Contenta F, Balbinot E, Petts JA, Read JI, Gieles M, Collins MLM, Peñarrubia J, Delorme M, Gualandris A (2018) Probing dark matter with star clusters: a dark matter core in the ultra-faint dwarf Eridanus II. MNRAS 476(3):3124–3136. https://doi.org/10.1093/mnras/sty424. arXiv:1705.01820 [astro-ph.GA]

Contopoulos G (2002) Order and chaos in dynamical astronomy. Springer, New York

Contopoulos G, Lukes-Gerakopoulos G, Apostolatos TA (2011) Orbits in a non-Kerr dynamical system. Int J Bifurcat Chaos 21(8):2261. https://doi.org/10.1142/S0218127411029768. arXiv:1108.5057 [gr-qc]

Copperwheat CM, Marsh TR, Littlefair SP, Dhillon VS, Ramsay G, Drake AJ, Gänsicke BT, Groot PJ, Hakala P, Koester D et al (2011) SDSS J0926+3624: the shortest period eclipsing binary star. MNRAS 410(2):1113–1129. https://doi.org/10.1111/j.1365-2966.2010.17508.x. arXiv:1008.1907 [astro-ph.SR]

Cornish N, Robson T (2017) Galactic binary science with the new LISA design. J Phys Conf Ser 840:012024. https://doi.org/10.1088/1742-6596/840/1/012024. arXiv:1703.09858 [astro-ph.IM]

Cornish NJ (2011) Detection strategies for extreme mass ratio inspirals. Class Quantum Grav 28 (9):094016. https://doi.org/10.1088/0264-9381/28/9/094016. arXiv:0804.3323 [gr-qc]

Cornish NJ, Crowder J (2005) LISA data analysis using Markov chain Monte Carlo methods. Phys Rev D 72(4):043005. https://doi.org/10.1103/PhysRevD.72.043005. arXiv:gr-qc/0506059 [astro-ph]

Cornish NJ, Larson SL (2003) LISA data analysis: source identification and subtraction. Phys Rev D 67 (10):103001. https://doi.org/10.1103/PhysRevD.67.103001. arXiv:astro-ph/0301548 [astro-ph]

Cornish NJ, Littenberg TB (2007) Tests of Bayesian model selection techniques for gravitational wave astronomy. Phys Rev D 76(8):083006. https://doi.org/10.1103/PhysRevD.76.083006. arXiv:0704. 1808 [gr-qc]

Cornish NJ, Shuman K (2020) Black hole hunting with LISA. Phys Rev D 101(12):124008. https://doi.org/ 10.1103/PhysRevD.101.124008. arXiv:2005.03610 [gr-qc]

Corrales L, Mills BS, Heinz S, Williger GM (2019) The X-ray variable sky as seen by MAXI: the future of dust-echo tomography with bright galactic X-ray bursts. ApJ 874(2):155. https://doi.org/10.3847/ 1538-4357/ab0c9b. arXiv:1903.08299 [astro-ph.HE]

Corrales LR, Haiman Z, MacFadyen A (2010) Hydrodynamical response of a circumbinary gas disc to black hole recoil and mass loss. MNRAS 404(2):947–962. https://doi.org/10.1111/j.1365-2966.2010. 16324.x. arXiv:0910.0014 [astro-ph.HE]

Coughlin MW, Dietrich T, Doctor Z, Kasen D, Coughlin S, Jerkstrand A, Leloudas G, McBrien O, Metzger BD, O'Shaughnessy R et al (2018) Constraints on the neutron star equation of state from AT2017gfo using radiative transfer simulations. MNRAS 480(3):3871–3878. https://doi.org/10.1093/mnras/ sty2174. arXiv:1805.09371 [astro-ph.HE]

Cresswell P, Dirksen G, Kley W, Nelson RP (2007) On the evolution of eccentric and inclined protoplanets embedded in protoplanetary disks. A&A 473(1):329–342. https://doi.org/10.1051/0004-6361: 20077666. arXiv:0707.2225 [astro-ph]

Cromartie HT, Fonseca E, Ransom SM, Demorest PB, Arzoumanian Z, Blumer H, Brook PR, DeCesar ME, Dolch T, Ellis JA et al (2020) Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar. Nat Astron 4:72–76. https://doi.org/10.1038/s41550-019-0880-2. arXiv:1904. 06759 [astro-ph.HE]

Croton DJ, Springel V, White SDM, De Lucia G, Frenk CS, Gao L, Jenkins A, Kauffmann G, Navarro JF, Yoshida N (2006) The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies. MNRAS 365(1):11–28. https://doi.org/10.1111/j.1365-2966. 2005.09675.x. arXiv:astro-ph/0508046 [astro-ph]

Cuadra J, Armitage PJ, Alexander RD, Begelman MC (2009) Massive black hole binary mergers within subparsec scale gas discs. MNRAS 393(4):1423–1432. https://doi.org/10.1111/j.1365-2966.2008. 14147.x. arXiv:0809.0311 [astro-ph]

Cunningham EC, Garavito-Camargo N, Deason AJ, Johnston KV, Erkal D, Laporte CFP, Besla G, Luger R, Sanderson RE (2020) Quantifying the stellar Halo’s response to the LMC’s infall with spherical harmonics. ApJ 898(1):4. https://doi.org/10.3847/1538-4357/ab9b88. arXiv:2006.08621 [astro-ph. GA]

Cusin G, Dvorkin I, Pitrou C, Uzan JP (2020) Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies. MNRAS 493(1):L1–L5. https://doi.org/10.1093/mnrasl/ slz182. arXiv:1904.07757 [astro-ph.CO]

Cutler C, Flanagan ÉE (1994) Gravitational waves from merging compact binaries: how accurately can one extract the binary’s parameters from the inspiral waveform? Phys Rev D 49(6):2658–2697. https:// doi.org/10.1103/PhysRevD.49.2658. arXiv:gr-qc/9402014 [gr-qc]
Cutler C, Berti E, Holley-Bockelmann K, Jani K, Kovetz ED, Larson SL, Littenberg T, McWilliams ST, Mueller G, Randall L et al (2019) What can we learn from multi-band observations of black hole binaries? BAAS 51(3):109 arXiv:1903.04069 [astro-ph.HE]

Dabringhausen J, Kroupa P, Baumgardt H (2009) A top-heavy stellar initial mass function in starbursts as an explanation for the high mass-to-light ratios of ultra-compact dwarf galaxies. MNRAS 394 (3):1529–1543. https://doi.org/10.1111/j.1365-2966.2009.14425.x. arXiv:0901.0915 [astro-ph.GA]

Dage KC, Zepf SE, Bahramian A, Strader J, Maccarone TJ, Peacock MB, Kundu A, Steele MM, Britt CT (2019) Slow decline and rise of the broad [O III] emission line in globular cluster black hole candidate RZ2109. MNRAS 489(4):4783–4790. https://doi.org/10.1093/mnras/stz2514. arXiv:1909.02683 [astro-ph.HE]

Dai L, McKinney JC, Roth N, Ramirez-Ruiz E, Miller MC (2018) A unified model for tidal disruption events. ApJ 859(2):L20. https://doi.org/10.3847/2041-8213/aab429. arXiv:1803.03265 [astro-ph.HE]

Dal Canton T, Mangiagli A, Noble SC, Schnittman J, Ptak A, Klein A, Sesana A, Camp J (2019) Detectability of modulated x-rays from LISA's supermassive black hole mergers. ApJ 886(2):146. https://doi.org/10.3847/1538-4357/ab505a

Dall'Osso S, Rossi EM (2013) Tidal torque induced by orbital decay in compact object binaries. MNRAS 428(1):518–531. https://doi.org/10.1093/mnras/sts037. arXiv:1203.3440 [astro-ph.HE]

Dall'Osso S, Rossi EM (2014) Constraining white dwarf viscosity through tidal heating in detached binary systems. MNRAS 443(2):1057–1064. https://doi.org/10.1093/mnras/stu901. arXiv:1308.1664 [astro-ph.HE]

Daly RA (2011) Estimates of black hole spin properties of 55 sources. MNRAS 414(2):1253–1262. https://doi.org/10.1111/j.1365-2966.2011.18452.x. arXiv:1103.0940 [astro-ph.CO]

Damour T, Gopakumar A (2006) Gravitational recoil during binary black hole coalescence using the effective one body approach. Phys Rev D 73(12):124006. https://doi.org/10.1103/PhysRevD.73.124006. arXiv:gr-qc/0602117 [gr-qc]

Dan M, Rosswog S, Guillochon J, Ramirez-Ruiz E (2011) Prelude to a double degenerate merger: the onset of mass transfer and its impact on gravitational waves and surface detonations. ApJ 737(2):89. https://doi.org/10.1088/0004-637X/737/2/89. arXiv:1101.5132 [astro-ph.HE]

D'Angelo G, Lubow SH, Bate MR (2006) Evolution of giant planets in eccentric disks. ApJ 652(2):1698–1714. https://doi.org/10.1086/508451. arXiv:astro-ph/0608355 [astro-ph]

Danielski C, Tamanini N (2020) Will gravitational waves discover the first extra-galactic planetary system? Int J Mod Phys D 29:2043007. https://doi.org/10.1142/S0218271820430075. arXiv:2007.07010 [astro-ph.IM]

Danielski C, Korol V, Tamanini N, Rossi EM (2019) Circumbinary exoplanets and brown dwarfs with the Laser Interferometer Space Antenna. A&A 632:A113. https://doi.org/10.1051/0004-6361/201936729. arXiv:1910.05414 [astro-ph.EP]

d'Ascoli S et al (2018) Electromagnetic emission from supermassive binary black holes approaching merger. ApJ 865:140. https://doi.org/10.3847/1538-4357/aa08b4. arXiv:1806.05697 [astro-ph.HE]

Datta S, Gupta A, Kastha S, Arun KG, Sathyaprakash BS (2021) Tests of general relativity using multiband observations of intermediate mass binary black hole mergers. Phys Rev D 103(2):024036. https://doi.org/10.1103/PhysRevD.103.024036. arXiv:2006.12137 [gr-qc]

Davé R, Anglés-Alcázar D, Narayanan D, Li Q, Rafieferantsoa MH, Appleby S (2019) SIMBA: cosmological simulations with black hole growth and feedback. MNRAS 486(2):2827–2849. https://doi.org/10.1093/mnras/stz937. arXiv:1901.10203 [astro-ph.GA]

Davies MB, Lin DNC (2020) Making massive stars in the Galactic Centre via accretion onto low-mass stars within an accretion disc. MNRAS https://doi.org/10.1093/mnras/staa2590 [astro-ph.GA]

Davies MB, Miller MC, Bellovary JM (2011) Supermassive black hole formation via gas accretion in nuclear stellar clusters. ApJ 740(2):L42. https://doi.org/10.1088/2041-8205/740/2/L42. arXiv:1106.5943 [astro-ph.CO]

Davies RI, Müller Sánchez F, Genzel R, Tacconi LJ, Hicks EKS, Friedrich S, Sternberg A (2007) A close look at star formation around active galactic nuclei. ApJ 671(2):1388–1412. https://doi.org/10.1086/523032. arXiv:0704.1374 [astro-ph]

Davis BL, Graham AW, Seigar MS (2017) Updating the (supermassive black hole mass)-(spiral arm pitch angle) relation: a strong correlation for galaxies with pseudobulges. MNRAS 471(2):2187–2203. https://doi.org/10.1093/mnras/stx1794. arXiv:1707.04001 [astro-ph.GA]
Davis BL, Graham AW, Cameron E (2018) Black hole mass scaling relations for spiral galaxies. II. $M_{BH-M_{tot}}$ and $M_{BH-M_{disk}}$. ApJ 869(2):113. https://doi.org/10.3847/1538-4357/aae820. arXiv:1810.04888 [astro-ph.GA]

Davis BL, Graham AW, Cameron E (2019) Black hole mass scaling relations for spiral galaxies. I. $M_{BH-M_{sph}}$. ApJ 873(1):85. https://doi.org/10.3847/1538-4357/aaf3b8. arXiv:1810.04887 [astro-ph.GA]

Davis BL, Graham AW, Combes F (2019) A consistent set of empirical scaling relations for spiral galaxies: the $(v_{max}, M_{oM})-(\sigma_0, M_{BH}, \phi)$ relations. ApJ 877(1):64. https://doi.org/10.3847/1538-4357/ab1aa4. arXiv:1901.06509 [astro-ph.GA]

Dayal P, Ferrara A (2018) Early galaxy formation and its large-scale effects. Phys Rep 780:1-64. https://doi.org/10.1016/j.physrep.2018.10.002. arXiv:1809.09136 [astro-ph.GA]

Dayal P, Rossi EM, Shiralilou B, Piana O, Choudhury TR, Volonteri M (2019) The hierarchical assembly of galaxies and black holes in the first billion years: predictions for the era of gravitational wave astronomy. MNRAS 486(2):2336-2350. https://doi.org/10.1093/mnras/stz897. arXiv:1810.11033 [astro-ph.GA]

De S, MacLeod M, Everson RW, Antoni A, Mandel I, Ramirez-Ruiz E (2020) Common envelope wind tunnel: the effects of binary mass ratio and implications for the accretion-driven growth of LIGO binary black holes. ApJ 897(2):130. https://doi.org/10.3847/1538-4357/ab9ac6. arXiv:1910.13333 [astro-ph.SR]

De Luca V, Franciolini G, Pani P, Riotto A (2020) Constraints on primordial black holes: the importance of accretion. Phys Rev D 102(4):043505. https://doi.org/10.1103/PhysRevD.102.043505. arXiv:2003.12589 [astro-ph.CO]

De Luca V, Franciolini G, Riotto A (2021) NANOGrav data hints at primordial black holes as dark matter. Phys Rev Lett 126(4):041303. https://doi.org/10.1103/PhysRevLett.126.041303. arXiv:2009.08268 [astro-ph.CO]

De Marco O, Passy JC, Moe M, Herwig F, Mac Low MM, Paxton B (2011) On the $\alpha$ formalism for the common envelope interaction. MNRAS 411(4):2277-2292. https://doi.org/10.1111/j.1365-2966.2010.17891.x. arXiv:1010.4374 [astro-ph.SR]

de Mink SE, Cantiello M, Langer N, Pols OR, Brott I, Yoon SC (2009) Rotational mixing in massive binaries. Detached short-period systems. A&A 497(1):243-253. https://doi.org/10.1051/0004-6361/200811439. arXiv:0902.1751 [astro-ph.SR]

De Rosa A, Uttley P, Gou L, Liu Y, Bambi C, Barret D, Belloni T, Berti E, Bianchi S, Caiazzo I et al (2019) Accretion in strong field gravity with eXTP. Sci China Phys Mech Astron 62(2):29504. https://doi.org/10.1007/s11433-018-9297-0. arXiv:1812.04022 [astro-ph.HE]

De Rosa A, Vignali C, Bogdanović T, Capelo PR, Charisi M, Dotti M, Husemann B, Lusso E, Mayer L, Paragi Z et al (2019) The quest for dual and binary supermassive black holes: a multi-messenger view. New A Rev 86:101525. https://doi.org/10.1016/j.newar.2020.101525. arXiv:2001.06293 [astro-ph.GA]

de Val-Borro M, Karovska M, Sasselov DD, Stone JM (2017) Three-dimensional hydrodynamical models of wind and outburst-related accretion in symbiotic systems. MNRAS 468(3):3408-3417. https://doi.org/10.1093/mnras/stx684. arXiv:1704.03460 [astro-ph.SR]

Deane RP, Paragi Z, Jarvis MJ, Coriat M, Bernardi G, Fender RP, Frey S, Heywood I, Klöckner HR, Grainge K et al (2014) A close-pair binary in a distant triple supermassive black hole system. Nature 511(7507):57-60. https://doi.org/10.1038/nature13454. arXiv:1406.6365 [astro-ph.GA]

Decarli R, Dotti M, Fumagalli M, Tsalmantza P, Montuori C, Lusso E, Hogg DW, Prochaska JX (2013) The nature of massive black hole binary candidates—I. Spectral properties and evolution. MNRAS 433(2):1492-1504. https://doi.org/10.1093/mnras/stt831. arXiv:1305.4941 [astro-ph.CO]

Decarli R, Dotti M, Mazzucchelli C, Montuori C, Volonteri M (2014) New insights on the recoiling/binary black hole candidate J0927+2943 via molecular gas observations. MNRAS 445(2):1558-1566. https://doi.org/10.1093/mnras/stu1810. arXiv:1409.1585 [astro-ph.GA]

Decarli R, Walter F, Venemans BP, Bañados E, Bertoldi F, Carilli C, Fan X, Farina EP, Mazzucchelli C, Riechers D et al (2018) An ALMA [C II] survey of 27 quasars at $z > 5.94$. ApJ 854(2):97. https://doi.org/10.3847/1538-4357/aaa5aa. arXiv:1801.02641 [astro-ph.GA]

Decarli R, Aravena M, Boogaard L, Carilli C, González-López J, Walter F, Cortes PC, Cox P, da Cunha E, Daddi E et al (2020) The ALMA spectroscopic survey in the hubble ultra deep field: multiband constraints on line-luminosity functions and the cosmic density of molecular gas. ApJ 902(2):110. https://doi.org/10.3847/1538-4357/abaa3b. arXiv:2009.10744 [astro-ph.GA]
DeGraf C, Sijacki D (2020) Cosmological simulations of massive black hole seeds: predictions for next-generation electromagnetic and gravitational wave observations. MNRAS 491(4):4973-4992. https://doi.org/10.1093/mnras/stz3309. arXiv:1906.11271 [astro-ph.GA]

DeGraf C, Sijacki D, Di Matteo T, Holley-Bockelmann K, Snyder G, Springel V (2021) Morphological evolution of supermassive black hole merger hosts and multimessenger signatures. MNRAS 503 (3):3629-3642. https://doi.org/10.1093/mnras/stab721. arXiv:2012.00775 [astro-ph.GA]

del Valle L, Volonteri M (2018) The effect of AGN feedback on the migration time-scale of supermassive black holes binaries. MNRAS 480(1):439-450. https://doi.org/10.1093/mnras/sty1815. arXiv:1807.03844 [astro-ph.GA]

del Valle L, Escala A, Maureira-Fredes C, Molina J, Cuadra J, Amaro-Seoane P (2015) Supermassive black holes in a star-forming gaseous circumnuclear disk. ApJ 811(1):59. https://doi.org/10.1088/0004-637X/811/1/59. arXiv:1503.01664 [astro-ph.GA]

Deloye CJ, Taam RE (2006) The turn-on of mass transfer in AM CVn binaries: implications for RX J0806+1527 and RX J1914+2456. ApJ 649(2):L99-L102. https://doi.org/10.1086/508372. arXiv:astro-ph/0608442 [astro-ph]

Deme B, Hoang BM, Naoz S, Kocsis B (2020) Detecting Kozai-Lidov imprints on the gravitational waves of intermediate-mass black holes in galactic nuclei. ApJ 901(2):125. https://doi.org/10.3847/1538-4357/abafa3. arXiv:2005.03677 [astro-ph.HE]

Deme B, Meiron Y, Kocsis B (2020) Intermediate-mass black holes’ effects on compact object binaries. ApJ 892(2):130. https://doi.org/10.3847/1538-4357/ab7921. arXiv:1909.04678 [astro-ph.GA]

Derdzinski A, D'Orazio D, Duffell P, Haiman Z, MacFadyen A (2021) Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band. MNRAS 501(3):3540-3557. https://doi.org/10.1093/mnras/staa3976. arXiv:2005.11333 [astro-ph.HE]

Derdzinski AM, D'Orazio D, Duffell P, Haiman Z, MacFadyen A (2019) Probing gas disc physics with LISA: simulations of an intermediate mass ratio inspiral in an accretion disc. MNRAS 486(2):2754-2765. https://doi.org/10.1093/mnras/stz1026. arXiv:1810.03623 [astro-ph.HE]

DESI Collaboration, Aghamousa A, Aguilar J, Ahlen S, Alam S, Allen LE, Allende Prieto C, Annis J, Bailey S, Balland C et al (2016) The DESI experiment part I: science, targeting, and survey design. arXiv e-prints arXiv:1611.00036 [astro-ph.IM]

Dessart L, Burrows A, Ott CD, Livne E, Yoon SC, Langer N (2006) Multidimensional simulations of the accretion-induced collapse of white dwarfs to neutron stars. ApJ 644(2):1063-1084. https://doi.org/10.1086/503626. arXiv:astro-ph/0601603 [astro-ph]

Destounis K, Kokkotas KD (2021) Gravitational-wave glitches: resonant islands and frequency jumps in nonintegrable extreme-mass-ratio inspirals. Phys Rev D 104(6):064023. https://doi.org/10.1103/PhysRevD.104.064023. arXiv:2108.02782 [gr-qc]

Destounis K, Suvorov AG, Kokkotas KD (2020) Testing spacetime symmetry through gravitational waves from extreme-mass-ratio inspirals. Phys Rev D 102:064041. https://doi.org/10.1103/PhysRevD.102.064041

Destounis K, Suvorov AG, Kokkotas KD (2021) Gravitational wave glitches in chaotic extreme-mass-ratio inspirals. Phys Rev Lett 126(14):141102. https://doi.org/10.1103/PhysRevLett.126.141102. arXiv:2103.05643 [gr-qc]

Desvignes G, Caballero RN, Lentati L, Verbiest JPW, Champion DJ, Stappers BW, Janssen GH, Lazarus P, Oslowski S, Babak S et al (2016) High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array. MNRAS 458(3):3341-3380. https://doi.org/10.1093/mnras/stw483. arXiv:1602.08511 [astro-ph.HE]

Devecchi B, Volonteri M (2009) Formation of the first nuclear clusters and massive black holes at high redshift. ApJ 694(1):302-313. https://doi.org/10.1088/0004-637X/694/1/302. arXiv:0810.1057 [astro-ph]

Dewdney PE, Hall PJ, Schilizzi RT, Lazio TJLW (2009) The square kilometre array. IEEE Proc 97 (8):1482-1496. https://doi.org/10.1109/JPROC.2009.2021005

Dewi JDM, Pols OR (2003) The late stages of evolution of helium star-neutron star binaries and the formation of double neutron star systems. MNRAS 344(2):629-643. https://doi.org/10.1046/j.1365-8711.2003.06844.x. arXiv:astro-ph/0306066 [astro-ph]

Dewi JDM, Podsiadlowski P, Pols OR (2005) The spin period-eccentricity relation of double neutron stars: evidence for weak supernova kicks? MNRAS 363(1):L71-L75. https://doi.org/10.1111/j.1745-3933.2005.00085.x. arXiv:astro-ph/0507628 [astro-ph]
Di Carlo UN, Giacobbo N, Mapelli M, Pasquato M, Spera M, Wang L, Haardt F (2019) Merging black holes in young star clusters. MNRAS 487(2):2947-2960. https://doi.org/10.1093/mnras/stz1453. arXiv:1901.00863 [astro-ph.HE]

Di Carlo UN, Mapelli M, Bouffanais Y, Giacobbo N, Santoliquido F, Bressan Ar, Spera M, Haardt F (2020) Binary black holes in the pair instability mass gap. MNRAS 497(1):1043-1049. https://doi.org/10.1093/mnras/staa1997. arXiv:1911.01434 [astro-ph.HE]

Di Carlo UN, Mapelli M, Giacobbo N, Spera M, Bouffanais Y, Rastello S, Santoliquido F, Pasquato M, Ballone Ar, Trani AA et al (2020) Binary black holes in young star clusters: the impact of metallicity. MNRAS 498(1):495-506. https://doi.org/10.1093/mnras/staa2286. arXiv:2004.09525 [astro-ph.HE]

Di Carlo UN, Mapelli M, Pasquato M, Rastello S, Ballone A, Dall'Amico M, Giacobbo N, Iorio G, Spera M, Torniamenti S et al (2021) Intermediate-mass black holes from stellar mergers in young star clusters. MNRAS 507(4):5132-5143. https://doi.org/10.1093/mnras/stab2390. arXiv:2105.01085 [astro-ph.GA]

Di Cintio A, Tremmel M, Governato F, Pontzen A, Zavala J, Fry Ae Bastidas, Brooks A, Vogelsberger M (2017) A rumble in the dark: signatures of self-interacting dark matter in supermassive black hole dynamics and galaxy density profiles. MNRAS 469(3):2845-2854. https://doi.org/10.1093/mnras/stx1043. arXiv:1701.04410 [astro-ph.GA]

Di Matteo T, Springel V, Hernquist L (2005) Energy input from quasars regulates the growth and activity of black holes and their host galaxies. Nature 433(7026):604-607. https://doi.org/10.1038/nature03335. arXiv:astro-ph/0502199 [astro-ph]

Dieball A, Knigge C, Zurek DR, Shara MM, Long KS, Charles PA, Hannikainen DC, van Zyl L (2005) An ultracompact X-ray binary in the globular cluster M15 (NGC 7078). ApJ 634(1):L105-L108. https://doi.org/10.1086/498712. arXiv:astro-ph/0510430 [astro-ph]

Dijkstra M, Haiman Z, Mesinger A, Wyithe JSB (2008) Fluctuations in the high-redshift Lyman-Werner background: close halo pairs as the origin of supermassive black holes. MNRAS 391:1961-1972. https://doi.org/10.1111/j.1365-2966.2008.14031.x. arXiv:0810.0014

Dijkstra M, Ferrara A, Mesinger A (2014) Feedback-regulated supermassive black hole seed formation. MNRAS 442(3):2036-2047. https://doi.org/10.1093/mnras/stu1007. arXiv:1405.6743 [astro-ph.GA]

Dittmann AJ, Miller MC (2020) Star formation in accretion discs and SMBH growth. MNRAS 493 (3):3732-3743. https://doi.org/10.1093/mnras/staa463. arXiv:1911.08685 [astro-ph.HE]

Domcke V, Muia F, Pieroni M, Witkowski LT (2017) PBH dark matter from axion inflation. J Cosmol Astropart Phys 07:048. https://doi.org/10.1088/1475-7516/2017/07/048. arXiv:1704.03464 [astro-ph.CO]

Dominik M, Belczynski K, Fryer C, Holz DE, Berti E, Bulik T, el Mand I, O'Shaughnessy R (2013) Double compact objects. II. Cosmological merger rates. ApJ 779(1):72. https://doi.org/10.1088/0004-637X/779/1/72. arXiv:1308.1546 [astro-ph.HE]

D'Orazio DJ, Di Stefano R (2018) Periodic self-lensing from accreting massive black hole binaries. MNRAS 474(3):2975-2986. https://doi.org/10.1093/mnras/stx2936. arXiv:1707.02335 [astro-ph.HE]

D'Orazio DJ, Loeb A (2018) Repeated imaging of massive black hole binary orbits with millimeter interferometry: measuring black hole masses and the Hubble constant. ApJ 863(2):185. https://doi.org/10.3847/1538-4357/aad413. arXiv:1712.02362 [astro-ph.HE]

D'Orazio DJ, Samsing J (2018) Black hole mergers from globular clusters observable by LISA II. Resolved eccentric sources and the gravitational wave background. MNRAS 481(4):4775-4785. https://doi.org/10.1093/mnras/sty2568. arXiv:1805.06194 [astro-ph.HE]

D'Orazio DJ, Haiman Z, MacFadyen A (2013) Accretion into the central cavity of a circumbinary disc. MNRAS 436(4):2997-3020. https://doi.org/10.1093/mnras/stt1787. arXiv:1210.0536 [astro-ph.GA]

D'Orazio DJ, Haiman Z, Schiminovich D (2015) Relativistic boost as the cause of periodicity in a massive black-hole binary candidate. Nature 525(7569):351-353. https://doi.org/10.1038/nature15262. arXiv:1509.04301 [astro-ph.HE]

D'Orazio DJ, Haiman Z, Duffell P, MacFadyen A, Farris B (2016) A transition in circumbinary accretion discs at a binary mass ratio of 1:25. MNRAS 459(3):2379-2393. https://doi.org/10.1093/mnras/stw792. arXiv:1512.05788 [astro-ph.HE]

Dosopoulou F, Antonini F (2017) Dynamical friction and the evolution of supermassive black hole binaries: the final hundred-parsec problem. ApJ 840(1):31. https://doi.org/10.3847/1538-4357/aa6b58. arXiv:1611.06573 [astro-ph.GA]
Dotti M, Colpi M, Haardt F (2006) Laser interferometer space antenna double black holes: dynamics in gaseous nuclear discs. MNRAS 367(1):103–112. https://doi.org/10.1111/j.1365-2966.2005.09956.x. arXiv:astro-ph/0509813 [astro-ph]

Dotti M, Colpi M, Haardt F, Mayer L (2007) Supermassive black hole binaries in gaseous and stellar circumnuclear discs: orbital dynamics and gas accretion. MNRAS 379(3):956–962. https://doi.org/10.1111/j.1365-2966.2007.12010.x. arXiv:astro-ph/0612505 [astro-ph]

Dotti M, Volonteri M, Perego A, Colpi M, Ruszkowski M, Haardt F (2010) Dual black holes in merger remnants—II. Spin evolution and gravitational recoil. MNRAS 402(1):682–690. https://doi.org/10.1111/j.1365-2966.2009.15922.x. arXiv:0910.5729 [astro-ph.HE]

Dotti M, Sesana A, Decarli R (2012) Massive black hole binaries: dynamical evolution and observational signatures. Adv Astron 2012:940568. https://doi.org/10.1155/2012/940568. arXiv:1111.0664 [astro-ph.CO]

Dotti M, Colpi M, Pallini S, Perego A, Volonteri M (2013) On the orientation and magnitude of the black hole spin in galactic nuclei. ApJ 762(2):68. https://doi.org/10.1088/0004-637X/762/2/68. arXiv:1211.4871 [astro-ph.CO]

Dovciak M, Matt G, Bianchi S, Boller T, Brenneman L, Bursa M, D'Ai A, di Salvo T, de Marco B, Goosmann R et al (2013) The hot and energetic universe: the close environments of supermassive black holes. arXiv e-prints arXiv:1306.2331 [astro-ph.HE]

Dovčiak M, Muleri F, Goosmann RW, Karas V, Matt G (2008) Thermal disc emission from a rotating black hole: X-ray polarization signatures. MNRAS 391(1):32–38. https://doi.org/10.1111/j.1365-2966.2008.13872.x. arXiv:0809.0418 [astro-ph]

Drasco S (2009) Verifying black hole orbits with gravitational spectroscopy. Phys Rev D 79(10):104016. https://doi.org/10.1103/PhysRevD.79.104016. arXiv:0711.4644 [gr-qc]

du Buisson L, Marchant P, Podsiadlowski P, Kobayashi C, Abdalla FB, Taylor P, Mandel I, de Mink SE, Moriya TJ, Langer N (2020) Cosmic rates of black hole mergers and pair-instability supernovae from chemically homogeneous binary evolution. MNRAS 499:5941–5959. https://doi.org/10.1093/mnras/sta3225. arXiv:2002.11630 [astro-ph.HE]

Dubois Y, Devriendt J, Slyz A, Teyssier R (2012) Self-regulated growth of supermassive black holes by a dual jet-heating active galactic nucleus feedback mechanism: methods, tests and implications for cosmological simulations. MNRAS 420(3):2662–2683. https://doi.org/10.1111/j.1365-2966.2011.20236.x. arXiv:1108.0110 [astro-ph.CO]

Dubois Y, Pichon C, Devriendt J, Silk J, Haehnelt M, Kimm T, Slyz A (2013) Blowing cold flows away: the impact of early AGN activity on the formation of a brightest cluster galaxy progenitor. MNRAS 428(4):2885–2900. https://doi.org/10.1093/mnras/sts224. arXiv:1206.5838 [astro-ph.CO]

Dubois Y, Pichon C, Welker C, Le Borgne D, Devriendt J, Laigle C, Codis S, Pogosyan D, Arnouts S, Benabed K et al (2014) Dancing in the dark: galactic properties trace spin swings along the cosmic web. MNRAS 444(2):1453–1468. https://doi.org/10.1093/mnras/stu1227. arXiv:1402.1165 [astro-ph.CO]

Dubois Y, Volonteri M, Silk J (2014) Black hole evolution—III. Statistical properties of mass growth and spin evolution using large-scale hydrodynamical cosmological simulations. MNRAS 440(2):1590–1606. https://doi.org/10.1093/mnras/stu373. arXiv:1304.4583 [astro-ph.CO]

Dubois Y, Volonteri M, Silk J, Devriendt J, Slyz A, Teyssier R (2015) Black hole evolution—I. Supernova-regulated black hole growth. MNRAS 452(2):1502–1518. https://doi.org/10.1093/mnras/stv1416. arXiv:1504.00018 [astro-ph.GA]

Dubois Y, Beckmann R, Bournaud F, Choi H, Devriendt J, Jackson R, Kaviraj S, Kimm T, Kraljic K, Laigle C et al (2021) Introducing the NEWHORIZON simulation: galaxy properties with resolved internal dynamics across cosmic time. A&A 651:A109. https://doi.org/10.1051/0004-6361/202039429. arXiv:2009.10578 [astro-ph.GA]

Duechting N (2004) Supermassive black holes from primordial black hole seeds. Phys Rev D 70:064015. https://doi.org/10.1103/PhysRevD.70.064015. arXiv:astro-ph/0406260

Duez MD, Zlochower Y (2019) Numerical relativity of compact binaries in the 21st century. Rep Prog Phys 82(1):016902. https://doi.org/10.1088/1361-6633/aadb16. arXiv:1808.06011 [gr-qc]

Duffell PC (2015) Halting migration: numerical calculations of corotation torques in the weakly nonlinear regime. ApJ 806(2):182. https://doi.org/10.1088/0004-637X/806/2/182. arXiv:1412.8092 [astro-ph. EP]

Duffell PC, D'Orazio D, Derdzinski A, Haiman Z, MacFadyen A, Rosen AL, Zrake J (2020) Circumbinary disks: accretion and torque as a function of mass ratio and disk viscosity. ApJ 901(1):25. https://doi.org/10.3847/1538-4357/abab95. arXiv:1911.05506 [astro-ph.SR]
Dullo BT (2019) The most massive galaxies with large depleted cores: structural parameter relations and black hole masses. ApJ 886(2):80. https://doi.org/10.3847/1538-4357/ab4d4f. arXiv:1910.10240 [astro-ph.GA]

Dullo BT, Graham AW (2013) Central stellar mass deficits in the bulges of local lenticular galaxies, and the connection with compact z −1.5 galaxies. ApJ 768(1):36. https://doi.org/10.1088/0004-637X/768/1/ 36. arXiv:1303.1273 [astro-ph.CO]

Dullo BT, Graham AW (2014) Depleted cores, multicomponent fits, and structural parameter relations for luminous early-type galaxies. MNRAS 444(3):2700–2722. https://doi.org/10.1093/mnras/stu1590. arXiv:1310.5867 [astro-ph.CO]

Duncan MJ, Lissauer JJ (1998) The effects of post-main-sequence solar mass loss on the stability of our planetary system. Icarus 134(2):303–310. https://doi.org/10.1006/icar.1998.5962

Dunhill AC, Alexander RD, Armitage PJ (2013) A limit on eccentricity growth from global 3D simulations of disc-planet interactions. MNRAS 428(4):3072–3082. https://doi.org/10.1093/mnras/sts254. arXiv: 1210.6035 [astro-ph.EP]

Dunlop JS, Abraham RG, Ashby MLN, Bagley M, Best PN, Bongiorno A, Bouwens R, Bowler RAA, Brammer G, Bremer M, et al (2021) PRIMER: public release IMaging for extragalactic research. JWST proposal. Cycle 1, ID. #1837

Dunn G, Bellovary J, Holley-Bockelmann K, Christensen C, Quinn T (2018) Sowing black hole seeds: direct collapse black hole formation with realistic Lyman–Werner radiation in cosmological simulations. ApJ 861(1):39. https://doi.org/10.3847/1538-4357/aac7c2. arXiv:1803.01007 [astro-ph. GA]

Dunn G, Holley-Bockelmann K, Bellovary J (2020) The role of gravitational recoil in the assembly of massive black hole seeds. ApJ 896(1):72. https://doi.org/10.3847/1538-4357/ab7cd2. arXiv:2002. 04740 [astro-ph.GA]

Dvorkin I, Uzan JP, Vangioni E, Silk J (2016) Synthetic model of the gravitational wave background from evolving binary compact objects. Phys Rev D 94(10):103011. https://doi.org/10.1103/PhysRevD.94. 103011. arXiv:1607.06818 [astro-ph.HE]

Dvorkin I, Vangioni E, Silk J, Uzan JP, Olive KA (2016) Metallicity-constrained merger rates of binary black holes and the stochastic gravitational wave background. MNRAS 461(4):3877–3885. https:// doi.org/10.1093/mnras/stw1477. arXiv:1604.04288 [astro-ph.HE]

Eatough RP, Kramer M, Lyne AG, Keith MJ (2013) A coherent acceleration search of the Parkes multibeam pulsar survey—techniques and the discovery and timing of 16 pulsars. MNRAS 431 (1):292–307. https://doi.org/10.1093/mnras/stt161. arXiv:1301.6346 [astro-ph.IM]

Ebisuzaki T, Makino J, Okumura SK (1991) Merging of two galaxies with central black holes. Nature 354 (6350):212–214. https://doi.org/10.1038/354212a0

Ebisuzaki T, Makino J, Tsuru TG, Funato Y, Portegies Zwart S, Hut P, McMillan S, Matsushita S, Matsumoto H, Kawabe R (2001) Missing link found? The “runaway” path to supermassive black holes. ApJ 562(1):L19–L22. https://doi.org/10.1086/338118. arXiv:astro-ph/0106252 [astro-ph]

Eda K, Itoh Y, Kuroyanagi S, Silk J (2013) New probe of dark-matter properties: gravitational waves from an intermediate-mass black hole embedded in a dark-matter minispike. Phys Rev Lett 110 (22):221101. https://doi.org/10.1103/PhysRevLett.110.221101. arXiv:1301.5971 [gr-qc]

Edlund JA, Tinto M, Królak A, Nelemans G (2005) White-dwarf white-dwarf galactic background in the LISA data. Phys Rev D 71(12):122003. https://doi.org/10.1103/PhysRevD.71.122003. arXiv:gr-qc/ 0504112 [gr-qc]

Edwards LOV, Patton DR (2012) Close companions to brightest cluster galaxies: support for minor mergers and downsizing. MNRAS 425(1):287–295. https://doi.org/10.1111/j.1365-2966.2012.21457. x. arXiv:1206.1612 [astro-ph.CO]

Eggleton P (2006) Evolutionary processes in binary and multiple stars. Cambridge University Press, Cambridge

Eggleton PP (1983) Aproximations to the radii of Roche lobes. ApJ 268:368–369. https://doi.org/10.1086/ 160960

Eilon E, Kupi G, Alexander T (2009) The efficiency of resonant relaxation around a massive black hole. ApJ 698(1):641–647. https://doi.org/10.1088/0004-637X/698/1/641. arXiv:0807.1430 [astro-ph]

Elbert OD, Bullock JS, Kaplinghat M (2018) Counting black holes: the cosmic stellar remnant population and implications for LIGO. MNRAS 473(1):1186–1194. https://doi.org/10.1093/mnras/stx1959. arXiv:1703.02551 [astro-ph.GA]

Eldridge JJ, Stanway ER (2016) BPASS predictions for binary black hole mergers. MNRAS 462(3):3302– 3313. https://doi.org/10.1093/mnras/stw1772. arXiv:1602.03790 [astro-ph.HE]
Enoki M, Inoue KT, Nagashima M, Sugiyama N (2005) Gravitational waves from coalescing supermassive black hole binaries in a hierarchical galaxy formation model. Annu Rep Natl Astron Observ Jpn 7:34 arXiv:astro-ph/0502529 [astro-ph]

Eracleous M, Boroson TA, Halpern JP, Liu J (2012) A large systematic search for close supermassive binary and rapidly recoiling black holes. ApJS 201(2):23. https://doi.org/10.1088/0067-0049/201/2/23. arXiv:1106.2952 [astro-ph.CO]

Espaillat C, Patterson J, Warner B, Woudt P (2005) The helium-rich cataclysmic variable ES Ceti. PASP 117(828):189–198. https://doi.org/10.1086/427959. arXiv:astro-ph/0412068 [astro-ph]

Euclid Collaboration, Barnett R, Warren SJ, Mortlock DJ, Cuby JG, Conselice C, Hewett PC, Willott CJ, Auricchio N, Balaguera-Antolinez A et al (2019) Euclid preparation. V. Predicted yield of redshift $7<z<9$ quasars from the wide survey. A&A 631:A85. https://doi.org/10.1051/0004-6361/201936427. arXiv:1908.04310 [astro-ph.GA]

Everson RW, MacLeod M, De S, Macias P, Ramirez-Ruiz E (2020) Common envelope wind tunnel: range of applicability and self-similarity in realistic stellar envelopes. ApJ 899(1):77. https://doi.org/10.3847/1538-4357/aba75c. arXiv:2006.07471 [astro-ph.SR]

Fabian AC (2012) Observational evidence of active galactic nuclei feedback. ARA&A 50:455–489. https://doi.org/10.1146/annurev-astro-081811-125521. arXiv:1204.4114 [astro-ph.CO]

Fabian AC, Pringle JE, Rees MJ (1975) Tidal capture formation of binary systems and X-ray sources in globular clusters. MNRAS 172:15. https://doi.org/10.1093/mnras/172.1.15P

Fabian AC, Iwasawa K, Reynolds CS, Young AJ (2000) Broad iron lines in active galactic nuclei. PASP 112(775):1145–1161. https://doi.org/10.1086/316610. arXiv:astro-ph/0004366 [astro-ph]

Fabj G, Nasim SS, Caban F, Ford KES, McKernan B, Bellovary JM (2020) Aligning nuclear cluster orbits with an active galactic nucleus accretion disk. MNRAS 499(2). https://doi.org/10.1093/mnras/staa3004. arXiv:2006.11229 [astro-ph.GA]

Fabrycky D, Tremaine S (2007) Shrinking binary and planetary orbits by Kozai cycles with tidal friction. ApJ 669(2):1298–1315. https://doi.org/10.1086/521702. arXiv:0705.4285 [astro-ph]

Fairhurst S (2009) Triangulation of gravitational wave sources with a network of detectors. New J Phys 11:123006

Fakhouri O, Ma CP, Boylan-Kolchin M (2010) The merger rates and mass assembly histories of dark matter haloes in the two Millennium simulations. MNRAS 406(4):2267–2278. https://doi.org/10.1111/j.1365-2966.2010.16859.x. arXiv:1001.2304 [astro-ph.CO]

Falta D, Fisher R, Khanna G (2011) Gravitational wave emission from the single-degenerate channel of type Ia supernovae. Phys Rev Lett 106(20):201103. https://doi.org/10.1103/PhysRevLett.106.201103. arXiv:1011.6387 [astro-ph.HE]

Fan X, Strauss MA, Schneider DP, Becker RH, White RL, Haiman Z, Gregg M, Pentericci L, Grebel EK, Narayanan VK et al (2003) A survey of $z > 5.7$ quasars in the Sloan digital sky survey. II. Discovery of three additional quasars at $z > 6$. AJ 125(4):1649–1659. https://doi.org/10.1086/368246. arXiv:astro-ph/0301135 [astro-ph]

Fan X, Carilli CL, Keating B (2006) Observational constraints on cosmic reionization. ARA&A 44(1):415–462. https://doi.org/10.1146/annurev.astro.44.051905.092514. arXiv:astro-ph/0602375 [astro-ph]

Fan X, Barth A, Banados E, De Rosa G, Decarli R, Eilers AC, Farina EP, Greene J, Habouzit M, Jiang L et al (2019) The first luminous quasars and their host galaxies. BAAS 51(3):121 arXiv:1903.04078 [astro-ph.GA]

Farihi J, Becklin EE, Zuckerman B (2005) Low-luminosity companions to white dwarfs. ApJS 161(2):394–428. https://doi.org/10.1086/444362. arXiv:astro-ph/0506017 [astro-ph]

Farihi J, Jura M, Zuckerman B (2009) Infrared signatures of disrupted minor planets at white dwarfs. ApJ 694(2):805–819. https://doi.org/10.1088/0004-637X/694/2/805. arXiv:0901.0973 [astro-ph.EP]

Farmer AJ, Phinney ES (2003) The gravitational wave background from cosmological compact binaries. MNRAS 346(4):1197–1214. https://doi.org/10.1111/j.1365-2966.2003.07176.x. arXiv:astro-ph/0304393 [astro-ph]

Farmer R, Renzo M, de Mink SE, Marchant P, Justham S (2019) Mind the gap: the location of the lower edge of the pair-instability supernova black hole mass gap. ApJ 887(1):53. https://doi.org/10.3847/1538-4357/ab518b. arXiv:1910.12874 [astro-ph.SR]

Farr WM, Stevenson S, Miller MC, Mandel I, Farr B, Vecchio A (2017) Distinguishing spin-aligned and isotropic black hole populations with gravitational waves. Nature 548:426–429. https://doi.org/10.1038/nature23453. arXiv:1706.01385 [astro-ph.HE]
Farris BD, Liu YT, Shapiro SL (2010) Binary black hole mergers in gaseous environments: “Binary Bondi” and “binary Bondi–Hoyle–Lyttleton” accretion. *Phys Rev D* 81(8):084008. https://doi.org/10.1103/PhysRevD.81.084008. arXiv:0912.2096 [astro-ph.HE]

Farris BD, Gold R, Paschalidis V, Etienne ZB, Shapiro SL (2012) Binary black-hole mergers in magnetized disks: simulations in full general relativity. *Phys Rev Lett* 109(22):221102. https://doi.org/10.1103/PhysRevLett.109.221102. arXiv:1207.3354 [astro-ph.HE]

Farris BD, Duffell P, MacFadyen AI, Haiman Z (2015) Binary black hole accretion during inspiral and merger. MNRAS 447:L80–L84. https://doi.org/10.1093/mnrasl/slu184. arXiv:1409.5124 [astro-ph. HE]

Farris BD, Duffell P, MacFadyen AI, Haiman Z (2015) Characteristic signatures in the thermal emission from accreting binary black holes. MNRAS 446:L36–L40. https://doi.org/10.1093/mnrasl/slu160. arXiv:1406.0007 [astro-ph.HE]

Farrow N, Zhu XJ, Thrane E (2019) The mass distribution of galactic double neutron stars. ApJ 876(1):18. https://doi.org/10.3847/1538-4357/ab12e3. arXiv:1902.03300 [astro-ph.HE]

Faulkner J (1971) Ultrashort-period binaries, gravitational radiation, and mass transfer. I. The standard model, with applications to WZ Sagittae and Z camelopardalis. ApJ 170:L99. https://doi.org/10.1086/180848

Feng H, Soria R (2011) Ultraluminous X-ray sources in the Chandra and XMM-Newton era. New A Rev 55(5):166–183. https://doi.org/10.1016/j.newar.2011.08.002. arXiv:1109.1610 [astro-ph.HE]

Fernández R, Metzger BD (2013) Nuclear dominated accretion flows in two dimensions. I. Torus evolution with parametric microphysics. ApJ 763(2):108. https://doi.org/10.1088/0004-637X/763/2/108. arXiv:1209.2712 [astro-ph.HE]

Fernandez R, Bryan GL, Haiman Z, Li M (2014) H₂ suppression with shocking inflows: testing a pathway for supermassive black hole formation. MNRAS 439:3798–3807. https://doi.org/10.1093/mnras/stu230. arXiv:1401.5803 [astro-ph.CO]

Ferrara A, Salvadori S, Yue B, Schleicher D (2014) Initial mass function of intermediate-mass black hole seeds. MNRAS 443(3):2410–2425. https://doi.org/10.1093/mnras/stu1280. arXiv:1406.6685 [astro-ph.GA]

Ferrarese L, Merritt D (2000) A fundamental relation between supermassive black holes and their host galaxies. ApJ 539(1):L9–L12. https://doi.org/10.1086/312838. arXiv:astro-ph/0006053 [astro-ph]

Ferrario L, de Martino D, Gänsicke BT (2015) Magnetic white dwarfs. Space Sci Rev 191(1–4):111–169. https://doi.org/10.1007/s11214-015-0152-0. arXiv:1504.08072 [astro-ph.SR]

Fiacconi D, Mayer L, Roškar R, Colpi M (2013) Massive black hole pairs in clumpy, self-gravitating circumnuclear disks: stochastic orbital decay. ApJ 777(1):L14. https://doi.org/10.1088/2041-8205/777/1/L14. arXiv:1307.0822 [astro-ph.CO]

Fiacconi D, Mayer L, Madau P, Lupi A, Dotti M, Haardt F (2017) Young and turbulent: the early life of massive galaxy progenitors. MNRAS 467(4):4080–4100. https://doi.org/10.1093/mnras/stx335. arXiv:1609.09499 [astro-ph.GA]

Fiacconi D, Sijacki D, Pringle JE (2018) Galactic nuclei evolution with spinning black holes: method and implementation. MNRAS 477(3):3807–3835. https://doi.org/10.1093/mnras/sty893. arXiv:1712.00023 [astro-ph.GA]

Fink M, Röpke FK, Hillebrandt W, Seitenzahl IR, Sim SA, Kromer M (2010) Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core? A&A 514:A53. https://doi.org/10.1051/0004-6361/200913892. arXiv:1002.2173 [astro-ph.SR]

Finkelstein SL, Papovich C, Pirzkal N, Bagley M, Berg D, Castellano M, Chavez Ortiz OA, Chworowsky K, Dave R, Dickinson M et al (2021) The Webb deep extragalactic exploratory public (WDEEP) survey: feedback in low-mass galaxies from cosmic dawn to dusk. JWST proposal. Cycle 1, ID. #2079

Fiore F, Puccetti S, Brusa M, Salvato M, Zamorani G, Aldcroft T, Aussel H, Brunner H, Capak P, Cappelluti N et al (2009) Chasing highly obscured QSOs in the COSMOS field. ApJ 693(1):447–462. https://doi.org/10.1088/0004-637X/693/1/447. arXiv:0810.0720 [astro-ph]

Fitchett MJ (1983) The influence of gravitational wave momentum losses on the centre of mass motion of a Newtonian binay system. MNRAS 203:1049–1062. https://doi.org/10.1093/mnras/203.4.1049

Flanagan ÉÉ, Hinderer T (2008) Constraining neutron-star tidal Love numbers with gravitational-wave detectors. Phys Rev D 77(2):021502. https://doi.org/10.1103/PhysRevD.77.021502. arXiv:0709.1915 [astro-ph]
Flanagan ÉÉ, Hinderer T (2012) Transient resonances in the inspirals of point particles into black holes. Phys Rev Lett 109(7):071102. https://doi.org/10.1103/PhysRevLett.109.071102. arXiv:1009.4923 [gr-qc]

Fluri J, Kacprzak T, Lucchi A, Refregier A, Amara A, Hofmann T, Schneider A (2019) Cosmological constraints with deep learning from KiDS-450 weak lensing maps. Phys Rev D 100(6):063514. https://doi.org/10.1103/PhysRevD.100.063514. arXiv:1906.03156 [astro-ph.CO]

Fontaine G, Brassard P, Green EM, Charpinet S, Dufour P, Hubeny I, Steeghs D, Aerts C, Randall SK, Bergeron P et al (2011) Discovery of a new AM CVn system with the Kepler satellite. ApJ 726(2):92. https://doi.org/10.1088/0004-637X/726/2/92

Fontecilla C, Chen X, Cuadra J (2017) A second decoupling between merging binary black holes and the inner disc—impact on the electromagnetic counterpart. MNRAS 468(1):L50–L54. https://doi.org/10.1093/mnrasl/slw258. arXiv:1610.09382 [astro-ph.HE]

Ford EB, Kozinsky B, Rasio FA (2000) Secular evolution of hierarchical triple star systems. ApJ 535 (1):385–401. https://doi.org/10.1086/308815

Fouvry JB, Bar-Or B, Chavanis PH (2019) Vector resonant relaxation of stars around a massive black hole. ApJ 883(2):161. https://doi.org/10.3847/1538-4357/ab2f78. arXiv:1812.07053 [astro-ph.GA]

Fragione G (2022) Mergers of supermassive and intermediate-mass black holes in galactic nuclei from disruptions of star clusters. ApJ 939:97. https://doi.org/10.3847/1538-4357/ac98b6. arXiv:2202.05618 [astro-ph.HE]

Fragione G, Kocsis B (2019) Black hole mergers from quadruples. MNRAS 486(4):4781–4789. https://doi.org/10.1093/mnras/stz1175. arXiv:1903.03112 [astro-ph.GA]

Fragione G, Loeb A (2019) Black hole-neutron star mergers from triples. MNRAS 486(3):4443–4450. https://doi.org/10.1093/mnras/stz1131. arXiv:1903.10511 [astro-ph.GA]

Fragione G, Silk J (2020) Repeated mergers and ejection of black holes within nuclear star clusters. MNRAS https://doi.org/10.1093/mnras/staa2629. arXiv:2006.01867 [astro-ph.GA]

Fragione G, Ginsburg I, Kocsis B (2018) Gravitational waves and intermediate-mass black hole retention in globular clusters. ApJ 856(2):92. https://doi.org/10.3847/1538-4357/aab368. arXiv:1711.00483 [astro-ph.GA]

Fragione G, Grishin E, Leigh NWC, Perets HB, Perna R (2019) Black hole and neutron star mergers in galactic nuclei. MNRAS 488(1):47–63. https://doi.org/10.1093/mnras/stz1651. arXiv:1811.10627 [astro-ph.GA]

Fragione G, Martinez MAS, Kremer K, Chatterjee S, Rodriguez CL, Ye CS, Weatherford NC, Naoz S, Rasio FA (2020) Demographics of triple systems in dense star clusters. ApJ 900(1):16. https://doi.org/10.3847/1538-4357/aba89b. arXiv:2007.11605 [astro-ph.GA]

Fragos T, Andrews JJ, Ramirez-Ruiz E, Meynet G, Kalogera V, Taam RE, Zezas A (2019) The complete evolution of a neutron-star binary through a common envelope phase using 1D hydrodynamic simulations. ApJ 883(2):L45. https://doi.org/10.3847/2041-8213/ab40d1. arXiv:1907.12573 [astro-ph.HE]

Fragos T, Andrews JJ, Bavera SS, Berry CPL, Coughlin S, Dotter A, Giri P, Kalogera V, Katsaggelos A, Kovlakas K et al (2022) POSYDON: a general-purpose population synthesis code with detailed binary-evolution simulations. arXiv e-prints arXiv:2202.05892 [astro-ph.SR]

Franchini A, Sesana A, Dotti M (2021) Circumbinary disc self-gravity governing supermassive black hole binary mergers. MNRAS 507(1):1458–1467. https://doi.org/10.1093/mnras/stab2234. arXiv:2106.13253 [astro-ph.HE]

Franchini A, Lupi A, Sesana A (2022) Resolving massive black hole binary evolution via adaptive particle splitting. ApJ 929(1):L13. https://doi.org/10.3847/2041-8213/ac63a2. arXiv:2201.05619 [astro-ph.HE]

Frank J, Rees MJ (1976) Effects of massive black holes on dense stellar systems. MNRAS 176:633–647. https://doi.org/10.1093/mnras/176.3.633

Frank J, King A, Raine DJ (2002) Accretion power in astrophysics, 3rd edn. Cambridge University Press, Cambridge

Freitag M (2001) Monte Carlo cluster simulations to determine the rate of compact star inspiralling to a central galactic black hole. Class Quantum Grav 18(19):4033–4038. https://doi.org/10.1088/0264-9381/18/19/309. arXiv:astro-ph/0107193 [astro-ph]

Freitag M, Gürkan MA, Rasio FA (2006) Runaway collisions in young star clusters—II. Numerical results. MNRAS 368(1):141–161. https://doi.org/10.1111/j.1365-2966.2006.10096.x. arXiv:astro-ph/0503130 [astro-ph]
Freitag M, Rasio FA, Baumgardt H (2006) Runaway collisions in young star clusters—I. Methods and tests. MNRAS 368(1):121–140. https://doi.org/10.1111/j.1365-2966.2006.10095.x. arXiv:astro-ph/0503129 [astro-ph]

French KD, Arcavi I, Zabludoff A (2016) Tidal disruption events prefer unusual host galaxies. ApJ 818(1): L21. https://doi.org/10.3847/2041-8205/818/1/L21. arXiv:1601.04705 [astro-ph.GA]

Fruchter AS, Stinebring DR, Taylor JH (1988) A millisecond pulsar in an eclipsing binary. Nature 333 (6170):237–239. https://doi.org/10.1038/333237a0

Fryer CL, Belczynski K, Wiktorowicz G, Dominik M, Kalogera V, Holz DE (2012) Compact remnant mass function: dependence on the explosion mechanism and metallicity. ApJ 749(1):91. https://doi.org/10.1088/0004-6367X/749/1/91. arXiv:1110.1726 [astro-ph.SR]

Fujita R (2015) Gravitational waves from a particle in circular orbits around a rotating black hole to the 11th post-Newtonian order. Prog Theor Exp Phys 2015(3):033E01. https://doi.org/10.1093/ptv012. arXiv:1412.5689 [gr-qc]

Fuller J, Lai D (2012) Dynamical tides in compact white dwarf binaries: tidal synchronization and dissipation. MNRAS 421(1):426–445. https://doi.org/10.1111/j.1365-2966.2011.20320.x. arXiv:1108.4910 [astro-ph.SR]

Gabbard H, Williams M, Hayes F, Messenger C (2018) Matching matched filtering with deep networks for gravitational-wave astronomy. Phys Rev Lett 120(14):141103. https://doi.org/10.1103/PhysRevLett. 120.141103. arXiv:1712.06041 [astro-ph.IM]

Gaia Collaboration, Brown AGA, Vallenari A, Prusti T, de Bruijne JHJ, Babusiaux C, Bailer-Jones CAL, Biermann M, Evans DW, Eyer L et al (2018) Gaia data release 2. Summary of the contents and survey properties. A&A 616:A1. https://doi.org/10.1051/0004-6361/201833051. arXiv:1804.09365 [astro-ph.GA]

Gaia Collaboration, Katz D, Antoja T, Romero-Gómez M, Drimmel R, Reylé C, Seabroke GM, Soubiran C, Babusiaux C, Di Matteo P et al (2018) Gaia data release 2. Mapping the milky way disc kinematics. A&A 616:A11. https://doi.org/10.1051/0004-6361/201832865. arXiv:1804.09380 [astro-ph.GA]

Gaia Collaboration, Brown AGA, Vallenari A, Prusti T, de Bruijne JHJ, Babusiaux C, Biermann M (2021) Gaia early data release 3: summary of the contents and survey properties. A&A 649:A1. https://doi.org/10.1051/0004-6361/202039657. arXiv:2012.01533 [astro-ph.GA]

Gair J, Jones G (2007) Detecting extreme mass ratio inspiral events in LISA data using the hierarchical algorithm for clusters and ridges (HACR). Class Quantum Grav 24(5):1145–1168. https://doi.org/10.1088/0264-9381/24/5/007. arXiv:gr-qc/0610046 [gr-qc]

Gair JR, Barack L, Creighton T, Cutler C, Larson SL, Phinney ES, Vallisneri M (2004) Event rate estimates for LISA extreme mass ratio capture sources. Class Quantum Grav 21(20):S1595–S1606. https://doi.org/10.1088/0264-9381/21/20/003. arXiv:gr-qc/0405137 [gr-qc]

Gair JR, Mandel I, Wen L (2008) Improved time frequency analysis of extreme-mass-ratio inspiral signals in mock LISA data. Class Quantum Grav 25(18):184031. https://doi.org/10.1088/0264-9381/25/18/184031. arXiv:0804.1084 [gr-qc]

Gair JR, Mandel I, Wen L (2008) Time-frequency analysis of extreme-mass-ratio inspiral signals in mock LISA data. J Phys Conf Ser 122:012037. https://doi.org/10.1088/1742-6596/122/1/012037. arXiv:0710.5250 [gr-qc]

Gair JR, Porter E, Babak S, Barack L (2008) A constrained metropolis Hastings search for EMRIs in the mock LISA data challenge 1B. Class Quantum Grav 25(18):184030. https://doi.org/10.1088/0264-9381/25/18/184030. arXiv:0804.3322 [gr-qc]

Gair JR, Mandel I, Miller MC, Volonteri M (2011) Exploring intermediate and massive black-hole binaries with the Einstein Telescope. Gen Relativ Gravit 43(2):485–518. https://doi.org/10.1007/s10714-010-1104-3. arXiv:0907.5450 [astro-ph.CO]

Galaudage S, Adamcewicz C, Zhu XJ, Stevenson S, Thrane E (2021) Heavy double neutron stars: birth, midlife, and death. ApJ 909(2):L19. https://doi.org/10.3847/2041-8213/abe7f6. arXiv:2011.01495 [astro-ph.HE]

Gallego-Cano E, Schödel R, Dong H, Nogueras-Lara F, Gallego-Calvente AT, Amaro-Seoane P, Baumgardt H (2018) The distribution of stars around the Milky Way’s central black hole. I. Deep star counts. A&A 609:A26. https://doi.org/10.1051/0004-6361/201730451. arXiv:1701.03816 [astro-ph.GA]

Gammie CF, Shapiro SL, McKinney JC (2004) Black hole spin evolution. ApJ 602(1):312–319. https://doi.org/10.1086/380996. arXiv:astro-ph/0310886 [astro-ph]
Gandhi P, Rao A, Johnson MAC, Paice JA, Maccarone TJ (2019) Gaia Data Release 2 distances and peculiar velocities for Galactic black hole transients. MNRAS 485(2):2642–2655. https://doi.org/10.1093/mnras/stz438. arXiv:1804.11349 [astro-ph.HE]

Gänsicke BT, Marsh TR, Southworth J, Rebassa-Mansergas A (2006) A gaseous metal disk around a white dwarf. Science 314(5807):1908. https://doi.org/10.1126/science.1135033. arXiv:astro-ph/0612697 [astro-ph]

Gänsicke BT, Schreiber MR, Toloza O, Gentile Fusillo NP, Koester D, Manser CJ (2019) Accretion of a giant planet onto a white dwarf star. Nature 576(7785):61–64. https://doi.org/10.1038/s41586-019-1789-8. arXiv:1912.01611 [astro-ph.EP]

Garavito-Camargo N, Besla G, Laporte CFP, Johnston KV, Gómez FA, Watkins LL (2019) Hunting for the dark matter wake induced by the large magellanic cloud. ApJ 884(1):51. https://doi.org/10.3847/1538-4357/ab32eb. arXiv:1902.05089 [astro-ph.GA]

Garavito-Camargo N, Besla G, Laporte CFP, Price-Whelan AM, Cunningham EC, Johnston KV, Weinberg M, Gómez FA (2021) Quantifying the impact of the large magellanic cloud on the structure of the milky way’s dark matter halo using basis function expansions. ApJ 919(2):109. https://doi.org/10.3847/1538-4357/ac0b44. arXiv:2010.00816 [astro-ph.GA]

García JA, Fabian AC, Kallman TR, Dauser T, Parker ML, McClintock JE, Steiner JF, Wilms J (2016) The effects of high density on the X-ray spectrum reflected from accretion discs around black holes. MNRAS 462(1):751–760. https://doi.org/10.1093/mnras/stw1696. arXiv:1603.05259 [astro-ph.HE]

García-Bellido J, Peloso M, Unal C (2016) Gravitational waves at interferometer scales and primordial black holes in axion inflation. J Cosmol Astropart Phys 12:031. https://doi.org/10.1088/1475-7516/2016/12/031. arXiv:1610.03763 [astro-ph.CO]

García-Bellido J, Peloso M, Unal C (2017) Gravitational Wave signatures of inflationary models from Primordial Black Hole Dark Matter. J Cosmol Astropart Phys 09:013. https://doi.org/10.1088/1475-7516/2017/09/013. arXiv:1707.02441 [astro-ph.CO]

Gardner JP, Mather JC, Clampin M, Doyon R, Greenhouse MA, Hammel HB, Hutchings JB, Jakobsen P, Lilly SJ, Long KS et al (2006) The James Webb space telescope. Space Sci Rev 123(4):485–606. https://doi.org/10.1007/s11214-006-8315-7. arXiv:astro-ph/0606175 [astro-ph]

Gaskin JA, Swartz DA, Vikhlinin A, Özel F, Gelmis KE, Arenberg JW, Bandler SR, Bautz MW, Civitani MM, Dominguez A et al (2019) Lynx X-ray observatory: an overview. J Astron Telesc Instr Syst 5:021001. https://doi.org/10.1117/1.JATIS.5.2.021001

Gaspari M, Ruszkowski M, Sharma P (2012) Cause and effect of feedback: multiphase gas in cluster cores heated by AGN jets. ApJ 746(1):94. https://doi.org/10.1088/0004-637X/746/1/94. arXiv:1110.6063 [astro-ph.CO]

Gaspari M, Ruszkowski M, Oh SP (2013) Chaotic cold accretion on to black holes. MNRAS 432(4):3401–3422. https://doi.org/10.1093/mnras/stt692. arXiv:1301.3130 [astro-ph.CO]

Gaspari M, Brighenti F, Temi P (2015) Chaotic cold accretion on to black holes in rotating atmospheres. A&A 579:A62. https://doi.org/10.1051/0004-6361/201526151. arXiv:1407.7531 [astro-ph.GA]

Gaspari M, Temi P, Brighenti F (2017) Raining on black holes and massive galaxies: the top-down multiphase condensation model. MNRAS 466(1):677–704. https://doi.org/10.1093/mnras/stw3108. arXiv:1608.08216 [astro-ph.GA]

Gaspari M, Eckert D, Ettori S, Tozzi P, Bassini L, Rasia E, Brighenti F, Sun M, Borgani S, Johnson SD et al (2019) The X-ray halo scaling relations of supermassive black holes. ApJ 884(2):169. https://doi.org/10.3847/1538-4357/ab3c5d. arXiv:1904.10972 [astro-ph.GA]

Gaspari M, Tombesi F, Cappi M (2020) Linking macro-, meso- and microscales in multiphase AGN feeding and feedback. Nat Astron 4:10–13. https://doi.org/10.1038/s41550-019-0970-1. arXiv:2001.04985 [astro-ph.GA]

Gatti M, Lamastra A, Menci N, Bongiorno A, Fiore F (2015) Physical properties of AGN host galaxies as a probe of supermassive black hole feeding mechanisms. A&A 576:A32. https://doi.org/10.1051/0004-6361/201425094. arXiv:1412.7660 [astro-ph.GA]

Gavazzi G, Consolandi G, Dotti M, Fanali R, Fossati M, Fumagalli M, Viscardi E, Savorgnan G, Boselli A, Gutiérrez L et al (2015) Hα: an Hα imaging survey of HI selected galaxies from ALFALFA. VI. The role of bars in quenching star formation from z = 3 to the present epoch. A&A 580:A116. https://doi.org/10.1051/0004-6361/201425351. arXiv:1505.07836 [astro-ph.GA]

Ge H, Webbink RF, Han Z (2020) The thermal equilibrium mass-loss model and its applications in binary evolution. ApJS 249(1):9. https://doi.org/10.3847/1538-4365/ab98f6. arXiv:2006.00774 [astro-ph. SR]
Gebhardt K, Bender R, Bower G, Dressler A, Faber SM, Filippenko AV, Green R, Grillmair C, Ho LC, Kormendy J et al (2000) A relationship between nuclear black hole mass and galaxy velocity dispersion. ApJ 539(1):L13–L16. https://doi.org/10.1086/312840. arXiv:astro-ph/0006289 [astro-ph]

Geha M, Brown TM, Tumlinson J, Kalirai JS, Simon JD, Kirby EN, Vand enBerg DA, Muñoz RR, Avila RJ, Guhathakurta P et al (2013) The stellar initial mass function of ultra-faint dwarf galaxies: evidence for IMF variations with galactic environment. ApJ 771(1):29. https://doi.org/10.1088/0004-637X/771/1/29. arXiv:1304.7769 [astro-ph.CO]

Geier S, Marsh TR, Wang B, Dunlap B, Barlow BN, Schaffenroth V, Chen X, Irrgang A, Maxted PFL et al (2013) A progenitor binary and an ejected mass donor remnant of faint type Ia supernovae. A&A 554:A54. https://doi.org/10.1051/0004-6361/201321395. arXiv:1304.4452 [astro-ph.SR]

Gendreau KC, Arzoumanian Z, Adkins PW, Albert CL, Anders JF, Aylward AT, Baker CL, Balsamo ER, Bamford WA, Benegalrao SS et al (2016) The neutron star interior composition explorer (NICER): design and development. In: den Herder JWA, Takahashi T, Bautz M (eds) Space telescopes and instrumentation 2016: ultraviolet to gamma ray. Society of photo-optical instrumentation engineers (SPIE) conference series, vol 9905. p 99051H. https://doi.org/10.1117/12.2231304

Generozov A, Madigan AM (2020) The hills mechanism and the galactic center S-stars. ApJ 896(2):137. https://doi.org/10.3847/1538-4357/ab94bc. arXiv:2002.10547 [astro-ph.GA]

Generozov A, Stone NC, Metzger BD, Ostriker JP (2018) An overabundance of black hole X-ray binaries in the Galactic Centre from tidal captures. MNRAS 478(3):4030–4051. https://doi.org/10.1093/mnras/sty1262. arXiv:1804.01543 [astro-ph.HE]

Genzel R, Eisenhauer F, Gillessen S (2010) The Galactic Center massive black hole and nuclear star cluster. Rev Mod Phys 82(4):3121–3195. https://doi.org/10.1103/RevModPhys.82.3121. arXiv:1006.0064 [astro-ph.GA]

Georgakarakos N (2008) Stability criteria for hierarchical triple systems. Celest Mech Dyn Astron 100 (2):151–168. https://doi.org/10.1007/s10569-007-9109-2. arXiv:1408.5431 [astro-ph.EP]

George D, Shen H, Huerta EA (2018) Classification and unsupervised clustering of LIGO data with Deep Transfer Learning. Phys Rev D 97(10):101501. https://doi.org/10.1103/PhysRevD.97.101501. arXiv:1706.07446 [gr-qc]

Gergely LÁ, Biermann PL, Caramete LI (2010) Supermassive black hole spin-flip during the inspiral. Class Quantum Grav 27(19):194009. https://doi.org/10.1088/0264-9381/27/19/194009. arXiv:1005.2287 [astro-ph.CO]

Gerosa D, Kesden M (2016) Precession: dynamics of spinning black-hole binaries with python. Phys Rev D 93(12):124066. https://doi.org/10.1103/PhysRevD.93.124066. arXiv:1605.01067 [astro-ph.HE]

Gerosa D, Moore CJ (2016) Black hole kicks as new gravitational wave observables. Phys Rev Lett 117 (1):011101. https://doi.org/10.1103/PhysRevLett.117.011101. arXiv:1606.04226 [gr-qc]

Gerosa D, Sesana A (2015) Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature. MNRAS 446(1):38–55. https://doi.org/10.1093/mnras/stu2049. arXiv:1405.2072 [astro-ph.GA]

Gerosa D, Kesden M, Berti E, O'Shaughnessy R, Sperhake U (2013) Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation. Phys Rev D 87(10):104028. https://doi.org/10.1103/PhysRevD.87.104028. arXiv:1302.4442 [gr-qc]

Gerosa D, Kesden M, Sperhake U, Berti E, O'Shaughnessy R (2015) Multi-timescale analysis of phase transitions in precessing black-hole binaries. Phys Rev D 92(6):064016. https://doi.org/10.1103/PhysRevD.92.064016. arXiv:1506.03492 [gr-qc]

Gerosa D, Veronesi B, Lodato G, Rosotti G (2015) Spin alignment and differential accretion in merging black hole binaries. MNRAS 451(4):3941–3954. https://doi.org/10.1093/mnras/stv1214. arXiv:1503.06807 [astro-ph.GA]

Gerosa D, Berti E, O'Shaughnessy R, Belczynski K, Kesden M, Wysocki D, Gladysz W (2018) Spin orientations of merging black holes formed from the evolution of stellar binaries. Phys Rev D 98 (8):084036. https://doi.org/10.1103/PhysRevD.98.084036. arXiv:1808.02491 [astro-ph.HE]

Gerosa D, Hébert F, Stein LC (2018) Black-hole kicks from numerical-relativity surrogate models. Phys Rev D 97(10):104049. https://doi.org/10.1103/PhysRevD.97.104049. arXiv:1802.04276 [gr-qc]

Gerosa D, Ma S, Wong KWK, Berti E, O'Shaughnessy R, Chen Y, Belczynski K (2019) Multiband gravitational-wave event rates and stellar physics. Phys Rev D 99(10):103004. https://doi.org/10.1103/PhysRevD.99.103004. arXiv:1902.00021 [astro-ph.HE]

Gerosa D, Rosotti G, Barbieri R (2020) The Bardeen–Petterson effect in accreting supermassive black hole binaries: a systematic approach. MNRAS 496(3):3060–3075. https://doi.org/10.1093/mnras/staa1693. arXiv:2004.02894 [astro-ph.GA]
Giacobbo N, Mapelli M (2018) The progenitors of compact-object binaries: impact of metallicity, common envelope and natal kicks. MNRAS 480(2):2011–2030. https://doi.org/10.1093/mnras/sty1999. arXiv: 1806.00001 [astro-ph.HE]

Giacobbo N, Mapelli M (2020) Revising natal kick prescriptions in population synthesis simulations. ApJ 891(2):141. https://doi.org/10.3847/1538-4357/ab7335. arXiv:1909.06385 [astro-ph.HE]

Giacobbo N, Mapelli M, Spera M (2018) Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor. MNRAS 474(3):2959–2974. https://doi.org/10.1093/mnras/stx2933. arXiv:1711.03556 [astro-ph.SR]

Giacomazzo B, Baker JG, Miller MC, Reynolds CS, van Meter JR (2012) General relativistic simulations of magnetized plasmas around merging supermassive black holes. ApJ 752(1):L15. https://doi.org/10.1088/2041-8205/752/1/L15. arXiv:1203.6108 [astro-ph.HE]

Giammichele N, Bergeron P, Dufour P (2012) Know your neighborhood: a detailed model atmosphere analysis of nearby white dwarfs. ApJS 199(2):29. https://doi.org/10.1088/0067-0049/199/2/29. arXiv:1202.5581 [astro-ph.SR]

Giblin J, John T, Price LR, Siemens X, Vlcek B (2012) Gravitational waves from global second order phase transitions. J Cosmol Astropart Phys 11:006. https://doi.org/10.1088/1475-7516/2012/11/006. arXiv:1111.4014 [astro-ph.CO]

Gieles M, Bastian N (2008) An alternative method to study star cluster disruption. A&A 482(1):165–171. https://doi.org/10.1051/0004-6361:20078909. arXiv:0802.3387 [astro-ph]

Giersz M, Heggie DC, Hurley JR, Hypki A (2013) MOCCA code for star cluster simulations—II. Comparison with N-body simulations. MNRAS 431(3):2184–2199. https://doi.org/10.1093/mnras/stt307. arXiv:1112.6246 [astro-ph.GA]

Giersz M, Leigh N, Hypki A, Lützgendorf N, Askar A (2015) MOCCA code for star cluster simulations—IV. A new scenario for intermediate mass black hole formation in globular clusters. MNRAS 454 (3):3150–3165. https://doi.org/10.1093/mnras/stv2162. arXiv:1506.05234 [astro-ph.GA]

Giersz M, Askar A, Wang L, Hypki A, Leveque A, Spurzem R (2019) MOCCA survey data base-I. Dissolution of tidally filling star clusters harbouring black hole subsystems. MNRAS 487(2):2412–2423. https://doi.org/10.1093/mnras/stz1460. arXiv:1904.01227 [astro-ph.GA]

Gillessen S, Plewa PM, Eisenhauer F, Sari R, Waisberg I, Habibi M, Pfuhl O, George E, Dexter J, von Fellenberg S et al (2017) An update on monitoring stellar orbits in the galactic center. ApJ 837(1):30. https://doi.org/10.3847/1538-4357/aa5c41. arXiv:1611.09144 [astro-ph.GA]

Gilli R, Daddi E, Zamorani G, Tozzi P, Borgani S, Bergeron J, Giacconi R, Hasinger G, Mainieri V, Norman C et al (2005) The spatial clustering of X-ray selected AGN and galaxies in the Chandra Deep Field South and North. A&A 430:811–825. https://doi.org/10.1051/0004-6361:20041375. arXiv:astro-ph/0409759 [astro-ph]

Gilli R, Norman C, Calura F, Vito F, Decarli R, Marchesi S, Iwasawa K, Comastri A, Lanzuisi G, Pozzi F et al (2022) Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies interstellar medium. A&A 666:A17. https://doi.org/10.1051/0004-6361/202243708. arXiv:2206.03508 [astro-ph.GA]

Ginat YB, Glanz H, Perets HB, Grishin E, Desjacques V (2020) Gravitational waves from in-spirals of compact objects in binary common-envelope evolution. MNRAS 493(4):4861–4867. https://doi.org/10.1093/mnras/staa465. arXiv:1903.11072 [astro-ph.SR]

Girardi M, Fadda D, Giuricin G, Mardirossian F, Mezzetti M, Biviano A (1996) Velocity dispersions and X-ray temperatures of galaxy clusters. ApJ 457:61. https://doi.org/10.1086/176711. arXiv:astro-ph/9507031 [astro-ph]

Glanz H, Perets HB (2021) Simulations of common envelope evolution in triple systems: circumstellar case. MNRAS 500(2):1921–1932. https://doi.org/10.1093/mnras/staa3242. arXiv:2004.00020 [astro-ph.SR]

Gnedin OY, Ostriker JP, Tremaine S (2014) Co-evolution of galactic nuclei and globular cluster systems. ApJ 785(1):71. https://doi.org/10.1088/0004-637X/785/1/71. arXiv:1308.0021 [astro-ph.CO]

Gnocchi G, Maselli A, Abdelsalhin T, Giacobbo N, Mapelli M (2019) Bounding alternative theories of gravity with multiband GW observations. Phys Rev D 100(6):064024. https://doi.org/10.1103/PhysRevD.100.064024. arXiv:1905.13460 [gr-qc]

Goicovic FG, Cuadra J, Sesana A, Stasyszyn F, Amaro-Seoane P, Tanaka TL (2016) Infalling clouds on to supermassive black hole binaries—I. Formation of discs, accretion and gas dynamics. MNRAS 455 (2):1989–2003. https://doi.org/10.1093/mnras/stv2470. arXiv:1507.05596 [astro-ph.HE]
Goicovic FG, Sesana A, Cuadra J, Stasyszyn F (2017) Infalling clouds on to supermassive black hole binaries—II. Binary evolution and the final parsec problem. MNRAS 472(1):514–531. https://doi.org/10.1093/mnras/stx1996. arXiv:1602.01966 [astro-ph.HE]

Goicovic FG, Maureira-Fredes C, Sesana A, Amaro-Seoane P, Cuadra J (2018) Accretion of clumpy cold gas onto massive black hole binaries: a possible fast route to binary coalescence. MNRAS 479 (3):3438–3455. https://doi.org/10.1093/mnras/sty1709. arXiv:1801.04937 [astro-ph.HE]

Gokhale V, Peng Xa, Frank J (2007) Evolution of close white dwarf binaries. ApJ 655(2):1010–1024. https://doi.org/10.1086/510119. arXiv:astro-ph/0610919 [astro-ph]

Gold R, Paschalidis V, Etienne ZB, Shapiro SL, Pfeiffer HP (2014) Accretion disks around binary black holes of unequal mass: general relativistic magnetohydrodynamic simulations near decoupling. Phys Rev D 89(6):064060. https://doi.org/10.1103/PhysRevD.89.064060. arXiv:1312.0600 [astro-ph.HE]

Gold R, Paschalidis V, Ruiz M, Shapiro SL, Etienne ZB, Pfeiffer HP (2014) Accretion disks around binary black holes of unequal mass: general relativistic MHD simulations of postdecoupling and merger. Phys Rev D 90(10):104030. https://doi.org/10.1103/PhysRevD.90.104030. arXiv:1410.1543 [astro-ph.GA]

Gondolo P, Silk J (1999) Dark matter annihilation at the galactic center. Phys Rev Lett 83(9):1719–1722. https://doi.org/10.1103/PhysRevLett.83.1719. arXiv:astro-ph/9906391 [astro-ph]

González E, Kremer K, Chatterjee S, Fragione G, Rodriguez CL, Weatherford NC, Ye CS, Rasio FA (2021) Intermediate-mass black holes from high massive-star binary fractions in young star clusters. ApJ 908(2):L29. https://doi.org/10.3847/2041-8213/abdf5b. arXiv:2012.10497 [astro-ph.HE]

González JA, Hannam M, Sperhake U, Brügmann B, Husa S (2007) Supermassive recoil velocities for binary black-hole mergers with antialigned spins. Phys Rev Lett 98(23):231101. https://doi.org/10.1103/PhysRevLett.98.231101. arXiv:gr-qc/0702052 [gr-qc]

González JA, Sperhake U, Brügmann B, Hannam M, Husa S (2007) Maximum kick from nonspinning black-hole binary inspiral. Phys Rev Lett 98(9):091101. https://doi.org/10.1103/PhysRevLett.98.091101. arXiv:gr-qc/0610154 [gr-qc]

González Delgado RM, Pérez E, Cid Fernandes R, Schmitt H (2008) HST/WFPC2 imaging of the circumnuclear structure of low-luminosity active galactic nuclei. I. Data and nuclear morphology. AJ 135(3):747–765. https://doi.org/10.1088/0004-6256/135/3/747. arXiv:0710.4450 [astro-ph]

Goodman J (2003) Self-gravity and quasi-stellar object discs. MNRAS 339(4):937–948. https://doi.org/10.1046/j.1365-8711.2003.06241.x. arXiv:astro-ph/0201001 [astro-ph]

Goodman J, Hut P (1993) Binary-single-star scattering. V. Steady state binary distribution in a homogeneous static background of single stars. ApJ 403:271. https://doi.org/10.1086/172200. arXiv:astro-ph/0201001 [astro-ph]

Goodman J, Tan JC (2004) Supermassive stars in quasar disks. ApJ 608(1):108–118. https://doi.org/10.1086/386360. arXiv:astro-ph/0307361 [astro-ph]

Götberg Y, Korol V, Lamberts A, Kupfer T, Breivik K, Ludwig B, Drout MR (2020) Stars stripped in binaries—the living gravitational wave sources. ApJ 904:56. https://doi.org/10.3847/1538-4357/abbd5a. arXiv:2006.07382 [astro-ph.SR]

Goulding AD, Greene JE, Bezanson R, Greco J, Johnson S, Leauthaud A, Matsuoka Y, Medezinski E, Price-Whelan AM (2018) Galaxy interactions trigger rapid black hole growth: an unprecedented view from the Hyper Suprime-Cam survey. PASJ 70:S37. https://doi.org/10.1093/pasj/psx135. arXiv:1706.07436 [astro-ph.GA]

Gourgoulhon E, Le Tiec A, Vincent FH, Warburton N (2019) Gravitational waves from bodies orbiting the Galactic center black hole and their detectability by LISA. A&A 627:A92. https://doi.org/10.1051/0004-6361/201935406. arXiv:1903.02049 [gr-qc]

Governato F, Brook C, Mayer L, Brooks A, Rhee G, Wadsley J, Jonsson P, Willman B, Stinson G, Quinn T et al (2010) Bulgeless dwarf galaxies and dark matter cores from supernova-driven outflows. Nature 463(7278):203–206. https://doi.org/10.1038/nature08640. arXiv:0911.2237 [astro-ph.CO]

Gow AD, Byrnes CT, Cole PS, Young S (2021) The power spectrum on small scales: robust constraints and comparing PBH methodologies. J Cosmol Astropart Phys 2:002. https://doi.org/10.1088/1475-7516/2021/02/002. arXiv:2008.03289 [astro-ph.CO]

Goździewski K, Słowikowska A, Dimitrov D, Krzeszowski K, Zejmo M, Kanbach G, Burwitz V, Rau A, Irawati P, Richichi A et al (2015) The HU Aqr planetary system hypothesis revisited. MNRAS 448 (2):1118–1136. https://doi.org/10.1093/mnras/stu2728. arXiv:1412.5899 [astro-ph.EP]

Graham AW (2004) Core depletion from coalescing supermassive black holes. ApJ 613(1):L33–L36. https://doi.org/10.1086/424928. arXiv:astro-ph/0503177 [astro-ph]
Graham AW (2016a) Black hole and nuclear cluster scaling relations: $M_{bh} - M_{nc}^{2.7+/-0.7}$. Proc Int Astron Union 10(S312):269-273. https://doi.org/10.1017/S1743921315008017. arXiv:1412.5715 [astro-ph. GA]

Graham AW (2016b) Galaxy bulges and their massive black holes: a review. In: Laurikainen E, Peletier R, Gadotti D (eds) Galactic bulges. Astrophysics and Space Science Library, vol 418. Springer, pp 263-313. https://doi.org/10.1007/978-3-319-19378-6_11

Graham AW, Driver SP (2007) A log-quadratic relation for predicting supermassive black hole masses from the host bulge Sérsic index. ApJ 655(1):77-87. https://doi.org/10.1086/509758. arXiv:astro-ph/0607378 [astro-ph]

Graham AW, Scott N (2015) The (black hole)-bulge mass scaling relation at low masses. ApJ 798(1):54. https://doi.org/10.1088/0004-637X/798/1/54. arXiv:1412.3091 [astro-ph.GA]

Graham AW, Soria R (2019) Expected intermediate-mass black holes in the Virgo cluster—I. Early-type galaxies. MNRAS 484(1):794-813. https://doi.org/10.1093/mnras/sty3398. arXiv:1812.01231 [astro-ph.HE]

Graham AW, Spitler LR (2009) Quantifying the coexistence of massive black holes and dense nuclear star clusters. MNRAS 397(4):2148-2162. https://doi.org/10.1111/j.1365-2966.2009.15118.x. arXiv:0907.5250 [astro-ph.CO]

Graham AW, Erwin P, Trujillo I, Asensio Ramos A (2003) A new empirical model for the structural analysis of early-type galaxies, and a critical review of the Nuker model. AJ 125(6):2951-2963. https://doi.org/10.1086/375320. arXiv:astro-ph/0306023 [astro-ph]

Graham AW, Driver SP, Allen PD, Liske J (2007) The Millennium Galaxy Catalogue: the local supermassive black hole mass function in early- and late-type galaxies. MNRAS 378(1):198-210. https://doi.org/10.1111/j.1365-2966.2007.11770.x. arXiv:0704.0316 [astro-ph]

Graham AW, Soria R, Davis BL (2019) Expected intermediate-mass black holes in the Virgo cluster—II. Late-type galaxies. MNRAS 484(1):814-831. https://doi.org/10.1093/mnras/sty3068. arXiv:1811.03232 [astro-ph.GA]

Graham MJ, Djorgovski SG, Stern D, Drake AJ, Mahabal AA, Donalek C, Glikman E, Larson S, Christensen E (2015) A systematic search for close supermassive black hole binaries in the Catalina Real-time Transient Survey. MNRAS 453(2):1562-1576. https://doi.org/10.1093/mnras/stv1726. arXiv:1507.07603 [astro-ph.GA]

Graham MJ, Ford KES, McKernan B, Ross NP, Stern D, Burdge K, Coughlin M, Djorgovski SG, Drake AJ, Duev D et al (2020) Candidate electromagnetic counterpart to the binary black hole merger gravitational-wave event S190521g*. Phys Rev Lett 124(25):251102. https://doi.org/10.1103/PhysRevLett.124.251102. arXiv:2006.14122 [astro-ph.HE]

Graziani L (2019) Hunting for dwarf galaxies hosting the formation and coalescence of compact binaries. Physics 1(3):412-429. https://doi.org/10.3390/physics1030030

Graziani L, Salvadori S, Schneider R, Kawata D, de Bennassuti M, Maselli A (2015) Galaxy formation with radiative and chemical feedback. MNRAS 449(3):3137-3148. https://doi.org/10.1093/mnras/stv494. arXiv:1502.07344 [astro-ph.GA]

Graziani L, de Bennassuti M, Schneider R, Kawata D, Salvadori S (2017) The history of the dark and luminous side of Milky Way-like progenitors. MNRAS 469(1):1101-1116. https://doi.org/10.1093/mnras/stx900. arXiv:1704.02983 [astro-ph.GA]

Graziani L, Schneider R, Marassi S, Del Pozzo W, Mapelli M, Giacobbo N (2020) Cosmic archaeology with massive stellar black hole binaries. MNRAS 495(1):L81-L85. https://doi.org/10.1093/mnrasl/sla063. arXiv:2004.03603 [astro-ph.GA]

Green J, Schechter P, Baltay C, Bean R, Bennett D, Brown R, Conselice C, Donahue M, Fan X, Gaudí BS et al (2012) Wide-field infrared survey telescope (WFIRST) final report. arXiv e-prints arXiv:1208.4012 [astro-ph.IM]

Green MJ, Hermes JJ, Marsh TR, Steeghs DTH, Bell KJ, Littlefair SP, Parsons SG, Dennihy E, Fuchs JT, Reding JS et al (2018) A 15.7-minAM CVn binary discovered in K2. MNRAS 477(4):5646-5656. https://doi.org/10.1093/mnras/sty1032. arXiv:1804.07138 [astro-ph.SR]

Green MJ, Marsh TR, Steeghs DTH, Kupfer T, Ashley RP, Bloemen S et al (2018) High-speed photometry of Gaia14aae: an eclipsing AM CVn that challenges formation models. MNRAS 476(2):1663-1679. https://doi.org/10.1093/mnras/sty299. arXiv:1802.00499 [astro-ph.SR]

Green SR, Gair J (2020) Complete parameter inference for GW150914 using deep learning. arXiv e-prints arXiv:2008.03312 [astro-ph.IM]
Greene JE (2012) Low-mass black holes as the remnants of primordial black hole formation. Nat Commun 3:1304. https://doi.org/10.1038/ncomms2314. arXiv:1211.7082 [astro-ph.CO]

Greene JE, Strader J, Ho LC (2020) Intermediate-mass black holes. ARA&A 58:257–312. https://doi.org/10.1146/annurev-astro-032620-021835. arXiv:1911.09678 [astro-ph.GA]

Grefenstette BW, Harrison FA, Boggs SE, Reynolds SP, Fryer CL, Madsen KK, Wik DR et al (2014) Asymmetries in core-collapse supernovae from maps of radioactive $^{44}$Ti in CassiopeiaA. Nature 506 (7488):339–342. https://doi.org/10.1038/nature12997. arXiv:1403.4978 [astro-ph.HE]

Gregely LA, Biermann PL (2009) The spin flip phenomenon and supermassive black hole binary systems. ApJ 697:1621–1633. https://doi.org/10.1088/0004-637X/697/2/1621

Greiner J, Schwarz R, Zharikov S, Orio M (2000) RX J1420.4+5334—another tidal disruption event? A&A 362:L25–L28 arXiv:astro-ph/0009430 [astro-ph]

Grindlay JE, Cool AM, Callanan PJ, Bailyn CD, Cohn HN, Lugger PM (1995) Spectroscopic identification of probable cataclysmic variables in the globular cluster NGC 6397. ApJ 455:L47. https://doi.org/10.1086/309806

Grover K, Fairhurst S, Farr BF et al (2014) Comparison of gravitational wave detector network sky localization approximations. Phys Rev D 89(4):042004. https://doi.org/10.1103/PhysRevD.89.042004. arXiv:1310.7454 [gr-qc]

Grupe D, Thomas HC, Leighly KM (1999) RX J1624.9+7554: a new X-ray transient AGN. A&A 350: L31–L34 arXiv:astro-ph/9909101 [astro-ph]

Gruzinov A, Levin Y, Matzner CD (2020) Negative dynamical friction on compact objects moving through dense gas. MNRAS 492(2):2755–2761. https://doi.org/10.1093/mnras/staa013. arXiv:1906.01186 [astro-ph.HE]

Gualandris A, Merritt D (2008) Ejection of supermassive black holes from galaxy cores. ApJ 678(2):780–797. https://doi.org/10.1086/586877. arXiv:0708.0771 [astro-ph]

Gualandris A, Merritt D (2009) Perturbations of intermediate-mass black holes on stellar orbits in the galactic center. ApJ 705(1):361–371. https://doi.org/10.1088/0004-637X/705/1/361. arXiv:0905.4514 [astro-ph.GA]

Gualandris A, Dotti M, Sesana A (2012) Massive black hole binary plane reorientation in rotating stellar systems. MNRAS 420(1):L38–L42. https://doi.org/10.1111/j.1745-3933.2011.01188.x. arXiv:1109.3707 [astro-ph.GA]

Gualandris A, Read JI, Dehnen W, Bortolas E (2017) Collisionless loss-cone refilling: there is no final parsec problem. MNRAS 464(2):2301–2310. https://doi.org/10.1093/mnras/stw2528. arXiv:1609.09383 [astro-ph.GA]

Gualtieri L, Berti E, Cardoso V, Sperhake U (2008) Transformation of the multipolar components of gravitational radiation under rotations and boosts. Phys Rev D 78(4):044024. https://doi.org/10.1103/PhysRevD.78.044024. arXiv:0805.1017 [gr-qc]

Guillochon J, Ramirez-Ruiz E, Rosswog S, Kasen D (2009) Three-dimensional simulations of tidally disrupted solar-type stars and the observational signatures of shock breakout. ApJ 705(1):844–853. https://doi.org/10.1088/0004-637X/705/1/844. arXiv:0811.1370 [astro-ph]

Guillochon J, Dan M, Ramirez-Ruiz E, Rosswog S (2010) Surface detonations in double degenerate binary systems triggered by accretion stream instabilities. ApJ 709(1):L64–L69. https://doi.org/10.1088/2041-8205/709/1/L64. arXiv:0911.0416 [astro-ph.HE]

Gültekin K, Richstone DO, Gebhardt K, Lauer TR, Tremaine S, Aller MC, Bender R, Dressler A, Faber SM, Filippenko AV et al (2009) The M-σ and M-L relations in galactic bulges, and determinations of their intrinsic scatter. ApJ 698(1):198–221. https://doi.org/10.1088/0004-637X/698/1/198. arXiv:0903.4897 [astro-ph.GA]

Gunn JE, Ostriker JP (1970) On the nature of pulsars. III. Analysis of observations. ApJ 160:979. https://doi.org/10.1086/150487

Guo H, Liu X, Shen Y, Loeb A, Monroe T, Prochaska JX (2019) Constraining sub-parsec binary supermassive black holes in quasars with multi-epoch spectroscopy—III. Candidates from continued radial velocity tests. MNRAS 482(3):3288–3307. https://doi.org/10.1093/mnras/sty2920. arXiv:1809.04610 [astro-ph.GA]

Gürkan MA, Freitag M, Rasio FA (2004) Formation of massive black holes in dense star clusters. I. Mass segregation and core collapse. ApJ 604(2):632–652. https://doi.org/10.1086/381968. arXiv:astro-ph/0308449 [astro-ph]

Gürkan MA, Fregeau JM, Rasio FA (2006) Massive black hole binaries from collisional runaways. ApJ 640(1):L39–L42. https://doi.org/10.1086/503295. arXiv:astro-ph/0512642 [astro-ph]
Habets GMHJ (1986) The evolution of a single and a binary helium star of 2.5 solar mass up to neon ignition. A&A 165:95-109

Habouzit M, Volonteri M, Latif M, Dubois Y, Peirani S (2016) On the number density of ‘direct collapse’ black hole seeds. MNRAS 463(1):529–540. https://doi.org/10.1093/mnras/stw1924. arXiv:1601.00557 [astro-ph.GA]

Habouzit M, Volonteri M, Dubois Y (2017) Blossoms from black hole seeds: properties and early growth regulated by supernova feedback. MNRAS 468(4):3935–3948. https://doi.org/10.1093/mnras/stx666. arXiv:1605.09394 [astro-ph.GA]

Hachisu I, Kato M, Nomoto K (1999) A wide symbiotic channel to type IA supernovae. ApJ 522(1):487–503. https://doi.org/10.1086/307608. arXiv:astro-ph/9902304 [astro-ph]

Haehnelt MG (1994) Low-frequency gravitational waves from supermassive black-holes. MNRAS 269:199. https://doi.org/10.1093/mnras/269.1.199. arXiv:astro-ph/9405032 [astro-ph]

Haehnelt MG, Natarajan P, Rees MJ (1998) High-redshift galaxies, their active nuclei and central black holes. MNRAS 300(3):817–827. https://doi.org/10.1046/j.1365-8711.1998.01951.x. arXiv:astro-ph/9712259 [astro-ph]

Haemmerlé L, Woods TE, Klessen RS, Heger A, Whalen DJ (2018) The evolution of supermassive Population III stars. MNRAS 474(2):2757–2773. https://doi.org/10.1093/mnras/stx2919. arXiv:1705.09301 [astro-ph.SR]

Haemmerlé L, Klessen RS, Mayer L, Zwick L (2021) Maximum accretion rate of supermassive stars. A&A 652(L7):L7–L11. https://doi.org/10.1051/0004-6361/202141376. arXiv:arXiv:2105.13373 [astro-ph. SR]

Haiman Z (2004) Constraints from gravitational recoil on the growth of supermassive black holes at high redshift. ApJ 613(1):36–40. https://doi.org/10.1086/422910. arXiv:astro-ph/0404196 [astro-ph]

Haiman Z (2017) Electromagnetic chirp of a compact binary black hole: A phase template for the gravitational wave inspiral. Phys Rev D 96(2):023004. https://doi.org/10.1103/PhysRevD.96.023004. arXiv:1705.06765 [astro-ph.HE]

Haiman Z, Loeb A (2001) What is the highest plausible redshift of luminous quasars? ApJ 552(2):459–463. https://doi.org/10.1086/320586. arXiv:astro-ph/0011529 [astro-ph]

Haiman Z, Kocsis B, Menou K (2009) The population of viscosity- and gravitational wave-driven supermassive black hole binaries among luminous active galactic nuclei. ApJ 700(2):1952–1969. https://doi.org/10.1088/0004-637X/700/2/1952. arXiv:0904.1383 [astro-ph.CO]

Halpern JP, Holt SS (1992) Discovery of soft X-ray pulsations from the γ-ray source Geminga. Nature 357 (6375):222–224. https://doi.org/10.1038/357222a0

Hamers AS (2017) On the formation of hot and warm Jupiters via secular high-eccentricity migration in stellar triples. MNRAS 466(4):4107–4120. https://doi.org/10.1093/mnras/stx035. arXiv:1701.01733 [astro-ph.EP]

Hamers AS, Portegies Zwart SF (2016) White dwarf pollution by planets in stellar binaries. MNRAS 462 (1):L84–L87. https://doi.org/10.1093/mnrasl/slw134. arXiv:1607.01397 [astro-ph.EP]

Hamers AS, Safarzadeh M (2020) Was GW190412 born from a hierarchical 3 + 1 quadruple configuration? ApJ 898(2):99. https://doi.org/10.3847/1538-4357/ab9b27. arXiv:2005.03045 [astro-ph.HE]

Hamers AS, Pols OR, Claeys JSW, Nelemans G (2013) Population synthesis of triple systems in the context of mergers of carbon-oxygen white dwarfs. MNRAS 430(3):2262–2280. https://doi.org/10.1093/mnras/stt046. arXiv:1301.1469 [astro-ph.SR]

Hamers AS, Portegies Zwart SF, Merritt D (2014) Relativistic dynamics of stars near a supermassive black hole. MNRAS 443(1):355–387. https://doi.org/10.1093/mnras/stu1126. arXiv:1406.2846 [astro-ph. GA]

Hamilton C, Heinemann T (2020) Noise and waves: a unified kinetic theory for stellar systems. arXiv e-prints arXiv:2011.14812 [astro-ph.GA]

Hamilton C, Rafikov RR (2019) Compact object binary mergers driven by cluster tides: a new channel for LIGO/Virgo gravitational-wave events. ApJ 881(1):L13. https://doi.org/10.3847/2041-8213/ab3468. arXiv:1907.00994 [astro-ph.GA]

Hamilton C, Rafikov RR (2019) Secular dynamics of binaries in stellar clusters—I. General formulation and dependence on cluster potential. MNRAS 488(4):5489–5511. https://doi.org/10.1093/mnras/stz1730. arXiv:1902.01344 [astro-ph.GA]

Han WB, Chen X (2019) Testing general relativity using binary extreme-mass-ratio inspirals. MNRAS 485 (1):L29–L33. https://doi.org/10.1093/mnrasl/slz021. arXiv:1801.07060 [gr-qc]
Han WB, Fan XL (2018) Determining the nature of white dwarfs from low-frequency gravitational waves. ApJ 856(1):82. https://doi.org/10.3847/1538-4357/aab03c. arXiv:1711.08628 [astro-ph.HE]

Han WB, Zhong XY, Chen X, Xin S (2020) Very extreme mass-ratio bursts in the Galaxy and neighbouring galaxies in relation to space-borne detectors. MNRAS 498(1):L61–L65. https://doi.org/10.1093/mnrasl/slaa115. arXiv:2004.04016 [gr-qc]

Hannuksela OA, Wong KW, Brito R, Berti E, Li TG (2019) Probing the existence of ultralight bosons with a single gravitational-wave measurement. Nat Astron 3(5):447–451. https://doi.org/10.1038/s41550-019-0712-4. arXiv:1804.09659 [astro-ph.HE]

Hannuksela OA, Ng KCY, Li TGF (2020) Extreme dark matter tests with extreme mass ratio inspirals. Phys Rev D 102(10):103022. https://doi.org/10.1103/PhysRevD.102.103022. arXiv:1906.11845 [astro-ph.CO]

Hansen BMS, Milosavljević M (2003) The need for a second black hole at the galactic center. ApJ 593(2): L77–L80. https://doi.org/10.1086/378182. arXiv:astro-ph/0306074 [astro-ph]

Hansen RO (1972) Post-Newtonian gravitational radiation from point masses in a hyperbolic kepler orbit. Phys Rev D 5(4):1021–1023. https://doi.org/10.1103/PhysRevD.5.1021

Harko T, Kovács Z, Lobo FSN (2010) Thin accretion disk signatures in dynamical Chern–Simons–modified gravity. Class Quantum Grav 27(10):105010. https://doi.org/10.1088/0264-9381/27/10/105010. arXiv:0909.1267 [gr-qc]

Hartnett JG, Luiten AN (2011) Colloquium: comparison of astrophysical and terrestrial frequency standards. Rev Mod Phys 83(1):1–9. https://doi.org/10.1103/RevModPhys.83.1. arXiv:1004.0115 [astro-ph.IM]

Haster CJ, Antonini F, Kalogera V, el Mand I (2016) N-body dynamics of intermediate mass-ratio inspirals in star clusters. ApJ 832(2):192. https://doi.org/10.3847/0004-6367X/832/2/192. arXiv:1606.07097 [astro-ph.HE]

Haster CJ, Wang Z, Berry CPL, Stevenson S, Veitch J, Mandel I (2016) Inference on gravitational waves from coalescences of stellar-mass compact objects and intermediate-mass black holes. MNRAS 457 (4):4499–4506. https://doi.org/10.1093/mnras/stw233. arXiv:1511.01431 [astro-ph.HE]

He MY, Petrovich C (2018) On the stability and collisions in triple stellar systems. MNRAS 474(1):20–31. https://doi.org/10.1093/mnras/stx2718. arXiv:1710.04698 [astro-ph.SR]

Heath RM, Nixon CJ (2020) On the orbital evolution of binaries with circumbinary discs. A&A 641:A64. https://doi.org/10.1051/0004-6361/202038548. arXiv:2007.11592 [astro-ph.HE]

Heber U (2016) Hot subluminous stars. PASP 128(966):082001. https://doi.org/10.1088/1538-3873/128/966/082001. arXiv:1604.07749 [astro-ph.SR]

Heckman TM, Best PN (2014) The coevolution of galaxies and supermassive black holes: insights from surveys of the contemporary universe. ARA&A 52:589–660. https://doi.org/10.1146/annurev-astro-081913-035722. arXiv:1403.4620 [astro-ph.GA]

Heger A, Fryer CL, Woosley SE, Langer N, Hartmann DH (2003) How massive single stars end their life. ApJ 591:288–300. https://doi.org/10.1086/375341. arXiv:astro-ph/0212469

Heggie D, Hut P (2003) The gravitational million-body problem: a multidisciplinary approach to star cluster dynamics. Cambridge University Press, Cambridge

Heggie DC (1975) Binary evolution in stellar dynamics. MNRAS 173:729–787. https://doi.org/10.1093/mnras/173.3.729

Heinämäki P (2001) Symmetry of black hole ejections in mergers of galaxies. A&A 371:795–805. https://doi.org/10.1051/0004-6361:20010460

Heinke CO, Grindlay JE, Lugger PM, Cohn HN, Edmonds PD, Lloyd DA, Cool AM (2003) Analysis of the quiescent low-mass X-ray binary population in galactic globular clusters. ApJ 598(1):501–515. https://doi.org/10.1086/378885. arXiv:astro-ph/0305445 [astro-ph]

Heinke CO, Ivanova N, Engel MC, Pavlovskii K, Sivakoff GR, Cartwright TF, Gladstone JC (2013) Galactic ultracompact X-ray binaries: disk stability and evolution. ApJ 768(2):184. https://doi.org/10.1088/0004-6367X/768/2/184. arXiv:1303.5864 [astro-ph.HE]

Hellings RW, Downs GS (1983) Upper limits on the isotopic gravitational radiation background from pulsar timing analysis. ApJ 265:L39–L42. https://doi.org/10.1086/183954

Hennawi JF, Prochaska JX, Cantalupo S, Arrigoni-Battaia F (2015) Quasar quartet embedded in giant nebula reveals rare massive structure in distant universe. Science 348(6236):779–783. https://doi.org/10.1126/science.aaa5397. arXiv:1505.03786 [astro-ph.GA]

Hermes JJ, Kilic M, Brown WR, Winget DE, Allende Prieto C, Gianninas A, Mukadam AS, Cabrera-Lavers A, Kenyon SJ (2012) Rapid orbital decay in the 12.75-minute binary white dwarf J0651+2844. ApJ 757(2):L21. https://doi.org/10.1088/2041-8205/757/2/L21. arXiv:1208.5051 [astro-ph.SR]
Hickox RC, Jones C, Forman WR, Murray SS, Kochanek CS, Eisenstein D, Jannuzi BT, Dey A, Brown MJI, Stern D et al (2009) Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and infrared-selected AGNs. ApJ 696(1):891–919. https://doi.org/10.1088/0004-637X/696/1/891. arXiv:0901.4121 [astro-ph.GA]

Hicks WM, Wells A, Norman ML, Wise JH, Smith BD, O’Shea BW (2021) External enrichment of mini halos by the first supernovae. ApJ 909(1):70. https://doi.org/10.3847/1538-4357/abda3a. arXiv:2009.05499 [astro-ph.GA]

Hild S et al (2011) Sensitivity studies for third-generation gravitational wave observatories. Class Quantum Grav 28(9):094013. https://doi.org/10.1088/0264-9381/28/9/094013. arXiv:1012.0908 [gr-qc]

Hilditch RW (2001) An introduction to close binary stars. Cambridge University Press, Cambridge

Hills JG (1976) The formation of binaries containing black holes by the exchange of companions and the X-ray sources in globular clusters. MNRAS 175:1P-4P. https://doi.org/10.1093/mnras/175.1.1P

Hills JG, Fullerton LW (1980) Computer simulations of close encounters between single stars and hard binaries. AJ 85:1281–1291. https://doi.org/10.1086/112798

Hills D, Bender PL, Webbink RF (1990) Gravitational radiation from the galaxy. ApJ 360:75. https://doi.org/10.1086/169098

Hinderer T, Flanagan ÉÉ (2008) Two-timescale analysis of extreme mass ratio inspirals in Kerr spacetime: orbital motion. Phys Rev D 78(6):064028. https://doi.org/10.1103/PhysRevD.78.064028. arXiv:0805.3337 [gr-qc]

Hirano S, Hosokawa T, Yoshida N, Umeda H, Omukai K, Chiaki G, Yorke HW (2014) One hundred first stars: protostellar evolution and the final masses. ApJ 781(2):60. https://doi.org/10.1088/0004-637X/781/2/60. arXiv:1308.4456 [astro-ph.CO]

Hirschmann M, Dolag K, Saro A, Bachmann L, Borgani S, Burkert A (2014) Cosmological simulations of black hole growth: AGN luminosities and downsizing. MNRAS 442(3):2304–2324. https://doi.org/10.1093/mnras/stu1023. arXiv:1308.0333 [astro-ph.CO]

Hjellming MS, Webbink RF (1987) Thresholds for rapid mass transfer in binary system. I. Polytropic models. ApJ 318:794. https://doi.org/10.1086/165412

Hoang BM, Naoz S, Kocsis B, Rasio FA, Dosopoulou F (2018) Black hole mergers in galactic nuclei induced by the eccentric Kozai–Lidov effect. ApJ 856(2):140. https://doi.org/10.3847/1538-4357/aaace. arXiv:1706.09896 [astro-ph.HE]

Hoang BM, Naoz S, Kocsis B, Farr WM, McIver J (2019) Detecting supermassive black hole-induced binary eccentricity oscillations with LISA. ApJ 875(2):L31. https://doi.org/10.3847/2041-8213/ab14f7. arXiv:1903.00134 [astro-ph.HE]

Hobbs A, Power C, Nayakshin S, King AR (2012) Modelling supermassive black hole growth: towards an improved sub-grid prescription. MNRAS 421(4):3443–3449. https://doi.org/10.1111/j.1365-2966.2012.20563.x. arXiv:1202.4725 [astro-ph.IM]

Hobbs G, Lorimer DR, Lyne AG, Kramer M (2005) A statistical study of 233 pulsar proper motions. MNRAS 360(3):974–992. https://doi.org/10.1111/j.1365-2966.2005.09087.x. arXiv:astro-ph/0504584 [astro-ph]

Hoffman L, Loeb A (2007) Dynamics of triple black hole systems in hierarchically merging massive galaxies. MNRAS 377(3):957–976. https://doi.org/10.1111/j.1365-2966.2007.11694.x. arXiv:astro-ph/0612517 [astro-ph]

Hofmann F, Barausse E, Rezzolla L (2016) The final spin from binary black holes in quasi-circular orbits. ApJ 825(2):L19. https://doi.org/10.3847/2041-8205/825/2/L19. arXiv:1605.01938 [gr-qc]

Holley-Bockelmann K, Khan FM (2015) Galaxy rotation and rapid supermassive binary coalescence. ApJ 810(2):139. https://doi.org/10.1088/0004-637X/810/2/139. arXiv:1505.06203 [astro-ph.GA]

Holley-Bockelmann K, Gültekin K, Shoemaker D, Yunes N (2008) Gravitational wave recoil and the retention of intermediate-mass black holes. ApJ 686(2):829–837. https://doi.org/10.1086/591218. arXiv:0707.1334 [astro-ph]

Hong J, Lee HM (2015) Black hole binaries in galactic nuclei and gravitational wave sources. MNRAS 448(1):754–770. https://doi.org/10.1093/mnras/stv035. arXiv:1501.02717 [astro-ph.GA]

Hong J, Askar A, Giersz M, Hypki A, Yoon SJ (2020) MOCCA-SURVEY database I: binary black hole mergers from globular clusters with intermediate mass black holes. MNRAS. https://doi.org/10.1093/mnras/staa2677. arXiv:2008.10823 [astro-ph.HE]

Hopkins PF, Quataert E (2010) How do massive black holes get their gas? MNRAS 407(3):1529–1564. https://doi.org/10.1111/j.1365-2966.2010.17064.x. arXiv:0912.3257 [astro-ph.CO]
Hopkins PF, Richards GT, Hernquist L (2007) An observational determination of the bolometric quasar luminosity function. ApJ 654(2):731–753. https://doi.org/10.1086/509629. arXiv:astro-ph/0605678 [astro-ph]

Hopkins PF, Kereš D, Oñorbe J, Faucher-Giguère CA, Quataert E, Murray N, Bullock JS (2014) Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation. MNRAS 445(1):581–603. https://doi.org/10.1093/mnras/stu1738. arXiv:1311.2073 [astro-ph.CO]

Hopkins PF, Wetzel A, Kereš D, Faucher-Giguère CA, Quataert E, Boylan-Kolchin M, Murray N, Hayward CC, Garrison-Kimmel S, Hummels C et al (2018) FIRE-2 simulations: physics versus numerics in galaxy formation. MNRAS 480(1):800–863. https://doi.org/10.1093/mnras/sty1690. arXiv:1702.06148 [astro-ph.GA]

Hopman C, Alexander T (2006) Resonant relaxation near a massive black hole: the stellar distribution and gravitational wave sources. ApJ 645(2):1152–1163. https://doi.org/10.1086/504400. arXiv:astro-ph/0601161 [astro-ph]

Hopman C, Freitag M, Larson SL (2007) Gravitational wave bursts from the Galactic massive black hole. MNRAS 378(1):129–136. https://doi.org/10.1111/j.1365-2966.2007.11758.x. arXiv:astro-ph/0612337 [astro-ph]

Horton MA, Hardcastle MJ, Read SC, Krause MHG (2020) A Markov chain Monte Carlo approach for measurement of jet precession in radio-loud active galactic nuclei. MNRAS 493(3):3911–3919. https://doi.org/10.1093/mnras/staa429. arXiv:2002.04966 [astro-ph.GA]

Howitt G, Stevenson S, Vigna-Gómez Ar, Justham S, Ivanova N, Woods TE, Neijssel CJ, Mandel I (2020) Luminous Red Novae: population models and future prospects. MNRAS 492(3):3229–3240. https://doi.org/10.1093/mnras/stz3542. arXiv:1912.07771 [astro-ph.HE]

Hoyle F, Lyttleton RA (1939) The effect of interstellar matter on climatic variation. Proc Camb Philos Soc 35(3):405. https://doi.org/10.1017/S0305004100021150

Hu BX, D'Orazio DJ, Haiman Z, Smith KL, Snios B, Charisi M, Di Stefano R (2020) Spikey: self-lensing flares from eccentric SMBH binaries. MNRAS 495(4):4061–4070. https://doi.org/10.1093/mnras/sta1312. arXiv:1910.05348 [astro-ph.HE]

Hu XC, Li XH, Wang Y, Feng WF, Zhou MY, Hu YM, Hu SC, Mei JW, Shao CG (2018) Fundamentals of the orbit and response for TianQin. Class Quantum Grav 35(9):095008. https://doi.org/10.1088/1361-6382/aab52f. arXiv:1803.03368 [gr-qc]

Huang G, Wu X (2014) Dynamics of the post-Newtonian circular restricted three-body problem with compact objects. Phys Rev D 89(12):124034. https://doi.org/10.1103/PhysRevD.89.124034

Huang SJ, Hu YM, Korol V, Li PC, Liang ZC, Lu Y, Wang HT, Yu S, Mei J (2020) Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries. Phys Rev D 102:063021. https://doi.org/10.1103/PhysRevD.102.063021. arXiv:2005.07889 [astro-ph.HE]

Hughes SA, Blandford RD (2003) Black hole mass and spin coevolution by mergers. ApJ 585(2):L101–L104. https://doi.org/10.1086/375495. arXiv:astro-ph/0208484 [astro-ph]

Hui CY, Wu K, Han Q, Kong AKH, Tam PHT (2018) On the orbital properties of millisecond pulsar binaries. ApJ 864(1):30. https://doi.org/10.3847/1538-4357/aad5ec. arXiv:1807.09001 [astro-ph.HE]

Hui L, Ostriker JP, Tremaine S, Witten E (2017) Ultralight scalars as cosmological dark matter. Phys Rev D 95(4):043541. https://doi.org/10.1103/PhysRevD.95.043541. arXiv:1610.08297 [astro-ph.CO]

Hulse RA, Taylor JH (1975) Discovery of a pulsar in a binary system. ApJ 195:L51–L53. https://doi.org/10.1086/181708

Hurley JR, Tout CA, Pols OR (2002) Evolution of binary stars and the effect of tides on binary populations. MNRAS 329(4):897–928. https://doi.org/10.1046/j.1365-8711.2002.05038.x. arXiv:astro-ph/0201220 [astro-ph]

Hut P (1981) Tidal evolution in close binary systems. A&A 99:126–140

Hut P, Bahcall JN (1983) Binary-single star scattering. I—Numerical experiments for equal masses. ApJ 268:319–341. https://doi.org/10.1086/160956

Hut P, Paczynski B (1984) Effects of encounters with field stars on the evolution of low-mass semidetached binaries. ApJ 284:675–684. https://doi.org/10.1086/162450

Hut P, McMillan S, Goodman J, Mateo M, Phinney ES, Pryor C, Richer HB, Verbunt F, Weinberg M (1992) Binaries in globular clusters. PASP 104:981. https://doi.org/10.1086/133085

Hypki A, Giersz M (2013) MOCCA code for star cluster simulations—I. Blue stragglers, first results. MNRAS 429(2):1221–1243. https://doi.org/10.1093/mnras/sts415. arXiv:1207.6700 [astro-ph.GA]
Iaconi R, De Marco O, Passy JC, Staff J (2018) The effect of binding energy and resolution in simulations of the common envelope binary interaction. MNRAS 477(2):2349–2365. https://doi.org/10.1093/mnras/sty974. arXiv:1706.09786 [astro-ph.SR]

Iben J Icko, Webbink RF (1987) On the formation and properties of close binary white dwarfs. In: Philip AGD, Hayes DF, Liebert JW (eds) The second conference on faint blue stars. IAU colloquia, vol 95. L. Davis Press, Schenectady, NY, p 401

Icko Iben J, Tutukov AV, Fedorova ArV (1998) On the luminosity of white dwarfs in close binaries merging under the influence of gravitational wave radiation. ApJ 503(1):344–349. https://doi.org/10.1086/305972

Inayoshi K, Haiman Z, Ostriker JP (2016) Hyper-Eddington accretion flows on to massive black holes. MNRAS 459:3738–3755. https://doi.org/10.1093/mnras/stw836. arXiv:1511.02116 [astro-ph.HE]

Inayoshi K, Hirai R, Kinugawa T, Hotokezaka K (2017) Formation pathway of Population III coalescing binary black holes through stable mass transfer. MNRAS 468(4):5020–5032. https://doi.org/10.1093/mnras/stx757. arXiv:1701.04823 [astro-ph.HE]

Inayoshi K, Tamanini N, Caprini C, Haiman Z (2017) Probing stellar binary black hole formation in galactic nuclei via the imprint of their center of mass acceleration on their gravitational wave signal. Phys Rev D 96(6):063014. https://doi.org/10.1103/PhysRevD.96.063014. arXiv:1702.06529 [astro-ph.HE]

Inayoshi K, Visbal E, Haiman Z (2020) The assembly of the first massive black holes. ARA&A 58:27–97. https://doi.org/10.1146/annurev-astro-120419-014455. arXiv:1911.05791 [astro-ph.GA]

Inman D, Ali-Haïmoud Y (2019) Early structure formation in primordial black hole cosmologies. Phys Rev D 100(8):083528. https://doi.org/10.1103/PhysRevD.100.083528. arXiv:1907.08129 [astro-ph.CO]

Inomata K, Nakama T (2019) Gravitational waves induced by scalar perturbations as probes of the small-scale primordial spectrum. Phys Rev D 99(4):043511. https://doi.org/10.1103/PhysRevD.99.043511. arXiv:1812.00674 [astro-ph.CO]

Inomata K, Kawasaki M, Mukaida K, Tada Y, Yanagida TT (2017) Inflationary primordial black holes for the LIGO gravitational wave events and pulsar timing array experiments. Phys Rev D 95(12):123510. https://doi.org/10.1103/PhysRevD.95.123510. arXiv:1611.06130 [astro-ph.CO]

in't Zand JJM, Cumming A, van der Sluys MV, Verbunt F, Pols OR (2005) On the possibility of a helium white dwarf donor in the presumed ultracompact binary 2S 0918–549. A&A 441(2):675–684. https://doi.org/10.1051/0004-6361:20053002. arXiv:astro-ph/0506666 [astro-ph]

Iorio L (2012) General relativistic spin-orbit and spin-spin effects on the motion of rotating particles in an external gravitational field. Gen Relativ Gravit 44(3):719–736. https://doi.org/10.1007/s10714-011-1302-7. arXiv:1012.5622 [gr-qc]

Ishibashi W, Fabian AC (2016) AGN-starburst evolutionary connection: a physical interpretation based on radiative feedback. MNRAS 463(2):1291–1296. https://doi.org/10.1093/mnras/stw2063. arXiv:1609.08963 [astro-ph.GA]

Isoyama S, Nakano H, Nakamura T (2018) Multiband gravitational-wave astronomy: observing binary inspirals with a decihertz detector, B-DECIGO. PTEP 2018(7):073E01. https://doi.org/10.1093/ptep/pty078. arXiv:1802.06977 [gr-qc]

Istrate AG, Tauris TM, Langer N (2014) The formation of low-mass helium white dwarfs orbiting pulsars. Evolution of low-mass X-ray binaries below the bifurcation period. A&A 571:A45. https://doi.org/10.1051/0004-6361/201424680

Istrate AG, Tauris TM, Langer N, Antoniadis J (2014) The timescale of low-mass proto-helium white dwarf evolution. A&A 571:L3. https://doi.org/10.1051/0004-6361/201424681. arXiv:1410.5471 [astro-ph.SR]

Istrate AG, Marchant P, Tauris TM, Langer N, Stancliffe RJ, Grassitelli L (2016) Models of low-mass helium white dwarfs including gravitational settling, thermal and chemical diffusion, and rotational mixing. A&A 595:A35. https://doi.org/10.1051/0004-6361/201628874. arXiv:1606.04947 [astro-ph.SR]

Ivanov PB, Papaloizou JCB, Paardekooper SJ, Polnarev AG (2015) The evolution of a binary in a retrograde circular orbit embedded in an accretion disk. A&A 576:A29. https://doi.org/10.1051/0004-6361/201424359. arXiv:1410.3250 [astro-ph.HE]

Ivanova N, Belczynski K, Kalogera V, Rasio FA, Taam RE (2003) The role of helium stars in the formation of double neutron stars. ApJ 592(1):475–485. https://doi.org/10.1086/375578. arXiv:astro-ph/0210267 [astro-ph]
Ivanova N, Heinke CO, Rasio FA, Taam RE, Belczynski K, Fregeau J (2006) Formation and evolution of compact binaries in globular clusters—I. Binaries with white dwarfs. MNRAS 372(3):1043–1059.
https://doi.org/10.1111/j.1365-2966.2006.10876.x. arXiv:astro-ph/0604085 [astro-ph]

Ivanova N, Justham S, Chen X, De Marco O, Fryer CL, Gaburov E, Ge H, Glebbeek E, Han Z, Li XD et al (2013) Common envelope evolution: where we stand and how we can move forward. A&A Rev 21:59. https://doi.org/10.1007/s00159-013-0059-2. arXiv:1209.4302 [astro-ph.HE]

Ivanova N, Justham S, Ricker P (2020) Common envelope evolution. IOP Publishing. https://doi.org/10.1088/2514-3433/abb6f0

Ivezić Ž, Kahn SM, Tyson JA, Abel B, Acosta E, Allsman R, Alonso D, AlSayyad Y, Anderson SF, Andrew J et al (2019) LSST: from science drivers to reference design and anticipated data products. ApJ 873(2):111. https://doi.org/10.3847/1538-4357/ab042c. arXiv:0805.2366 [astro-ph]

Izquierdo-Villalba D, Bonoli S, Dotti M, Sesana A, Rosas-Guevara Y, Spinoso D (2020) From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments. MNRAS 495(4):4681–4706. https://doi.org/10.1093/mnras/staa1399. arXiv:2001.10548 [astro-ph.GA]

Izzard RG (2004) Nucleosynthesis in binary stars. PhD thesis, University of Cambridge

Izzard RG, Dray LM, Karakas AI, Lugaro M, Tout CA (2006) Population nucleosynthesis in single and binary stars. I. Model. A&A 460(2):565–572. https://doi.org/10.1051/0004-6361/20066129

Izzard RG, Glebbeek E, Stancliffe RJ, Pols OR (2009) Population synthesis of binary carbon-enhanced metal-poor stars. A&A 508(3):1359–1374. https://doi.org/10.1051/0004-6361/200912827. arXiv:0910.2158 [astro-ph.SR]

Jani K, Shoemaker D, Cutler C (2019) Detectability of intermediate-mass black holes in multiband gravitational wave astronomy. Nat Astron 4:260–265. https://doi.org/10.1038/s41550-019-0932-7. arXiv:1908.04985 [gr-qc]

Janka HT (2012) Explosion mechanisms of core-collapse supernovae. Annu Rev Nucl Part Sci 62(1):407–451. https://doi.org/10.1146/annurev-nucl-102711-094901. arXiv:1206.2503 [astro-ph.SR]

Janka HT (2017) Neutron star kicks by the gravitational tug-boat mechanism in asymmetric supernova explosions: progenitor and explosion dependence. ApJ 837(1):84. https://doi.org/10.3847/1538-4357/aa618e. arXiv:1611.07562 [astro-ph.HE]

Jha SW, Maguire K, Sullivan M (2019) Observational properties of thermonuclear supernovae. Nat Astron 3:706–716. https://doi.org/10.1038/s41550-019-0858-0. arXiv:1908.02303 [astro-ph.HE]

Jia K, Li XD (2016) Evolution of low-mass X-ray binaries: the effect of donor evaporation. ApJ 830 (2):153. https://doi.org/10.3847/0004-637X/830/2/153. arXiv:1608.01076 [astro-ph.HE]

Jiang YF, Blaes O (2020) Opacity-driven convection and variability in accretion disks around supermassive black holes. ApJ 900(1):25. https://doi.org/10.3847/1538-4357/aba4b7. arXiv:2006.08657 [astro-ph.HE]

Jiang YF, Stone JM, Davis SW (2014) A global three-dimensional radiation magneto-hydrodynamic simulation of super-eddington accretion disks. ApJ 796(2):106. https://doi.org/10.1088/0004-637X/796/2/106. arXiv:1410.0678 [astro-ph.HE]

Jiang YF, Davis SW, Stone JM (2016) Iron opacity bump changes the stability and structure of accretion disks in active galactic nuclei. ApJ 827(1):10. https://doi.org/10.3847/0004-637X/827/1/10. arXiv:1601.06836 [astro-ph.HE]

Jiang YF, Blaes O, Stone JM, Davis SW (2019) Global radiation magnetohydrodynamic simulations of sub-Eddington accretion disks around supermassive black holes. ApJ 885(2):144. https://doi.org/10.3847/1538-4357/ab4a00. arXiv:1904.01674 [astro-ph.HE]

Johannsen T (2013) Regular black hole metric with three constants of motion. Phys Rev D 88(4):044002.
https://doi.org/10.1103/PhysRevD.88.044002. arXiv:1501.02809 [gr-qc]

Johnson JL, Haardt F (2016) The early growth of the first black holes. PASA 33:e007. https://doi.org/10.1017/pasa.2016.4. arXiv:1601.05473 [astro-ph.GA]

Johnson M, Haworth K, Pesce DW, Palumbo DCM, Blackburn L, Akiyama K, Boroson D, Bouman KL, Farah JR, Fish VL et al (2019) Studying black holes on horizon scales with space-VLBI. In: Bulletin of the American Astronomical Society, vol 51, p 235. arXiv:1909.01405 [astro-ph.IM]

Jones S, Hirsch R, Nomoto K, Fischer T, Timmes FX, Herwig F, Paxton B, Toki H, Suzuki T, Martínez-Pinedo G et al (2013) Advanced burning stages and fate of 8–10 M⊙ stars. ApJ 772(2):150. https://doi.org/10.1088/0004-637X/772/2/150. arXiv:1306.2030 [astro-ph.SR]

Ju W, Greene JE, Rafikov RR, Bickerton SJ, Badenes C (2013) Search for supermassive black hole binaries in the Sloan digital sky survey spectroscopic sample. ApJ 777(1):44. https://doi.org/10.1088/0004-637X/777/1/44. arXiv:1306.4987 [astro-ph.CO]
Juett AM, Psaltis D, Chakrabarty D (2001) Ultracompact X-ray binaries with neon-rich degenerate donors. ApJ 560(1):L59-L63. https://doi.org/10.1086/324225. arXiv:astro-ph/0108102 [astro-ph]

Just A, Yurin D, Makukov M, Berczik P, Omarov C, Spurzem R, Vilkoviskij EY (2012) Enhanced accretion rates of stars on supermassive black holes by star-disk interactions in galactic nuclei. ApJ 758(1):51. https://doi.org/10.1088/0004-637X/758/1/51. arXiv:1208.4954 [astro-ph.CO]

Kahabka P, van den Heuvel EPJ (1997) Luminous supersoft X-ray sources. ARA&A 35:69-100. https://doi.org/10.1146/annurev.astro.35.1.69

Kalaja A, Bellomo N, Bartolo N, Bertacca D, Matarrese S, Musco I, Raccanelli A, Verde L (2019) From primordial black holes abundance to primordial curvature power spectrum (and back). J Cosmol Astropart Phys 10:031. https://doi.org/10.1088/1475-7516/2019/10/031. arXiv:1908.03596 [astro-ph.CO]

Kalfountzou E, Santos Lleo M, Trichas M (2017) SDSS J1056+5516: a triple AGN or an SMBH recoil candidate? ApJ 851(1):L15. https://doi.org/10.3847/2041-8213/aa9b2d. arXiv:1712.03909 [astro-ph.GA]

Kalogera V, Belczynski K, Kim C, O'Shaughnessy R, Willems B (2007) Formation of double compact objects. Phys Rep 442(1-6):75-108. https://doi.org/10.1016/j.physrep.2007.02.008. arXiv:astro-ph/0612144 [astro-ph]

Karnesis N, Lilley M, Petiteau A (2020) Assessing the detectability of a Stochastic Gravitational Wave Background with LISA, using an excess of power approach. Class Quantum Grav 37:215017. https://doi.org/10.1088/1361-6382/abb637. arXiv:1906.09027 [astro-ph.IM]

Karnesis N, Babak S, Pieroni M, Cornish N, Littenberg T (2021) Characterization of the stochastic signal originating from compact binary populations as measured by LISA. Phys Rev D 104(4):043019. https://doi.org/10.1103/PhysRevD.104.043019. arXiv:2103.14598 [astro-ph.IM]

Kato M, Hachisu I (1999) A new estimation of mass accumulation efficiency in helium shell flashestoward type IA supernova explosions. ApJ 513(1):L41-L44. https://doi.org/10.1086/311893. arXiv:astro-ph/9901080 [astro-ph]

Katz H, Sijacki D, Haehnelt MG (2015) Seeding high-redshift QSOs by collisional runaway in primordial star clusters. MNRAS 451(3):2352-2369. https://doi.org/10.1093/mnras/stv1048. arXiv:1502.03448 [astro-ph.GA]

Katz ML, Kelley LZ, Dosopoulou F, Berry S, Blecha L, Larson SL (2020) Probing massive black hole binary populations with LISA. MNRAS 491(2):2301-2317. https://doi.org/10.1093/mnras/stz3102. arXiv:1908.05779 [astro-ph.HE]

Kauffmann G, Haehnelt M (2000) A unified model for the evolution of galaxies and quasars. MNRAS 311 (3):576-588. https://doi.org/10.1046/j.1365-8711.2000.03077.x. arXiv:astro-ph/9906493 [astro-ph]

Kauffmann G, White SDM, Guiderdoni B (1993) The formation and evolution of galaxies within merging dark matter haloes. MNRAS 264:201-218. https://doi.org/10.1093/mnras/264.1.201

Kavanagh BJ, Nichols DA, Bertone G, Gaggero D (2020) Detecting dark matter around black holes with gravitational waves: effects of dark-matter dynamics on the gravitational waveform. Phys Rev D 102 (8):083006. https://doi.org/10.1103/PhysRevD.102.083006. arXiv:2002.12811 [gr-qc]

Kawamura S, Ando M, Seto N, Sato S, Nakamura T, Tsubono K, Kand AN, Tanaka T, Yokoyama J, Funaki I, et al (2011) The Japanese space gravitational wave antenna: DECIGO. CQGra 28 (9):094011. https://doi.org/10.1088/0264-9381/28/9/094011

Kawamura S, Ando M, Seto N, Sato S, Musha M, Kawano I, Yokoyama J, Tanaka T, Ioka K, Akutsu T et al (2020) Current status of space gravitational wave antenna DECIGO and B-DECIGO. arXiv e-prints arXiv:2006.13545 [gr-qc]

Kawanaka N, Yamaguchi M, Piran T, Bulik T (2017) Prospects for the discovery of black hole binaries without mass accretion with Gaia. In: Gomboc A (ed) New frontiers in black hole astrophysics. IAU symposium, vol 324, pp 41-42. https://doi.org/10.1017/S1743921316012606

Kawka A, Vennes S, Ferrario L (2020) An ancient double degenerate merger in the Milky Way halo. MNRAS 491(1):L40-L45. https://doi.org/10.1093/mnrasl/slz165. arXiv:1910.13053 [astro-ph.SR]

Keane E, Bhattacharyya B, Kramer M, Stappers B, Keane EF, Bhattacharyya B, Kramer M, Stappers BW et al (2015) A cosmic census of radio pulsars with the SKA. In: Advancing astrophysics with the square kilometre array (AASKA14), p 40. arXiv:1501.00056 [astro-ph.IM]

Kelley L, Charisi M, Burke-Spolaor S, Simon J, Blecha L, Bogdanovic T, Colpi M, Comerford J, D'Orazio D, Dotti M et al (2019) Multi-messenger astrophysics with pulsar timing arrays. BAAS 51(3):490 arXiv:1903.07644 [astro-ph.HE]
Kelley LZ, Blecha L, Hernquist L (2017) Massive black hole binary mergers in dynamical galactic environments. MNRAS 464(3):3131–3157. https://doi.org/10.1093/mnras/stw2452. arXiv:1606.01900 [astro-ph.HE]

Kelley LZ, Blecha L, Hernquist L, Sesana A, Taylor SR (2017) The gravitational wave background from massive black hole binaries in Illustris: spectral features and time to detection with pulsar timing arrays. MNRAS 471(4):4508–4526. https://doi.org/10.1093/mnras/stx1638. arXiv:1702.02180 [astro-ph.HE]

Kelley LZ, Blecha L, Hernquist L, Sesana A, Taylor SR (2018) Single sources in the low-frequency gravitational wave sky: properties and time to detection by pulsar timing arrays. MNRAS 477 (1):964–976. https://doi.org/10.1093/mnras/sty689. arXiv:1711.00075 [astro-ph.HE]

Kelly BJ, Baker JG, Etienne ZB, Giacomazzo B, Schnittman J (2017) Prompt electromagnetic transients from binary black hole mergers. Phys Rev D 96(12):123003. https://doi.org/10.1103/PhysRevD.96.123003. arXiv:1710.02132 [astro-ph.HE]

Kennedy GF, Meiron Y, Shukirgaliyev B, Panamarev T, Berczik P, Just A, Spurzem R (2016) Star-disc interaction in galactic nuclei: orbits and rates of accreted stars. MNRAS 460(1):240–255. https://doi.org/10.1093/mnras/stw908. arXiv:1604.05309 [astro-ph.GA]

Kerr M, Reardon DJ, Hobbs G, Shannon RM, Manchester RN, Dai S, Russell CJ, Zhang S, van Straten W, Oslowski S et al (2020) The Parkes Pulsar Timing Array project: second data release. PASA 37:e020. https://doi.org/10.1017/pasa.2020.11. arXiv:2003.09780 [astro-ph.IM]

Kesden M, Sperhake U, Berti E (2010) Final spins from the merger of precessing binary black holes. Phys Rev D 81(8):084054. https://doi.org/10.1103/PhysRevD.81.084054. arXiv:1002.2643 [astro-ph.GA]

Kesden M, Sperhake U, Berti E (2010) Relativistic suppression of black hole recoils. ApJ 715(2):1006–1011. https://doi.org/10.1088/0004-637X/715/2/1006. arXiv:1003.4993 [astro-ph.CO]

Kesden M, Gerosa D, O’Shaughnessy R, Berti E, Sperhake U (2015) Effective potentials and morphological transitions for binary black hole spin precession. Phys Rev Lett 114(8):081103. https://doi.org/10.1103/PhysRevLett.114.081103. arXiv:1411.0674 [gr-qc]

Khan A, Paschalidis V, Ruiz M, Shapiro SL (2018) Disks around merging binary black holes: from GW150914 to supermassive black holes. Phys Rev D 97(4):044036. https://doi.org/10.1103/PhysRevD.97.044036. arXiv:1801.02624 [astro-ph.HE]

Khan FM, Just A, Merritt D (2011) Efficient merger of binary supermassive black holes in merging galaxies. ApJ 732(2):89. https://doi.org/10.1088/0004-637X/732/2/89. arXiv:1103.0272 [astro-ph.CO]

Khan FM, Preto M, Berczik P, Berentzen I, Just A, Spurzem R (2012) Mergers of unequal-mass galaxies: supermassive black hole binary evolution and structure of merger remnants. ApJ 749(2):147. https://doi.org/10.1088/0004-637X/749/2/147. arXiv:1202.2124 [astro-ph.CO]

Khan FM, Fiacconi D, Mayer L, Berczik P, Just A (2016) Swift coalescence of supermassive black holes in cosmological mergers of massive galaxies. ApJ 828(2):73. https://doi.org/10.3847/0004-637X/828/2/73. arXiv:1604.00015 [astro-ph.GA]

Khan FM, Berczik P, Just A (2018) Gravitational wave driven mergers and coalescence time of supermassive black holes. A&A 615:A71. https://doi.org/10.1051/0004-6361/201730489. arXiv:1803.11394 [astro-ph.GA]

Khan FM, Capelo PR, Mayer L, Berczik P (2018) Dynamical evolution and merger timescales of LISA massive black hole binaries in disk galaxy mergers. ApJ 868(2):97. https://doi.org/10.3847/1538-4357/aae77b. arXiv:1807.11004 [astro-ph.GA]

Khan FM, Mirza MA, Holley-Bockelmann K (2020) Inward bound: the incredible journey of massive black holes as they pair and merge—I. The effect of mass ratio in flattened rotating galactic nuclei. MNRAS 492(1):256–267. https://doi.org/10.1093/mnras/stz3360. arXiv:1911.07946 [astro-ph.GA]

Kidder LE (1995) Coalescing binary systems of compact objects to (post)5/2–Newtonian order. V. Spin effects. Phys Rev D 52(2):821–847. https://doi.org/10.1103/PhysRevD.52.821. arXiv:gr-qc/9506022 [gr-qc]

Kilic M, Brown WR, Hermes JJ, Allende Prieto C, Kenyon SJ, Winget DE, Winget KI (2011) SDSS J163030.58+423305.8: a 40-min orbital period detached white dwarf binary. MNRAS 418(1):L157–L161. https://doi.org/10.1111/j.1745-3933.2011.01165.x. arXiv:1109.6339 [astro-ph.GA]

Kilic M, Brown WR, Allende Prieto C, Kenyon SJ, Heinke CO, Agüeros MA, Kleinman SJ (2012) The ELM survey. IV. 24 white dwarf merger systems. ApJ 751(2):141. https://doi.org/10.1088/0004-637X/751/2/141. arXiv:1204.0028 [astro-ph.GA]
Kilic M, Brown WR, Gianninas A, Hermes JJ, Allende Prieto C, Kenyon SJ (2014) A new gravitational wave verification source. MNRAS 444:L1–L5. https://doi.org/10.1093/mnrasl/slu093. arXiv:1406.3346 [astro-ph.SR]

Kilic M, Brown WR, Gianninas A, Curd B, Bell KJ, Allende Prieto C (2017) A Gemini snapshot survey for double degenerates. MNRAS 471(4):4218–4227. https://doi.org/10.1093/mnras/stx1886. arXiv:1707.08948 [astro-ph.SR]

Kim C, Kalogera V, Lorimer DR (2003) The probability distribution of binary pulsar coalescence rates. I. Double neutron star systems in the galactic field. ApJ 584(2):985–995. https://doi.org/10.1086/345740. arXiv:astro-ph/0207408 [astro-ph]

Kim DC, Yoon I, Privon GC, Evans AS, Harvey D, Stierwalt S, Kim JH (2017) A potential recoiling supermassive black hole, CXO J101527.2+625911. ApJ 840(2):71. https://doi.org/10.3847/1538-4357 aa6030. arXiv:1704.05549 [astro-ph.GA]

Kimpson T, Wu K, Zane S (2019) Pulsar timing in extreme mass ratio binaries: a general relativistic approach. MNRAS 486(1):360–377. https://doi.org/10.1093/mnras/stz845. arXiv:1903.08258 [astro-ph.HE]

Kimpson T, Wu K, Zane S (2019) Spatial dispersion of light rays propagating through a plasma in Kerr space-time. MNRAS 484(2):2411–2419. https://doi.org/10.1093/mnras/stz138. arXiv:1901.03733 [astro-ph.HE]

Kimpson T, Wu K, Zane S (2020) Gravitational burst radiation from pulsars in the Galactic centre and stellar clusters. MNRAS 495(1):600–613. https://doi.org/10.1093/mnras/staa1259. arXiv:2005.02053 [astro-ph.HE]

Kimpson T, Wu K, Zane S (2020) Orbital spin dynamics of a millisecond pulsar around a massive BH with a general mass quadrupole. MNRAS 497(4):5421–5431. https://doi.org/10.1093/mnras/staa2103. arXiv:2007.05219 [astro-ph.HE]

King A (2003) Black holes, galaxy formation, and the $M_{BH}-\sigma$ relation. ApJ 596(1):L27–L29. https://doi.org/10.1086/379143. arXiv:astro-ph/0308342 [astro-ph]

King AR, Pringle JE (2006) Growing supermassive black holes by chaotic accretion. MNRAS 373(1): L90–L92. https://doi.org/10.1111/j.1745-3933.2006.00249.x. arXiv:astro-ph/0609598 [astro-ph]

King AR, Frank J, Whitehurst R (1990) Synchronous rotation in AM Herculis systems-I. Equilibrium configurations. MNRAS 244:731

King AR, Pringle JE, Hofmann JA (2008) The evolution of black hole mass and spin in active galactic nuclei. MNRAS 385(3):1621–1627. https://doi.org/10.1111/j.1365-2966.2008.12943.x. arXiv:0801.1564 [astro-ph]

Kiseleva LG, Eggleton PP, Orlov VV (1994) Instability of close triple systems with coplanar initial doubly circular motion. MNRAS 270:936–946. https://doi.org/10.1093/mnras/270.4.936

Kiseleva LG, Eggleton PP, Mikkola S (1998) Tidal friction in triple stars. MNRAS 300(1):292–302. https://doi.org/10.1046/j.1365-8711.1998.01903.x

Kiuchi K, Maeda KI (2004) Gravitational waves from a chaotic dynamical system. Phys Rev D 70 (6):064036. https://doi.org/10.1103/PhysRevD.70.064036. arXiv:gr-qc/0404124 [gr-qc]

Kiuchi K, Shibata M, Montero PJ, Font JA (2011) Gravitational waves from the Papaloizou-Pringle instability in black-hole-torus systems. Phys Rev Lett 106(25):251102. https://doi.org/10.1103/PhysRevLett.106.251102. arXiv:1105.5035 [astro-ph.HE]

Klein A, Barausse E, Sesana A, Petiteau A, Berti E, Babak S, Gair J, Aoudia S, Hinder I, Ohme F et al (2016) Science with the space-based interferometer eLISA: supermassive black hole binaries. Phys Rev D 93(2):024003. https://doi.org/10.1103/PhysRevD.93.024003. arXiv:1511.05581 [gr-qc]

Klencki J, Moe M, Gladysz W, Chruslinska M, Holz DE, Belczynski K (2018) Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers. A&A 619:A77. https://doi.org/10.1051/0004-6361/201833025. arXiv:1808.07889 [astro-ph.HE]

Klugge C, Baraffe I, Patterson J (2011) The evolution of cataclysmic variables as revealed by their donor stars. ApJS 194(2):28. https://doi.org/10.1088/0067-0049/194/2/28. arXiv:1102.2440 [astro-ph.SR]

Kobayashi S, Laguna P, Phinney ES, Mészáros P (2004) Gravitational waves and X-ray signals from stellar disruption by a massive black hole. ApJ 615(2):855–865. https://doi.org/10.1086/424684. arXiv:astro-ph/0404173 [astro-ph]

Kochanek CS (1992) Coalescing binary neutron stars. ApJ 398:234. https://doi.org/10.1086/171851

Kochanek CS, Shapiro SL, Teukolsky SA, Chernoff DF (1990) Gravitational radiation from colliding clusters: Newtonian simulations in three dimensions. ApJ 358:81. https://doi.org/10.1086/168964

Kocsis B, Tremaine S (2015) A numerical study of vector resonant relaxation. MNRAS 448(4):3265–3296. https://doi.org/10.1093/mnras/stv057. arXiv:1406.1178 [astro-ph.GA]
Kocsis B, Gáspár ME, Márka S (2006) Detection rate estimates of gravity waves emitted during parabolic encounters of stellar black holes in globular clusters. ApJ 648(1):411–429. https://doi.org/10.1086/505641. arXiv:astro-ph/0603441 [astro-ph]

Kocsis B, Yunes N, Loeb A (2011) Observable signatures of extreme mass-ratio inspiral black hole binaries embedded in thin accretion disks. Phys Rev D 84(2):024032. https://doi.org/10.1103/PhysRevD.84.024032. arXiv:1104.2322 [astro-ph.GA]

Koester D, Gänsicke BT, Farihi J (2014) The frequency of planetary debris around young white dwarfs. A&A 566:A34. https://doi.org/10.1051/0004-6361/201423691. arXiv:1404.2617 [astro-ph.SR]

Kohri K, Terada T (2021) Solar-mass primordial black holes explain NANOGrav hint of gravitational waves. Phys Lett B 813:136040. https://doi.org/10.1016/j.physletb.2020.136040. arXiv:2009.11853 [astro-ph.CO]

Kolb U (1993) A model for the intrinsic population of cataclysmic variables. A&A 271:149

Koliopanos F, Ciambur BC, Graham AW, Webb NA, Coriat M, Mutlu-Pakdil B, Davis BL, Godet O, Barret D, Seigar MS (2017) Searching for intermediate-mass black holes in galaxies with low-luminosity AGN: a multiple-method approach. A&A 601:A20. https://doi.org/10.1051/0004-6361/201630061. arXiv:1612.06794 [astro-ph.GA]

Koliopanos F, Peault M, Vasilopoulos G, Webb N (2020) The chemical composition of the accretion disk and donor star in Ultra Compact X-ray Binaries: a comprehensive X-ray analysis. MNRAS 501:548–563. https://doi.org/10.1093/mnras/staa3474. arXiv:2001.00716 [astro-ph.HE]

Kollmeier JA, Zasowski G, Rix HW, Johns M, Anderson SF, Drory N, Johnson JA, Pogge RW, Bird JC, Blanc GA et al (2017) SDSS-V: pioneering panoptic spectroscopy. arXiv e-prints arXiv:1711.03234 [astro-ph.GA]

Komossa S (2012) Recoiling black holes: electromagnetic signatures, candidates, and astrophysical implications. Adv Astron 2012:364973. https://doi.org/10.1155/2012/364973. arXiv:1202.1977 [astro-ph.CO]

Komossa S, Greiner J (1999) Discovery of a giant and luminous X-ray outburst from the optically inactive galaxy pair RX J1242.6-1119. A&A 349:L45–L48 arXiv:astro-ph/9908216 [astro-ph]

Komossa S, Zhou H, Lu H (2008) A recoiling supermassive black hole in the quasar SDSS J092712.65+294344.0? ApJ 678(2):L81. https://doi.org/10.1086/588656. arXiv:0804.4585 [astro-ph]

Konstantinidis S, Amaro-Seoane P, Kokkotas KD (2013) Investigating the retention of intermediate-mass black holes in star clusters using N-body simulations. A&A 557:A135. https://doi.org/10.1051/0004-6361/201219620. arXiv:1108.5175 [astro-ph.CO]

Kormendy J (2004) The stellar-dynamical search for supermassive black holes in galactic nuclei. In: Ho LC (ed) Coevolution of black holes and galaxies, p 1. arXiv:astro-ph/0306353 [astro-ph]

Kormendy J, Ho LC (2013) Coevolution (or not) of supermassive black holes and host galaxies. ARA&A 51(1):511–653. https://doi.org/10.1146/annurev-astro-082708-101811. arXiv:1304.7762 [astro-ph.CO]

Kormendy J, Richstone D (1995) Inward bound-the search for supermassive black holes in galactic nuclei. A&A&A 33:581. https://doi.org/10.1146/annurev.aa.33.090195.003053

Korol V, Safarzadeh M (2021) How can LISA probe a population of GW190425-like binary neutron stars in the Milky Way? MNRAS 502(4):5576–5583. https://doi.org/10.1093/mnras/stab310. arXiv:2012.03070 [astro-ph.HE]

Korol V, Rossi EM, Groot PJ, Nelemans G, Toonen S, Brown AGA (2017) Prospects for detection of detached double white dwarf binaries with Gaia, LSST and LISA. MNRAS 470(2):1894–1910. https://doi.org/10.1093/mnras/stx1285. arXiv:1703.02555 [astro-ph.HE]

Korol V, Koop O, Rossi EM (2018) Detectability of double white dwarfs in the local group with LISA. ApJ 866(2):L20. https://doi.org/10.3847/2041-8213/aae587. arXiv:1808.05959 [astro-ph.HE]

Korol V, Rossi EM, Barausse E (2019) A multimessenger study of the Milky Way’s stellar disc and bulge with LISA, Gaia, and LSST. MNRAS 483(4):5518–5533. https://doi.org/10.1093/mnras/sty3440. arXiv:1806.03306 [astro-ph.GA]

Korol V, Toonen S, Klein A, Belokurov V, Vincenzo F, Buscicchio R, Gerosa D, Moore CJ, Roebber E, Rossi EM et al (2020) Populations of double white dwarfs in Milky Way satellites and their detectability with LISA. A&A 638:A153. https://doi.org/10.1051/0004-6361/202037764. arXiv:2002.10462 [astro-ph.GA]

Korol V, Belokurov V, Moore CJ, Toonen S (2021) Weighing Milky Way satellites with LISA. MNRAS 502(1):L55–L60. https://doi.org/10.1093/mnrasl/slab003. arXiv:2010.05918 [astro-ph.GA]
Koss M, Blecha L, Mushotzky R, Hung CL, Veilleux S, Trakhtenbrot B, Schawinski K, Stern D, Smith N, Li Y et al (2014) SDSS1133: an unusually persistent transient in a nearby dwarf galaxy. MNRAS 445 (1):515–527. https://doi.org/10.1093/mnras/stu1673. arXiv:1401.6798 [astro-ph.GA]

Kostov VB, Moore K, Tamayo D, Jayawardhana R, Rinehart SA (2016) Tatooine's future: the eccentric response of Kepler's circumbinary planets to common-envelope evolution of their host stars. ApJ 832 (2):183. https://doi.org/10.3847/0004-6367X/832/2/183. arXiv:1610.03436 [astro-ph.EP]

Kozai Y (1962) Secular perturbations of asteroids with high inclination and eccentricity. AJ 67:591–598. https://doi.org/10.1086/108790

Kramer M, Schneider FRN, Ohlmann ST, Geier S, Schaffenroth V, Pakmor R, Röpke FK (2020) Formation of sdB-stars via common envelope ejection by substellar companions. A&A 642:A97. https://doi.org/10.1051/0004-6361/202038702. arXiv:2007.00019 [astro-ph.SR]

Kremer K, Breivik K, Larson SL, Kalogera V (2017) Accreting double white dwarf binaries: implications for LISA. ApJ 846(2):95. https://doi.org/10.3847/1538-4357/aa8557. arXiv:1707.01104 [astro-ph.HE]

Kremer K, Chatterjee S, Breivik K, Rodriguez CL, Larson SL, Rasio FA (2018) LISA sources in milky way globular clusters. Phys Rev Lett 120(19):191103. https://doi.org/10.1103/PhysRevLett.120. 191103. arXiv:1802.05661 [astro-ph.HE]

Kremer K, Chatterjee S, Rodriguez CL, Rasio FA (2018) Accreting black hole binaries in globular clusters. ApJ 852(1):29. https://doi.org/10.3847/1538-4357/aa99df. arXiv:1709.05444 [astro-ph.HE]

Kremer K, Chatterjee S, Ye CS, Rodriguez CL, Rasio FA (2019) How initial size governs core collapse in globular clusters. ApJ 871(1):38. https://doi.org/10.3847/1538-4357/aaf646. arXiv:1808.02204 [astro-ph.GA]

Kremer K, Rodriguez CL, Amaro-Seoane P, Breivik K, Chatterjee S, Katz ML, Larson SL, Rasio FA, Samsing J, Ye CS et al (2019) Post-Newtonian dynamics in dense star clusters: binary black holes in the LISA band. Phys Rev D 99(6):063003. https://doi.org/10.1103/PhysRevD.99.063003. arXiv: 1811.11812 [astro-ph.HE]

Kremer K, Spera M, Becker D, Chatterjee S, Di Carlo UN, Fragione G, Rodriguez CL, Ye CS, Rasio FA (2020a) Populating the upper black hole mass gap through stellar collisions in dense star clusters. ApJ 903:45. https://doi.org/10.3847/1538-4357/abb945. arXiv:2006.10771 [astro-ph.HE]

Kremer K, Ye CS, Rui NZ, Weatherford NC, Chatterjee S, Fragione G, Rodriguez CL, Spera M, Rasio FA (2020b) Modeling dense star clusters in the milky way and beyond with the CMC cluster catalog. ApJS 247(2):48. https://doi.org/10.3847/1538-4365/ab7919. arXiv:1911.00018 [astro-ph.HE]

Krolik JH, Volonteri M, Dubois Y, Devriendt J (2019) Population estimates for electromagnetically distinguishable supermassive binary black holes. ApJ 879(2):110. https://doi.org/10.3847/1538-4357/ ab24c9. arXiv:1905.10450 [astro-ph.GA]

Kroupa P (2001) On the variation of the initial mass function. MNRAS 322(2):231–246. https://doi.org/10. 1046/j.1365-8711.2001.04022.x. arXiv:astro-ph/0009005 [astro-ph]

Kruckow MU, Tauris TM, Langer N, Szécsi D, Marchant P, Podsiadlowski P (2016) Common-envelope ejection in massive binary stars. Implications for the progenitors of GW150914 and GW151226. A&A 596:A58. https://doi.org/10.1051/0004-6361/201629420. arXiv:1610.04417 [astro-ph.SR]

Kruckow MU, Tauris TM, Langer N, Kramer M, Izzard RG (2018) Progenitors of gravitational wave mergers: binary evolution with the stellar grid-based code COMBINE. MNRAS 481(2):1908–1949. https://doi.org/10.1093/mnras/sty2190. arXiv:1801.05433 [astro-ph.SR]

Krumholz MR (2014) The big problems in star formation: the star formation rate, stellar clustering, and the initial mass function. Phys Rep 539:49–134. https://doi.org/10.1016/j.physrep.2014.02.001. arXiv: 1402.0867 [astro-ph.GA]

Kuhlen M, Vogelsberger M, Angulo R (2012) Numerical simulations of the dark universe: state of the art and the next decade. Phys Dark Universe 1(1–2):50–93. https://doi.org/10.1016/j.dark.2012.10.002. arXiv:1209.5745 [astro-ph.CO]

Kuin NPM, Wu K, Oates S, Lien A, Emery S, Kennea JA, de Pasquale M, Han Q, Brown PJ, Tohuvavohu A et al (2019) Swift spectra of AT2018cow: a white dwarf tidal disruption event? MNRAS 487 (2):2505–2521. https://doi.org/10.1093/mnras/stz053. arXiv:1808.08492 [astro-ph.HE]

Kulkarni G, Loeb A (2012) Formation of galactic nuclei with multiple supermassive black holes at high redshifts. MNRAS 422(2):1306–1323. https://doi.org/10.1111/j.1365-2966.2012.20699.x. arXiv: 1107.0517 [astro-ph.CO]

Kulkarni SR, Ofek EO, Rau A, Cenko SB, Soderberg AM, Fox DB, Gal-Yam A, Capak PL, Moon DS, Li W et al (2007) An unusually brilliant transient in the galaxy M85. Nature 447(7143):458–460. https:// doi.org/10.1038/nature05822. arXiv:0705.3668 [astro-ph]
Kumamoto J, Fujii MS, Tanikawa A (2019) Gravitational-wave emission from binary black holes formed in open clusters. MNRAS 486(3):3942–3950. https://doi.org/10.1093/mnras/stz1068. arXiv:1811.06726 [astro-ph.HE]

Kumamoto J, Fujii MS, Tanikawa A (2020) Merger rate density of binary black holes formed in open clusters. MNRAS 495(4):4268–4278. https://doi.org/10.1093/mnras/staa1440. arXiv:2001.10690 [astro-ph.HE]

Kupfer T, Groot PJ, Bloemen S, Levitan D, Steeghs D, Marsh TR, Rutten RGM, Nelemans G, Prince TA, Fürst F et al (2015) Phase-resolved spectroscopy and Kepler photometry of the ultracompact AM CVn binary SDSS J190817.07+394036.4. MNRAS 453(1):483–496. https://doi.org/10.1093/mnras/stv1609. arXiv:1507.03926 [astro-ph.SR]

Kupfer T, Ramsay G, van Roestel J, Brooks J, MacFarlane SA, Toma R, Groot PJ, Woudt PA, Bildsten L et al (2017) The OmegaWhite survey for short-period variable stars. V. Discovery of an ultracompact hot subdwarf binary with a compact companion in a 44-minute orbit. ApJ 851(1):28. https://doi.org/10.3847/1538-4357/aa9522. arXiv:1710.07287 [astro-ph.SR]

Kupfer T, Korol V, Shah S, Nelemans G, Marsh TR, Ramsay G, Groot PJ, Steeghs DTH, Rossi EM (2018) LISA verification binaries with updated distances from Gaia Data Release 2. MNRAS 480(1):302–309. https://doi.org/10.1093/mnras/sty1545. arXiv:1805.00482 [astro-ph.SR]

Kupfer T, Bauer EB, Burdge KB, Roestel Jv, Bellm EC, Fuller J, Hermes J, Marsh TR et al (2020) A new class of Roche lobe-filling hot subdwarf binaries. ApJ 898(1):L25. https://doi.org/10.3847/2041-8213/aba3c2. arXiv:2007.05349 [astro-ph.SR]

Kupfer T, Bauer EB, Marsh TR, van Roestel J, Bellm EC, Burge KB, Coughlin MW, Fuller J et al (2020) The first ultracompact Roche lobe-filling hot subdwarf binary. ApJ 891(1):45. https://doi.org/10.3847/1538-4357/ab72ff. arXiv:2002.01485 [astro-ph.SR]

Kupfer T, Prince TA, van Roestel J, Bellm EC, Bildsten L, Coughlin MW, Drake AJ, Graham MJ, Klein C, Kulkarni SR et al (2021) Year 1 of the ZTF high-cadence Galactic plane survey: strategy, goals, and early results on new single-mode hot subdwarf B-star pulsators. MNRAS 505(1):1254–1267. https://doi.org/10.1093/mnras/stab1344. arXiv:2105.02758 [astro-ph.SR]

Kupi G, Amaro-Seoane P, Spurzem R (2006) Dynamics of compact object clusters: a post-Newtonian study. MNRAS 371(1):L45–L49. https://doi.org/10.1111/j.1745-3933.2006.00205.x. arXiv:astro-ph/0602125 [astro-ph]

Kuroda T, Arcones A, Takiwaki T, Kotake K (2020) Magnetorotational explosion of a massive star supported by neutrino heating in general relativistic three-dimensional simulations. ApJ 896(2):102. https://doi.org/10.3847/1538-4357/ab9308. arXiv:2003.02004 [astro-ph.HE]

Kuruwita RL, Staff J, De Marco O (2016) Considerations on the role of fall-back discs in the final stages of the common envelope binary interaction. MNRAS 461(1):486–496. https://doi.org/10.1093/mnras/stw1414. arXiv:1606.04635 [astro-ph.SR]

Kushnir D, Katz B, Dong S, Livne E, Fernández R (2013) Head-on collisions of white dwarfs in triple systems could explain type Ia supernovae. ApJ 778(2):L37. https://doi.org/10.1088/2041-8205/778/2/L37. arXiv:1303.1180 [astro-ph.HE]

Kuulkers E, den Hartog PR, in't Zand JJM, Verbunt FWM, Harris WE, Cocchi M (2003) Photospheric radius expansion X-ray bursts as standard candles. A&A 399:663–680. https://doi.org/10.1051/0004-6361:20021781. arXiv:astro-ph/0212028 [astro-ph]

Kyutoku K, Seto N (2016) Concise estimate of the expected number of detections for stellar-mass binary black holes by eLISA. MNRAS 462(2):2177–2183. https://doi.org/10.1093/mnras/stw1767. arXiv:1606.02298 [astro-ph.HE]

Kyutoku K, Nishino Y, Seto N (2019) How to detect the shortest period binary pulsars in the era of LISA. MNRAS 483(2):2615–2620. https://doi.org/10.1093/mnras/sty3322. arXiv:1812.02177 [astro-ph.HE]

Lacey C, Cole S (1993) Merger rates in hierarchical models of galaxy formation. MNRAS 262(3):627–649. https://doi.org/10.1093/mnras/262.3.627

Lacy M, Ridgway SE, Sajina A, Petric AO, Gates EL, Urrutia T, Storrie-Lombardi LJ (2015) The Spitzer mid-infrared AGN survey. II. The demographics and cosmic evolution of the AGN population. ApJ 802(2):102. https://doi.org/10.1088/0004-637X/802/2/102. arXiv:1501.04118 [astro-ph.GA]

Lai D, Shapiro SL (1995) Hydrodynamics of coalescing binary neutron stars: ellipsoidal treatment. ApJ 443:705. https://doi.org/10.1086/175562. arXiv:astro-ph/9408054 [astro-ph]

Lai D, Rasio FA, Shapiro SL (1994) Hydrodynamics of rotating stars and close binary interactions: compressible ellipsoid models. ApJ 437:742. https://doi.org/10.1086/175036. arXiv:astro-ph/9404031 [astro-ph]
Lai D, Chernoff DF, Cordes JM (2001) Pulsar jets: implications for neutron star kicks and initial spins. ApJ 549(2):1111–1118. https://doi.org/10.1086/319455. arXiv:astro-ph/0007272 [astro-ph]

Lamberts A, Garrison-Kimmel S, Clausen DR, Hopkins PF (2016) When and where did GW150914 form? MNRAS 463(1):L31–L35. https://doi.org/10.1093/mnrassl/slw152. arXiv:1605.08783 [astro-ph.HE]

Lamberts A, Garrison-Kimmel S, Hopkins PF, Quataert E, Bullock JS, Faucher-Giguère CA, Wetzel A, Kereš D, Drango K, Sanderson RE (2018) Predicting the binary black hole population of the Milky Way with cosmological simulations. MNRAS 480(2):2704–2718. https://doi.org/10.1093/mnras/sty2035. arXiv:1801.03099 [astro-ph.GA]

Lamberts A, Blunt S, Littenberg TB, Garrison-Kimmel S, Kupfer T, Sanderson RE (2019) Predicting the LISA white dwarf binary population in the Milky Way with cosmological simulations. MNRAS 490 (4):5888–5903. https://doi.org/10.1093/mnras/stz2834. arXiv:1907.00014 [astro-ph.HE]

Lasky PD, Mingarelli CMF, Smith TL et al (2016) Gravitational-wave cosmology across 29 decades in frequency. Phys Rev X 6(1):011035. https://doi.org/10.1103/PhysRevX.6.011035. arXiv:1511.05994

Lattimer JM, Prakash M (2016) The equation of state of hot, dense matter and neutron stars. Phys Rep 621:127–164. https://doi.org/10.1016/j.physrep.2015.12.005. arXiv:1512.07820 [astro-ph.SR]

Lau MYM, Mandel I, Vigna-Gómez A, Neijssel CJ, Stevenson S, Sesana A (2020) Detecting double neutron stars with LISA. MNRAS 492(3):3061–3072. https://doi.org/10.1093/mnras/staa002. arXiv: 1910.12422 [astro-ph.HE]

Law-Smith JAP, Everson RW, Ramirez-Ruiz E, de Mink SE, van Son LAC, Götzberg Y, Zellmann S, Vigna-Gómez A, Renzo M, Wu S et al (2020) Successful common envelope ejection and binary neutron star formation in 3D hydrodynamics. arXiv e-prints arXiv:2011.06630 [astro-ph.HE]

Lee HM (1995) Evolution of galactic nuclei with 10-Mblack holes. MNRAS 272(3):605–617. https://doi. org/10.1093/mnras/272.3.605. arXiv:astro-ph/9409073 [astro-ph]

Leigh NWC, Geller AM (2013) The dynamical significance of triple star systems in star clusters. MNRAS 432(3):2474–2479. https://doi.org/10.1093/mnras/stt617. arXiv:1304.2775 [astro-ph.SR]

Leigh NWC, Böker T, Maccarone TJ, Perets HB (2013) Gas depletion in primordial globular clusters due to accretion on to stellar-mass black holes. MNRAS 429(4):2997–3006. https://doi.org/10.1093/ mnras/sts554. arXiv:1212.1461 [astro-ph.SR]

Leigh NWC, Lützgendorf N, Geller AM, Maccarone TJ, Heinke C, Sesana A (2014) On the coexistence of stellar-mass and intermediate-mass black holes in globular clusters. MNRAS 444(1):29–42. https:// doi.org/10.1093/mnras/stu1437. arXiv:1407.4459 [astro-ph.SR]

Leitao L, Mégevand A, Sánchez AD (2012) Gravitational waves from the electroweak phase transition. J Cosmol Astropart Phys 10:024. https://doi.org/10.1088/1475-7516/2012/10/024. arXiv:1205.3070 [astro-ph.CO]

Lena D, Robinson A, Marconi A, Axon DJ, Capetti A, Merritt D, Batcheldor D (2014) Recoiling supermassive black holes: a search in the nearby universe. ApJ 795(2):146. https://doi.org/10.1088/ 0004-637X/795/2/146. arXiv:1409.3976 [astro-ph.GA]

Lenon AK, Nitz AH, Brown DA (2020) Measuring the eccentricity of GW170817 and GW190425. MNRAS 497(2):1966–1971. https://doi.org/10.1093/mnras/staa2120. arXiv:2005.14146 [astro-ph. HE]

Leung GYC, Leaman R, van de Ven G, Battaglia G (2020) A dwarf-dwarf merger and dark matter core as a solution to the globular cluster problems in the Fornax dSph. MNRAS 493(1):320–336. https://doi. org/10.1093/mnras/stz3017. arXiv:1911.09167 [astro-ph.GA]

Leveque A, Giersz M, Arca-Sedda M, Askar A (2022) MOCCA-survey data base: extra galactic globular clusters—II. Milky way and andromeda. MNRAS 514(4):5751–5766. https://doi.org/10.1093/mnras/ stac1694

Levin L, Bailes M, Barsdell BR, Bates SD, Bhat NDR, Burgay M, Burke-Spolaor S, Champion DJ, Coster P, D'Amico N et al (2013) The high time resolution universe pulsar survey—VIII. The galactic millisecond pulsar population. MNRAS 434(2):1387–1397. https://doi.org/10.1093/mnras/stt1103. arXiv:1306.4190 [astro-ph.SR]

Levin Y (2007) Starbursts near supermassive black holes: young stars in the Galactic Centre, and gravitational waves in LISA band. MNRAS 374(2):515–524. https://doi.org/10.1111/j.1365-2966. 2006.11155.x. arXiv:astro-ph/0603583 [astro-ph]

Levin Y, Beloborodov AM (2003) Stellar disk in the galactic center: a remnant of a dense accretion disk? ApJ 590(1):L33–L36. https://doi.org/10.1086/376675. arXiv:astro-ph/0303436 [astro-ph]

Levine R, Gnedin NY, Hamilton AJS (2010) Measuring gas accretion and angular momentum near simulated supermassive black holes. ApJ 716(2):1386–1396. https://doi.org/10.1088/0004-637X/716/ 2/1386. arXiv:1004.3785 [astro-ph.CO]
Levitan D, Kupfer T, Groot PJ, Margon B, Prince TA, Kulkarni SR, Hallinan G, Harding LK, Kyne G, Laher R et al (2014) PTF1 J191905.19+481506.2—a partially eclipsing AM CVn system discovered in the Palomar transient factory. ApJ 785(2):114. https://doi.org/10.1088/0004-637X/785/2/114. arXiv:1402.7129 [astro-ph.SR]

Lezhnin K, Vasiliev E (2016) Tidal disruption rates in non-spherical galactic nuclei formed by galaxy mergers. ApJ 831(1):84. https://doi.org/10.3847/0004-637X/831/1/84. arXiv:1609.00009 [astro-ph. GA]

Li K, Bogdanović T, Ballantyne DR (2020) Pairing of massive black holes in merger galaxies driven by dynamical friction. ApJ 896(2):113. https://doi.org/10.3847/1538-4357/ab93c6. arXiv:2006.08520 [astro-ph.GA]

Li K, Bogdanović T, Ballantyne DR (2020) The pairing probability of massive black holes in merger galaxies in the presence of radiative feedback. ApJ 905(2):123. https://doi.org/10.3847/1538-4357/ abc555. arXiv:2007.02051 [astro-ph.GA]

Li KJ, Wu K, Singh D (2019) Spin dynamics of a millisecond pulsar orbiting closely around a massive black hole. MNRAS 485(1):1053–1066. https://doi.org/10.1093/mnras/stz389. arXiv:1902.03146 [astro-ph.HE]

Li LX, Narayan R, McClintock JE (2009) Inferring the inclination of a black hole accretion disk from observations of its polarized continuum radiation. ApJ 691(1):847–865. https://doi.org/10.1088/0004- 637X/691/1/847. arXiv:0809.0866 [astro-ph]

Li S, Liu FK, Berczik P, Spurzem R (2017) Boosted tidal disruption by massive black hole binaries during galaxy mergers from the view of N-body simulation. ApJ 834(2):195. https://doi.org/10.3847/1538- 4357/834/2/195. arXiv:1509.00158 [astro-ph.GA]

Li TS, Simon JD, Kuehn K, Pace AB, Erkal D, Bechtol K, Yanny B, Drlica-Wagner A, Marshall JL, Lidman C et al (2018) The first tidally disrupted ultra-faint dwarf galaxy? A spectroscopic analysis of the Tucana III stream. ApJ 866(1):22. https://doi.org/10.3847/1538-4357/aadf91. arXiv:1804.07761 [astro-ph.GA]

Li Y, Ni Y, Croft RAC, Di Matteo T, Bird S, Feng Y (2021) AI-assisted superresolution cosmological simulations. Proc Natl Acad Sci 118(19):e2022038118. https://doi.org/10.1073/pnas.2022038118. arXiv:2010.06608 [astro-ph.CO]

Lidov ML (1962) The evolution of orbits of artificial satellites of planets under the action of gravitational perturbations of external bodies. Planet Space Sci 9(10):719–759. https://doi.org/10.1016/0032-0633 (62)90129-0

Lim H, Rodriguez CL (2020) Relativistic three-body effects in hierarchical triples. Phys Rev D 102 (6):064033. https://doi.org/10.1103/PhysRevD.102.064033. arXiv:2001.03654 [astro-ph.HE]

Lippai Z, Frei Z, Haiman Z (2008) Prompt shocks in the gas disk around a recoiling supermassive black hole binary. ApJ 676(1):L5. https://doi.org/10.1086/587034. arXiv:0801.0739 [astro-ph]

Liptai D, Price DJ (2019) General relativistic smoothed particle hydrodynamics. MNRAS 485(1):819–842. https://doi.org/10.1093/mnras/stz111. arXiv:1901.08064 [astro-ph.IM]

Lipunov VM, Postnov KA, Prokhorov ME (1996) The scenario machine: binary star population synthesis. Harwood Academic, Amsterdam

Lipunov VM, Postnov KA, Prokhorov ME, Bogomazov AI (2009) Description of the “scenario machine”. Astron Rep 53(10):915–940. https://doi.org/10.1134/S1063772909100047. arXiv:0704.1387 [astro-ph]

Littenberg TB, Cornish NJ (2019) Prospects for gravitational wave measurement of ZTF J1539+5027. ApJ 881(2):L43. https://doi.org/10.3847/2041-8213/ab385f. arXiv:1908.00678 [astro-ph.IM]

Littenberg TB, Larson SL, Nelemans G, Cornish NJ (2013) Prospects for observing ultracompact binaries with space-based gravitational wave interferometers and optical telescopes. MNRAS 429(3):2361– 2365. https://doi.org/10.1093/mnras/sts507. arXiv:1207.4848 [astro-ph.IM]

Littenberg TB, Cornish NJ, Lackeos K, Robson T (2020) Global analysis of the gravitational wave signal from Galactic binaries. Phys Rev D 101(12):123021. https://doi.org/10.1103/PhysRevD.101.123021. arXiv:2004.08464 [gr-qc]

Liu B, Lai D (2017) Spin-orbit misalignment of merging black hole binaries with tertiary companions. ApJ 846(1):L11. https://doi.org/10.3847/2041-8213/aa8727. arXiv:1706.02309 [astro-ph.HE]

Liu B, Lai D (2018) Black hole and neutron star binary mergers in triple systems: merger fraction and spin-orbit misalignment. ApJ 863(1):68. https://doi.org/10.3847/1538-4357/aad09f. arXiv:1805.03202 [astro-ph.HE]
Liu C, Shao L, Zhao J, Gao Y (2020) Multiband observation of LIGO/Virgo binary black hole mergers in the gravitational-wave transient catalog GWTC-1. MNRAS 496(1):182–196. https://doi.org/10.1093/mnras/staa1512. arXiv:2004.12096 [astro-ph.HE]

Liu J, Han Z, Zhang F, Zhang Y (2010) A comprehensive study of close double white dwarfs as gravitational wave sources: evolutionary channels, birth rates, and physical properties. ApJ 719 (2):1546–1552. https://doi.org/10.1088/0004-637X/719/2/1546

Liu J, Zhang H, Howard AW, Bai Z, Lu Y, Soria R, Justham S, Li X, Zheng Z (2019) A wide star-black-hole binary system from radial-velocity measurements. Nature 575(7784):618–621. https://doi.org/10.1038/s41586-019-1766-2. arXiv:1911.11989 [astro-ph.SR]

Liu T, Gezari S, Ayers M, Burgett W, Chambers K, Hodapp K, Huber ME, Kudritzki RP, Metcalfe N, Tonry J et al (2019) Supermassive black hole binary candidates from the pan-STARRS1 medium deep survey. ApJ 884(1):36. https://doi.org/10.3847/1538-4357/ab40cb. arXiv:1906.08315 [astro-ph. HE]

Liu X, Shen Y, Bian F, Loeb A, Tremaine S (2014) Constraining sub-parsec binary supermassive black holes in quasars with multi-epoch spectroscopy. II. The population with kinematically offset broad Balmer emission lines. ApJ 789(2):140. https://doi.org/10.1088/0004-637X/789/2/140. arXiv:1312.6694 [astro-ph.CO]

Liu YT, Shapiro SL, Stephens BC (2007) Magnetorotational collapse of very massive stars in full general relativity. Phys Rev D 76:084017. https://doi.org/10.1103/PhysRevD.76.084017. arXiv:0706.2360 [astro-ph]

Livio M, Soker N (1984) Star-planet systems as possible progenitors of cataclysmic binaries. MNRAS 208:763–781. https://doi.org/10.1093/mnras/208.4.763

Lodato G, Gerosa D (2013) Black hole mergers: do gas discs lead to spin alignment? MNRAS 429:L30–L34. https://doi.org/10.1093/mnrasl/slsl018. arXiv:1211.0284 [astro-ph.CO]

Lodato G, Natarajan P (2006) Supermassive black hole formation during the assembly of pre-galactic discs. MNRAS 371(4):1813–1823. https://doi.org/10.1111/j.1365-2966.2006.10801.x. arXiv:astro-ph/0606159 [astro-ph]

Lodato G, Rossi EM (2011) Multiband light curves of tidal disruption events. MNRAS 410(1):359–367. https://doi.org/10.1111/j.1365-2966.2010.17448.x. arXiv:1008.4589 [astro-ph.CO]

Lodato G, Nayakshin S, King AR, Pringle JE (2009) Black hole mergers: can gas discs solve the ‘final parsec’ problem? MNRAS 398(3):1392–1402. https://doi.org/10.1111/j.1365-2966.2009.15179.x. arXiv:0906.0737 [astro-ph.CO]

Lops G, Izquierdo-Villalba D, Colpi M, Bonoli S, Sesana A, Mangiagli A (2022) Galaxy fields of LISA massive black hole mergers in a simulated universe. arXiv e-prints arXiv:2207.10683 [astro-ph.GA]

Lousto CO, Zlochower Y (2008) Further insight into gravitational recoil. Phys Rev D 77(4):044028. https://doi.org/10.1103/PhysRevD.77.044028. arXiv:0708.4048 [gr-qc]

Lousto CO, Zlochower Y (2011) Hangup kicks: still larger recoils by partial spin-orbit alignment of black-hole binaries. Phys Rev Lett 107(23):231102. https://doi.org/10.1103/PhysRevLett.107.231102. arXiv:1108.2009 [gr-qc]

Lousto CO, Zlochower Y (2013) Nonlinear gravitational recoil from the mergers of precessing black-hole binaries. Phys Rev D 87(8):084027. https://doi.org/10.1103/PhysRevD.87.084027. arXiv:1211.7099 [gr-qc]

Lousto CO, Campanelli M, Zlochower Y, Nakano H (2010) Remnant masses, spins and recoils from the merger of generic black hole binaries. Class Quantum Grav 27(11):114006. https://doi.org/10.1088/0264-9381/27/11/114006. arXiv:0904.3541 [gr-qc]

Lousto CO, Zlochower Y, Dotti M, Volonteri M (2012) Gravitational recoil from accretion-aligned black-hole binaries. Phys Rev D 85(8):084015. https://doi.org/10.1103/PhysRevD.85.084015. arXiv:1201.1923 [gr-qc]

Lovelace G, Scheel MA, Szilágyi B (2011) Simulating merging binary black holes with nearly extremal spins. Phys Rev D 83(2):024010. https://doi.org/10.1103/PhysRevD.83.024010. arXiv:1010.2777 [gr-qc]

Loveridge AJ, van der Sluys MV, Kalogera V (2011) Analytical expressions for the envelope binding energy of giants as a function of basic stellar parameters. ApJ 743(1):49. https://doi.org/10.1088/0004-637X/743/1/49. arXiv:1009.5400 [astro-ph.SR]

LSST Science Collaboration, Abell PA, Allison J, Anderson SF, Andrew JR, Angel JRP, Armus L, Arnett D, Asztalos SJ, Axelrod TS et al (2009) LSST science book, version 2.0. arXiv e-prints arXiv:0912.0201 [astro-ph.IM]
Lu W, Beniamini P, Bonnerot C (2020) On the formation of GW190814. MNRAS 500:1817–1832. https://doi.org/10.1093/mnras/staa3372. arXiv:2009.10082 [astro-ph.HE]

Lukes-Gerakopoulos G, Witzany V (2021) Nonlinear effects in EMRI dynamics and their imprints on gravitational waves. In: Bambi C, Katsanevas S, Kokkotas KD (eds) Handbook of gravitational wave astronomy. Springer, p 42. https://doi.org/10.1007/978-981-15-4702-7_42-1

Lukes-Gerakopoulos G, Apostolatos TA, Contopoulos G (2010) Observable signature of a background deviating from the Kerr metric. Phys Rev D 81(12):124005. https://doi.org/10.1103/PhysRevD.81.124005. arXiv:1003.3120 [gr-qc]

Lukes-Gerakopoulos G, Seyrich J, Kunst D (2014) Investigating spinning test particles: spin supplementary conditions and the Hamiltonian formalism. Phys Rev D 90(10):104019. https://doi.org/10.1103/PhysRevD.90.104019. arXiv:1409.4314 [gr-qc]

Luo J, Chen LS, Duan HZ, Gong YG, Hu S, Ji J, Liu Q, Mei J, Milyukov V, Sazhin M et al (2016) TianQin: a space-borne gravitational wave detector. Class Quantum Grav 33(3):035010. https://doi.org/10.1088/0264-9381/33/3/035010. arXiv:1512.02076 [astro-ph.IM]

Lupi A, Haardt F, Dotti M, Fiacconi D, Mayer L, Madau P (2016) Growing massive black holes through supercritical accretion of stellar-mass seeds. MNRAS 456:2993–3003. https://doi.org/10.1093/mnras/stv2877. arXiv:1512.02651

Luyten WJ (1949) An Atlas of identification charts of white dwarfs. ApJ 109:528. https://doi.org/10.1086/145156

Lyne AG, Burgay M, Kramer M, Possenti A, Manchester RN, Camilo F, McLaughlin MA, Lorimer DR, D'Amico N, Joshi BC et al (2004) A double-pulsar system: a rare laboratory for relativistic gravity and plasma physics. Science 303(5661):1153–1157. https://doi.org/10.1126/science.1094645. arXiv:astro-ph/0401086 [astro-ph]

Lynx Team (2018) The Lynx mission concept study interim report. arXiv e-prints arXiv:1809.09642 [astro-ph.IM]

Ma L, Hopkins PF, Ma X, Anglés-Alcázar D, Faucher-Giguère CA, Kelley LZ (2021) Seeds don't sink: even massive black hole “seeds” cannot migrate to galaxy centres efficiently. MNRAS 508(2):1973–1985. https://doi.org/10.1093/mnras/stab2713. arXiv:2101.02727 [astro-ph.GA]

Maccarone TJ, Kundu A, Zepf SE, Rhode KL (2007) A black hole in a globular cluster. Nature 445(7124):183–185. https://doi.org/10.1038/nature05434. arXiv:astro-ph/0701310 [astro-ph]

MacFadyen AI, Milosavljević M (2008) An eccentric circumbinary accretion disk and the detection of binary massive black holes. ApJ 672(1):83–93. https://doi.org/10.1086/523869. arXiv:astro-ph/0607467 [astro-ph]

Macfarlane SA, Toma R, Ramsay G, Groot PJ, Woudt PA, Drew JE, Barentsen G, Eislöffel J (2015) The OmegaWhite survey for short-period variable stars—I. Overview and first results. MNRAS 454(1):507–530. https://doi.org/10.1093/mnras/stv1989. arXiv:1508.06277 [astro-ph.SR]

Mack KJ, Ostriker JP, Ricotti M (2007) Growth of structure seeded by primordial black holes. Astrophys J 665:1277–1287. https://doi.org/10.1086/518998. arXiv:astro-ph/0608642

Mackey AD, Wilkinson MI, Davies MB, Gilmore GF (2007) The effect of stellar-mass black holes on the structural evolution of massive star clusters. MNRAS 379(1):L40–L44. https://doi.org/10.1111/j.1745-3933.2007.00330.x. arXiv:0704.2494 [astro-ph]

Mackey AD, Wilkinson MI, Davies MB, Gilmore GF (2008) Black holes and core expansion in massive star clusters. MNRAS 386(1):65–95. https://doi.org/10.1111/j.1365-2966.2008.13052.x. arXiv:0802.0513 [astro-ph]

MacLeod CL, Hogan CJ (2008) Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information. Phys Rev D 77:043512. https://doi.org/10.1103/PhysRevD.77.043512. arXiv:0712.0618 [astro-ph]

MacLeod M, Lin DNC (2020) The effect of star-disk interactions on highly eccentric stellar orbits in active galactic nuclei: a disk loss cone and implications for stellar tidal disruption events. ApJ 889(2):94. https://doi.org/10.3847/1538-4357/ab64db. arXiv:1909.09645 [astro-ph.SR]

MacLeod M, Ramirez-Ruiz E (2015) On the accretion-fed growth of neutron stars during common envelope. ApJ 798(1):L19. https://doi.org/10.1088/2041-8205/798/1/L19. arXiv:1410.5421 [astro-ph.SR]

MacLeod M, Guillochon J, Ramirez-Ruiz E, Kasen D, Rosswog S (2016) Optical thermonuclear transients from tidal compression of white dwarfs as tracers of the low end of the massive black hole mass function. ApJ 819(1):3. https://doi.org/10.3847/0004-637X/819/1/3. arXiv:1508.02399 [astro-ph.HE]

MacLeod M, Trenti M, Ramirez-Ruiz E (2016) The close stellar companions to intermediate-mass black holes. ApJ 819(1):70. https://doi.org/10.3847/0004-637X/819/1/70. arXiv:1508.07000 [astro-ph.HE]
MacLeod M, Antoni A, Murguia-Berthier A, Macias P, Ramirez-Ruiz E (2017) Common envelope wind tunnel: coefficients of drag and accretion in a simplified context for studying flows around objects embedded within stellar envelopes. ApJ 838(1):56. https://doi.org/10.3847/1538-4357/aa6117. arXiv: 1704.02372 [astro-ph.SR]

Madau P, Dickinson M (2014) Cosmic star-formation history. ARA&A 52:415-486. https://doi.org/10.1146/annurev-astro-081811-125615. arXiv:1403.0007 [astro-ph.CO]

Madau P, Fragos T (2017) Radiation backgrounds at cosmic dawn: X-rays from compact binaries. ApJ 840 (1):39. https://doi.org/10.3847/1538-4357/aa6af9. arXiv:1606.07887 [astro-ph.GA]

Madau P, Rees MJ (2001) Massive black holes as population III remnants. ApJ 551(1):L27-L30. https://doi.org/10.1086/319848. arXiv:astro-ph/0101223 [astro-ph]

Madej OK, Jonker PG, Groot PJ, van Haaften LM, Nelemans G, Maccarone TJ (2013) Time-resolved X-shooter spectra and RXTE light curves of the ultra-compact X-ray binary candidate 4U 0614+091. MNRAS 429(4):2986-2996. https://doi.org/10.1093/mnras/sts550. arXiv:1212.0862 [astro-ph.HE]

Madigan AM, Hopman C, Levin Y (2011) Secular stellar dynamics near a massive black hole. ApJ 738 (1):99. https://doi.org/10.1088/0004-637X/738/1/99. arXiv:1010.1535 [astro-ph.GA]

Maggiore M (2000) Stochastic backgrounds of gravitational waves. arXiv e-prints arXiv:gr-qc/0008027 [astro-ph]

Magorrian J, Tremaine S, Richstone D, Bender R, Bower G, Dressler A, Faber SM, Gebhardt K, Green R, Grillmair C et al (1998) The demography of massive dark objects in galaxy centers. AJ 115(6):2285-2305. https://doi.org/10.1086/300353. arXiv:astro-ph/9708072 [astro-ph]

Maguire K, Eracleous M, Jonker PG, MacLeod M, Rosswog S (2020) Tidal disruptions of white dwarfs: theoretical models and observational prospects. Space Sci Rev 216(3):39. https://doi.org/10.1007/s11214-020-00661-2. arXiv:2004.00146 [astro-ph.HE]

Maio U, Dotti M, Petkova M, Perego A, Volonteri M (2013) Effects of circumnuclear disk gas evolution on the spin of central black holes. ApJ 767(1):37. https://doi.org/10.1088/0004-637X/767/1/37. arXiv:1203.1877 [astro-ph.HE]

Makino J, Funato Y (2004) Evolution of massive black hole binaries. ApJ 602(1):93-102. https://doi.org/10.1086/380917. arXiv:astro-ph/0307327 [astro-ph]

Manchester RN, Hobbs GB, Teoh A, Hobbs M (2005) The Australia telescope national facility pulsar catalogue. AJ 129(4):1993-2006. https://doi.org/10.1086/428488. arXiv:astro-ph/0412641 [astro-ph]

Mandel I (2016) Estimates of black hole natal kick velocities from observations of low-mass X-ray binaries. MNRAS 456(1):578-581. https://doi.org/10.1093/mnras/stv2733. arXiv:1510.03871 [astro-ph.HE]

Mandel I, de Mink SE (2016) Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries. MNRAS 458(3):2634-2647. https://doi.org/10.1093/mnras/stw379. arXiv:1601.00007 [astro-ph.HE]

Mandel I, Müller B (2020) Simple recipes for compact remnant masses and natal kicks. MNRAS 499:3214-3221. https://doi.org/10.1093/mnras/staa3043. arXiv:2006.08360 [astro-ph.HE]

Mandel I, Brown DA, Gair JR, Müller MC (2008) Rates and characteristics of intermediate mass ratio Inspirals detectable by advanced LIGO. ApJ 681:1431-1447. https://doi.org/10.1086/588246. arXiv:0705.0285

Mandel I, Sesana A, Vecchio A (2018) The astrophysical science case for a decihertz gravitational-wave detector. Class Quantum Grav 35(5):054004. https://doi.org/10.1088/1361-6382/aaa7e0. arXiv:1710.11187 [astro-ph.HE]

Mandic V, Thrane E, Giampanis S, Regimbau T (2012) Parameter estimation in searches for the stochastic gravitational-wave background. Phys Rev Lett 109(17):171102. https://doi.org/10.1103/PhysRevLett.109.171102. arXiv:1209.3847 [astro-ph.CO]

Mangiagli A, Klein A, Sesana A, Barausse E, Colpi M (2019) Post-Newtonian phase accuracy requirements for stellar black hole binaries with LISA. Phys Rev D 99(6):064056. https://doi.org/10.1103/PhysRevD.99.064056. arXiv:1811.01805 [gr-qc]

Mangiagli A, Klein A, Bonetti M, Katz ML, Sesana A, Volonteri M, Colpi M, Marsat S, Babak S (2020) Observing the inspiral of coalescing massive black hole binaries with LISA in the era of multimessenger astrophysics. Phys Rev D 102(8):084056. https://doi.org/10.1103/PhysRevD.102.084056. arXiv:2006.12513 [astro-ph.HE]

Mangiagli A, Caprini C, Volonteri M, Marsat S, Vergani S, Tamanini N, Inchauspé H (2022) Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts. Phys Rev D 106:103017. https://doi.org/10.1103/PhysRevD.106.103017. arXiv:2207.10678 [astro-ph.HE]
Mannerkoski M, Johansson PH, Pihajoki P, Rantala A, Naab T (2019) Gravitational waves from the inspiral of supermassive black holes in galactic-scale simulations. ApJ 887(1):35. https://doi.org/10.3847/1538-4357/ab52f9. arXiv:1909.01373 [astro-ph.GA]

Mannerkoski M, Johansson PH, Rantala A, Naab T, Liao S (2021) Resolving the complex evolution of a supermassive black hole triplet in a cosmological simulation. ApJ 912(2):L20. https://doi.org/10.3847/2041-8213/abf9a5. arXiv:2103.16254 [astro-ph.GA]

Manser CJ, Gänsicke BT, Marsh TR, Veras D, Koester D, Breedt E, Pala AF, Parsons SG, Southworth J (2016) Doppler imaging of the planetary debris disc at the white dwarf SDSS J122859.93+104032.9. MNRAS 455(4):4467-4478. https://doi.org/10.1093/mnras/stv2603. arXiv:1511.02230 [astro-ph.SR]

Manser CJ, Gänsicke BT, Eggl S, Hollands M, Izquierdo P, Koester D, Landstreet JD, Lyra W, Marsh TR, Meru F et al (2019) A planetesimal orbiting within the debris disc around a white dwarf star. Science 364(6435):66-69. https://doi.org/10.1126/science.aat5330. arXiv:1904.02163 [astro-ph.EP]

Mapelli M (2016) Massive black hole binaries from runaway collisions: the impact of metallicity. MNRAS 459(4):3432-3446. https://doi.org/10.1093/mnras/stw869. arXiv:1604.03559 [astro-ph.GA]

Mapelli M, Giacobbo N (2018) The cosmic merger rate of neutron stars and black holes. MNRAS 479 (4):4391-4398. https://doi.org/10.1093/mnras/sty1613. arXiv:1806.04866 [astro-ph.HE]

Mapelli M, Ripamonti E, Vecchio A, Graham AW, Gualandris A (2012) A cosmological view of extreme mass-ratio inspirals in nuclear star clusters. A&A 542:A102. https://doi.org/10.1051/0004-6361/201118444. arXiv:1205.2702 [astro-ph.CO]

Mapelli M, Giacobbo N, Ripamonti E, Spera M (2017) The cosmic merger rate of stellar black hole binaries from the Illustrus simulation. MNRAS 472(2):2422-2435. https://doi.org/10.1093/mnras/stx2123. arXiv:1708.05722 [astro-ph.GA]

Mapelli M, Santoliquido F, Bouffanais Y, Arca Sedda M, Giacobbo N, Artale MC, Ballone A (2021) Mass and rate of hierarchical black hole mergers in young, globular and nuclear star clusters. Symmetry 13:1678. https://doi.org/10.3390/sym13091678. arXiv:2007.15022 [astro-ph.HE]

Marassi S, Schneider R, Corvino G, Ferrari V, Portegies Zwart S (2011) Imprint of the merger and ring-down on the gravitational wave background from black hole binaries coalescence. Phys Rev D 84 (12):124037. https://doi.org/10.1103/PhysRevD.84.124037. arXiv:1111.6125 [astro-ph.CO]

Marassi S, Graziani L, Ginolfi M, Schneider R, Mapelli M, Spera M, Alparone M (2019) Evolution of dwarf galaxies hosting GW150914-like events. MNRAS 484(3):3219-3232. https://doi.org/10.1093/mnras/stz170. arXiv:1901.04494 [astro-ph.GA]

Marchant P, Langer N, Podsiadlowski P, Tauris TM, Moriya TJ (2016) A new route towards merging massive black holes. A&A 588:A50. https://doi.org/10.1051/0004-6361/201628133. arXiv:1601.03718 [astro-ph.SR]

Marconi A, Risaliti G, Gilli R, Hunt LK, Maiolino R, Salvati M (2004) Local supermassive black holes, relics of active galactic nuclei and the X-ray background. MNRAS 351(1):169-185. https://doi.org/10.1111/j.1365-2966.2004.07765.x. arXiv:astro-ph/0311619 [astro-ph]

Mardling R, Aarseth S (1999) Dynamics and stability of three-body systems. In: Steves BA, Roy AE (eds) The dynamics of small bodies in the solar system, a major key to solar system studies. NATO Advanced Study Institute (ASI) Series C, vol 522, p 385

Marelli M, Mignani RP, De Luca A, Saz Parkinson PM, Salvetti D, Den Hartog PR, Wolff MT (2015) Radio-quiet and radio-loud pulsars: similar in gamma-rays but different in X-rays. ApJ 802(2):78. https://doi.org/10.1088/0004-637X/802/2/78. arXiv:1501.06215 [astro-ph.HE]

Margalit B, Metzger BD (2019) The multi-messenger matrix: the future of neutron star merger constraints on the nuclear equation of state. ApJ 880(1):L15. https://doi.org/10.3847/2041-8213/ab2ae2. arXiv:1904.11995 [astro-ph.HE]

Marinacci F, Sales LV, Vogelsberger M, Torrey P, Springel V (2019) Simulating the interstellar medium and stellar feedback on a moving mesh: implementation and isolated galaxies. MNRAS 489(3):4233-4260. https://doi.org/10.1093/mnras/stz2391. arXiv:1905.08806 [astro-ph.GA]

Marronetti P, Tichy W, Brügmann B, González J, Sperhake U (2008) High-spin binary black hole mergers. Phys Rev D 77(6):064010. https://doi.org/10.1103/PhysRevD.77.064010. arXiv:0709.2160 [gr-qc]

Marsh TR, Steeghs D (2002) V407 Vul: a direct impact accretor. MNRAS 331(1):L7-L11. https://doi.org/10.1046/j.1365-8711.2002.05346.x. arXiv:astro-ph/0201309 [astro-ph]

Marsh TR, Dhillon VS, Duck SR (1995) Low-mass white dwarfs need friends—five new double-degenerate close binary stars. MNRAS 275:828. https://doi.org/10.1093/mnras/275.3.828

Marsh TR, Nelemans G, Steeghs D (2004) Mass transfer between double white dwarfs. MNRAS 350 (1):113-128. https://doi.org/10.1111/j.1365-2966.2004.07564.x. arXiv:astro-ph/0312577 [astro-ph]
Martinez MAS, Fragione G, Kremer K, Chatterjee S, Rodriguez CL, Samsing J, Ye CS, Weatherford NC, Zevin M, Naoz S et al (2020) Black hole mergers from hierarchical triples in dense star clusters. ApJ 903:67. https://doi.org/10.3847/1538-4357/abba25. arXiv:2009.08468 [astro-ph.GA]

Martinez-Valpuesta I, Aguerri J, González-García C (2016) Characterization of bars induced by interactions. Galaxies 4(2):7. https://doi.org/10.3390/galaxies4020007

Marulli F, Bonoli S, Branchini E, Moscardini L, Springel V (2008) Modelling the cosmological co-evolution of supermassive black holes and galaxies—I. BH scaling relations and the AGN luminosity function. MNRAS 385(4):1846–1858. https://doi.org/10.1111/j.1365-2966.2008.12988.x. arXiv:0711.2053 [astro-ph]

Masci FJ, Laher RR, Rusholme B, Shupe DL, Groom S, Surace J, Jackson E, Monkewitz S, Beck R, Flynn D et al (2019) The Zwicky transient facility: data processing, products, and archive. PASP 131 (995):018003. https://doi.org/10.1088/1538-3873/aae8ac. arXiv:1902.01872 [astro-ph.IM]

Mashian N, Loeb A (2017) Hunting black holes with Gaia. MNRAS 470(3):2611–2616. https://doi.org/10.1093/mnras/stx1410. arXiv:1704.03455 [astro-ph.HE]

Mastrobuono-Battisti A, Perets HB, Loeb A (2014) Effects of intermediate mass black holes on nuclear star clusters. ApJ 796(1):40. https://doi.org/10.1088/0004-637X/796/1/40. arXiv:1403.3094 [astro-ph.GA]

Mathis S (2019) Tidal dissipation in stars and giant planets: Jean-Paul Zahn’s pioneering work and legacy. In: EAS publications series. EAS Publications Series, vol 82, pp 5–33. https://doi.org/10.1051/eas/1982002

Matsubayashi T, Shinkai Ha, Ebisuzaki T (2004) Gravitational waves from merging intermediate-mass black holes. ApJ 614(2):864–868. https://doi.org/10.1086/423796

Matsubayashi T, Makino J, Ebisuzaki T (2007) Orbital evolution of an IMBH in the galactic nucleus with a massive central black hole. ApJ 656(2):879–896. https://doi.org/10.1086/510344. arXiv:astro-ph/0511782 [astro-ph]

Matsuoka Y, Iwasawa K, Onoue M, Kashikawa N, Strauss MA, Lee CH, Imanishi M, Nagao T, Akiyama M, Asami N et al (2019) Subaru high-z exploration of low-luminosity quasars (SHELLQs). X. Discovery of 35 quasars and luminous galaxies at 5.7 $\le$ z $\le$ 7.0. ApJ 883(2):183. https://doi.org/10.3847/1538-4357/ab3c60. arXiv:1908.07910 [astro-ph.GA]

Maureira-Fredes C, Goicovic FG, Amaro-Seoane P, Sesana A (2018) Accretion of clumpy cold gas on to massive black hole binaries: the challenging formation of extended circumbinary structures. MNRAS 478(2):1726–1748. https://doi.org/10.1093/mnras/sty1105. arXiv:1801.06179 [astro-ph.HE]

Maxted PFL, Marsh TR, Moran CKJ (2000) Radial velocity measurements of white dwarfs. MNRAS 319 (1):305–317. https://doi.org/10.1046/j.1365-8711.2000.03840.x. arXiv:astro-ph/0007129 [astro-ph]

Maxted PFL, Marsh TR, Moran CKJ, Han Z (2000) The triple degenerate star WD 1704+481. MNRAS 314(2):334–337. https://doi.org/10.1046/j.1365-8711.2000.03343.x. arXiv:astro-ph/0001212 [astro-ph]

Maxted PFL, Marsh TR, Moran CKJ (2002) The mass ratio distribution of short-period double degenerate stars. MNRAS 332(3):745–753. https://doi.org/10.1046/j.1365-8711.2002.05368.x. arXiv:astro-ph/0201411 [astro-ph]

Maxted PFL, Napiwotzki R, Dobbie PD, Burleigh MR (2006) Survival of a brown dwarf after engulfment by a red giant star. Nature 442(7102):543–545. https://doi.org/10.1038/nature04987. arXiv:astro-ph/0608054 [astro-ph]

Mayer L (2013) Massive black hole binaries in gas-rich galaxy mergers; multiple regimes of orbital decay and interplay with gas inflows. Class Quantum Grav 30(24):244008. https://doi.org/10.1088/0264-9381/30/24/244008. arXiv:1308.0431 [astro-ph.CO]

Mayer L (2017) Multiple regimes and coalescence timescales for massive black hole pairs; the critical role of galaxy formation physics. J Phys Conf Ser 840:012025. https://doi.org/10.1088/1742-6596/840/1/012025. arXiv:1703.00661 [astro-ph.GA]

Mayer L, Wadsley J (2004) The formation and evolution of bars in low surface brightness galaxies with cold dark matter haloes. MNRAS 347(1):277–294. https://doi.org/10.1111/j.1365-2966.2004.07202.x. arXiv:astro-ph/0303239 [astro-ph]

Mayer L, Kazantzidis S, Madau P, Colpi M, Quinn T, Wadsley J (2007) Rapid formation of supermassive black hole binaries in galaxy mergers with gas. Science 316(5833):1874. https://doi.org/10.1126/science.1141858. arXiv:0706.1562 [astro-ph]

Mayer L, Kazantzidis S, Escala A, Callegari S (2010) Direct formation of supermassive black holes via multi-scale gas inflows in galaxy mergers. Nature 466(7310):1082–1084. https://doi.org/10.1038/nature09294. arXiv:0912.4262 [astro-ph.CO]
Mayer L, Fiacconi D, Bonoli S, Quinn T, Roškar R, Shen S, Wadsley J (2015) Direct formation of supermassive black holes in metal-enriched gas at the heart of high-redshift galaxy mergers. ApJ 810:51. https://doi.org/10.1088/0004-637X/810/1/51. arXiv:1411.5683

Mazeh T, Shaham J (1979) The orbital evolution of close triple systems: the binary eccentricity. A&A 77:145

McClintock JE, Remillard RA (2006) Black hole binaries. In: Compact stellar X-ray sources. Cambridge astrophysics series. Cambridge University Press, vol 39, pp 157–213. https://doi.org/10.1017/CBO9780511536281.005

McClintock JE, Narayan R, Davis SW, Gou L, Kulkarni A, Orosz JA, Penna RF, Remillard RA, Steiner JF (2011) Measuring the spins of accreting black holes. Class Quantum Grav 28(11):114009. https://doi.org/10.1088/0264-9381/28/11/114009. arXiv:1101.0811 [astro-ph.HE]

McConnell NJ, Ma CP (2013) Revisiting the scaling relations of black hole masses and host Galaxy properties. ApJ 764(2):184. https://doi.org/10.1088/0004-637X/764/2/184. arXiv:1211.2816 [astro-ph.CO]

McConnell NJ, Ma CP, Gebhardt K, Wright SA, Murphy JD, Lauer TR, Graham JR, Richstone DO (2011) Two ten-billion-solar-mass black holes at the centres of giant elliptical galaxies. Nature 480 (7376):215–218. https://doi.org/10.1038/nature10636. arXiv:1112.1078 [astro-ph.CO]

McGee S, Sesana A, Vecchio A (2020) Linking gravitational waves and X-ray phenomena with joint LISA and Athena observations. Nat Astron 4:26–31. https://doi.org/10.1038/s41550-019-0969-7. arXiv: 1811.00050 [astro-ph.HE]

McGee SL (2013) The strong environmental dependence of black hole scaling relations. MNRAS 436 (3):2708–2721. https://doi.org/10.1093/mnras/stt1769. arXiv:1302.6237 [astro-ph.CO]

McKernan B, Ford KES (2015) Detection of radial velocity shifts due to black hole binaries near merger. MNRAS 452:L1–L5. https://doi.org/10.1093/mnras/slv076. arXiv:1505.04120 [astro-ph.HE]

McKernan B, Ford KES, Lyra W, Perets HB (2012) Intermediate mass black holes in AGN discs—I. Production and growth. MNRAS 425(1):460–469. https://doi.org/10.1111/j.1365-2966.2012.21486.x. arXiv:1206.2309 [astro-ph.GA]

McKernan B, Ford KES, Kocsis B, Haiman Z (2013) Ripple effects and oscillations in the broad Fe Kα line as a probe of massive black hole mergers. MNRAS 432(2):1468–1482. https://doi.org/10.1093/mnras/stt567. arXiv:1303.7206 [astro-ph.HE]

McKernan B, Ford KES, Kocsis B, Lyra W, Winter LM (2014) Intermediate-mass black holes in AGN discs—II. Model predictions and observational constraints. MNRAS 441(1):900–909. https://doi.org/10.1093/mnras/stu553. arXiv:1403.6433 [astro-ph.GA]

McKernan B, Ford KES, Bartos I, Graham MJ, Lyra W, Marka S, Marka Z, Ross NP, Stern D, Yang Y (2019) Ram-pressure stripping of a kicked hill sphere: prompt electromagnetic emission from the merger of stellar mass black holes in an AGN accretion disk. ApJ 884(2):L50. https://doi.org/10.3847/2041-8213/ab4886. arXiv:1907.03746 [astro-ph.HE]

McKernan B, Ford KES, O'Shaughnessy R (2020) Black hole, neutron star, and white dwarf merger rates in AGN discs. MNRAS 498(3):4088–4094. https://doi.org/10.1093/mnras/staa2681. arXiv:2002.00046 [astro-ph.HE]

McKernan B, Ford KES, O'Shaughnessy R, Wysocki D (2020) Monte Carlo simulations of black hole mergers in AGN discs: low $\chi_{eff}$ mergers and predictions for LIGO. MNRAS 494(1):1203–1216. https://doi.org/10.1093/mnras/staa740. arXiv:1907.04356 [astro-ph.HE]

McKinney JC, Dai L, Avara MJ (2015) Efficiency of super-Eddington magnetically-arrested accretion. MNRAS 454(1):L6–L10. https://doi.org/10.1093/mnras/slv115. arXiv:1508.02433 [astro-ph.HE]

McMillan S, Hut P, Makino J (1991) Star cluster evolution with primordial binaries. II. Detailed analysis. ApJ 372:111. https://doi.org/10.1086/169958

McNeill LO, Mardling RA, Müller B (2020) Gravitational waves from dynamical tides in white-dwarf binaries. MNRAS 491(2):3000–3012. https://doi.org/10.1093/mnras/stz3215. arXiv:1901.09045 [astro-ph.HE]

Mei J, Bai YZ, Bao J, Barausse E, Cai L, Canuto E, Cao B, Chen WM et al (2020) The TianQin project: current progress on science and technology. PTEP 2021:05A107. https://doi.org/10.1093/ptep/ptaa114. arXiv:2008.10332 [gr-qc]

Meiron Y, Kocsis B, Loeb A (2017) Detecting triple systems with gravitational wave observations. ApJ 834(2):200. https://doi.org/10.3847/1538-4357/834/2/200. arXiv:1604.02148 [astro-ph.HE]

Melvin T, Masters K, Lintott C, Nichol RC, Simmons B, Bamford SP, Casteels KRV, Cheung E, Edmondson EM, Fortson L et al (2014) Galaxy Zoo: an independent look at the evolution of the bar
fraction over the last eight billion years from HST-COSMOS. MNRAS 438(4):2882-2897. https://doi.org/10.1093/mnras/stt2397. arXiv:1401.3334 [astro-ph.GA]

Memmesheimer RM, Gopakumar A, Schäfer G (2004) Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits. Phys Rev D 70(10):104011. https://doi.org/10.1103/PhysRevD.70.104011 (gr-qc/0407049)

Menci N, Gatti M, Fiore F, Lamastra A (2014) Triggering active galactic nuclei in hierarchical galaxy formation: disk instability vs. interactions. A&A 569:A37. https://doi.org/10.1051/0004-6361/201424217. arXiv:1406.7740 [astro-ph.GA]

Menou K, Haiman Z, Kocsis B (2008) Cosmological physics with black holes (and possibly white dwarfs). New A Rev 51(10-12):884-890. https://doi.org/10.1016/j.newar.2008.03.020. arXiv:0803.3627 [astro-ph]

Merloni A, Heinz S (2008) A synthesis model for AGN evolution: supermassive black holes growth and feedback modes. MNRAS 388(3):1011-1030. https://doi.org/10.1111/j.1365-2966.2008.13472.x. arXiv:0805.2499 [astro-ph]

Merritt D (2001) Brownian motion of a massive binary. ApJ 556(1):245-264. https://doi.org/10.1086/321550. arXiv:astro-ph/0012264 [astro-ph]

Merritt D (2004) Evolution of the dark matter distribution at the galactic center. Phys Rev Lett 92 (20):201304. https://doi.org/10.1103/PhysRevLett.92.201304. arXiv:astro-ph/0311594 [astro-ph]

Merritt D (2013) Dynamics and evolution of galactic nuclei. Princeton University Press, Princeton

Merritt D (2015) Gravitational encounters and the evolution of galactic nuclei. I. Method. ApJ 804(1):52. https://doi.org/10.1088/0004-637X/804/1/52. arXiv:1505.07516 [astro-ph.GA]

Merritt D, Milosavljević M (2005) Massive black hole binary evolution. Living Rev Relativ 8:8. https://doi.org/10.12942/lrr-2005-8. arXiv:astro-ph/0410364 [astro-ph]

Merritt D, Poon MY (2004) Chaotic loss cones and black hole fueling. ApJ 606(2):788-798. https://doi.org/10.1086/382497. arXiv:astro-ph/0302296 [astro-ph]

Merritt D, Vasiliev E (2011) Orbits around black holes in triaxial nuclei. ApJ 726(2):61. https://doi.org/10.1088/0004-637X/726/2/61. arXiv:1005.0040 [astro-ph.GA]

Merritt D, Milosavljević M, Verde L, Jimenez R (2002) Dark matter spikes and annihilation radiation from the galactic center. Phys Rev Lett 88(19):191301. https://doi.org/10.1103/PhysRevLett.88.191301. arXiv:astro-ph/0201376 [astro-ph]

Merritt D, Milosavljević M, Favata M, Hughes SA, Holz DE (2004) Consequences of gravitational radiation recoil. ApJ 607(1):L9-L12. https://doi.org/10.1086/421551. arXiv:astro-ph/0402057 [astro-ph]

Merritt D, Alexander T, Mikkola S, Will CM (2011) Stellar dynamics of extreme-mass-ratio inspirals. Phys Rev D 84(4):044024. https://doi.org/10.1103/PhysRevD.84.044024. arXiv:1102.3180 [astro-ph.CO]

Metzger BD (2012) Nuclear-dominated accretion and subluminous supernovae from the merger of a white dwarf with a neutron star or black hole. MNRAS 419(1):827-840. https://doi.org/10.1111/j.1365-2966.2011.19747.x. arXiv:1105.6096 [astro-ph.HE]

Metzger BD (2019) Kilonovae. Living Rev Relativ 23:1. https://doi.org/10.1007/s41114-019-0024-0. arXiv:1910.01617 [astro-ph.HE]

Metzger BD, Stone NC (2016) A bright year for tidal disruptions. MNRAS 461(1):948-966. https://doi.org/10.1093/mnras/stw1394. arXiv:1506.03453 [astro-ph.HE]

Mezcua M (2017) Observational evidence for intermediate-mass black holes. Int J Mod Phys D 26 (11):1730021. https://doi.org/10.1142/S021827181730021X. arXiv:1705.09667 [astro-ph.GA]

Mezcua M, Domínguez Sánchez H (2020) Hidden AGNs in dwarf galaxies revealed by MaNGA: light echoes, off-nuclear wanderers, and a new broad-line AGN. ApJ 898(2):L30. https://doi.org/10.3847/2041-8213/aba199. arXiv:2007.08527 [astro-ph.GA]

Mezcua M, Civano F, Fabbiano G, Miyaji T, Marchesi S (2016) A population of intermediate-mass black holes in dwarf starburst galaxies up to redshift~2.4 in the Chandra COSMOS-Legacy Survey. MNRAS 478 (2):2576-2591. https://doi.org/10.1093/mnras/sty1163. arXiv:1802.01567 [astro-ph.GA]

Mezcua M, Civano F, Marchesi S, Suh H, Fabbiano G, Volonteri M (2018) Intermediate-mass black holes in dwarf galaxies out to redshift ~2.4 in the Chandra COSMOS-Legacy Survey. MNRAS 478 (2):2576-2591. https://doi.org/10.1093/mnras/sty1163. arXiv:1802.01567 [astro-ph.GA]

Michaely E, Perets HB (2014) Secular dynamics in hierarchical three-body systems with mass loss and mass transfer. ApJ 794(2):122. https://doi.org/10.1088/0004-637X/794/2/122. arXiv:1406.3035 [astro-ph.SR]

Mikkola S (1983) Encounters of binaries. I—equal energies. MNRAS 203:1107-1121. https://doi.org/10.1093/mnras/203.4.1107
Mikkola S (1984) Encounters of binaries. II—unequal energies. MNRAS 207:115–126. https://doi.org/10.1093/mnras/207.1.115

Mikkola S, Valtonen MJ (1990) The slingshot ejections in merging galaxies. ApJ 348:412. https://doi.org/10.1086/168250

Mikkola S, Valtonen MJ (1992) Evolution of binaries in the field of light particles and the problem of two black holes. MNRAS 259(1):115–120. https://doi.org/10.1093/mnras/259.1.115

Miller J, Wardell B, Pound A (2016) Second-order perturbation theory: the problem of infinite mode coupling. Phys Rev D 94(10):104018. https://doi.org/10.1103/PhysRevD.94.104018. arXiv:1608.06783 [gr-qc]

Miller JM (2007) Relativistic X-ray lines from the inner accretion disks around black holes. ARA&A 45 (1):441–479. https://doi.org/10.1146/annurev.astro.45.051806.110555. arXiv:0705.0540 [astro-ph]

Miller MC (2005) Probing general relativity with mergers of supermassive and intermediate-mass black holes. ApJ 618(1):426–431. https://doi.org/10.1086/425910. arXiv:astro-ph/0409331 [astro-ph]

Miller MC, Colbert EJM (2004) Intermediate-mass black holes. Int J Mod Phys D 13:1–64. https://doi.org/10.1142/S0218271804004426. arXiv:astro-ph/0308042

Miller MC, Davies MB (2012) An upper limit to the velocity dispersion of relaxed stellar systems without massive black holes. ApJ 755(1):81. https://doi.org/10.1088/0004-637X/755/1/81. arXiv:1206.6167 [astro-ph.GA]

Miller MC, Hamilton DP (2002) Four-body effects in globular cluster black hole coalescence. ApJ 576 (2):894–898. https://doi.org/10.1086/341788. arXiv:astro-ph/0202298 [astro-ph]

Miller MC, Hamilton DP (2002) Production of intermediate-mass black holes in globular clusters. MNRAS 330(1):232–240. https://doi.org/10.1046/j.1365-8711.2002.05112.x. arXiv:astro-ph/0106188 [astro-ph]

Miller MC, Krolik JH (2013) Alignment of supermassive black hole binary orbits and spins. ApJ 774 (1):43. https://doi.org/10.1088/0004-637X/774/1/43. arXiv:1307.6569 [astro-ph.HE]

Miller MC, Lauburg VM (2009) Mergers of stellar-mass black holes in nuclear star clusters. ApJ 692 (1):917–923. https://doi.org/10.1088/0004-637X/692/1/917. arXiv:0804.2783 [astro-ph]

Miller MC, Freitag M, Hamilton DP, Lauburg VM (2005) Binary encounters with supermassive black holes: zero-eccentricity LISA events. ApJ 631(2):L117–L120. https://doi.org/10.1086/497335. arXiv:astro-ph/0507133 [astro-ph]

Miller MC, Lamb FK, Dittmann AJ, Bogdanov S, Arzoumanian Z, Gendreau KC, Guillot S, Harding AK, Ho WCG, Lattimer JM et al (2019) PSR J0030+0451 mass and radius from NICER data and implications for the properties of neutron star matter. ApJ 887(1):L24. https://doi.org/10.3847/2041-8213/ab50c5. arXiv:1912.05705 [astro-ph.HE]

Miller-Jones JCA, Strader J, Heinke CO, Maccarone TJ, van den Berg M, Knigge C, Chomiu k L, Noyola E, Russell TD, Seth AC et al (2015) Deep radio imaging of 47 Tuc identifies the peculiar X-ray source X9 as a new black hole candidate. MNRAS 453(4):3918–3931. https://doi.org/10.1093/mnras/stv1869. arXiv:1509.02579 [astro-ph.HE]

Miller-Jones JCA, Bahramian A, Orosz JA, Mandel I, Gou L, Maccarone TJ, Neijssel CJ, Zhao X, Ziółkowski J, Reid MJ et al (2021) Cygnus X-1 contains a 21-solar mass black hole—implications for massive star winds. Science 371(6533):1046–1049. https://doi.org/10.1126/science.abb3363. arXiv:2102.09091 [astro-ph.HE]

Milosavljević M, Merritt D (2001) Formation of galactic nuclei. ApJ 563(1):34–62. https://doi.org/10.1086/323830. arXiv:astro-ph/0103350 [astro-ph]

Milosavljević M, Merritt D (2003) Long-term evolution of massive black hole binaries. ApJ 596(2):860–878. https://doi.org/10.1086/378086. arXiv:astro-ph/0212459 [astro-ph]

Milosavljević M, Phinney ES (2005) The afterglow of massive black hole coalescence. ApJ 622(2):L93–L96. https://doi.org/10.1086/429618. arXiv:astro-ph/0410343 [astro-ph]

Mingarelli CMF, Lazio TJW, Sesana A, Greene JE, Ellis JA, Ma CP, Croft S, Burke-Spolaor S, Taylor SR (2017) The local nanohertz gravitational-wave landscape from supermassive black hole binaries. Nat Astron 1:886–892. https://doi.org/10.1038/s41550-017-0299-6. arXiv:1708.03491 [astro-ph.GA]

Mirabel F (2017) The formation of stellar black holes. New A Rev 78:1–15. https://doi.org/10.1016/j.newar.2017.04.002

Miralda-Escudé J, Kollmeier JA (2005) Star captures by quasar accretion disks: a possible explanation of the M-σ relation. ApJ 619(1):30–40. https://doi.org/10.1086/426467. arXiv:astro-ph/0310717 [astro-ph]
Mirza MA, Tahir A, Khan FM, Holley-Bockelmann H, Baig AM, Berczik P, Chishtie F (2017) Galaxy rotation and supermassive black hole binary evolution. MNRAS 470(1):940–947. https://doi.org/10.1093/mnras/stx1248. arXiv:1704.03490 [astro-ph.GA]

Misra D, Fragos T, Tauris TM, Zapartas E, Aguilera-Dena DR (2020) The origin of pulsating ultra-luminous X-ray sources: low- and intermediate-mass X-ray binaries containing neutron star accretors. A&A 642:A174. https://doi.org/10.1051/0004-6361/202038070. arXiv:2004.01205 [astro-ph.HE]

Montuori C, Dotti M, Colpi M, Decarli R, Haardt F (2011) Search for sub-parsec massive binary black holes through line diagnosis. MNRAS 412(1):26–32. https://doi.org/10.1111/j.1365-2966.2010.17888.x. arXiv:1010.4303 [astro-ph.CO]

Montuori C, Dotti M, Haardt F, Colpi M, Decarli R (2012) Search for sub-parsec massive binary black holes through line diagnosis—II. MNRAS 425(3):1633–1639. https://doi.org/10.1111/j.1365-2966.2012.21530.x. arXiv:1207.0813 [astro-ph.CO]

Moody MSL, Shi JM, Stone JM (2019) Hydrodynamic torques in circumbinary accretion disks. ApJ 875 (1):66. https://doi.org/10.3847/1538-4357/ab09ee. arXiv:1903.00008 [astro-ph.HE]

Moore B (1994) Evidence against dissipation-less dark matter from observations of galaxy haloes. Nature 370(6491):629–631. https://doi.org/10.1038/370629a0

Moore CJ, Cole RH, Berry CPL (2015) Gravitational-wave sensitivity curves. Class Quantum Grav 32 (1):015014. https://doi.org/10.1088/0264-9381/32/1/015014. arXiv:1408.0740 [gr-qc]

Moore CJ, Mihaylov DP, Lasenby A, Gilmore G (2017) Astrometric search method for individually resolvable gravitational wave sources with Gaia. Phys Rev Lett 119(26):261102. https://doi.org/10.1103/PhysRevLett.119.261102. arXiv:1707.06239 [astro-ph.IM]

Moore CJ, Gerosa D, Klein A (2019) Are stellar-mass black-hole binaries too quiet for LISA? MNRAS 488(1):L94–L98. https://doi.org/10.1093/mnrasl/slz104. arXiv:1905.11998 [astro-ph.HE]

Moran EC, Shahinyan K, Sugarman HR, Vélez DO, Eracleous M (2014) Black holes at the centers of nearby dwarf galaxies. AJ 148(6):136. https://doi.org/10.1088/0004-6256/148/6/136. arXiv:1408.4451 [astro-ph.GA]

Morawski J, Giersz M, Askar A, Belczynski K (2018) MOCCA-SURVEY Database I: assessing GW kick retention fractions for BH-BH mergers in globular clusters. MNRAS 481(2):2168–2179. https://doi.org/10.1093/mnras/sty2401. arXiv:1802.01192 [astro-ph.GA]

Morris M (1993) Massive star formation near the galactic center and the fate of the stellar remnants. ApJ 408:496. https://doi.org/10.1086/172607

Morscher M, Umbreit S, Farr WM, Rasio FA (2013) Retention of Stellar-mass black holes in globular clusters. ApJ 763(1):L15. https://doi.org/10.1088/2041-8205/763/1/L15. arXiv:1211.3372 [astro-ph.GA]

Morscher M, Pattabiraman B, Rodriguez C, Rasio FA, Umbreit S (2015) The dynamical evolution of stellar black holes in globular clusters. ApJ 800(1):9. https://doi.org/10.1088/0004-637X/800/1/9. arXiv:1409.0866 [astro-ph.GA]

Mortlock DJ, Warren SJ, Venemans BP, Patel M, Hewett PC, McMahon RG, Simpson C, Theuns T, Gonzáles-Solares EA, Adamson A et al (2011) A luminous quasar at a redshift of z = 7.085. Nature 474(7353):616–619. https://doi.org/10.1038/nature10159. arXiv:1106.6088 [astro-ph.CO]

Mösta P et al (2010) Vacuum electromagnetic counterparts of binary black-hole mergers. Phys Rev D 81:064017. https://doi.org/10.1103/PhysRevD.81.064017

Mösta P et al (2012) On the detectability of dual jets from binary black holes. ApJ 749(2):L32. https://doi.org/10.1088/2041-8205/749/2/L32

Motl PM, Frank J, Tohline JE, D'Souza MCR (2007) The stability of double white dwarf binaries undergoing direct-impact accretion. ApJ 670(2):1314–1325. https://doi.org/10.1086/522076. arXiv:astro-ph/0702388 [astro-ph]

Moxon J, Flanagan É (2018) Radiation-reaction force on a small charged body to second order. Phys Rev D 97(10):105001. https://doi.org/10.1103/PhysRevD.97.105001. arXiv:1711.05212 [gr-qc]

Muñoz DJ, Miranda R, Lai D (2019) Hydrodynamics of circumbinary accretion: angular momentum transfer and binary orbital evolution. ApJ 871(1):84. https://doi.org/10.3847/1538-4357/aaf867. arXiv:1810.04676 [astro-ph.HE]

Muñoz DJ, Lai D, Kratter K, Mirand AR (2020) Circumbinary accretion from finite and infinite disks. ApJ 889(2):114. https://doi.org/10.3847/1538-4357/ab5d33. arXiv:1910.04763 [astro-ph.HE]

Müller B, Tauris TM, Heger A, Banerjee P, Qian YZ, Powell J, Chan C, Gay DW, Langer N (2019) Three-dimensional simulations of neutrino-driven core-collapse supernovae from low-mass single and binary star progenitors. MNRAS 484(3):3307–3324. https://doi.org/10.1093/mnras/stz216. arXiv:1811.05483 [astro-ph.SR]
Munna C (2020) Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit nonspinning extreme-mass-ratio inspirals to the 19th order. Phys Rev D 102(12):124001. https://doi.org/10.1103/PhysRevD.102.124001. arXiv:2008.10622 [gr-qc]

Muratov AL, Gnedin OY (2010) Modeling the metallicity distribution of globular clusters. ApJ 718 (2):1266–1288. https://doi.org/10.1088/0004-637X/718/2/1266. arXiv:1002.1325 [astro-ph.GA]

Murguia-Berthier A, Batta A, Janiuk A, Ramirez-Ruiz E, Mandel I, Noble SC, Everson RW (2020) On the maximum stellar rotation to form a black hole without an accompanying luminous transient. ApJ 901 (2):L24. https://doi.org/10.3847/2041-8213/abb818. arXiv:2005.10212 [astro-ph.HE]

Murphy EJ, Bolatto A, Chatterjee S, Casey CM, Chomiu k L, Dale D, de Pater I, Dickinson M, Francesco JD, Hallinan G et al (2018) The ngVLA science case and associated science requirements. In: Murphy E (ed) Science with a next generation very large array. Astronomical society of the pacific conference series, vol 517, p 3. arXiv:1810.07524 [astro-ph.IM]

Murray CD, Dermott SF (1999) Solar system dynamics. Cambridge University Press, Cambridge

Mushotzky R (2018) AXIS: a probe class next generation high angular resolution x-ray imaging satellite. In: Space telescopes and instrumentation 2018: ultraviolet to gamma ray. Society of photo-optical instrumentation engineers (SPIE) conference series, vol 10699, p 1069929. https://doi.org/10.1117/ 12.2310003. arXiv:1807.02122 [astro-ph.HE]

Mushotzky R, Aird J, Barger AJ, Cappelluti N, Chartas G, Corrales L, Eufrasio R, Fabian AC, Falcone AD, Gallo E et al (2019) The advanced X-ray imaging satellite. In: Bulletin of the American astronomical society, vol 51, p 107. arXiv:1903.04083 [astro-ph.HE]

Nakama T, Suyama T, Yokoyama J (2016) Supermassive black holes formed by direct collapse of inflationary perturbations. Phys Rev D 94(10):103522. https://doi.org/10.1103/PhysRevD.94.103522. arXiv:1609.02245 [gr-qc]

Nakama T, Carr B, Silk J (2018) Limits on primordial black holes from $\mu$ distortions in cosmic microwave background. Phys Rev D 97(4):043525. https://doi.org/10.1103/PhysRevD.97.043525. arXiv:1710. 06945 [astro-ph.CO]

Nandez JLA, Ivanova N (2016) Common envelope events with low-mass giants: understanding the energy budget. MNRAS 460(4):3992–4002. https://doi.org/10.1093/mnras/stw1266. arXiv:1606.04922 [as- tro-ph.SR]

Nandez JLA, Ivanova N, Lombardi JCJ (2015) Recombination energy in double white dwarf formation. MNRAS 450:L39–L43. https://doi.org/10.1093/mnrasl/slv043. arXiv:1503.02750 [astro-ph.SR]

Nandra K, George IM, Mushotzky RF, Turner TJ, Yaqoob T (1997) ASCA observations of Seyfert 1 galaxies. II. Relativistic iron $K\alpha$ emission. ApJ 477(2):602–622. https://doi.org/10.1086/303721. arXiv:astro-ph/9606169 [astro-ph]

Nandra K, Barret D, Barcons X, Fabian A, den Herder JW, Piro L, Watson M, Adami C, Aird J, Afonso JM,et al (2013) The hot and energetic universe: a white paper presenting the science theme motivating the Athena+ mission. arXiv e-prints arXiv:1306.2307 [astro-ph.HE]

Naoz S (2016) The eccentric Kozai–Lidov effect and its applications. ARA&A 54:441–489. https://doi. org/10.1146/annurev-astro-081915-023315. arXiv:1601.07175 [astro-ph.EP]

Naoz S, Will CM, Ramirez-Ruiz E, Hees A, Ghez AM, Do T (2020) A hidden friend for the galactic center black hole, Sgr A*. ApJ 888(1):L8. https://doi.org/10.3847/2041-8213/ab5e3b. arXiv:1912.04910 [astro-ph.GA]

Napiwotzki R, Karl CA, Lisker T, Catalán S, Drechsel H, Heber U, Homeier D, Koester D, Leibundgut B, Marsh TR et al (2020) The ESO supernovae type Ia progenitor survey (SPY). The radial velocities of 643 DA white dwarfs. A&A 638:A131. https://doi.org/10.1051/0004-6361/201629648. arXiv:1906. 10977 [astro-ph.SR]

Narayan R, Yi I (1994) Advection-dominated accretion: a self-similar solution. ApJ 428:L13. https://doi. org/10.1086/187381. arXiv:astro-ph/9403052 [astro-ph]

Narayan R, Paczynski B, Piran T (1992) Gamma-ray bursts as the death throes of massive binary stars. ApJ 395:L83. https://doi.org/10.1086/186493. arXiv:astro-ph/9204001 [astro-ph]

Natarajan P (2021) A new channel to form IMBHs throughout cosmic time. MNRAS 501(1):1413–1425. https://doi.org/10.1093/mnras/staa3724. arXiv:2009.09156 [astro-ph.GA]

Natarajan P, Pacucci F, Ferrara A, Agarwal B, Ricarte A, Zackrisson E, Cappelluti N (2017) Unveiling the first black holes with JWST: multi-wavelength spectral predictions. ApJ 838(2):117. https://doi.org/ 10.3847/1538-4357/aa6330. arXiv:1610.05312 [astro-ph.GA]

Nayakshin S, Cuadra J, Springel V (2007) Simulations of star formation in a gaseous disc around Sgr A*— a failed active galactic nucleus. MNRAS 379(1):21–33. https://doi.org/10.1111/j.1365-2966.2007. 11938.x. arXiv:astro-ph/0701141 [astro-ph]
Negri A, Volonteri M (2017) Black hole feeding and feedback: the physics inside the 'sub-grid'. MNRAS 467(3):3475-3492. https://doi.org/10.1093/mnras/stx362. arXiv:1610.04753 [astro-ph.GA]

Neijssel CJ, Vigna-Gómez A, Stevenson S, Barrett JW, Gaebel SM, Broekgaarden FS, de Mink SE, Szécsi D, Vinciguerra S, Mandel I (2019) The effect of the metallicity-specific star formation history on double compact object mergers. MNRAS 490(3):3740-3759. https://doi.org/10.1093/mnras/stz2840. arXiv:1906.08136 [astro-ph.SR]

Nelemans G, Tauris TM (1998) Formation of undermassive single white dwarfs and the influence of planets on late stellar evolution. A&A 335:L85-L88 arXiv:astro-ph/9806011 [astro-ph]

Nelemans G, Verbunt F, Yungelson LR, Portegies Zwart SF (2000) Reconstructing the evolution of double helium white dwarfs: envelope loss without spiral-in. A&A 360:1011-1018 arXiv:astro-ph/0006216 [astro-ph]

Nelemans G, Portegies Zwart SF, Verbunt F, Yungelson LR (2001) Population synthesis for double white dwarfs. II. Semi-detached systems: AM CVn stars. A&A 368:939-949. https://doi.org/10.1051/0004-6361:20010049. arXiv:astro-ph/0101123 [astro-ph]

Nelemans G, Yungelson LR, Portegies Zwart SF (2001) The gravitational wave signal from the Galactic disk population of binaries containing two compact objects. A&A 375:890-898. https://doi.org/10.1051/0004-6361:20010683. arXiv:astro-ph/0105221 [astro-ph]

Nelemans G, Yungelson LR, Portegies Zwart SF, Verbunt F (2001) Population synthesis for double white dwarfs. I. Close detached systems. A&A 365:491-507. https://doi.org/10.1051/0004-6361:20000147. arXiv:astro-ph/0010457 [astro-ph]

Nelemans G, Jonker PG, Marsh TR, van der Klis M (2004) Optical spectra of the carbon-oxygen accretion discs in the ultra-compact X-ray binaries 4U 0614+09, 4U 1543-624 and 2S 0918-549. MNRAS 348(1):L7-L11. https://doi.org/10.1111/j.1365-2966.2004.07486.x. arXiv:astro-ph/0312008 [astro-ph]

Nelemans G, Yungelson LR, Portegies Zwart SF (2004) Short-period AM CVn systems as optical, X-ray and gravitational-wave sources. MNRAS 349(1):181-192. https://doi.org/10.1111/j.1365-2966.2004.07479.x. arXiv:astro-ph/0312193 [astro-ph]

Nelemans G, Napiwotzki R, Karl C, Marsh TR, Voss B, Roelofs G, Izzard RG, Montgomery M, Reerink T, Christlieb N et al (2005) Binaries discovered by the SPYproject. IV. Five single-lined DA double white dwarfs. A&A 440(3):1087-1095. https://doi.org/10.1051/0004-6361:20053174. arXiv:astro-ph/0506231 [astro-ph]

Nelemans G, Jonker PG, Steeghs D (2006) Optical spectroscopy of (candidate) ultracompact X-ray binaries: constraints on the composition of the donor stars. MNRAS 370(1):255-262. https://doi.org/10.1111/j.1365-2966.2006.10496.x. arXiv:astro-ph/0604597 [astro-ph]

Nelemans G, Yungelson LR, van der Sluys MV, Tout CA (2010) The chemical composition of donors in AM CVn stars and ultracompact X-ray binaries: observational tests of their formation. MNRAS 401 (2):1347-1359. https://doi.org/10.1111/j.1365-2966.2009.15731.x. arXiv:0909.3376 [astro-ph.SR]

Nelson LA, Rappaport SA, Joss PC (1986) The evolution of ultrashort period binary systems. ApJ 304:231. https://doi.org/10.1086/164156

Neumayer N, Seth A, Böker T (2020) Nuclear star clusters. A&A Rev 28(1):4. https://doi.org/10.1007/s00159-020-00125-0. arXiv:2001.03626 [astro-ph.GA]

Nevin R, Blecha L, Comerford J, Greene J (2019) Accurate identification of galaxy mergers with imaging. ApJ 872(1):76. https://doi.org/10.3847/1538-4357/aafd34. arXiv:1901.01975 [astro-ph.GA]

Nguyen K, Bogdanović T (2016) Emission signatures from sub-parsec binary supermassive black holes. I. Diagnostic power of broad emission lines. ApJ 828(2):68. https://doi.org/10.3847/0004-637X/828/2/68. arXiv:1605.09389 [astro-ph.HE]

Nguyen K, Bogdanović T, Runnoe JC, Eracleous M, Sigurdsson S, Boroson T (2019) Emission signatures from sub-parsec binary supermassive black holes. II. Effect of accretion disk wind on broad emission lines. ApJ 870(1):16. https://doi.org/10.3847/1538-4357/aaeff0. arXiv:1807.09782 [astro-ph.HE]

Nguyen K, Bogdanović T, Runnoe JC, Eracleous M, Sigurdsson S, Boroson T (2020) Emission signatures from subparsec binary supermassive black holes. III. Comparison of models with observations. ApJ 894(2):105. https://doi.org/10.3847/1538-4357/ab88b5. arXiv:1908.01799 [astro-ph.HE]

Nishizawa A, Berti E, Klein A, Sesana A (2016) eLISA eccentricity measurements as tracers of binary black hole formation. Phys Rev D 94(6):064020. https://doi.org/10.1103/PhysRevD.94.064020. arXiv:1605.01341 [gr-qc]

Nishizawa A, Sesana A, Berti E, Klein A (2017) Constraining stellar binary black hole formation scenarios with eLISA eccentricity measurements. MNRAS 465(4):4375-4380. https://doi.org/10.1093/mnras/stw2993. arXiv:1606.09295 [astro-ph.HE]
Nissanke S, Vallisneri M, Nelemans G, Prince TA (2012) Gravitational-wave emission from compact galactic binaries. ApJ 758(2):131. https://doi.org/10.1088/0004-637X/758/2/131. arXiv:1201.4613 [astro-ph.GA]

Nitadori K, Aarseth SJ (2012) Accelerating NBODY6 with graphics processing units. MNRAS 424 (1):545–552. https://doi.org/10.1111/j.1365-2966.2012.21227.x. arXiv:1205.1222 [astro-ph.IM]

Noble SC, Mundim BC, Nakano H, Krolik JH, Campanelli M, Zlochower Y, Yunes N (2012) Circumbinary magnetohydrodynamic accretion into inspiraling binary black holes. ApJ 755(1):51. https://doi.org/10.1088/0004-637X/755/1/51. arXiv:1204.1073 [astro-ph.HE]

Nomoto K, Saio H, Kato M, Hachisu I (2007) Thermal stability of white dwarfs accreting hydrogen-rich matter and progenitors of type Ia supernovae. ApJ 663(2):1269–1276. https://doi.org/10.1086/518465. arXiv:astro-ph/0603351 [astro-ph]

Noutsos A, Kramer M, Carr P, Johnston S (2012) Pulsar spin-velocity alignment: further results and discussion. MNRAS 423(3):2736–2752. https://doi.org/10.1111/j.1365-2966.2012.21083.x. arXiv: 1205.2305 [astro-ph.GA]

Novikov ID, Thorne KS (1973) Astrophysics of black holes. In: Black holes (Les Astres Occlus), pp 343–450

Obergaulinger M, Aloy MÁ (2020) Magnetorotational core collapse of possible GRB progenitors—I. Explosion mechanisms. MNRAS 492(4):4613–4634. https://doi.org/10.1093/mnras/staa096. arXiv: 1909.01105 [astro-ph.HE]

Oesch P, Bouwens R, Brammer G, Chisholm J, Fudamoto Y, Illingworth GD, Kerutt J, Labbe I, Magee DK, Marchesini D et al (2021) FRESCO: the first reionization epoch spectroscopic complete survey. JWST proposal. Cycle 1, ID. #1895

Ogilvie GI (2013) Tides in rotating barotropic fluid bodies: the contribution of inertial waves and the role of internal structure. MNRAS 429(1):613–632. https://doi.org/10.1093/mnras/sts362. arXiv:1211. 0837 [astro-ph.EP]

Ogilvie GI (2014) Tidal dissipation in stars and giant planets. ARA&A 52:171–210. https://doi.org/10. 1146/annurev-astro-081913-035941. arXiv:1406.2207 [astro-ph.SR]

Ogiya G, Hahn O, Mingarelli CFM, Volonteri M (2020) Accelerated orbital decay of supermassive black hole binaries in merging nuclear star clusters. MNRAS 493(3):3676–3689. https://doi.org/10.1093/ mnras/staa444. arXiv:1911.11526 [astro-ph.GA]

SH Oh, Hunter DA, Brinks E, Elmegreen BG, Schruba A, Walter F, Rupen MP, Young LM, Simpson CE, Johnson MC et al (2015) High-resolution mass models of dwarf galaxies from LITTLE THINGS. AJ 149(6):180. https://doi.org/10.1088/0004-6256/149/6/180. arXiv:1502.01281 [astro-ph.GA]

Oh SP, Haiman Z (2003) Fossil H II regions: self-limiting star formation at high redshift. MNRAS 346 (2):456–472. https://doi.org/10.1046/j.1365-2966.2003.07103.x. arXiv:astro-ph/0307135 [astro-ph]

Ohlmann ST (2016) Hydrodynamics of the common envelope phase in binary stellar evolution. PhD thesis

Ohlmann ST, Röpke FK, Pakmor R, Springel V (2016) Hydrodynamic moving-mesh simulations of the common envelope phase in binary stellar systems. ApJ 816(1):L9. https://doi.org/10.3847/2041- 8205/816/1/L9. arXiv:1512.04529 [astro-ph.SR]

Ohlmann ST, Röpke FK, Pakmor R, Springel V, Müller E (2016) Magnetic field amplification during the common envelope phase. MNRAS 462(1):L121–L125. https://doi.org/10.1093/mnrasl/slw144. arXiv:1607.05996 [astro-ph.SR]

Oka T, Tsujimoto S, Iwata Y, Nomura M, Takekawa S (2017) Millimetre-wave emission from an intermediate-mass black hole candidate in the Milky Way. Nat Astron 1:709–712. https://doi.org/10. 1038/s41550-017-0224-z. arXiv:1707.07603 [astro-ph.GA]

O'Leary JA, Moster BP, Naab T, Somerville RS (2021) EMERGE: empirical predictions of galaxy merger rates since z ~ 6. MNRAS 501(3):3215–3237. https://doi.org/10.1093/mnras/staa3746. arXiv:2001. 02687

Omukai K, Si Inutsuka (2002) An upper limit on the mass of a primordial star due to the formation of an Hii region: the effect of ionizing radiation force. MNRAS 332(1):59–64. https://doi.org/10.1046/j. 1365-8711.2002.05276.x. arXiv:astro-ph/0112345 [astro-ph]

Omukai K, Palla F (2003) Formation of the first stars by accretion. ApJ 589(2):677–687. https://doi.org/10. 1086/374810. arXiv:astro-ph/0302345 [astro-ph]

Omukai K, Schneider R, Haiman Z (2008) Can supermassive black holes form in metal-enriched high- redshift protogalaxies? ApJ 686(2):801–814. https://doi.org/10.1086/591636. arXiv:0804.3141 [as- tro-ph]