[1076] Z.L. Wen, J.L. Han, Clusters of galaxies up to z=1.5 identified from photometric data of the Dark Energy Survey and unWISE, Mon. Not. R. Astron. Soc. 513 (3) (2022) 3946-3959, arXiv:2204.11215 [astro-ph.CO].

[1077] M. Maturi, F. Bellagamba, M. Radovich, M. Roncarelli, M. Sereno, L. Moscardini, S. Bardelli, E. Puddu, AMICO galaxy clusters in KiDS-DR3: sample properties and selection function, Mon. Not. R. Astron. Soc. 485 (2019) 498, arXiv:1810.02811 [astro-ph.CO].

[1078] M. Oguri, et al., An optically-selected cluster catalog at redshift 0.1< z < 1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data, Publ. Astron. Soc. Jap. 70 (2018) S20, arXiv:1701.00818 [astro-ph.CO].

[1079] Z.L. Wen, J.L. Han, A catalog of 1.58 million clusters of galaxies identified from the DESI legacy imaging surveys, Astrophys. J. Suppl. 272 (2) (2024) 39, arXiv:2404.02002 [astro-ph.CO].

[1080] M. Simet, T. McClintock, R. Mandelbaum, E. Rozo, E. Rykoff, E. Sheldon, R.H. Wechsler, Weak lensing measurement of the mass-richness relation of SDSS redMaPPer clusters, Mon. Not. R. Astron. Soc. 466 (3) (2017) 3103-3118, arXiv:1603.06953 [astro-ph.CO].

[1081] DES Collaboration, T. McClintock, et al., Dark energy survey year 1 results: weak lensing mass calibration of redMaPPer galaxy clusters, Mon. Not. R. Astron. Soc. 482 (1) (2019) 1352-1378, arXiv:1805.00039 [astro-ph.CO].

[1082] C. Ge, M. Sun, E. Rozo, N. Sehgal, A. Vikhlinin, W. Forman, C. Jones, D. Nagai, X-ray scaling relations from a complete sample of the richest maxBCG clusters, Mon. Not. R. Astron. Soc. 484 (2) (2019) 1946-1971, arXiv:1803.05007 [astro-ph.GA].

[1083] DES Collaboration, V. Wetzell, et al., Velocity dispersions of clusters in the Dark Energy Survey Y3 redMaPPer catalogue, Mon. Not. R. Astron. Soc. 514 (4) (2022) 4696-4717, arXiv:2107.07631 [astro-ph.CO].

[1084] S. Miyazaki, T. Hamana, R.S. Ellis, N. Kashikawa, R.J. Massey, J. Taylor, A. Refregier, A subaru weak lensing survey I: cluster candidates and spectroscopic verification, Astrophys. J. 669 (2007) 714, arXiv:0707.2249 [astro-ph].

[1085] S. Miyazaki, et al., A large sample of shear selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S16A wide field mass maps, Publ. Astron. Soc. Jap. 70 (2018) S27, arXiv:1802.10290 [astro-ph.CO].

[1086] K.-F. Chen, et al., Weak-lensing shear-selected galaxy clusters from the hyper suprime-cam subaru strategic program: I. Cluster catalog, selection function and mass-observable relation, 2024, arXiv:2406.11966 [astro-ph.CO].

[1087] G. Leroy, S. Pires, G.W. Pratt, C. Giocoli, Fast multi-scale galaxy cluster detection with weak lensing: Towards a mass-selected sample, Astron. Astrophys. 678 (2023) A125, arXiv:2304.01812 [astro-ph.CO].

[1088] M.E. Ramos-Ceja, et al., The eROSITA Final Equatorial-Depth Survey (eFEDS) - A complete census of X-ray properties of Subaru Hyper Suprime-Cam weak lensing shear-selected clusters in the eFEDS footprint, Astron. Astrophys. 661 (2022) A14, arXiv:2109.07836 [astro-ph.CO].

[1089] I.-N. Chiu, et al., Weak-lensing shear-selected galaxy clusters from the hyper suprime-cam subaru strategic program: II. Cosmological constraints from the cluster abundance, 2024, arXiv:2406.11970 [astro-ph.CO].

[1090] K.-F. Chen, M. Oguri, Y.-T. Lin, S. Miyazaki, Mass bias of weak lensing shear-selected galaxy cluster samples, Astrophys. J. 891 (2) (2020) 139, arXiv:1911.11480 [astro-ph.GA].

[1091] K. Umetsu, Cluster-galaxy weak lensing, Astron. Astrophys. Rev. 28 (1) (2020) 7, arXiv:2007.00506 [astro-ph.CO].

[1092] DES Collaboration, H.-Y. Wu, et al., Optical selection bias and projection effects in stacked galaxy cluster weak lensing, Mon. Not. R. Astron. Soc. 515 (3) (2022) 4471-4486, arXiv:2203.05416 [astro-ph.CO].

[1093] DES, eROSITA-DE Collaboration, S. Grandis, et al., The SRG/eROSITA All-Sky Survey - Dark Energy Survey year 3 weak gravitational lensing by eRASS1 selected galaxy clusters, Astron. Astrophys. 687 (2024) A178, arXiv:2402.08455 [astro-ph.CO].

[1094] H. Hoekstra, How well can we determine cluster mass profiles from weak lensing? Mon. Not. R. Astron. Soc. 339 (2003) 1155, arXiv:astro-ph/0208351.

[1095] D. Gruen, S. Seitz, M.R. Becker, O. Friedrich, A. Mana, Cosmic variance of the galaxy cluster weak lensing signal, Mon. Not. R. Astron. Soc. 449 (4) (2015) 4264-4276, arXiv:1501.01632 [astro-ph.CO].

[1096] D.E. Applegate, A. von der Linden, P.L. Kelly, M.T. Allen, S.W. Allen, P.R. Burchat, D.L. Burke, H. Ebeling, A. Mantz, R.G. Morris, Weighing the Giants - III. Methods and measurements of accurate galaxy cluster weak-lensing masses, Mon. Not. R. Astron. Soc. 439 (1) (2014) 48-72, arXiv:1208.0605 [astro-ph.CO].

[1097] SPT Collaboration, J.P. Dietrich, et al., Sunyaev-Zel'dovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters, Mon. Not. R. Astron. Soc. 483 (3) (2019) 2871-2906, arXiv:1711.05344 [astro-ph.CO].

[1098] S. Grandis, S. Bocquet, J.J. Mohr, M. Klein, K. Dolag, Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing, Mon. Not. R. Astron. Soc. 507 (4) (2021) 5671-5689, arXiv:2103.16212 [astro-ph.CO].

[1099] M.R. Becker, A.V. Kravtsov, On the accuracy of weak lensing cluster mass reconstructions, Astrophys. J. 740 (2011) 25, arXiv:1011.1681 [astro-ph.CO].

[1100] Y.M. Bahe, I.G. McCarthy, L.J. King, Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration, Mon. Not. R. Astron. Soc. 421 (2012) 1073-1088, arXiv:1106.2046 [astro-ph.CO].

[1101] Euclid Collaboration, C. Giocoli, et al., Euclid preparation - XXXII. Evaluating the weak-lensing cluster mass biases using the Three Hundred Project hydro-dynamical simulations, Astron. Astrophys. 681 (2024) A67, arXiv:2302.00687 [astro-ph.CO].

[1102] I.-N. Chiu, et al., The eROSITA Final Equatorial-Depth Survey (eFEDS) - X-ray observable-to-mass-and-redshift relations of galaxy clusters and groups with weak-lensing mass calibration from the Hyper Suprime-Cam Subaru Strategic Program survey, Astron. Astrophys. 661 (2022) A11, arXiv:2107.05652 [astro-ph.CO].

[1103] F. Kleinebreil, et al., The SRG/eROSITA All-Sky Survey - Weak lensing of eRASS1 galaxy clusters in KiDS-1000 and consistency checks with DES Y3 and HSC-Y3, Astron. Astrophys. 695 (2025) A216, arXiv:2402.08456 [astro-ph.CO].

[1104] F. Bellagamba, et al., AMICO galaxy clusters in KiDS-DR3: weak-lensing mass calibration, Mon. Not. R. Astron. Soc. 484 (2) (2019) 1598-1615, arXiv:1810.02827 [astro-ph.CO].

[1105] W. Cui, S. Borgani, K. Dolag, G. Murante, L. Tornatore, The effects of baryons on the halo mass function, Mon. Not. R. Astron. Soc. 423 (2012) 2279, arXiv:1111.3066 [astro-ph.CO].

[1106] S. Bocquet, A. Saro, K. Dolag, J.J. Mohr, Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology, Mon. Not. R. Astron. Soc. 456 (3) (2016) 2361-2373, arXiv:1502.07357 [astro-ph.CO].

[1107] T. Castro, S. Borgani, K. Dolag, V. Marra, M. Quartin, A. Saro, E. Sefusatti, On the impact of baryons on the halo mass function, bias, and cluster cosmology, Mon. Not. R. Astron. Soc. 500 (2) (2020) 2316-2335, arXiv:2009.01775 [astro-ph.CO].

[1108] DES, SPT Collaboration, M. Costanzi, et al., Cosmological constraints from DES Y1 cluster abundances and SPT multiwavelength data, Phys. Rev. D 103 (4) (2021) 043522, arXiv:2010.13800 [astro-ph.CO].

[1109] C.T. Mpetha, et al., Cosmology from UNIONS weak lensing profiles of galaxy clusters, 2025, arXiv:2501.09147 [astro-ph.CO].

[1110] SPT Collaboration, A.B. Mantz, et al., Cosmological constraints from gas mass fractions of massive, relaxed galaxy clusters, Mon. Not. R. Astron. Soc. 510 (1) (2021) 131-145, arXiv:2111.09343 [astro-ph.CO].

[1111] F. Schmidt, Cosmological simulations of normal-branch braneworld gravity, Phys. Rev. D 80 (2009) 123003, arXiv:0910.0235 [astro-ph.CO].

[1112] M. Kopp, S.A. Appleby, I. Achitouv, J. Weller, Spherical collapse and halo mass function in $f(R)$ theories, Phys. Rev. D 88 (8) (2013) 084015, arXiv:1306.3233 [astro-ph.CO].

[1113] S. Hagstotz, M. Costanzi, M. Baldi, J. Weller, Joint halo-mass function for modified gravity and massive neutrinos - I. Simulations and cosmological forecasts, Mon. Not. R. Astron. Soc. 486 (3) (2019) 3927-3941, arXiv:1806.07400 [astro-ph.CO].

[1114] S. Gupta, W.A. Hellwing, M. Bilicki, J.E. García-Farieta, Universality of the halo mass function in modified gravity cosmologies, Phys. Rev. D 105 (4) (2022) 043538, arXiv:2112.03699 [astro-ph.CO].

[1115] M. Sereno, A. Veropalumbo, F. Marulli, G. Covone, L. Moscardini, A. Cimatti, New constraints on $\sigma_8$ from a joint analysis of stacked gravitational lensing and clustering of galaxy clusters, Mon. Not. R. Astron. Soc. 449 (4) (2015) 4147-4161, arXiv:1410.5438 [astro-ph.CO].

[1116] F. Marulli, A. Veropalumbo, J.E. García-Farieta, M. Moresco, L. Moscardini, A. Cimatti, C3 cluster clustering cosmology I. New constraints on the cosmic growth rate at $z \sim 0.3$ from redshift-space clustering anisotropies, Astrophys. J. 920 (1) (2021) 13, arXiv:2010.11206 [astro-ph.CO].

[1117] G.F. Lesci, et al., AMICO galaxy clusters in KiDS-DR3: Constraints on cosmological parameters and on the normalisation of the mass-richness relation from clustering, Astron. Astrophys. 665 (2022) A100, arXiv:2203.07398 [astro-ph.CO].

[1118] M. Romanello, et al., AMICO galaxy clusters in KiDS-DR3: Cosmological constraints from the angular power spectrum and correlation function, Astron. Astrophys. 682 (2024) A72, arXiv:2310.12224 [astro-ph.CO].

[1119] M.C.A. Cerbolini, B. Sartoris, J.-Q. Xia, A. Biviano, S. Borgani, M. Viel, Constraining neutrino properties with a Euclid-like galaxy cluster survey, J. Cosmol. Astropart. Phys. 06 (2013) 020, arXiv:1303.4550 [astro-ph.CO].

[1120] B. Sartoris, et al., Next generation cosmology: constraints from the euclid galaxy cluster survey, Mon. Not. R. Astron. Soc. 459 (2) (2016) 1764-1780, arXiv:1505.02165 [astro-ph.CO].

[1121] L. Moscardini, S. Matarrese, H.J. Mo, Constraining cosmological parameters with the clustering properties of galaxy clusters in optical and x-ray bands, Mon. Not. R. Astron. Soc. 327 (2001) 422, arXiv:astro-ph/0009006.

[1122] R.K. Sheth, H.J. Mo, G. Tormen, Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes, Mon. Not. R. Astron. Soc. 323 (2001) 1, arXiv:astro-ph/9907024.

[1123] E. Branchini, S. Camera, A. Cuoco, N. Fornengo, M. Regis, M. Viel, J.-Q. Xia, Cross-correlating the $\gamma$-ray sky with catalogs of galaxy clusters, Astrophys. J. Suppl. 228 (1) (2017) 8, arXiv:1612.05788 [astro-ph.CO].

[1124] K. Paech, N. Hamaus, B. Hoyle, M. Costanzi, T. Giannantonio, S. Hagstotz, G. Sauerwein, J. Weller, Cross-correlation of galaxies and galaxy clusters in the Sloan Digital Sky Survey and the importance of non-Poissonian shot noise, Mon. Not. R. Astron. Soc. 470 (3) (2017) 2566-2577, arXiv:1612.02018 [astro-ph.CO].
[1125] J.L. Tinker, B.E. Robertson, A.V. Kravtsov, A. Klypin, M.S. Warren, G. Yepes, S. Gottlober, The large scale bias of dark matter halos: numerical calibration and model tests, Astrophys. J. 724 (2010) 878–886, arXiv:1001.3162 [astro-ph.CO].

[1126] N. Okabe, Y.-Y. Zhang, A. Finoguenov, M. Takada, G.P. Smith, K. Umetsu, T. Futamase, LoCuSS: calibrating mass-observables scaling relations for cluster cosmology with subaru weak lensing observations, Astrophys. J. 721 (2010) 875–885, arXiv:1007.3816 [astro-ph.CO].

[1127] S. Giodini, L. Lovisari, E. Pointecouteau, S. Ettori, T.H. Reiprich, H. Hoekstra, Scaling relations for galaxy clusters: properties and evolution, Space Sci. Rev. 177 (2013) 247–282, arXiv:1305.3286 [astro-ph.CO].

[1128] A. Veropalumbo, F. Marulli, L. Moscardini, M. Moresco, A. Cimatti, An improved measurement of baryon acoustic oscillations from the correlation function of galaxy clusters at z ~ 0.3, Mon. Not. R. Astron. Soc. 442 (4) (2014) 3275–3283, arXiv:1311.5895 [astro-ph.CO].

[1129] F. Marulli, A. Veropalumbo, L. Moscardini, A. Cimatti, K. Dolag, Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections, Astron. Astrophys. 599 (2017) A106, arXiv:1505.01170 [astro-ph.CO].

[1130] M. Moresco, A. Veropalumbo, F. Marulli, L. Moscardini, A. Cimatti, C3: cluster clustering cosmology. II. First detection of the baryon acoustic oscillations peak in the three-point correlation function of galaxy clusters, Astrophys. J. 919 (2) (2021) 144, arXiv:2011.04665 [astro-ph.CO].

[1131] C. Alcock, B. Paczynski, An evolution free test for non-zero cosmological constant, Nature 281 (1979) 358–359.

[1132] F. Marulli, D. Bianchi, E. Branchini, L. Guzzo, L. Moscardini, R.E. Angulo, Cosmology with clustering anisotropies: disentangling dynamic and geometric distortions in galaxy redshift surveys, Mon. Not. R. Astron. Soc. 426 (2012) 2566, arXiv:1203.1002 [astro-ph.CO].

[1133] BOSS Collaboration, F. Beutler, et al., The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles, Mon. Not. R. Astron. Soc. 443 (2) (2014) 1065–1089, arXiv:1312.4611 [astro-ph.CO].

[1134] F. Marulli, et al., The XXL Survey: XVI. The clustering of X-ray selected galaxy clusters at z~0.3, Astron. Astrophys. 620 (2018) A1, arXiv:1807.04760 [astro-ph.CO].

[1135] A. Veropalumbo, F. Marulli, L. Moscardini, M. Moresco, A. Cimatti, Measuring the distance–redshift relation with the baryon acoustic oscillations of galaxy clusters, Mon. Not. R. Astron. Soc. 458 (2) (2016) 1909–1920, arXiv:1510.08852 [astro-ph.CO].

[1136] G.F. Lesci, A. Veropalumbo, M. Sereno, F. Marulli, L. Moscardini, C. Giocoli, Mass bias and cosmological constraints from Planck cluster clustering, Astron. Astrophys. 674 (2023) A80, arXiv:2302.14074 [astro-ph.CO].

[1137] V. Lindholm, A. Finoguenov, J. Comparat, C.C. Kirkpatrick, E. Rykoff, N. Clerc, C. Collins, S. Damsted, J.I. Chitham, N. Padilla, Clustering of CODEX clusters, Astron. Astrophys. 646 (2021) A8, arXiv:2012.00090 [astro-ph.CO].

[1138] P.J.E. Peebles, Statistical analysis of catalogs of extragalactic objects. I. Theory, Astrophys. J. 185 (1973) 413–440.

[1139] eBOSS Collaboration, A. Tamone, et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample, Mon. Not. R. Astron. Soc. 499 (4) (2020) 5527–5546, arXiv:2007.0909 [astro-ph.CO].

[1140] Z. Li, Y.P. Jing, P. Zhang, D. Cheng, Measurement of redshift-space power spectrum for BOSS galaxies and the growth rate at redshift 0.57, Astrophys. J. 833 (2) (2016) 287, arXiv:1609.03697 [astro-ph.CO].

[1141] S. Alam, S. Ho, M. Vargas-Magaña, D.P. Schneider, Testing general relativity with growth rate measurement from Sloan Digital Sky Survey – III. Baryon Oscillations Spectroscopic Survey galaxies, Mon. Not. R. Astron. Soc. 453 (2) (2015) 1754–1767, arXiv:1504.02100 [astro-ph.CO].

[1142] ACT Collaboration, G.S. Farren, et al., The atacama cosmology telescope: cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing, Astrophys. J. 966 (2) (2024) 157, arXiv:2309.05659 [astro-ph.CO].

[1143] G. Piccirilli, G. Fabbian, D. Alonso, K. Storey-Fisher, J. Carron, A. Lewis, C. García-García, Growth history and quasar bias evolution at z < 3 from Quaia, J. Cosmol. Astropart. Phys. 06 (2024) 012, arXiv:2402.05761 [astro-ph.CO].

[1144] D. Alonso, G. Fabbian, K. Storey-Fisher, A.-C. Eilers, C. García-García, D.W. Hogg, H.-W. Rix, Constraining cosmology with the Gaia-unWISE Quasar Catalog and CMB lensing: structure growth, J. Cosmol. Astropart. Phys. 11 (2023) 043, arXiv:2306.17748 [astro-ph.CO].

[1145] BOSS Collaboration, S. Alam, et al., The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample, Mon. Not. R. Astron. Soc. 470 (3) (2017) 2617–2652, arXiv:1607.03155 [astro-ph.CO].

[1146] DESI Collaboration, A. Dey, et al., Overview of the DESI legacy imaging surveys, Astron. J. 157 (5) (2019) 168, arXiv:1804.08657 [astro-ph.IM].

[1147] C.S. Saraf, P. Bielewicz, M. Chodorowski, Effect of redshift bin mismatch on the cross correlation between the DESI Legacy Imaging Survey and the Planck CMB lensing potential, Astron. Astrophys. 690 (2024) A338, arXiv:2406.02857 [astro-ph.CO].

[1148] S.J. Nakoneczny, et al., Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background, Astron. Astrophys. 681 (2024) A105, arXiv:2310.07642 [astro-ph.CO]; Astron. Astrophys. 686 (2024) C2 (erratum).

[1149] DES, SPT Collaboration, C. Chang, et al., Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. II. Cross-correlation measurements and cosmological constraints, Phys. Rev. D 107 (2) (2023) 023530, arXiv:2203.12440 [astro-ph.CO].

[1150] M. White, et al., Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing, J. Cosmol. Astropart. Phys. 02 (02) (2022) 007, arXiv:2111.09898 [astro-ph.CO].

[1151] Z. Sun, J. Yao, F. Dong, X. Yang, L. Zhang, P. Zhang, Cross-correlation of Planck cosmic microwave background lensing with DESI galaxy groups, Mon. Not. R. Astron. Soc. 511 (3) (2022) 3548–3560, arXiv:2109.07387 [astro-ph.CO].

[1152] A. Krolewski, S. Ferraro, M. White, Cosmological constraints from unWISE and Planck CMB lensing tomography, J. Cosmol. Astropart. Phys. 12 (12) (2021) 028, arXiv:2105.03421 [astro-ph.CO].

[1153] Q. Hang, S. Alam, J.A. Peacock, Y.-C. Cai, Galaxy clustering in the DESI Legacy Survey and its imprint on the CMB, Mon. Not. R. Astron. Soc. 501 (1) (2021) 1481–1498, arXiv:2010.00466 [astro-ph.CO].

[1154] J.A. Peacock, M. Bilicki, Wide-area tomography of CMB lensing and the growth of cosmological density fluctuations, Mon. Not. R. Astron. Soc. 481 (1) (2018) 1133–1148, arXiv:1805.11525 [astro-ph.CO].

[1155] DES Collaboration, T. Giannantonio, et al., CMB lensing tomography with the DES Science Verification galaxies, Mon. Not. R. Astron. Soc. 456 (3) (2016) 3213–3244, arXiv:1507.05551 [astro-ph.CO].

[1156] N. Sailer, et al., Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6, 2024, arXiv:2407.04607 [astro-ph.CO].

[1157] C.S. Saraf, P. Bielewicz, Tomographic cross correlations between galaxy surveys and the CMB gravitational lensing potential - Effect of the redshift bin mismatch, Astron. Astrophys. 687 (2024) A150, arXiv:2311.15261 [astro-ph.CO].

[1158] T. Simon, P. Zhang, V. Poulin, Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis, J. Cosmol. Astropart. Phys. 07 (2023) 041, arXiv:2210.14931 [astro-ph.CO].

[1159] Y. Kobayashi, T. Nishimichi, M. Takada, H. Miyatake, Full-shape cosmology analysis of the SDSS-III BOSS galaxy power spectrum using an emulator-based halo model: A 5% determination of σ8, Phys. Rev. D 105 (8) (2022) 083517, arXiv:2110.06969 [astro-ph.CO].

[1160] S.-F. Chen, Z. Vlah, M. White, A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO, J. Cosmol. Astropart. Phys. 02 (02) (2022) 008, arXiv:2110.05530 [astro-ph.CO].

[1161] M.M. Ivanov, O.H.E. Philcox, G. Cabass, T. Nishimichi, M. Simonović, M. Zaldarriaga, Cosmology with the galaxy bispectrum multipoles: Optimal estimation and application to BOSS data, Phys. Rev. D 107 (8) (2023) 083515, arXiv:2302.04414 [astro-ph.CO].

[1162] O.H.E. Philcox, M.M. Ivanov, BOSS DR12 full-shape cosmology: ΛCDM constraints from the large-scale galaxy power spectrum and bispectrum monopole, Phys. Rev. D 105 (4) (2022) 043517, arXiv:2112.04515 [astro-ph.CO].

[1163] S. Joudaki, et al., KiDS-450 + 2dFlenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering, Mon. Not. R. Astron. Soc. 474 (4) (2018) 4894–4924, arXiv:1707.06627 [astro-ph.CO].

[1164] E. van Uitert, et al., KiDS+GAMA: cosmology constraints from a joint analysis of cosmic shear, galaxy–galaxy lensing, and angular clustering, Mon. Not. R. Astron. Soc. 476 (4) (2018) 4662–4689, arXiv:1706.05004 [astro-ph.CO].

[1165] DES Collaboration, T.M.C. Abbott, et al., Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing, Phys. Rev. D 98 (4) (2018) 043526, arXiv:1708.01530 [astro-ph.CO].

[1166] BOSS Collaboration, A.J. Ross, et al., The clustering of galaxies in the SDSS-III baryon oscillation spectroscopic survey: analysis of potential systematics, Mon. Not. R. Astron. Soc. 424 (2012) 564, arXiv:1203.6499 [astro-ph.CO].

[1167] C. Hahn, R. Scoccimarro, M.R. Blanton, J.L. Tinker, S.A. Rodriguez-Torres, The effect of fibre collisions on the galaxy power spectrum multipoles, Mon. Not. R. Astron. Soc. 467 (2) (2017) 1940–1956, arXiv:1609.01714 [astro-ph.CO].

[1168] A. de Mattia, V. Ruhlmann-Kleider, Integral constraints in spectroscopic surveys, J. Cosmol. Astropart. Phys. 08 (2019) 036, arXiv:1904.08851 [astro-ph.CO].

[1169] C.S. Saraf, P. Bielewicz, M. Chodorowski, Cross-correlation between Planck CMB lensing potential and galaxy catalogues from HELP, Mon. Not. R. Astron. Soc. 515 (2) (2022) 1993–2007, arXiv:2106.02551 [astro-ph.CO].

[1170] A.R. Pullen, S. Alam, S. He, S. Ho, Constraining gravity at the largest scales through CMB lensing and galaxy velocities, Mon. Not. R. Astron. Soc. 460 (4) (2016) 4098–4108, arXiv:1511.04457 [astro-ph.CO].

[1171] S. Joudaki, et al., CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics, Mon. Not. R. Astron. Soc. 465 (2) (2017) 2033–2052, arXiv:1601.05786 [astro-ph.CO].
[1172] M.M. Ivanov, M. Simonović, M. Zaldarriaga, Cosmological parameters from the BOSS galaxy power spectrum, J. Cosmol. Astropart. Phys. 05 (2020) 042, arXiv:1909.05277 [astro-ph.CO].

[1173] R. Gsponer, R. Zhao, J. Donald-McCann, D. Bacon, K. Koyama, R. Crittenden, T. Simon, E.-M. Mueller, Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16, Mon. Not. R. Astron. Soc. 530 (3) (2024) 3075-3099, arXiv:2312.01977 [astro-ph.CO].

[1174] S.-F. Chen, Z. Vlah, E. Castorina, M. White, Redshift-space distortions in lagrangian perturbation theory, J. Cosmol. Astropart. Phys. 03 (2021) 100, arXiv:2012.04636 [astro-ph.CO].

[1175] DESI Collaboration, S. Ramirez-Solano, et al., Full Modeling and parameter compression methods in configuration space for DESI 2024 and beyond, J. Cosmol. Astropart. Phys. 01 (2025) 129, arXiv:2404.07268 [astro-ph.CO].

[1176] M. Maus, et al., A comparison of effective field theory models of redshift space galaxy power spectra for DESI 2024 and future surveys, J. Cosmol. Astropart. Phys. 01 (2025) 134, arXiv:2404.07272 [astro-ph.CO].

[1177] D. Baumann, A. Nicolis, L. Senatore, M. Zaldarriaga, Cosmological non-linearities as an effective fluid, J. Cosmol. Astropart. Phys. 07 (2012) 051, arXiv:1004.2488 [astro-ph.CO].

[1178] J.J.M. Carrasco, M.P. Hertzberg, L. Senatore, The effective field theory of cosmological large scale structures, JHEP 09 (2012) 082, arXiv:1206.2926 [astro-ph.CO].

[1179] R.A. Porto, L. Senatore, M. Zaldarriaga, The lagrangian-space effective field theory of large scale structures, J. Cosmol. Astropart. Phys. 05 (2014) 022, arXiv:1311.2168 [astro-ph.CO].

[1180] M. Lewandowski, L. Senatore, F. Prada, C. Zhao, C.-H. Chuang, EFT of large scale structures in redshift space, Phys. Rev. D 97 (6) (2018) 063526, arXiv:1512.06831 [astro-ph.CO].

[1181] A. Lewis, A. Challinor, Weak gravitational lensing of the CMB, Phys. Rep. 429 (2006) 1-65, arXiv:astro-ph/0601594.

[1182] J. Carron, M. Mirmelstein, A. Lewis, CMB lensing from Planck PR4 maps, J. Cosmol. Astropart. Phys. 09 (2022) 039, arXiv:2206.07773 [astro-ph.CO].

[1183] ACT Collaboration, F.J. Qu, et al., The atacama cosmology telescope: a measurement of the DR6 CMB lensing power spectrum and its implications for structure growth, Astrophys. J. 962 (2) (2024) 112, arXiv:2304.05202 [astro-ph.CO].

[1184] SPT Collaboration, Z. Pan, et al., Measurement of gravitational lensing of the cosmic microwave background using SPT-3G 2018 data, Phys. Rev. D 108 (12) (2023) 122005, arXiv:2308.11608 [astro-ph.CO].

[1185] E. Di Valentino, A. Melchiorri, J. Silk, Planck evidence for a closed Universe and a possible crisis for cosmology, Nat. Astron. 4 (2) (2019) 196-203, arXiv:1911.02087 [astro-ph.CO].

[1186] W. Handley, Curvature tension: evidence for a closed universe, Phys. Rev. D 103 (4) (2021) L041301, arXiv:1908.09139 [astro-ph.CO].

[1187] G. Efstathiou, S. Gratton, The evidence for a spatially flat Universe, Mon. Not. R. Astron. Soc. 496 (1) (2020) L91-L95, arXiv:2002.06892 [astro-ph.CO].

[1188] A. Glanville, C. Howlett, T.M. Davis, Full-shape galaxy power spectra and the curvature tension, Mon. Not. R. Astron. Soc. 517 (2) (2022) 3087-3100, arXiv:2205.05892 [astro-ph.CO].

[1189] S. Vagnozzi, A. Loeb, M. Moresco, Eppur è piatto? The cosmic chronometers take on spatial curvature and cosmic concordance, Astrophys. J. 908 (1) (2021) 84, arXiv:2011.11645 [astro-ph.CO].

[1190] S. Vagnozzi, E. Di Valentino, S. Gariazzo, A. Melchiorri, O. Mena, J. Silk, The galaxy power spectrum take on spatial curvature and cosmic concordance, Phys. Dark Univ. 33 (2021) 100851, arXiv:2010.02230 [astro-ph.CO].

[1191] C.-G. Park, B. Ratra, Using the tilted flat-ΛCDM and the untilted non-flat ΛCDM inflation models to measure cosmological parameters from a compilation of observational data, Astrophys. J. 882 (2019) 158, arXiv:1801.00213 [astro-ph.CO].

[1192] C.-G. Park, B. Ratra, Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data, Astrophys. Space Sci. 364 (8) (2019) 134, arXiv:1809.03598 [astro-ph.CO].

[1193] WMAP Collaboration, C.L. Bennett, et al., Nine-year wilkinson microwave anisotropy probe (WMAP) observations: final maps and results, Astrophys. J. Suppl. 208 (2013) 20, arXiv:1212.5225 [astro-ph.CO].

[1194] Planck Collaboration, R. Adam, et al., Planck 2015 results. I. Overview of products and scientific results, Astron. Astrophys. 594 (2016) A1, arXiv:1502.01582 [astro-ph.CO].

[1195] WMAP Collaboration, G. Hinshaw, et al., First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: The Angular power spectrum, Astrophys. J. Suppl. 148 (2003) 135, arXiv:astro-ph/0302217.

[1196] C.R. Contaldi, M. Peloso, L. Kofman, A.D. Linde, Suppressing the lower multipoles in the CMB anisotropies, J. Cosmol. Astropart. Phys. 07 (2003) 002, arXiv:astro-ph/0303636.

[1197] J.M. Cline, P. Crotty, J. Lesgourgues, Does the small CMB quadrupole moment suggest new physics? J. Cosmol. Astropart. Phys. 09 (2003) 010, arXiv:astro-ph/0304558.

[1198] D.J. Schwarz, G.D. Starkman, D. Huterer, C.J. Copi, Is the low-l microwave background cosmic? Phys. Rev. Lett. 93 (2004) 221301, arXiv:astro-ph/0403353.

[1199] C.J. Copi, D. Huterer, D.J. Schwarz, G.D. Starkman. On the large-angle anomalies of the microwave sky, Mon. Not. R. Astron. Soc. 367 (2006) 79-102, arXiv:astro-ph/0508047.

[1200] A. de Oliveira-Costa, M. Tegmark, Cmb multipole measurements in the presence of foregrounds, Phys. Rev. D 74 (2006) 023005, arXiv:astro-ph/0603369.

[1201] A. Slosar, U. Seljak, Assessing the effects of foregrounds and sky removal in WMAP, Phys. Rev. D 70 (2004) 083002, arXiv:astro-ph/0404567.

[1202] A. Hajian, Analysis of the apparent lack of power in the cosmic microwave background anisotropy at large angular scales, 2007, arXiv:astro-ph/0702723.

[1203] Planck Collaboration, P.A.R. Ade, et al., Planck 2013 results. XXIII. Isotropy and statistics of the CMB, Astron. Astrophys. 571 (2014) A23, arXiv:1303.5083 [astro-ph.CO].

[1204] H.K. Eriksen, F.K. Hansen, A.J. Banday, K.M. Gorski, P.B. Lilje, Asymmetries in the cosmic microwave background anisotropy field, Astrophys. J. 605 (2004) 14-20, arXiv:astro-ph/0307507; Astrophys. J. 609 (2004) 1198 (erratum).

[1205] Planck Collaboration, P.A.R. Ade, et al., Planck 2015 results. XVI. Isotropy and statistics of the CMB, Astron. Astrophys. 594 (2016) A16, arXiv:1506.07135 [astro-ph.CO].

[1206] A.L. Erickcek, M. Kamionkowski, S.M. Carroll, A hemispherical power asymmetry from inflation, Phys. Rev. D 78 (2008) 123520, arXiv:0806.0377 [astro-ph].

[1207] F. Schmidt, L. Hui, Cosmic microwave background power asymmetry from non-gaussian modulation, Phys. Rev. Lett. 110 (2013) 011301, arXiv:1210.2965 [astro-ph.CO]; Phys. Rev. Lett. 110 (2013) 059902 (erratum).

[1208] F.K. Hansen, T. Trombetti, N. Bartolo, U. Natale, M. Liguori, A.J. Banday, K.M. Gorski, Isotropic non-Gaussian gNL-like toy models that reproduce cosmic microwave background anomalies, Astron. Astrophys. 626 (2019) A13, arXiv:1806.08531 [astro-ph.CO].

[1209] C. Gordon, W. Hu, A Low CMB quadrupole from dark energy isocurvature perturbations, Phys. Rev. D 70 (2004) 083003, arXiv:astro-ph/0406496.

[1210] K. Land, J. Magueijo, The axis of evil, Phys. Rev. Lett. 95 (2005) 071301, arXiv:astro-ph/0502237.

[1211] J. Kim, P. Naselsky, Lack of angular correlation and odd-parity preference in CMB data, Astrophys. J. 739 (2011) 79, arXiv:1011.0377 [astro-ph.CO].

[1212] A. Lue, L.-M. Wang, M. Kamionkowski, Cosmological signature of new parity violating interactions, Phys. Rev. Lett. 83 (1999) 1506-1509, arXiv:astro-ph/9812088.

[1213] S.H.S. Alexander, Is cosmic parity violation responsible for the anomalies in the WMAP data? Phys. Lett. B 660 (2008) 444-448, arXiv:hep-th/0601034.

[1214] P. Vielva, E. Martinez-Gonzalez, R.B. Barreiro, J.L. Sanz, L. Cayon, Detection of non-Gaussianity in the WMAP 1 - year data using spherical wavelets, Astrophys. J. 609 (2004) 22-34, arXiv:astro-ph/0310273.

[1215] M. Cruz, L. Cayon, E. Martinez-Gonzalez, P. Vielva, J. Jin, The non-gaussian cold spot in the 3-year wmap data, Astrophys. J. 655 (2007) 11-20, arXiv:astro-ph/0603859.

[1216] S. Nadathur, M. Lavinto, S. Hotchkiss, S. Räsänen, Can a supervoid explain the Cold Spot? Phys. Rev. D 90 (10) (2014) 103510, arXiv:1408.4720 [astro-ph.CO].

[1217] K.T. Inoue, J. Silk, Local voids as the origin of large-angle cosmic microwave background anomalies I, Astrophys. J. 648 (2006) 23-30, arXiv:astro-ph/0602478.

[1218] R. Holman, L. Mersini-Houghton, T. Takahashi, Cosmological avatars of the landscape I: Bracketing the SUSY breaking scale, Phys. Rev. D 77 (2008) 063510, arXiv:hep-th/0611223.

[1219] M. Cruz, M. Tucci, E. Martinez-Gonzalez, P. Vielva, The non-gaussian cold spot in wmap: significance, morphology and foreground contribution, Mon. Not. R. Astron. Soc. 369 (2006) 57-67, arXiv:astro-ph/0601427.

[1220] L. Rudnick, S. Brown, L.R. Williams, Extragalactic radio sources and the WMAP cold spot, Astrophys. J. 671 (2007) 40-44, arXiv:0704.0908 [astro-ph].

[1221] D.G. Lambas, F.K. Hansen, F. Toscano, H.E. Luparello, E.F. Boero, The CMB Cold Spot as predicted by foregrounds around nearby galaxies, Astron. Astrophys. 681 (2024) A2, arXiv:2310.13755 [astro-ph.CO].

[1222] I. Szapudi, et al., Detection of a supervoid aligned with the cold spot of the cosmic microwave background, Mon. Not. R. Astron. Soc. 450 (1) (2015) 288-294, arXiv:1405.1566 [astro-ph.CO].

[1223] R. Mackenzie, T. Shanks, M.N. Bremer, Y.-C. Cai, M.L.P. Gunawardhana, A. Kovács, P. Norberg, I. Szapudi, Evidence against a supervoid causing the CMB Cold Spot, Mon. Not. R. Astron. Soc. 470 (2) (2017) 2328-2338, arXiv:1704.03814 [astro-ph.CO].

[1224] H.M. Courtois, R.B. Tully, Y. Hoffman, D. Pomarede, R. Graziani, A. Dupuy, Cosmicflows-3: cold spot repeller? Astrophys. J. Lett. 847 (1) (2017) L6, arXiv:1708.07547 [astro-ph.CO].

[1225] DES Collaboration, A. Kovács, et al., The DES view of the Eridanus supervoid and the CMB cold spot, Mon. Not. R. Astron. Soc. 510 (1) (2022) 216-229, arXiv:2112.07699 [astro-ph.CO].

[1226] H.E. Luparello, E.F. Boero, M. Lares, A.G. Sánchez, D.G. Lambas, The cosmic shallows – I. Interaction of CMB photons in extended galaxy haloes, Mon. Not. R. Astron. Soc. 518 (4) (2022) 5643-5652, arXiv:2206.14217 [astro-ph.CO].
[1227] F.K. Hansen, E.F. Boero, H.E. Luparello, D.G. Lambas, A possible common explanation for several cosmic microwave background (CMB) anomalies: A strong impact of nearby galaxies on observed large-scale CMB fluctuations, Astron. Astrophys. 675 (2023) L7, arXiv:2305.00268 [astro-ph.CO].

[1228] J.P. Huchra, et al., The 2MASS redshift survey - description and data release, Astrophys. J. Suppl. 199 (2012) 26, arXiv:1108.0669 [astro-ph.CO].

[1229] M. Cruz, E. Martínez-González, C. Gimeno-Amo, B.J. Kavanagh, M. Tucci, Unexplained correlation between the Cosmic Microwave Background temperature and the local matter density distribution, J. Cosmol. Astropart. Phys. 04 (2025) 079, arXiv:2407.17599 [astro-ph.CO].

[1230] F.K. Hansen, D.G. Lambas, H.E. Luparello, F. Toscano, L.A. Pereyra, A $5\sigma$ detection confirming the existence of a possibly dark matter related CMB foreground in nearby cosmic filaments, 2024, arXiv:2411.15307 [astro-ph.CO].

[1231] F. Toscano, F.K. Hansen, D.G. Lambas, H. Luparello, P. Fosalba, E. Gaztañaga, Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies? Phys. Rev. D 111 (8) (2025) 083528, arXiv:2410.24026 [astro-ph.CO].

[1232] C.J. Copi, D. Huterer, D.J. Schwarz, G.D. Starkman, No large-angle correlations on the non-Galactic microwave sky, Mon. Not. R. Astron. Soc. 399 (2009) 295-303, arXiv:0808.3767 [astro-ph].

[1233] D. Sarkar, D. Huterer, C.J. Copi, G.D. Starkman, D.J. Schwarz, Missing power vs low-l alignments in the cosmic microwave background: no correlation in the standard cosmological model, Astropart. Phys. 34 (2011) 591-594, arXiv:1004.3784 [astro-ph.CO].

[1234] J.P. Luminet, J. Weeks, A. Riazuelo, R. Lehoucq, J.P. Uzan, Dodecahedral space topology as an explanation for weak wide - angle temperature correlations in the cosmic microwave background, Nature 425 (2003) 593, arXiv: astro-ph/0310253.

[1235] R. Aurich, H.S. Janzer, S. Lustig, F. Steiner, Do we live in a small universe? Cl. Quant. Grav. 25 (2008) 125006, arXiv:0708.1420 [astro-ph].

[1236] C. Copi, D. Huterer, D. Schwarz, G. Starkman, The uncorrelated universe: statistical anisotropy and the vanishing angular correlation function in WMAP years 1-3, Phys. Rev. D 75 (2007) 023507, arXiv:astro-ph/0605135.

[1237] C.J. Hogan, Gravitational waves from light cosmic strings: backgrounds and bursts with large loops, Phys. Rev. D 74 (2006) 043526, arXiv:astro-ph/0605567.

[1238] L.P. Chimento, M.I. Forte, Anisotropic k-essence cosmologies, Phys. Rev. D 73 (2006) 063502, arXiv:astro-ph/0510726.

[1239] S. Tsujikawa, M. Sami, R. Maartens, Observational constraints on braneworld inflation: the effect of a gauss-bonnet term, Phys. Rev. D 70 (2004) 063525, arXiv:astro-ph/0406078.

[1240] M.-a. Watanabe, S. Kanno, J. Soda, Inflationary universe with anisotropic hair, Phys. Rev. Lett. 102 (2009) 191302, arXiv:0902.2833 [hep-th].

[1241] J. Delabrouille, et al., The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths, Astron. Astrophys. 553 (2013) A96, arXiv:1207.3675 [astro-ph.CO].

[1242] L. Mersini-Houghton, Cosmological implications of the string theory landscape, AIP Conf. Proc. 878 (1) (2006) 315-322, arXiv:hep-ph/0609157.

[1243] L. Mersini-Houghton, Can we predict Lambda for the non-SUSY sector of the landscape, Cl. Quant. Grav. 22 (2005) 3481-3490, arXiv:hep-th/0504026.

[1244] A. Kobakhidze, L. Mersini-Houghton, Birth of the universe from the landscape of string theory, Eur. Phys. J. C 49 (2007) 869-873, arXiv:hep-th/0410213.

[1245] R. Holman, L. Mersini-Houghton, Why the universe started from a low entropy state, Phys. Rev. D 74 (2006) 123510, arXiv:hep-th/0511102.

[1246] R. Holman, L. Mersini-Houghton, T. Takahashi, Cosmological avatars of the landscape. II. CMB and LSS signatures, Phys. Rev. D 77 (2008) 063511, arXiv:hep-th/0612142.

[1247] E. Di Valentino, L. Mersini-Houghton, Testing predictions of the quantum landscape multiverse 1: the starobinsky inflationary potential, J. Cosmol. Astropart. Phys. 03 (2017) 002, arXiv:1612.09588 [astro-ph.CO].

[1248] E. Di Valentino, L. Mersini-Houghton, Testing predictions of the quantum landscape multiverse 2: the exponential inflationary potential, J. Cosmol. Astropart. Phys. 03 (2017) 020, arXiv:1612.08334 [astro-ph.CO].

[1249] E. Di Valentino, L. Mersini-Houghton, Testing predictions of the quantum landscape multiverse 3: the hilltop inflationary potential, Symmetry 11 (4) (2019) 520, arXiv:1807.10833 [astro-ph.CO].

[1250] L. Mersini-Houghton, Predictions of the quantum landscape multiverse, Cl. Quant. Grav. 34 (4) (2017) 047001, arXiv:1612.07129 [hep-th].

[1251] DESI Collaboration, K. Lodha, et al., DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data, Phys. Rev. D 111 (2) (2025) 023532, arXiv:2405.13588 [astro-ph.CO].

[1252] DESI Collaboration, M.A. Karim, et al., DESI DR2 results I: baryon acoustic oscillations from the lyman alpha forest, 2025, arXiv:2503.14739 [astro-ph.CO].

[1253] DESI Collaboration, U. Andrade, et al., Validation of the DESI DR2 measurements of baryon acoustic oscillations from galaxies and quasars, 2025, arXiv:2503.14742 [astro-ph.CO].

[1254] A. Brodzeller, et al., Construction of the damped Ly$\alpha$ absorber catalog for DESI DR2 Ly$\alpha$ BAO, 2025, arXiv:2503.14740 [astro-ph.CO].

[1255] DESI Collaboration, K. Lodha, et al., Extended dark energy analysis using DESI DR2 BAO measurements, 2025, arXiv:2503.14743 [astro-ph.CO].

[1256] D. Rubin, et al., Union through UNITY: cosmology with 2,000 SNe using a unified Bayesian framework, 2023, arXiv:2311.12098 [astro-ph.CO].

[1257] DES Collaboration, T.M.C. Abbott, et al., The dark energy survey: cosmology results with ~1500 new high-redshift type ia supernovae using the full 5 yr data set, Astrophys. J. Lett. 973 (1) (2024) L14, arXiv:2401.02929 [astro-ph.CO].

[1258] DES Collaboration, B.O. Sánchez, et al., The dark energy survey supernova program: light curves and 5 yr data release, Astrophys. J. 975 (1) (2024) 5, arXiv:2406.05046 [astro-ph.CO].

[1259] DES Collaboration, M. Vincenzi, et al., The dark energy survey supernova program: cosmological analysis and systematic uncertainties, Astrophys. J. 975 (1) (2024) 86, arXiv:2401.02945 [astro-ph.CO].

[1260] DESI Collaboration, K. Lodha, et al., Extended dark energy analysis using DESI DR2 BAO measurements, 2025, arXiv:2503.14743 [astro-ph.CO].

[1261] A. Vikman, Can dark energy evolve to the phantom? Phys. Rev. D 71 (2005) 023515, arXiv:astro-ph/0407107.

[1262] S.M. Carroll, M. Hoffman, M. Trodden, Can the dark energy equation-of-state parameter $w$ be less than -1? Phys. Rev. D 68 (2003) 023509, arXiv:astro-ph/0301273.

[1263] W. Hu, Crossing the phantom divide: Dark energy internal degrees of freedom, Phys. Rev. D 71 (2005) 047301, arXiv:astro-ph/0410680.

[1264] P. Creminelli, G. D'Amico, J. Norena, F. Vernizzi, The effective theory of quintessence: the w<-1 side unveiled, J. Cosmol. Astropart. Phys. 02 (2009) 018, arXiv:0811.0827 [astro-ph].

[1265] A. Chudaykin, M. Kunz, Modified gravity interpretation of the evolving dark energy in light of DESI data, Phys. Rev. D 110 (12) (2024) 123524, arXiv:2407.02558 [astro-ph.CO].

[1266] G. Ye, M. Martinelli, B. Hu, A. Silvestri, Non-minimally coupled gravity as a physically viable fit to DESI 2024 BAO, 2024, arXiv:2407.15832 [astro-ph.CO].

[1267] M. Ishak, et al., Modified gravity constraints from the full shape modeling of clustering measurements from DESI 2024, 2024, arXiv:2411.12026 [astro-ph.CO].

[1268] A. Chudaykin, M. Kunz, J. Carron, Modified gravity constraints with Planck ISW-lensing bispectrum, 2025, arXiv:2503.09893 [astro-ph.CO].

[1269] W.J. Wolf, P.G. Ferreira, C. García-García, Matching current observational constraints with nonminimally coupled dark energy, Phys. Rev. D 111 (4) (2025) L041303, arXiv:2409.17019 [astro-ph.CO].

[1270] A. Hernández-Almada, M.L. Mendoza-Martínez, M.A. García-Aspeitia, V. Motta, Phenomenological emergent dark energy in the light of DESI Data Release 1, Phys. Dark Univ. 46 (2024) 101668, arXiv:2407.09430 [astro-ph.CO].

[1271] DESI Collaboration, M. Malekjani, Z. Davari, S. Pourojaghi, Cosmological constraints on dark energy parametrizations after DESI 2024: Persistent deviation from standard ΛCDM cosmology, Phys. Rev. D 111 (8) (2025) 083547, arXiv:2407.09767 [astro-ph.CO].

[1272] O.F. Ramadan, J. Sakstein, D. Rubin, DESI constraints on exponential quintessence, Phys. Rev. D 110 (4) (2024) L041303, arXiv:2405.18747 [astro-ph.CO].

[1273] Y. Carloni, O. Luongo, M. Muccino, Does dark energy really revive using DESI 2024 data? Phys. Rev. D 111 (2) (2025) 023512, arXiv:2404.12068 [astro-ph.CO].

[1274] K.V. Berghaus, J.A. Kable, V. Miranda, Quantifying scalar field dynamics with DESI 2024 Y1 BAO measurements, Phys. Rev. D 110 (10) (2024) 103524, arXiv:2404.14341 [astro-ph.CO].

[1275] F.J. Qu, K.M. Surrao, B. Bolliet, J.C. Hill, B.D. Sherwin, H.T. Jense, Accelerated inference on accelerated cosmic expansion: New constraints on axion-like early dark energy with DESI BAO and ACT DR6 CMB lensing, 2024, arXiv:2404.16805 [astro-ph.CO].

[1276] A. Notari, M. Redi, A. Tesi, Consistent theories for the DESI dark energy fit, J. Cosmol. Astropart. Phys. 11 (2024) 025, arXiv:2406.08459 [astro-ph.CO].

[1277] P. Adolf, M. Hirsch, S. Krieg, H. Päs, M. Tabet, Fitting the DESI BAO data with dark energy driven by the Cohen-Kaplan-Nelson bound, J. Cosmol. Astropart. Phys. 08 (2024) 048, arXiv:2406.09964 [astro-ph.CO].

[1278] J.-Q. Jiang, D. Pedrotti, S.S. da Costa, S. Vagnozzi, Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data, Phys. Rev. D 110 (12) (2024) 123519, arXiv:2408.02365 [astro-ph.CO].

[1279] B.R. Dinda, R. Maartens, Model-agnostic assessment of dark energy after DESI DR1 BAO, J. Cosmol. Astropart. Phys. 01 (2025) 120, arXiv:2407.17252 [astro-ph.CO].

[1280] W.J. Wolf, C. García-García, P.G. Ferreira, Robustness of dark energy phenomenology across different parameterizations, 2025, arXiv:2502.04929 [astro-ph.CO].

[1281] A. Sousa-Neto, C. Bengaly, J.E. González, J. Alcaniz, No evidence for dynamical dark energy from DESI and SN data: a symbolic regression analysis, 2025, arXiv:2502.10506 [astro-ph.CO].

[1282] R. de Putter, E.V. Linder, Calibrating dark energy, J. Cosmol. Astropart. Phys. 10 (2008) 042, arXiv:0808.0189 [astro-ph].

[1283] W. Giarè, M. Najafi, S. Pan, E. Di Valentino, J.T. Firouzjaee, Robust preference for dynamical dark energy in DESI BAO and SN measurements, J. Cosmol. Astropart. Phys. 10 (2024) 035, arXiv:2407.16689 [astro-ph.CO].
[1284] Z. Wang, S. Lin, Z. Ding, B. Hu, The role of LRG1 and LRG2's monopole in inferring the DESI 2024 BAO cosmology, Mon. Not. R. Astron. Soc. 534 (4) (2024) 3869-3875, arXiv:2405.02168 [astro-ph.CO].

[1285] E.O. Colgáin, M.G. Dainotti, S. Capozziello, S. Pourojaghi, M.M. Sheikh-Jabbari, D. Stojkovic, Does DESI 2024 confirm $\Lambda$CDM? 2024, arXiv:2404.08633 [astro-ph.CO].

[1286] D. Naredo-Tuero, M. Escudero, E. Fernández-Martínez, X. Marcano, V. Poulin, Critical look at the cosmological neutrino mass bound, Phys. Rev. D 110 (12) (2024) 123537, arXiv:2407.13831 [astro-ph.CO].

[1287] D. Sapone, S. Nesseris, Outliers in DESI BAO: robustness and cosmological implications, 2024, arXiv:2412.01740 [astro-ph.CO].

[1288] W. Giarè, T. Mahassen, E. Di Valentino, S. Pan, An overview of what current data can (and cannot yet) say about evolving dark energy, Phys. Dark Univ. 48 (2025) 101906, arXiv:2502.10264 [astro-ph.CO].

[1289] DES Collaboration, T.M.C. Abbott, et al., Dark Energy Survey: implications for cosmological expansion models from the final DES Baryon Acoustic Oscillation and Supernova data, 2025, arXiv:2503.06712 [astro-ph.CO].

[1290] E.O. Colgáin, M.M. Sheikh-Jabbari, R. Solomon, M.G. Dainotti, D. Stojkovic, Putting flat $\Lambda$CDM in the (Redshift) bin, Phys. Dark Univ. 44 (2024) 101464, arXiv:2206.11447 [astro-ph.CO].

[1291] M. Malekjani, R.M. Conville, E.O. Colgáin, S. Pourojaghi, M.M. Sheikh-Jabbari, On redshift evolution and negative dark energy density in Pantheon + Supernovae, Eur. Phys. J. C 84 (3) (2024) 317, arXiv:2301.12725 [astro-ph.CO].

[1292] E.O. Colgáin, S. Pourojaghi, M.M. Sheikh-Jabbari, Implications of DES 5YR SNe dataset for $\Lambda$CDM, Eur. Phys. J. C 85 (3) (2025) 286, arXiv:2406.06389 [astro-ph.CO].

[1293] E.O. Colgáin, M.M. Sheikh-Jabbari, DESI and SNe: dynamical dark energy, $\Omega_m$ tension or systematics? 2024, arXiv:2412.12905 [astro-ph.CO].

[1294] A. Notari, M. Redi, A. Tesi, BAO vs. SN evidence for evolving dark energy, J. Cosmol. Astropart. Phys. 04 (2025) 048, arXiv:2411.11685 [astro-ph.CO].

[1295] G. Efstathiou, Evolving dark energy or supernovae systematics? Mon. Not. R. Astron. Soc. 538 (2) (2025) 875-882, arXiv:2408.07175 [astro-ph.CO].

[1296] DES Collaboration, M. Vincenzi, et al., Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: Investigation based on "Evolving Dark Energy or Supernovae systematics?", 2025, arXiv:2501.06664 [astro-ph.CO].

[1297] W. Giarè, Dynamical dark energy beyond planck? Constraints from multiple CMB probes, DESI BAO and type-ia supernovae, 2024, arXiv:2409.17074 [astro-ph.CO].

[1298] L.A. Escamilla, W. Giarè, E. Di Valentino, R.C. Nunes, S. Vagnozzi, The state of the dark energy equation of state circa 2023, J. Cosmol. Astropart. Phys. 05 (2024) 091, arXiv:2307.14802 [astro-ph.CO].

[1299] W. Giarè, E. Di Valentino, A. Melchiorri, Measuring the reionization optical depth without large-scale CMB polarization, Phys. Rev. D 109 (10) (2024) 103519, arXiv:2312.06482 [astro-ph.CO].

[1300] I. Ben-Dayan, U. Kumar, M. Shimon, A. Verma, Impact of low ell's on large scale structure anomalies, J. Cosmol. Astropart. Phys. 02 (2025) 069, arXiv:2409.15457 [astro-ph.CO].

[1301] Z.-Y. Peng, Y.-S. Piao, Dark energy and lensing anomaly in Planck CMB data, 2025, arXiv:2502.04641 [astro-ph.CO].

[1302] C.-G. Park, B. Ratra, Is excess smoothing of Planck CMB anisotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? 2025, arXiv:2501.03480 [astro-ph.CO].

[1303] C.-G. Park, J. de Cruz Perez, B. Ratra, Is the $w_0w_\Lambda$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data? 2024, arXiv:2410.13627 [astro-ph.CO].

[1304] E. Di Valentino, S. Garciazo, O. Mena, Most constraining cosmological neutrino mass bounds, Phys. Rev. D 104 (8) (2021) 083504, arXiv:2106.15267 [astro-ph.CO].

[1305] J.-Q. Jiang, W. Giarè, S. Garciazo, M.G. Dainotti, E. Di Valentino, O. Mena, D. Pedrotti, S.S. da Costa, S. Vagnozzi, Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations, J. Cosmol. Astropart. Phys. 01 (2025) 153, arXiv: 2407.18047 [astro-ph.CO].

[1306] E. Di Valentino, S. Garciazo, W. Giarè, O. Mena, Impact of the damping tail on neutrino mass constraints, Phys. Rev. D 108 (8) (2023) 083509, arXiv:2305.12989 [astro-ph.CO].

[1307] D. Wang, O. Mena, E. Di Valentino, S. Garciazo, Updating neutrino mass constraints with background measurements, Phys. Rev. D 110 (10) (2024) 103536, arXiv:2405.03368 [astro-ph.CO].

[1308] J. Hamann, J. Hasenkamp, A new life for sterile neutrinos: resolving inconsistencies using hot dark matter, J. Cosmol. Astropart. Phys. 10 (2013) 044, arXiv:1308.3255 [astro-ph.CO].

[1309] P.F. de Salas, D.V. Forero, S. Garciazo, P. Martínez-Miravé, O. Mena, C.A. Ternes, M. Tórtola, J.W.F. Valle, 2020 global reassessment of the neutrino oscillation picture, JHEP 02 (2021) 071, arXiv:2006.11237 [hep-ph].

[1310] I. Esteban, M.C. Gonzalez-Garcia, M. Maltoni, T. Schwetz, A. Zhou, The fate of hints: updated global analysis of three-flavor neutrino oscillations, JHEP 09 (2020) 178, arXiv:2007.14792 [hep-ph].

[1311] S. Garciazo, O. Mena, T. Schwetz, Quantifying the tension between cosmological and terrestrial constraints on neutrino masses, Phys. Dark Univ. 40 (2023) 101226, arXiv:2302.14159 [hep-ph].

[1312] E. di Valentino, S. Garciazo, O. Mena, Model marginalized constraints on neutrino properties from cosmology, Phys. Rev. D 106 (4) (2022) 043540, arXiv:2207.05167 [astro-ph.CO].

[1313] C.S. Lorenz, L. Funcke, E. Calabrese, S. Hannestad, Time-varying neutrino mass from a supercooled phase transition: current cosmological constraints and impact on the $\Omega_m-\sigma_8$ plane, Phys. Rev. D 99 (2) (2019) 023501, arXiv:1811.01991 [astro-ph.CO].

[1314] M. Escudero, J. Lopez-Pavon, N. Rius, S. Sandner, Relaxing cosmological neutrino mass bounds with unstable neutrinos, JHEP 12 (2020) 119, arXiv:2007.04994 [hep-ph].

[1315] Z. Chacko, A. Dev, P. Du, V. Poulin, Y. Tsai, Determining the neutrino lifetime from cosmology, Phys. Rev. D 103 (4) (2021) 043519, arXiv:2002.08401 [astro-ph.CO].

[1316] Z. Chacko, A. Dev, P. Du, V. Poulin, Y. Tsai, Cosmological Limits on the Neutrino Mass and Lifetime, JHEP 04 (2020) 020, arXiv:1909.05275 [hep-ph].

[1317] G. Franco Abellán, Z. Chacko, A. Dev, P. Du, V. Poulin, Y. Tsai, Improved cosmological constraints on the neutrino mass and lifetime, JHEP 08 (2022) 076, arXiv:2112.13862 [hep-ph].

[1318] C.D. Kreisch, F.-Y. Cyr-Racine, O. Doré, Neutrino puzzle: Anomalies, interactions, and cosmological tensions, Phys. Rev. D 101 (12) (2020) 123505, arXiv:1902.00534 [astro-ph.CO].

[1319] D. Camarena, F.-Y. Cyr-Racine, Strong constraints on a simple self-interacting neutrino cosmology, Phys. Rev. D 111 (2) (2025) 023504, arXiv:2403.05496 [astro-ph.CO].

[1320] I. Esteban, J. Salvado, Long range interactions in cosmology: implications for neutrinos, J. Cosmol. Astropart. Phys. 05 (2021) 036, arXiv:2101.05804 [hep-ph].

[1321] I.M. Oldengott, G. Barenboim, S. Kahlen, J. Salvado, D.J. Schwarz, How to relax the cosmological neutrino mass bound, J. Cosmol. Astropart. Phys. 04 (2019) 049, arXiv:1901.04352 [astro-ph.CO].

[1322] G. Dvali, L. Funcke, Small neutrino masses from gravitational $\theta$-term, Phys. Rev. D 93 (11) (2016) 113002, arXiv:1602.03191 [hep-ph].

[1323] G. Barenboim, H. Sanchis, W.H. Kinney, D. Rios, Bound on thermal y distortion of the cosmic neutrino background, Phys. Rev. D 110 (12) (2024) 123535, arXiv:2407.18102 [astro-ph.CO].

[1324] N. Craig, D. Green, J. Meyers, S. Rajendran, No vs is good news, JHEP 09 (2024) 097, arXiv:2405.00836 [astro-ph.CO].

[1325] A. Yadav, S. Kumar, C. Kibris, O. Akarsu, $\Lambda$CDM cosmology: alleviating major cosmological tensions by predicting standard neutrino properties, J. Cosmol. Astropart. Phys. 01 (2025) 042, arXiv:2406.18496 [astro-ph.CO].

[1326] KATRIN Collaboration, M. Aker, et al., Direct neutrino-mass measurement based on 259 days of KATRIN data, Science 388 (6743) (2025) adq9592, arXiv:2406.13516 [nucl-ex].

[1327] G. Drexlin, V. Hannen, S. Mertens, C. Weinheimer, Current direct neutrino mass experiments, Adv. High Energy Phys. 2013 (2013) 293986, arXiv:1307.0101 [physics.ins-det].

[1328] P.K. Aluri, et al., Is the observable Universe consistent with the cosmological principle? Cl. Quant. Grav. 40 (9) (2023) 094001, arXiv:2207.05765 [astro-ph.CO].

[1329] G. Ellis, R. Maartens, M. MacCallum, Relativistic Cosmology, Cambridge University Press, 2012, https://books.google.it/books?id=igkhAWAAQBAJ.

[1330] D.J. Schwarz, C.J. Copi, D. Huterer, G.D. Starkman, CMB Anomalies after Planck, Cl. Quant. Grav. 33 (18) (2016) 184001, arXiv:1510.07929 [astro-ph.CO].

[1331] P. Fleury, C. Clarkson, R. Maartens, How does the cosmic large-scale structure bias the Hubble diagram? J. Cosmol. Astropart. Phys. 03 (2017) 062, arXiv:1612.03726 [astro-ph.CO].

[1332] J. Jones, C.J. Copi, G.D. Starkman, Y. Akrami, The Universe is not statistically isotropic, 2023, arXiv:2310.12859 [astro-ph.CO].

[1333] P. Fosalba, E. Gaztanaga, Explaining cosmological anisotropy: evidence for causal horizons from CMB data, Mon. Not. R. Astron. Soc. 504 (4) (2021) 5840-5862, arXiv:2011.00910 [astro-ph.CO].

[1334] S. Yeung, M.-C. Chu, Directional variations of cosmological parameters from the Planck CMB data, Phys. Rev. D 105 (8) (2022) 083508, arXiv:2201.03799 [astro-ph.CO].

[1335] Euclid Collaboration, A. Kashlinsky, et al., Euclid preparation - XLVI. The near-infrared background dipole experiment with Euclid, Astron. Astrophys. 689 (2024) A294, arXiv:2401.17945 [astro-ph.CO].

[1336] M. Plionis, Large-scale optical dipole anisotropy, Mon. Not. R. Astro. Soc. 234 (1988) 401-416.

[1337] M. Plionis, R. Valdarnini, Evidence for large-scale structure on scales ≈300 h⁻¹Mpc, Mon. Not. R. Astro. Soc. 249 (1991) 46.

[1338] R. Scaramella, G. Vettolani, G. Zamorani, The distribution of clusters of galaxies within 300 MPC H-1 and the crossover to an isotropic and homogeneous universe, Astrophys. J. Lett. 376 (1991) L1.

[1339] E. Branchini, M. Plionis, Reconstructing positions and peculiar velocities of galaxy clusters within 20000 km/sec: I: the cluster 3-D dipole, Astrophys. J. 460 (1996) 569, arXiv:astro-ph/9501028.
[1340] M. Plionis, E. Kolokotronis, The x-ray cluster dipole, Astrophys. J. 500 (1998) 1, arXiv:astro-ph/9707147.

[1341] M. Rowan-Robinson, et al., The IRAS PSCz dipole, Mon. Not. R. Astron. Soc. 314 (2000) 375, arXiv:astro-ph/9912223.

[1342] D.D. Kocevksi, H. Ebeling, B. Tully, C.R. Mullis, The dipole anisotropy of the first all-sky X-ray cluster sample, in: A.P. Fairall, P.A. Woudt (Eds.), Nearby Large-Scale Structures and the Zone of Avoidance, in: Astronomical Society of the Pacific Conference Series, vol. 329, 2005, p. 89.

[1343] Y. Hoffman, D. Pomarede, R. Brent Tully, H. Courtois, The dipole re-
peller, 2017, http://dx.doi.org/10.1038/s41550-016-0036, arXiv:1702.02483
[astro-ph.CO].

[1344] M. Lopes, A. Bernui, C. Franco, F. Avila, Bulk flow motion detection in the local universe with pantheon+ type ia supernovae, Astrophys. J. 967 (1) (2024) 47, arXiv:2405.11077 [astro-ph.CO].

[1345] J.A.R. Cembranos, A.L. Maroto, H. Villarrubia-Rojo, Non-comoving cosmology, J. Cosmol. Astropart. Phys. 06 (2019) 041, arXiv:1903.11009 [astro-ph.CO].

[1346] C.G. Tsagas, M.I. Kazantzoglou, K. Asvesta, The deceleration parameter in "tilted" Friedmann universes: Newtonian vs relativistic treatment, Astrophys. Space Sci. 366 (9) (2021) 90, arXiv:2105.09267 [gr-qc].

[1347] C.G. Tsagas, The deceleration parameter in 'tilted' universes: generalising the Friedmann background, Eur. Phys. J. C 82 (6) (2022) 521, arXiv:2112.04313 [gr-qc].

[1348] K. Asvesta, L. Kazantzidis, L. Perivolaropoulos, C.G. Tsagas, Observational constraints on the deceleration parameter in a tilted universe, Mon. Not. R. Astron. Soc. 513 (2) (2022) 2394-2406, arXiv:2202.00962 [astro-ph.CO].

[1349] J. Santiago, C.G. Tsagas, Timelike vs null deceleration parameter in tilted Friedmann universes, 2022, arXiv:2203.01126 [gr-qc].

[1350] A.R. King, G.F.R. Ellis, Tilted homogeneous cosmological models, Comm. Math. Phys. 31 (1973) 209-242.

[1351] C.G. Tsagas, A. Challinor, R. Maartens, Relativistic cosmology and large-scale structure, Phys. Rep. 465 (2008) 61-147, arXiv:0705.4397 [astro-ph].

[1352] C. Krishnan, R. Mondol, M.M. Sheikh-Jabbari, Dipole cosmology: the Coper-
nican paradigm beyond FLRW, J. Cosmol. Astropart. Phys. 07 (2023) 020,
arXiv:2209.14918 [astro-ph.CO].

[1353] C. Krishnan, R. Mondol, M.M. Sheikh-Jabbari, A tilt instability in the cosmological principle, Eur. Phys. J. C 83 (9) (2023) 874, arXiv:2211.08093 [astro-ph.CO].

[1354] E. Ebrahimian, C. Krishnan, R. Mondol, M.M. Sheikh-Jabbari, Towards a realistic dipole cosmology: the dipole ΛCDM model, Cl. Quant. Grav. 41 (14) (2024) 145007, arXiv:2305.16177 [astro-ph.CO].

[1355] A. Allahyari, E. Ebrahimian, R. Mondol, M.M. Sheikh-Jabbari, Big Bang in dipole cosmology, Eur. Phys. J. C 85 (2) (2025) 119, arXiv:2307.15791 [astro-ph.CO].

[1356] C.G. Tsagas, M.I. Kazantzoglou, Deceleration parameter in tilted Friedmann universes, Phys. Rev. D 92 (4) (2015) 043515, arXiv:1507.04266 [gr-qc].

[1357] A. Heinesen, T. Buchert, Solving the curvature and Hubble parameter inconsistencies through structure formation-induced curvature, Cl. Quant. Grav. 37 (16) (2020) 164001, arXiv:2002.10831 [gr-qc]; Class. Quant. Grav. 37 (2020) 229601 (erratum).

[1358] A. Heinesen, Multipole decomposition of the general luminosity distance 'Hubble law' - a new framework for observational cosmology, J. Cosmol. Astropart. Phys. 05 (2021) 008, arXiv:2010.06534 [astro-ph.CO].

[1359] A. Heinesen, H.J. Macpherson, A prediction for anisotropies in the nearby Hubble flow, J. Cosmol. Astropart. Phys. 03 (03) (2022) 057, arXiv:2111.14423 [astro-ph.CO].

[1360] C. Guandalin, J. Piat, C. Clarkson, R. Maartens, Theoretical systematics in testing the cosmological principle with the kinematic quasar dipole, Astrophys. J. 953 (2) (2023) 144, arXiv:2212.04925 [astro-ph.CO].

[1361] R. Maartens, J. Santiago, C. Clarkson, B. Kalbouneh, C. Marinoni, Covariant cosmography: the observer-dependence of the Hubble parameter, J. Cosmol. Astropart. Phys. 09 (2024) 070, arXiv:2312.09875 [astro-ph.CO].

[1362] G.F.R. Ellis, J.E. Baldwin, On the expected anisotropy of radio source counts, Mon. Not. R. Astr. Soc. 206 (1984) 377-381.

[1363] L. Perivolaropoulos, F. Skara, Challenges for ΛCDM: an update, New Astron. Rev. 95 (2022) 101659, arXiv:2105.05208 [astro-ph.CO].

[1364] O. Akarsu, E. Di Valentino, S. Kumar, M. Ozyigit, S. Sharma, Testing spatial curvature and anisotropic expansion on top of the ΛCDM model, Phys. Dark Univ. 39 (2023) 101162, arXiv:2112.07807 [astro-ph.CO].

[1365] A. Mariano, L. Perivolaropoulos, CMB Maximum temperature asymmetry Axis: Alignment with other cosmic asymmetries, Phys. Rev. D 87 (4) (2013) 043511, arXiv:1211.5915 [astro-ph.CO].

[1366] J.K. Webb, J.A. King, M.T. Murphy, V.V. Flambaum, R.F. Carswell, M.B. Bainbridge, Indications of a spatial variation of the fine structure constant, Phys. Rev. Lett. 107 (2011) 191101, arXiv:1008.3907 [astro-ph.CO].

[1367] M.R. Wilczynska, et al., Four direct measurements of the fine-structure constant 13 billion years ago, Sci. Adv. 6 (17) (2020) eaay9672, arXiv:2003.07627 [astro-ph.CO].

[1368] R. Mohayaee, M. Rameez, S. Sarkar, Do supernovae indicate an accelerating universe? Eur. Phys. J. ST 230 (9) (2021) 2067-2076, arXiv:2106.03119 [astro-ph.CO].

[1369] J. Colin, R. Mohayaee, M. Rameez, S. Sarkar, Evidence for anisotropy of cosmic acceleration, Astron. Astrophys. 631 (2019) L13, arXiv:1808.04597 [astro-ph.CO].

[1370] R. Mohayaee, M. Rameez, S. Sarkar, Cosmological inference from within the peculiar local universe, Universe 10 (5) (2024) 209, arXiv:2003.10420 [astro-ph.CO].

[1371] A.K. Singal, Peculiar motion of Solar system from the Hubble diagram of supernovae Ia and its implications for cosmology, Mon. Not. R. Astron. Soc. 515 (4) (2022) 5969-5980, arXiv:2106.11968 [astro-ph.CO].

[1372] N. Horstmann, Y. Pietschke, D.J. Schwarz, Inference of the cosmic rest-frame from supernovae Ia, Astron. Astrophys. 668 (2022) A34, arXiv:2111.03055 [astro-ph.CO].

[1373] J.A. Cowell, S. Dhawan, H.J. Macpherson, Potential signature of a quadrupolar hubble expansion in Pantheon+supernovae, Mon. Not. R. Astron. Soc. 526 (1) (2023) 1482-1494, arXiv:2212.13569 [astro-ph.CO].

[1374] R. Mc Conville, E.O. Colgáin, Anisotropic distance ladder in Pantheon+su-
pernovae, Phys. Rev. D 108 (12) (2023) 123533, arXiv:2304.02718
[astro-ph.CO].

[1375] U. Andrade, C.A.P. Bengaly, J.S. Alcaniz, B. Santos, Isotropy of low redshift type Ia Supernova: A Bayesian analysis, Phys. Rev. D 97 (8) (2018) 083518, arXiv:1711.10536 [astro-ph.CO].

[1376] C.A.P. Bengaly, Evidence for cosmic acceleration with next-generation surveys: A model-independent approach, Mon. Not. R. Astron. Soc. 499 (1) (2020) L6-L10, arXiv:1912.05528 [astro-ph.CO].

[1377] W. Rahman, R. Trotta, S.S. Boruah, M.J. Hudson, D.A. van Dyk, New constraints on anisotropic expansion from supernovae Type Ia, Mon. Not. R. Astron. Soc. 514 (1) (2022) 139-163, arXiv:2108.12497 [astro-ph.CO].

[1378] A. Salehi, H. Farajollahi, M. Motahari, P. Pashamokhtari, M. Yarahmadi, S. Fathi, Are Type Ia supernova powerful tool to detect anisotropic expansion of the Universe? Eur. Phys. J. C 80 (8) (2020) 753.

[1379] J.P. Hu, Y.Y. Wang, F.Y. Wang, Testing cosmic anisotropy with Pantheon sample and quasars at high redshifts, Astron. Astrophys. 643 (2020) A93, arXiv:2008.12439 [astro-ph.CO].

[1380] N. Dhawan, A. Borderies, H.J. Macpherson, A. Heinesen, The quadrupole in the local Hubble parameter: first constraints using Type Ia supernova data and forecasts for future surveys, Mon. Not. R. Astron. Soc. 519 (4) (2023) 4841-4855, arXiv:2205.12692 [astro-ph.CO].

[1381] D. Sapone, S. Nesseris, C.A.P. Bengaly, Is there any measurable redshift dependence on the SN Ia absolute magnitude? Phys. Dark Univ. 32 (2021) 100814, arXiv:2006.05461 [astro-ph.CO].

[1382] C.A.P. Bengaly, J.S. Alcaniz, C. Pigozzo, Testing the isotropy of cosmic acceleration with the Pantheon+ and SHOES datasets: A cosmographic analysis, Phys. Rev. D 109 (12) (2024) 123533, arXiv:2402.17741 [astro-ph.CO].

[1383] I. Antoniou, L. Perivolaropoulos, Searching for a cosmological preferred axis: union2 data analysis and comparison with other probes, J. Cosmol. Astropart. Phys. 12 (2010) 012, arXiv:1007.4347 [astro-ph.CO].

[1384] A. Mariano, L. Perivolaropoulos, Is there correlation between fine structure and dark energy cosmic dipoles? Phys. Rev. D 86 (2012) 083517, arXiv:1206.4055 [astro-ph.CO].

[1385] C. Krishnan, R. Mohayaee, E.O. Colgáin, M.M. Sheikh-Jabbari, L. Yin, Hints of FLRW breakdown from supernovae, Phys. Rev. D 105 (6) (2022) 063514, arXiv:2106.02532 [astro-ph.CO].

[1386] B. Bahr-Kalus, D.J. Schwarz, M. Seikel, A. Wiegand, Constraints on anisotropic cosmic expansion from supernovae, Astron. Astrophys. 553 (2013) A56, arXiv: 1212.3691 [astro-ph.CO].

[1387] D. Zhao, Y. Zhou, Z. Chang, Anisotropy of the Universe via the Pantheon supernovae sample revisited, Mon. Not. R. Astron. Soc. 486 (4) (2019) 5679-5689, arXiv:1903.12401 [astro-ph.CO].

[1388] B. Kalbouneh, C. Marinoni, J. Bel, Multipole expansion of the local expansion rate, Phys. Rev. D 107 (2) (2023) 023507, arXiv:2210.11333 [astro-ph.CO].

[1389] L. Tang, H.-N. Lin, L. Liu, X. Li, Consistency of Pantheon+ supernovae with a large-scale isotropic universe*, Chin. Phys. C 47 (12) (2023) 125101, arXiv:2309.11320 [astro-ph.CO].

[1390] J.P. Hu, Y.Y. Wang, J. Hu, F.Y. Wang, Testing the cosmological principle with the Pantheon+ sample and the region-fitting method, Astron. Astrophys. 681 (2024) A88, arXiv:2310.11727 [astro-ph.CO].

[1391] F. Sorrenti, R. Durrer, M. Kunz, The dipole of the Pantheon+SHOES data, J. Cosmol. Astropart. Phys. 11 (2023) 054, arXiv:2212.10328 [astro-ph.CO].

[1392] L. Perivolaropoulos, Isotropy properties of the absolute luminosity magnitudes of SNIa in the Pantheon+ and SHOES samples, Phys. Rev. D 108 (6) (2023) 063509, arXiv:2305.12819 [astro-ph.CO].

[1393] G. Risaliti, E. Lusso, A hubble diagram for quasars, Astrophys. J. 815 (2015) 33, arXiv:1505.07118 [astro-ph.CO].

[1394] G. Risaliti, E. Lusso, Cosmological constraints from the Hubble diagram of quasars at high redshifts, Nat. Astron. 3 (3) (2019) 272-277, arXiv:1811.02590 [astro-ph.CO].

[1395] N. Khadka, B. Ratra, Do quasar X-ray and UV flux measurements provide a useful test of cosmological models? Mon. Not. R. Astron. Soc. 510 (2) (2022) 2753-2772, arXiv:2107.07600 [astro-ph.CO].
[1396] N. Khadka, M. Zajaˇ cek, R. Prince, S. Panda, B. Czerny, M.L. Martínez-Aldama, V.K. Jaiswal, B. Ratra, Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius–luminosity relation luminosity distances, Mon. Not. R. Astron. Soc. 522 (1) (2023) 1247–1264, arXiv:2212.10483 [astro-ph.CO].

[1397] E.O. Colgáin, M.M. Sheikh-Jabbari, L. Yin, Do high redshift QSOs and GRBs corroborate JWST? 2024, arXiv:2405.19953 [astro-ph.CO].

[1398] N.J. Secrest, S. von Hausegger, M. Rameez, R. Mohayae, S. Sarkar, J. Colin, A test of the cosmological principle with quasars, Astrophys. J. Lett. 908 (2) (2021) L51, arXiv:2009.14826 [astro-ph.CO].

[1399] A.K. Singal, Peculiar motion of the solar system derived from a dipole anisotropy in the redshift distribution of distant quasars, Mon. Not. R. Astron. Soc. 488 (1) (2019) L104–L108, arXiv:1405.4796 [astro-ph.CO].

[1400] L. Dam, G.F. Lewis, B.J. Brewer, Testing the cosmological principle with CatWISE quasars: a bayesian analysis of the number-count dipole, Mon. Not. R. Astron. Soc. 525 (1) (2023) 231–245, arXiv:2212.07733 [astro-ph.CO].

[1401] R. Kothari, M. Panwar, G. Singh, P. Tiwari, P. Jain, A study of dipolar signal in distant Quasars with various observables, Eur. Phys. J. C 84 (1) (2024) 75, arXiv:2208.14397 [astro-ph.CO].

[1402] A. Abghari, E.F. Bunn, L.T. Hergt, B. Li, D. Scott, R.M. Sullivan, D. Wei, Reassessment of the dipole in the distribution of quasars on the sky, J. Cosmol. Astropart. Phys. 11 (2024) 067, arXiv:2405.09762 [astro-ph.CO].

[1403] O. Luongo, M. Muccino, E.O. Colgáin, M.M. Sheikh-Jabbari, L. Yin, Larger H0 values in the CMB dipole direction, Phys. Rev. D 105 (10) (2022) 103510, arXiv:2108.13228 [astro-ph.CO].

[1404] C. Blake, J. Wall, Detection of the velocity dipole in the radio galaxies of the nrao vla sky survey, Nature 416 (2002) 150–152, arXiv:astro-ph/0203385.

[1405] J. Colin, R. Mohayae, M. Rameez, S. Sarkar, High redshift radio galaxies and divergence from the CMB dipole, Mon. Not. R. Astron. Soc. 471 (1) (2017) 1045–1055, arXiv:1703.09376 [astro-ph.CO].

[1406] A.K. Singal, Large peculiar motion of the solar system from the dipole anisotropy in sky brightness due to distant radio sources, Astrophys. J. Lett. 742 (2011) L23, arXiv:1110.6260 [astro-ph.CO].

[1407] M. Rubart, D.J. Schwarz, Cosmic radio dipole from NVSS and WENSS, Astron. Astrophys. 555 (2013) A117, arXiv:1301.5559 [astro-ph.CO].

[1408] C.A.P. Bengaly, T.M. Siewert, D.J. Schwarz, R. Maartens, Testing the standard model of cosmology with the SKA: the cosmic radio dipole, Mon. Not. R. Astron. Soc. 486 (1) (2019) 1350–1357, arXiv:1810.04960 [astro-ph.CO].

[1409] A.K. Singal, Large disparity in cosmic reference frames determined from the sky distributions of radio sources and the microwave background radiation, Phys. Rev. D 100 (6) (2019) 063501, arXiv:1904.11362 [physics.gen-ph].

[1410] T.M. Siewert, M. Schmidt-Rubart, D.J. Schwarz, Cosmic radio dipole: Estimators and frequency dependence, Astron. Astrophys. 653 (2021) A9, arXiv:2010.08366 [astro-ph.CO].

[1411] N.J. Secrest, S. von Hausegger, M. Rameez, R. Mohayae, S. Sarkar, A challenge to the standard cosmological model, Astrophys. J. Lett. 937 (2) (2022) L31, arXiv:2206.05624 [astro-ph.CO].

[1412] J.D. Wagenveld, H.-R. Klöckner, D.J. Schwarz, The cosmic radio dipole: Bayesian estimators on new and old radio surveys, Astron. Astrophys. 675 (2023) A72, arXiv:2305.15335 [astro-ph.CO].

[1413] A.K. Singal, Resolution of the incongruency of dipole asymmetries within various large radio surveys – implications for the Cosmological Principle, Mon. Not. R. Astron. Soc. 528 (4) (2024) 5679–5691, arXiv:2312.12785 [astro-ph.CO].

[1414] C. Gibelyou, D. Huterer, Dipoles in the sky, Mon. Not. R. Astron. Soc. 427 (2012) 1994–2021, arXiv:1205.6476 [astro-ph.CO].

[1415] C.A.P. Bengaly, R. Maartens, N. Randriamiarinarivo, A. Baloyi, Testing the cosmological principle in the radio sky, J. Cosmol. Astropart. Phys. 09 (2019) 025, arXiv:1905.12378 [astro-ph.CO].

[1416] C. Murray, The effects of lensing by local structures on the dipole of radio source counts, Mon. Not. R. Astron. Soc. 510 (2) (2022) 3098–3101, arXiv:2112.06689 [astro-ph.CO].

[1417] Y.-T. Cheng, T.-C. Chang, A. Lidz, Is the radio source dipole from NVSS consistent with the cosmic microwave background and ΛCDM? Astrophys. J. 965 (1) (2024) 32, arXiv:2309.02490 [astro-ph.CO].

[1418] P. da Silveira Ferreira, V. Marra, Tomographic redshift dipole: testing the cosmological principle, J. Cosmol. Astropart. Phys. 09 (2024) 077, arXiv:2403.14580 [astro-ph.CO].

[1419] O.T. Oayda, V. Mittal, G.F. Lewis, T. Murphy, A Bayesian approach to the cosmic dipole in radio galaxy surveys: joint analysis of NVSS & RACS, Mon. Not. R. Astron. Soc. 531 (4) (2024) 4545–4559, arXiv:2406.01871 [astro-ph.CO].

[1420] B.E. Schaefer, The hubble diagram to redshift >6 from 69 gamma-ray bursts, Astrophys. J. 660 (2007) 16–46, arXiv:astro-ph/0612285.

[1421] S. Basilakos, L. Perivolaropoulos, Testing GRBs as standard candles, Mon. Not. R. Astron. Soc. 391 (2008) 411–419, arXiv:0805.0875 [astro-ph].

[1422] N. Liang, W.K. Xiao, Y. Liu, S.N. Zhang, A cosmology independent calibration of gamma-ray burst luminosity relations and the hubble diagram, Astrophys. J. 685 (2008) 354, arXiv:0802.4262 [astro-ph].

[1423] S. Cao, N. Khadka, B. Ratra, Standardizing Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters, Mon. Not. R. Astron. Soc. 510 (2) (2022) 2928–2947, arXiv:2110.14840 [astro-ph.CO].

[1424] R.B. Tully, et al., Cosmicflows-4, Astrophys. J. 944 (1) (2023) 94, arXiv:2209.11238 [astro-ph.CO].

[1425] Y. Hoffman, A. Valade, N.I. Libeskind, J.G. Sorce, R.B. Tully, S. Pfeifer, S. Gottlöber, D. Pomarède, The large-scale velocity field from the Cosmicflows-4 data, Mon. Not. R. Astron. Soc. 527 (2) (2024) 3788–3805, arXiv:2311.01340 [astro-ph.CO].

[1426] R. Watkins, T. Allen, C.J. Bradford, A. Ramon, A. Walker, H.A. Feldman, R. Cionitti, Y. Al-Shorman, E. Kourkchi, R.B. Tully, Analysing the large-scale bulk flow using cosmicflows4: increasing tension with the standard cosmological model, Mon. Not. R. Astron. Soc. 524 (2) (2023) 1885–1892, arXiv:2302.02028 [astro-ph.CO].

[1427] A.M. Whitford, C. Howlett, T.M. Davis, Evaluating bulk flow estimators for CosmicFlows-4 measurements, Mon. Not. R. Astron. Soc. 526 (2) (2023) 3051–3071, arXiv:2306.11269 [astro-ph.CO].

[1428] S. Peery, R. Watkins, H.A. Feldman, Easily interpretable bulk flows: continuing tension with the standard cosmological model, Mon. Not. R. Astron. Soc. 481 (1) (2018) 1368–1375, arXiv:1808.07772 [astro-ph.CO].

[1429] A. Kashlinsky, F. Atrio-Barandela, D. Kocevski, H. Ebeling, A measurement of large-scale peculiar velocities of clusters of galaxies: results and cosmological implications, Astrophys. J. Lett. 686 (2009) L49–L52, arXiv:0809.3734 [astro-ph].

[1430] F. Atrio-Barandela, A. Kashlinsky, H. Ebeling, D.J. Fixsen, D. Kocevski, Probing the dark flow signal in Wmap 9-year and planck cosmic microwave background maps, Astrophys. J. 810 (2) (2015) 143, arXiv:1411.4180 [astro-ph.CO].

[1431] A. Kashlinsky, F. Atrio-Barandela, H. Ebeling, A. Edge, D. Kocevski, A new measurement of the bulk flow of X-ray luminous clusters of galaxies, Astrophys. J. Lett. 712 (2010) L81–L85, arXiv:0910.4958 [astro-ph.CO].

[1432] A. Kashlinsky, F. Atrio-Barandela, H. Ebeling, Measuring the dark flow with public X-ray cluster data, Astrophys. J. 732 (2011) 1, arXiv:1012.3214 [astro-ph.CO].

[1433] F. Atrio-Barandela, On the statistical significance of the bulk flow measured by the PLANCK satellite, Astron. Astrophys. 557 (2013) A116, arXiv:1303.6614 [astro-ph.CO].

[1434] Planck Collaboration, N. Aghanim, et al., Planck 2018 results. I. Overview and the cosmological legacy of Planck, Astron. Astrophys. 641 (2020) A1, arXiv:1807.06205 [astro-ph.CO].

[1435] J. Grande, L. Perivolaropoulos, Generalized LTB model with inhomogeneous isotropic dark energy: observational constraints, Phys. Rev. D 84 (2011) 023514, arXiv:1103.4143 [astro-ph.CO].

[1436] H. Alnes, M. Amarzguioui, O. Gron, Can a dust dominated Universe have accelerated expansion? J. Cosmol. Astropart. Phys. 01 (2007) 007, arXiv:astro-ph/0506449.

[1437] L. Ackerman, S.M. Carroll, M.B. Wise, Imprints of a primordial preferred direction on the microwave background, Phys. Rev. D 75 (2007) 083502, arXiv:astro-ph/0701357; Phys. Rev. D 80 (2009) 069901 (erratum).

[1438] R. Aurich, S. Lustig, F. Steiner, CMB anisotropy of the Poincare dodecahedron, Cl. Quant. Grav. 22 (2005) 2061–2083, arXiv:astro-ph/0412569.

[1439] COMPACT Collaboration, Y. Akrami, et al., Promise of future searches for cosmic topology, Phys. Rev. Lett. 132 (17) (2024) 171501, arXiv:2210.11426 [astro-ph.CO].

[1440] J.C. Bueno Sanchez, L. Perivolaropoulos, Topological quintessence, Phys. Rev. D 84 (2011) 123516, arXiv:1110.2587 [astro-ph.CO].

[1441] L. Perivolaropoulos, Topological quintessence: Generalizing Lambda CDM with inhomogeneous dark energy, Romanian J. Phys. 57 (2012) 950–968.

[1442] T. Koivisto, D.F. Mota, Dark energy anisotropic stress and large scale structure formation, Phys. Rev. D 73 (2006) 083502, arXiv:astro-ph/0512135.

[1443] R. Battye, A. Moss, Anisotropic dark energy and CMB anomalies, Phys. Rev. D 80 (2009) 023531, arXiv:0905.3403 [astro-ph.CO].

[1444] J.D. Barrow, Cosmological limits on slightly skew stresses, Phys. Rev. D 55 (1997) 7451–7460, arXiv:gr-qc/9701038.

[1445] J.D. Barrow, P.G. Ferreira, J. Silk, Constraints on a primordial magnetic field, Phys. Rev. Lett. 78 (1997) 3610–3613, arXiv:astro-ph/9701063.

[1446] L. Campanelli, A model of universe anisotropization, Phys. Rev. D 80 (2009) 063006, arXiv:0907.3703 [astro-ph.CO].

[1447] A. Maleknejad, M.M. Sheikh-Jabbari, J. Soda, Gauge fields and inflation, Phys. Rep. 528 (2013) 161–261, arXiv:1212.2921 [hep-th].

[1448] K. Dimopoulos, M. Karciauskas, J.M. Wagstaff, Vector curvaton with varying kinetic function, Phys. Rev. D 81 (2010) 023522, arXiv:0907.1838 [hep-ph].

[1449] M. Karciauskas, K. Dimopoulos, D.H. Lyth, Anisotropic non-Gaussianity from vector field perturbations, Phys. Rev. D 80 (2009) 023509, arXiv:0812.0264 [astro-ph]; Phys. Rev. D 85 (2012) 069905 (erratum).

[1450] C.G. Tsagas, Peculiar motions, accelerated expansion and the cosmological axis, Phys. Rev. D 84 (2011) 063503, arXiv:1107.4045 [astro-ph.CO].

[1451] T. Anton, T. Clifton, Modelling the emergence of cosmic anisotropy from non-linear structures, Cl. Quant. Grav. 40 (14) (2023) 145004, arXiv:2302.05715 [gr-qc].
[1452] E. Pastén, V.H. Cárdenas, Testing $\Lambda$CDM cosmology in a binned universe: Anomalies in the deceleration parameter, Phys. Dark Univ. 40 (2023) 101224, arXiv:2301.10740 [astro-ph.CO].

[1453] C.G. Tsagas, The peculiar Jeans length, Eur. Phys. J. C 81 (8) (2021) 753, arXiv:2103.15884 [gr-qc].

[1454] O. Roldan, A. Notari, M. Quartin, Interpreting the CMB aberration and Doppler measurements: boost or intrinsic dipole? J. Cosmol. Astropart. Phys. 06 (2016) 026, arXiv:1603.02664 [astro-ph.CO].

[1455] S. Yasini, E. Pierpaoli, Beyond the boost: measuring the intrinsic dipole of the cosmic microwave background using the spectral distortions of the monopole and quadrupole, Phys. Rev. Lett. 119 (22) (2017) 221102, arXiv:1610.00015 [astro-ph.CO].

[1456] P.d.S. Ferreira, M. Quartin, First constraints on the intrinsic CMB dipole and our velocity with doppler and aberration, Phys. Rev. Lett. 127 (10) (2021) 101301, arXiv:2011.08385 [astro-ph.CO].

[1457] M.I. Khan, R. Saha, Detection of dipole modulation in CMB temperature anisotropy maps from WMAP and planck using artificial intelligence, Astrophys. J. 947 (2) (2023) 47, arXiv:2212.04438 [astro-ph.CO].

[1458] C.E. Kester, A. Bernui, W.S. Hipólito-Ricaldi, Probing the statistical isotropy of the universe with Planck data of the cosmic microwave background, Astron. Astrophys. 683 (2024) A176, arXiv:2310.02928 [astro-ph.CO].

[1459] J.A. King, J.K. Webb, M.T. Murphy, V.V. Flambaum, R.F. Carswell, M.B. Bainbridge, M.R. Wilczynska, F.E. Koch, Spatial variation in the fine-structure constant – new results from VLT/UVES, Mon. Not. R. Astron. Soc. 422 (2012) 3370–3413, arXiv:1202.4758 [astro-ph.CO].

[1460] D.-C. Qiang, H.-K. Deng, H. Wei, Cosmic anisotropy and fast radio bursts, Cl. Quant. Grav. 37 (18) (2020) 185022, arXiv:1902.03580 [astro-ph.CO].

[1461] H.-N. Lin, Y. Sang, Probing the anisotropic distribution of baryon matter in the Universe using fast radio bursts *, Chin. Phys. C 45 (12) (2021) 125101, arXiv:2111.12934 [astro-ph.CO].

[1462] O.T. Oayda, G.F. Lewis, Testing the cosmological principle: on the time dilation of distant sources, Mon. Not. R. Astron. Soc. 523 (1) (2023) 667–675, arXiv:2305.06771 [astro-ph.CO].

[1463] V. Mittal, O.T. Oayda, G.F. Lewis, The cosmic dipole in the quaia sample of quasars: a Bayesian analysis, Mon. Not. R. Astron. Soc. 527 (3) (2024) 8497–8510, arXiv:2311.14938 [astro-ph.CO]; Mon. Not. Roy. Astron. Soc. 530 (2024) 4763–4764 (erratum).

[1464] F. Iocco, G. Mangano, G. Miele, O. Pisanti, P.D. Serpico, Primordial Nucleosynthesis: from precision cosmology to fundamental physics, Phys. Rep. 472 (2009) 1–76, arXiv:0809.0631 [astro-ph].

[1465] R.H. Cybert, B.D. Fields, K.A. Olive, T.-H. Yeh, Big bang nucleosynthesis: 2015, Rev. Modern Phys. 88 (2016) 015004, arXiv:1505.01076 [astro-ph.CO].

[1466] I. Tanihata, H. Toki, T. Kajino (Eds.), Big bang nucleosynthesis: in: Handbook of Nuclear Physics, Springer Nature Singapore, 2023, pp. 1–21, arXiv:2301.12299 [astro-ph.CO].

[1467] Particle Data Group Collaboration, R.L. Workman, et al., Review of particle physics, PTEP 2022 (2022) 083C01.

[1468] T.-H. Yeh, K.A. Olive, B.D. Fields, The impact of new $d(p,\gamma)$ rates on Big Bang Nucleosynthesis, J. Cosmol. Astropart. Phys. 03 (2021) 046, arXiv:2011.13874 [astro-ph.CO].

[1469] A. Coc, S. Goriely, Y. Xu, M. Saimpert, E. Vangioni, Standard Big-Bang Nucleosynthesis up to CNO with an improved extended nuclear network, Astrophys. J. 744 (2012) 158, arXiv:1107.1117 [astro-ph.CO].

[1470] R. Consiglio, P.F. de Salas, G. Mangano, G. Miele, S. Pastor, O. Pisanti, PArthEnOPE reloaded, Comput. Phys. Comm. 233 (2018) 237–242, arXiv:1712.04378 [astro-ph.CO].

[1471] C. Pitrou, A. Coc, J.-P. Uzan, E. Vangioni, A new tension in the cosmological model from primordial deuterium? Mon. Not. R. Astron. Soc. 502 (2) (2021) 2474–2481, arXiv:2011.11320 [astro-ph.CO].

[1472] V. Singh, D. Bhowmick, D.N. Basu, Re-examining the Lithium abundance problem in Big-Bang nucleosynthesis, Astropart. Phys. 162 (2024) 102995, arXiv:2304.08032 [nucl-th].

[1473] S. Gariazzo, P. F. de Salas, O. Pisanti, R. Consiglio, PArthEnOPE revolutions, Comput. Phys. Comm. 271 (2022) 108205, arXiv:2103.05027 [astro-ph.IM].

[1474] L. Sbordone, et al., The metal-poor end of the Spite plateau: 1: Stellar parameters, metallicities and lithium abundances, Astron. Astrophys. 522 (2010) A26, arXiv:1003.4510 [astro-ph.GA].

[1475] J.C. Howk, N. Lehner, B.D. Fields, G.J. Mathews, The detection of interstellar lithium in a low-metallicity galaxy, Nature 489 (2012) 121, arXiv:1207.3081 [astro-ph.CO].

[1476] L. Izzo, P. Molaro, G. Cescutti, E. Aydi, P. Selvelli, E. Harvey, A. Agnello, P. Bonifacio, M. Della Valle, E. Guido, M. Hernanz, Detection of $^7$Be II in the small magellanic cloud, Mon. Not. R. Astro. Soc. 510 (4) (2022) 5302–5314, arXiv:2112.11859 [astro-ph.SR].

[1477] B.D. Fields, The primordial lithium problem, Ann. Rev. Nucl. Part. Sci. 61 (2011) 47–68, arXiv:1203.3551 [astro-ph.CO].

[1478] F. Spite, M. Spite, Abundance of lithium in unevolved halo stars and old disk stars: Interpretation and consequences, Astron. Astrophys. 115 (1982) 357–366.

[1479] R. Rebolo, P. Molaro, J.E. Beckman, Lithium abundances in metal-deficient dwarfs, Astron. Astrophys. 192 (1988) 192–205.

[1480] F. Matteucci, M. Molero, D.S. Aguado, D. Romano, The evolution of Lithium: implications of a universal Spite plateau, Mon. Not. R. Astro. Soc. 505 (1) (2021) 200–206, arXiv:2104.11504 [astro-ph.GA].

[1481] T. Makki, M.E. Eid, G. Mathews, New insight concerning primordial lithium production, 2024, arXiv:2402.17871 [astro-ph.CO].

[1482] X. Fu, A. Bressan, P. Molaro, P. Marigo, Lithium evolution in metal-poor stars: from pre-main sequence to the Spite plateau, Mon. Not. R. Astro. Soc. 452 (3) (2015) 3256–3265, arXiv:1506.05993 [astro-ph.SR].

[1483] B.D. Fields, K.A. Olive, Implications of the non-observation of $^6$Li in halo stars for the primordial $^7$Li problem, J. Cosmol. Astropart. Phys. 10 (2022) 078, arXiv:2204.03167 [astro-ph.GA].

[1484] V.V. Smith, D.L. Lambert, P.E. Nissen, The 6Li/7Li ratio in the metal-poor halo dwarfs HD 19445 and HD 84937, Astrophys. J. 408 (1993) 262–276.

[1485] L.M. Hobbs, J.A. Thorburn, Lithium isotope ratios in six halo stars, Astrophys. J. Lett. 428 (1994) L25.

[1486] L.M. Hobbs, J.A. Thorburn, Lithium isotope ratios in halo stars. II, Astrophys. J. 491 (2) (1997) 772–788.

[1487] V.V. Smith, D.L. Lambert, P.E. Nissen, Isotopic lithium abundances in nine halo stars, Astrophys. J. 506 (1) (1998) 405–423.

[1488] L.M. Hobbs, J.A. Thorburn, L.M. Rebull, Lithium isotope ratios in halo stars. III, Astrophys. J. 523 (2) (1999) 797–804.

[1489] R. Cayrel, M. Spite, F. Spite, E. Vangioni-Flam, M. Casse, J.A.R. Cayrel, J. Audouze, New high s/n observations of the li-6/li-7 blend in hd 84937 and two other metal-poor stars, Astron. Astrophys. 343 (1999) 923, arXiv:astro-ph/9901205.

[1490] M. Asplund, D.L. Lambert, P.E. Nissen, F. Primas, V.V. Smith, Lithium isotopic abundances in metal-poor halo stars, Astrophys. J. 644 (2006) 229–259, arXiv:astro-ph/0510636.

[1491] M. Steffen, R. Cayrel, P. Bonifacio, H.G. Ludwig, E. Caffau, 6Li in metal-poor halo stars: real or spurious? IAU Symp. 265 (2010) 23, arXiv:0910.5917 [astro-ph.SR].

[1492] A.E.G. Perez, W. Aoki, S. Inoue, S.G. Ryan, T.K. Suzuki, M. Chiba, 6Li/7Li estimates for metal-poor stars, Astron. Astrophys. 504 (2009) 213, arXiv:0909.5163 [astro-ph.SR].

[1493] K. Lind, J. Melendez, M. Asplund, R. Collet, Z. Magic, The lithium isotopic ratio in very metal-poor stars, Astron. Astrophys. 554 (2013) A96, arXiv:1305.6564 [astro-ph.SR].

[1494] E.X. Wang, T. Nordlander, M. Asplund, K. Lind, Y. Zhou, H. Reggiani, Non-detection of 6Li in Spite plateau stars with ESPRESSO, Mon. Not. R. Astron. Soc. 509 (1) (2021) 1521–1535, arXiv:2110.03822.

[1495] A. Korn, The ups and downs of inferred cosmological lithium, EPJ Web Conf. 297 (2024) 01007, arXiv:2406.09974 [astro-ph.SR].

[1496] GALAH Collaboration, X. Gao, et al., The GALAH Survey: A new constraint on cosmological lithium and Galactic lithium evolution from warm dwarf stars, Mon. Not. R. Astron. Soc. 497 (1) (2020) L30–L34, arXiv:2006.05173 [astro-ph.SR].

[1497] K.A. Olive, P. Petitjean, E. Vangioni, J. Silk, Higher D or Li: probes of physics beyond the standard model, Mon. Not. R. Astron. Soc. 426 (2012) 1427, arXiv:1203.5701 [astro-ph.CO].

[1498] A. Coc, M. Pospelov, J.-P. Uzan, E. Vangioni, Modified big bang nucleosynthesis with nonstandard neutron sources, Phys. Rev. D 90 (8) (2014) 085018, arXiv:1405.1718 [hep-ph].

[1499] K. Jedamzik, Neutralinos and Big Bang nucleosynthesis, Phys. Rev. D 70 (2004) 083510, arXiv:astro-ph/0405583.

[1500] K. Jedamzik, Did something decay, evaporate, or annihilate during Big Bang nucleosynthesis? Phys. Rev. D 70 (2004) 063524, arXiv:astro-ph/0402344.

[1501] A. Goudelis, M. Pospelov, J. Pradler, Light particle solution to the cosmic lithium problem, Phys. Rev. Lett. 116 (21) (2016) 211303, arXiv:1510.08858 [hep-ph].

[1502] S.Q. Hou, J.J. He, A. Parikh, D. Kahl, C.A. Bertulani, T. Kajino, G.J. Mathews, G. Zhao, Non-extensive statistics to the cosmological lithium problem, Astrophys. J. 834 (2) (2017) 165, arXiv:1701.04149 [astro-ph.CO].

[1503] R. Nakamura, M.-a. Hasahimoto, R. Ichimasa, K. Arai, Big-Bang nucleosynthesis: Constraints on nuclear reaction rates, neutrino degeneracy, inhomogeneous and Brans-Dicke models, Int. J. Mod. Phys. E 26 (08) (2017) 1741003, arXiv:1710.08153 [astro-ph.CO].

[1504] D.G. Yamazaki, M. Kusakabe, T. Kajino, G.J. Mathews, M.-K. Cheoun, The new hybrid BBN model with the photon cooling, X particle, and the primordial magnetic field, Int. J. Mod. Phys. E 26 (08) (2017) 1741006.

[1505] T.R. Makki, M.F. El Eid, G.J. Mathews, Impact of neutrino properties and dark matter on the primordial lithium production, Int. J. Mod. Phys. E 28 (08) (2019) 1950065, arXiv:1901.03726 [astro-ph.CO].

[1506] T.R. Makki, M.F. El Eid, G.J. Mathews, A critical analysis of the Big Bang Nucleosynthesis, Modern Phys. Lett. A 34 (24) (2019) 1950194.

[1507] A.-K. Burns, V. Keus, M. Sher, T.M.P. Tait, Constraints on variation of the weak scale from big bang nucleosynthesis, Phys. Rev. D 109 (12) (2024) 123506, arXiv:2402.08626 [hep-ph].

[1508] G.-y. Huang, W. Rodejohann, Solving the Hubble tension without spoiling Big Bang Nucleosynthesis, Phys. Rev. D 103 (2021) 123007, arXiv:2102.04280 [hep-ph].
[1509] F.F. Deppisch, L. Graf, W. Rodejohann, X.-J. Xu, Neutrino self-interactions and double beta decay, Phys. Rev. D 102 (5) (2020) 051701, [arXiv:2004.11919 [hep-ph]].

[1510] G.J. Mathews, A. Kedia, N. Sasankan, M. Kusakabe, Y. Luo, T. Kajino, D. Yamazaki, T. Makki, M.E. Eid, Cosmological solutions to the lithium problem, JPS Conf. Proc. 31 (2020) 011033, [arXiv:1909.01245 [astro-ph.CO]].

[1511] T.M. Bania, R.T. Rood, D.S. Balser, The cosmological density of baryons from observations of 3He+ in the Milky Way, Nature 415 (2002) 54–57.

[1512] E. Aver, D.A. Berg, K.A. Olive, R.W. Pogge, J.J. Salzer, E.D. Skillman, Improving helium abundance determinations with Leo P as a case study, J. Cosmol. Astropart. Phys. 03 (2021) 027, [arXiv:2010.04180 [astro-ph.CO]].

[1513] M. Valerdi, A. Peimbert, M. Peimbert, A. Sixtos, Determination of the primordial helium abundance based on NGC 346, an H ii region of the small magellanic cloud, Astrophys. J. 876 (2) (2019) 98, [arXiv:1904.01594 [astro-ph.GA]].

[1514] V. Fernández, E. Terlevich, A.I. Díaz, R. Terlevich, A Bayesian direct method implementation to fit emission line spectra: Application to the primordial He abundance determination, Mon. Not. R. Astron. Soc. 487 (3) (2019) 3221–3238, [arXiv:1905.09215 [astro-ph.GA]].

[1515] O.A. Kurichin, P.A. Kislitsyn, V.V. Klimenko, S.A. Balashev, A.V. Ivanchik, A new determination of the primordial helium abundance using the analyses of H II region spectra from SDSS, Mon. Not. R. Astron. Soc. 502 (2) (2021) 3045–3056, [arXiv:2101.09127 [astro-ph.CO]].

[1516] T. Hsyu, R.J. Cooke, J.X. Prochaska, M. Bolte, The PHLEK survey: a new determination of the primordial helium abundance, Astrophys. J. 896 (1) (2020) 77, [arXiv:2005.12290 [astro-ph.GA]].

[1517] M. Valerdi, A. Peimbert, M. Peimbert, Chemical abundances in seven metal-poor H II regions and a determination of the primordial helium abundance, Mon. Not. R. Astron. Soc. 505 (3) (2021) 3624–3634, [arXiv:2105.12260 [astro-ph.GA]].

[1518] A. Matsumoto, et al., EMPRESS VIII. A new determination of primordial he abundance with extremely metal-poor galaxies: a suggestion of the lepton asymmetry and implications for the hubble tension, Astrophys. J. 941 (2) (2022) 167, [arXiv:2203.09617 [astro-ph.CO]].

[1519] T. Takahashi, S. Yamashita, Big bang nucleosynthesis and early dark energy in light of the EMPRESS Yp results and the H0 tension, Phys. Rev. D 107 (10) (2023) 103520, [arXiv:2211.04087 [astro-ph.CO]].

[1520] M. Escudero, A. Ibarra, V. Maura, Primordial lepton asymmetries in the precision cosmology era: Current status and future sensitivities from BBN and the CMB, Phys. Rev. D 107 (3) (2023) 035024, [arXiv:2208.03201 [hep-ph]].

[1521] Y.I. Izotov, T.X. Thuan, N.G. Guseva, A new determination of the primordial He abundance using the He i λ10830 Å emission line: cosmological implications, Mon. Not. R. Astron. Soc. 445 (1) (2014) 778–793, [arXiv:1408.6953 [astro-ph.CO]].

[1522] C. Pitrou, A. Coc, J.-P. Uzan, E. Vangioni, Resolving conclusions about the early Universe requires accurate nuclear measurements, Nat. Rev. Phys. 3 (4) (2021) 231–232, [arXiv:2104.11148 [astro-ph.CO]].

[1523] O. Pisanti, G. Mangano, G. Miele, P. Mazzella, Primordial Deuterium after LUNA: concordances and error budget, J. Cosmol. Astropart. Phys. 04 (2021) 020, [arXiv:2011.11537 [astro-ph.CO]].

[1524] E. Di Valentino, C. Gustavino, J. Lesgourgues, G. Mangano, A. Melchiorri, G. Miele, O. Pisanti, Probing nuclear rates with Planck and BICEP2, Phys. Rev. D 90 (2) (2014) 023543, [arXiv:1404.7848 [astro-ph.CO]].

[1525] G.E. Addison, G. Hinshaw, M. Halpern, Cosmological constraints from baryon acoustic oscillations and clustering of large-scale structure, Mon. Not. R. Astron. Soc. 436 (2013) 1674–1683, [arXiv:1304.6984 [astro-ph.CO]].

[1526] G.E. Addison, D.J. Watts, C.L. Bennett, M. Halpern, G. Hinshaw, J.L. Weiland, Elucidating ACDM: impact of baryon acoustic oscillation measurements on the hubble constant discrepancy, Astrophys. J. 853 (2) (2018) 119, [arXiv:1707.06547 [astro-ph.CO]].

[1527] eBOSS Collaboration, M. Blomqvist, et al., Baryon acoustic oscillations from the cross-correlation of Lyα absorption and quasars in eBOSS DR14, Astron. Astrophys. 629 (2019) A86, [arXiv:1904.03430 [astro-ph.CO]].

[1528] A. Cuceu, J. Farr, P. Lemos, A. Font-Ribera, Baryon acoustic oscillations and the hubble constant: past, present and future, J. Cosmol. Astropart. Phys. 10 (2019) 044, [arXiv:1906.11628 [astro-ph.CO]].

[1529] N. Schöneberg, L. Verde, H. Gil-Marín, S. Frieden, BAO+BBN revisited — growing the Hubble tension with a 0.7 km/s/Mpc constraint, J. Cosmol. Astropart. Phys. 11 (2022) 039, [arXiv:2209.14330 [astro-ph.CO]].

[1530] N. Schöneberg, L. Vacher, The mass effect — variations of the electron mass and their impact on cosmology, J. Cosmol. Astropart. Phys. 03 (2025) 004, [arXiv:2407.16845 [astro-ph.CO]].

[1531] B.D. Fields, K.A. Olive, T.-H. Yeh, C. Young, Big-Bang Nucleosynthesis after Planck, J. Cosmol. Astropart. Phys. 03 (2020) 010, [arXiv:1912.01132 [astro-ph.CO]]; JCAP 11 (2020) E02 (erratum).

[1532] M. McQuinn, The evolution of the intergalactic medium, Ann. Rev. Astron. Astrophys. 54 (2016) 313–362, [arXiv:1512.00086 [astro-ph.CO]].

[1533] eBOSS Collaboration, H. du Mas des Bourboux, et al., The completed SDSS-IV extended baryon oscillation spectroscopic survey: baryon acoustic oscillations with Lyα forests, Astrophys. J. 901 (2) (2020) 153, [arXiv:2007.08995 [astro-ph.CO]].

[1534] A. Cuceu, A. Font-Ribera, B. Joachimi, S. Nadathur, Cosmology beyond BAO from the 3D distribution of the Lyman-α forest, Mon. Not. R. Astron. Soc. 506 (4) (2021) 5439–5450, [arXiv:2103.14075 [astro-ph.CO]].

[1535] R. de Belsunce, O.H.E. Philcox, V. Irsic, P. McDonald, J. Guy, N. Palanque-Delabrouille, The 3D Lyman-α forest power spectrum from eBOSS DR16, Mon. Not. R. Astron. Soc. 533 (3) (2024) 3756–3770, [arXiv:2403.08241 [astro-ph.CO]].

[1536] DESI Collaboration, C. Ravoux, et al., The Dark Energy Spectroscopic Instrument: one-dimensional power spectrum from first Ly α forest samples with Fast Fourier Transform, Mon. Not. R. Astron. Soc. 526 (4) (2023) 5118–5140, [arXiv:2306.06311 [astro-ph.CO]].

[1537] N.G. Karaçaylı, et al., Optimal 1D Lyα forest power spectrum estimation – III. DESI early data, Mon. Not. R. Astron. Soc. 528 (3) (2024) 3941–3963, [arXiv:2306.06316 [astro-ph.CO]].

[1538] V.K. Narayanan, D.N. Spergel, R. Dave, C.-P. Ma, Constraints on the mass of warm dark matter particles and the shape of the linear power spectrum from the Lyα forest, Astrophys. J. Lett. 543 (2000) L103–L106, [arXiv:astro-ph/0005095].

[1539] U. Seljak, A. Slosar, P. McDonald, Cosmological parameters from combining the Lyman-alpha forest with CMB, galaxy clustering and SN constraints, J. Cosmol. Astropart. Phys. 10 (2006) 014, [arXiv:astro-ph/0604335].

[1540] M. Viel, J. Schaye, C.M. Booth, The impact of feedback from galaxy formation on the Lyman-alpha transmitted flux, Mon. Not. R. Astron. Soc. 429 (2013) 1734, [arXiv:1207.6567 [astro-ph.CO]].

[1541] V. Iršič, et al., The Lyman α forest power spectrum from the XQ-100 legacy survey, Mon. Not. R. Astron. Soc. 466 (4) (2017) 4332–4345, [arXiv:1702.01761 [astro-ph.CO]].

[1542] E. Boera, G.D. Becker, J.S. Bolton, F. Nasir, Revealing reionization with the thermal history of the intergalactic medium: new constraints from the Lyα flux power spectrum, Astrophys. J. 872 (1) (2019) 101, [arXiv:1809.06980 [astro-ph.CO]].

[1543] N.G. Karaçaylı, et al., Optimal 1D Lyα forest power spectrum estimation – II. KODIAQ, SQUAD, and XQ-100, Mon. Not. R. Astron. Soc. 509 (2) (2022) 2842–2855, [arXiv:2108.10870 [astro-ph.CO]].

[1544] B. Villasenor, B. Robertson, P. Madau, E. Schneider, New constraints on warm dark matter from the Lyman-α forest power spectrum, Phys. Rev. D 108 (2) (2023) 023502, [arXiv:2209.14220 [astro-ph.CO]].

[1545] E. Puchwein, et al., The Sherwood–Relics simulations: overview and impact of patchy reionization and pressure smoothing on the intergalactic medium, Mon. Not. R. Astron. Soc. 519 (4) (2023) 6162–6183, [arXiv:2207.13098 [astro-ph.CO]].

[1546] C.C. Doughty, J.F. Hennawi, F.B. Davies, Z. Lukić, J. Oñorbe, Convergence of small scale Lyα structure at high-z under different reionization scenarios, Mon. Not. R. Astron. Soc. 525 (3) (2023) 3790–3805, [arXiv:2305.16200 [astro-ph.CO]].

[1547] S. Bird, M. Fernandez, M.-F. Ho, M. Qezlou, R. Monadi, Y. Ni, N. Chen, R. Croft, T. Di Matteo, PRIYA: a new suite of Lyman-α forest simulations for cosmology, J. Cosmol. Astropart. Phys. 10 (2023) 037, [arXiv:2306.05471 [astro-ph.CO]].

[1548] SDSS Collaboration, P. McDonald, et al., The Linear theory power spectrum from the Lyman-alpha forest in the Sloan Digital Sky Survey, Astrophys. J. 635 (2005) 761–783, [arXiv:astro-ph/0407377].

[1549] C. Pedersen, A. Font-Ribera, N.Y. Gnedin, Compressing the cosmological information in one-dimensional correlations of the Lyα forest, Astrophys. J. 944 (2) (2023) 223, [arXiv:2209.09895 [astro-ph.CO]].

[1550] M. Viel, J. Lesgourgues, M.G. Haehnelt, S. Matarrese, A. Riotto, Constraining warm dark matter candidates including sterile neutrinos and light gravitinos with WMAP and the Lyman-alpha forest, Phys. Rev. D 71 (2005) 063534, [arXiv:astro-ph/0501562].

[1551] V. Iršič, M. Viel, M.G. Haehnelt, J.S. Bolton, G.D. Becker, First constraints on fuzzy dark matter from Lyman-α forest data and hydrodynamical simulations, Phys. Rev. Lett. 119 (3) (2017) 031302, [arXiv:1703.04683 [astro-ph.CO]].

[1552] E. Armengaud, N. Palanque-Delabrouille, C. Yèche, D.J.E. Marsh, J. Baur, Constraining the mass of light bosonic dark matter using SDSS Lyman-α forest, Mon. Not. R. Astron. Soc. 471 (4) (2017) 4606–4614, [arXiv:1703.09126 [astro-ph.CO]].

[1553] N. Palanque-Delabrouille, C. Yèche, N. Schöneberg, J. Lesgourgues, M. Walther, S. Chabanier, E. Armengaud, Hints, neutrino bounds and WDM constraints from SDSS DR14 Lyman-α and Planck full-survey data, J. Cosmol. Astropart. Phys. 04 (2020) 038, [arXiv:1911.09073 [astro-ph.CO]].

[1554] K.K. Rogers, H.V. Peiris, General framework for cosmological dark matter bounds using N-body simulations, Phys. Rev. D 103 (4) (2021) 043526, [arXiv:2007.13751 [astro-ph.CO]].

[1555] V. Iršič, et al., Unveiling dark matter free streaming at the smallest scales with the high redshift Lyman-alpha forest, Phys. Rev. D 109 (4) (2024) 043511, [arXiv:2309.04533 [astro-ph.CO]].

[1556] eBOSS Collaboration, S. Chabanier, et al., The one-dimensional power spectrum from the SDSS DR14 Lyα forests, J. Cosmol. Astropart. Phys. 07 (2019) 017, [arXiv:1812.03554 [astro-ph.CO]].
[1557] M.A. Fernandez, S. Bird, M.-F. Ho, Cosmological constraints from the eBOSS Lyman-α forest using the PRIYA simulations, J. Cosmol. Astropart. Phys. 07 (2024) 029, arXiv:2309.03943 [astro-ph.CO].

[1558] V. Iršič, et al., New Constraints on the free-streaming of warm dark matter from intermediate and small scale Lyman-α forest data, Phys. Rev. D 96 (2) (2017) 023522, arXiv:1702.01764 [astro-ph.CO].

[1559] C. Yèche, N. Palanque-Delabrouille, J. Baur, H. du Mas des Bouroux, Constraints on neutrino masses from Lyman-alpha forest power spectrum with BOSS and XQ-100, J. Cosmol. Astropart. Phys. 06 (2017) 047, arXiv:1702.03314 [astro-ph.CO].

[1560] M. Esposito, V. Iršič, M. Costanzi, S. Borgani, A. Saro, M. Viel, Weighing cosmic structures with clusters of galaxies and the intergalactic medium, Mon. Not. R. Astron. Soc. 515 (1) (2022) 857-870, arXiv:2202.00974 [astro-ph.CO].

[1561] S. Goldstein, J.C. Hill, V. Iršič, B.D. Sherwin, Canonical hubble-tension-resolving early dark energy cosmologies are inconsistent with the Lyman-α forest, Phys. Rev. Lett. 131 (20) (2023) 201001, arXiv:2303.00746 [astro-ph.CO].

[1562] K.K. Rogers, V. Poulin, 5σ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond ΛCDM, Phys. Rev. Res. 7 (1) (2025) L012018, arXiv:2311.16377 [astro-ph.CO].

[1563] T. Kobayashi, R. Murgia, A. De Simone, V. Iršič, M. Viel, Lyman-α constraints on ultralight scalar dark matter: Implications for the early and late universe, Phys. Rev. D 96 (12) (2017) 123514, arXiv:1708.00015 [astro-ph.CO].

[1564] J. Baur, N. Palanque-Delabrouille, C. Yèche, A. Boyarsky, O. Ruchayskiy, E. Armengaud, J. Lesgourgues, Constraints from Ly-α forests on non-thermal dark matter including resonantly-produced sterile neutrinos, J. Cosmol. Astropart. Phys. 12 (2017) 013, arXiv:1706.03118 [astro-ph.CO].

[1565] P. Gaikwad, et al., Probing the thermal state of the intergalactic medium at z > 5 with the transmission spikes in high-resolution Ly α forest spectra, Mon. Not. R. Astron. Soc. 494 (4) (2020) 5091-5109, arXiv:2001.10018 [astro-ph.CO].

[1566] P. Montero-Camacho, C.M. Hirata, P. Martini, K. Honscheid, Impact of inhomogeneous reionization on the Lyman-α forest, Mon. Not. R. Astron. Soc. 487 (1) (2019) 1047-1056, arXiv:1902.02892 [astro-ph.CO].

[1567] M. Molaro, V. Iršič, J.S. Bolton, M. Lieu, L.C. Keating, E. Puchwein, M.G. Haehnelt, M. Viel, Possible evidence for a large-scale enhancement in the Lyman-α forest power spectrum at redshift $z \ge 4$, Mon. Not. R. Astron. Soc. 521 (1) (2023) 1489-1501, arXiv:2303.05167 [astro-ph.CO].

[1568] J. Einasto, Dark Matter and Cosmic Web Story, World Scientific Publishing Co., 2014.

[1569] M. Einasto, J. Einasto, P. Tenjes, S. Korhonen, R. Kipper, E. Tempel, L.J. Liivamägi, P. Heinämäki, Galaxy groups and clusters and their brightest galaxies within the cosmic web, Astron. Astrophys. 681 (2024) A91, arXiv:2311.01868 [astro-ph.CO].

[1570] S. Sankhyayan, J. Bagchi, E. Tempel, S. More, M. Einasto, P. Dabhade, S. Raychaudhury, R. Athreya, P. Heinämäki, Identification of superclusters and their properties in the sloan digital sky survey using the WHL cluster catalog, Astrophys. J. 958 (1) (2023) 62, arXiv:2309.06251 [astro-ph.CO].

[1571] J. Einasto, I. Suhhonenko, L.J. Liivamägi, M. Einasto, Evolution of superclusters in the cosmic web, Astron. Astrophys. 623 (2019) A97, arXiv:1901.09378 [astro-ph.CO].

[1572] M. Einasto, J. Einasto, E. Tago, G.B. Dalton, H. Andernach, The structure of the universe traced by rich clusters of galaxies, Mon. Not. R. Astro. Soc. 269 (1994) 301-322.

[1573] H. Lietzen, E. Tempel, L.J. Liivamägi, A. Montero-Dorta, M. Einasto, A. Streblyanska, C. Maraston, J.A. Rubiño Martín, E. Saar, Discovery of a massive supercluster system at $z \sim 0.47$, Astron. Astrophys. 588 (2016) L4, arXiv:1602.08498 [astro-ph.CO].

[1574] M. Einasto, R. Kipper, P. Tenjes, H. Lietzen, E. Tempel, L.J. Liivamägi, J. Einasto, A. Tamm, P. Heinämäki, P. Nurmi, The Corona Borealis supercluster: connectivity, collapse, and evolution, Astron. Astrophys. 649 (2021) A51, arXiv:2103.02326 [astro-ph.CO].

[1575] N. Aghanim, T. Tuominen, V. Bonjean, C. Gouin, T. Bonnaire, M. Einasto, Dissecting a miniature universe: A multi-wavelength view of galaxy quenching in the Shapley supercluster, Astron. Astrophys. 689 (2024) A332, arXiv:2402.18455 [astro-ph.CO].

[1576] L.J. Liivamägi, E. Tempel, E. Saar, SDSS DR7 superclusters. The catalogues, Astron. Astrophys. 539 (2012) A80, arXiv:1012.1989 [astro-ph.CO].

[1577] R.B. Tully, H. Courtois, Y. Hoffman, D. Pomarède, The Laniakea supercluster of galaxies, Nature 513 (7516) (2014) 71, arXiv:1409.0880 [astro-ph.CO].

[1578] A. Dupuy, H.M. Courtois, Dynamic cosmography of the local Universe: Laniakea and five more watershed superclusters, Astron. Astrophys. 678 (2023) A176, arXiv:2305.02339 [astro-ph.CO].

[1579] M. Einasto, et al., The Sloan Great Wall. Morphology and galaxy content, Astrophys. J. 736 (2011) 51, arXiv:1105.1632 [astro-ph.CO].

[1580] J.M. Zúniga, C.A. Caretta, H. Andernach, Nucleation regions in the Large-Scale Structure I: A catalogue of cores in nearby rich superclusters, Publ. Astron. Soc. Austral. 41 (2024) e078, arXiv:2405.13280 [astro-ph.CO].

[1581] S. Lim, J. Lee, An analytic formula for the supercluster mass function, Astrophys. J. 783 (2014) 39, arXiv:1201.1382 [astro-ph.CO].

[1582] S. Nadathur, S. Hotchkiss, S. Sarkar, The integrated Sachs-Wolfe imprints of cosmic superstructures: a problem for ΛCDM, J. Cosmol. Astropart. Phys. 06 (2012) 042, arXiv:1109.4126 [astro-ph.CO].

[1583] B.R. Granett, M.C. Neyrinck, I. Szapudi, An imprint of super-structures on the microwave background due to the integrated Sachs-wolfe effect, Astrophys. J. Lett. 683 (2008) L99-L102, arXiv:0805.3695 [astro-ph].

[1584] I.D. Gialamas, G. Hütsi, K. Kannike, A. Racioppi, M. Raidal, M. Vasar, H. Veermaë, Interpreting DESI 2024 BAO: Late-time dynamical dark energy or a local effect? Phys. Rev. D 111 (4) (2025) 043540, arXiv:2406.07533 [astro-ph.CO].

[1585] M. Reyhani, M. Najafi, J.T. Firouzjaee, E. Di Valentino, Structure formation in various dynamical dark energy scenarios, Phys. Dark Univ. 44 (2024) 101477, arXiv:2403.15202 [astro-ph.CO].

[1586] R.K. Sachs, A.M. Wolfe, Perturbations of a cosmological model and angular variations of the microwave background, Astrophys. J. 147 (1967) 73-90.

[1587] M.J. Rees, D.W. Sciama, Large scale density inhomogeneities in the universe, Nature 217 (1968) 511-516.

[1588] S. Flender, S. Hotchkiss, S. Nadathur, The stacked ISW signal of rare superstructures in ΛCDM, J. Cosmol. Astropart. Phys. 02 (2013) 013, arXiv:1212.0776 [astro-ph.CO].

[1589] C. Hernandez-Monteagudo, R.E. Smith, On the signature of nearby superclusters and voids in the Integrated Sachs-Wolfe effect, Mon. Not. R. Astron. Soc. 435 (2013) 1094, arXiv:1212.1174 [astro-ph.CO].

[1590] S. Aiola, A. Kosowsky, B. Wang, Gaussian approximation of peak values in the integrated Sachs-wolfe effect, Phys. Rev. D 91 (2015) 043510, arXiv:1410.6138 [astro-ph.CO].

[1591] A.M. Soltan, ISW in ΛCDM or something else? Mon. Not. R. Astron. Soc. 488 (2) (2019) 2732-2742, arXiv:1812.09348 [astro-ph.CO].

[1592] Planck Collaboration, P.A.R. Ade, et al., Planck 2015 results. XXI. The integrated Sachs-Wolfe effect, Astron. Astrophys. 594 (2016) A21, arXiv:1502.01595 [astro-ph.CO].

[1593] Y.-C. Cai, M. Neyrinck, Q. Mao, J.A. Peacock, I. Szapudi, A.A. Berlind, The lensing and temperature imprints of voids on the Cosmic Microwave Background, Mon. Not. R. Astron. Soc. 466 (3) (2017) 3364-3375, arXiv:1609.00301 [astro-ph.CO].

[1594] A. Kovács, The part and the whole: voids, supervoids, and their ISW imprint, Mon. Not. R. Astron. Soc. 475 (2) (2018) 1777-1790, arXiv:1701.08583 [astro-ph.CO].

[1595] S. Nadathur, R. Crittenden, A detection of the integrated Sachs-Wolfe imprint of cosmic superstructures using a matched-filter approach, Astrophys. J. Lett. 830 (1) (2016) L19, arXiv:1608.08638 [astro-ph.CO].

[1596] DES Collaboration, A. Kovács, et al., Imprint of DES superstructures on the cosmic microwave background, Mon. Not. R. Astron. Soc. 465 (4) (2017) 4166-4179, arXiv:1610.00637 [astro-ph.CO].

[1597] DES Collaboration, A. Kovács, et al., More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey, Mon. Not. R. Astron. Soc. 484 (2019) 5267-5277, arXiv:1811.07812 [astro-ph.CO].

[1598] M. Cruz, E. Martinez-Gonzalez, P. Vielva, L. Cayon, Detection of a non-gaussian spot in wmap, Mon. Not. R. Astron. Soc. 356 (2005) 29-40, arXiv:astro-ph/0405341.

[1599] F. Finelli, J. García-Bellido, A. Kovács, F. Paci, I. Szapudi, Supervoids in the WISE-2MASS catalogue imprinting cold spots in the cosmic microwave background, Mon. Not. R. Astron. Soc. 455 (2) (2016) 1246-1256, arXiv:1405.1555 [astro-ph.CO].

[1600] A. Pataki, P. Raffai, I. Csabai, G. Rácz, I. Szapudi, Constraints on AvERA cosmologies from cosmic chronometers and type ia supernovae, 2025, arXiv:2503.21369 [astro-ph.CO].

[1601] S. Räsänen, Backreaction: directions of progress, Cl. Quant. Grav. 28 (2011) 164008, arXiv:1102.0408 [astro-ph.CO].

[1602] T. Buchert, et al., Is there proof that backreaction of inhomogeneities is irrelevant in cosmology? Cl. Quant. Grav. 32 (2015) 215021, arXiv:1505.07800 [gr-qc].

[1603] D.L. Wiltshire, Solution to the cosmological constant problem, 2024, arXiv:2404.02129 [gr-qc].

[1604] M.J. Williams, H.J. Macpherson, D.L. Wiltshire, C. Stevens, First investigation of void statistics in numerical relativity simulations, Mon. Not. R. Astron. Soc. 536 (2025) 2645-2660, arXiv:2403.15134 [astro-ph.CO].

[1605] A. Kovács, R. Beck, A. Smith, G. Rácz, I. Csabai, I. Szapudi, Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars, Mon. Not. R. Astron. Soc. 513 (1) (2022) 15-26, arXiv:2107.13038 [astro-ph.CO].

[1606] eBOSS Collaboration, A.D. Myers, et al., The SDSS-IV extended baryon oscillation spectroscopic survey: quasar target selection, Astrophys. J. Suppl. 221 (2) (2015) 27, arXiv:1508.04472 [astro-ph.CO].

[1607] J.R. Gott, III, M. Juric, D. Schlegel, F. Hoyle, M. Vogeley, M. Tegmark, N.A. Bahcall, J. Brinkmann, A map of the universe, Astrophys. J. 624 (2005) 463, arXiv:astro-ph/0310571.

[1608] M. Einasto, H. Lietzen, M. Gramann, E. Tempel, E. Saar, L.J. Liivamägi, P. Heinämäki, P. Nurmi, J. Einasto, Sloan Great Wall as a complex of superclusters with collapsing cores, Astron. Astrophys. 595 (2016) A70, arXiv:1608.04988 [astro-ph.CO].
[1609] M. Einasto, P. Tenjes, M. Gramann, H. Lietzen, R. Kipper, L.J. Liivamägi, E. Tempel, S. Sankhyayan, J. Einasto, The evolution of high-density cores of the BOSS Great Wall superclusters, Astron. Astrophys. 666 (2022) A52, arXiv:2204.08918 [astro-ph.CO].

[1610] J. Einasto, et al., Luminous superclusters: remnants from inflation, Astron. Astrophys. 459 (2006) L1, arXiv:astro-ph/0605393.

[1611] R.K. Sheth, A. Diaferio, How unusual are the shapley supercluster and the sloan great wall? Mon. Not. R. Astron. Soc. 417 (2011) 2938-2949, arXiv:1105.3378 [astro-ph.CO].

[1612] C. Park, Y.-Y. Choi, J. Kim, J.R. Gott III, S.S. Kim, K.-S. Kim, The challenge of the largest structures in the universe to cosmology, Astrophys. J. Lett. 759 (2012) L7, arXiv:1209.5659 [astro-ph.CO].

[1613] J. Einasto, R.H. Miller, Neighboring superclusters and their environs, in: G.O. Abell, G. Chincarini (Eds.), Early Evolution of the Universe and its Present Structure, in: IAU Symposium, vol. 104, 1983, p. 405.

[1614] P.A. Shaver, Radio surveys and large scale structure, Aust. J. Phys. 44 (6) (1991) 759.

[1615] H. Boehringer, G. Chon, J. Truemper, The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey - II. Unveiling a pancake structure with a 100 Mpc radius in the local Universe, Astron. Astrophys. 651 (2021) A15, arXiv:2105.13999 [astro-ph.CO].

[1616] P.J.E. Peebles, Flat patterns in cosmic structure, Mon. Not. R. Astron. Soc. 526 (3) (2023) 4490-4501, arXiv:2308.04245 [astro-ph.CO].

[1617] M. Einasto, E. Tago, J. Jaaniste, J. Einasto, H. Andernach, The supercluster-void network I. the supercluster catalogue and large scale distribution, Astron. Astrophys. Suppl. Ser. 123 (1997) 119, arXiv:astro-ph/9610088.

[1618] K. Dolag, J.G. Sorce, S. Pilipenko, E. Hernández-Martínez, M. Valentini, S. Gottlöber, N. Aghanim, I. Khabibullin, Simulating the Local Web (SLOW) - I. Anomalies in the local density field, Astron. Astrophys. 677 (2023) A169, arXiv:2302.10960 [astro-ph.CO].

[1619] P.J.E. Peebles, Improving physical cosmology: an empiricist's assessment, 2021, http://dx.doi.org/10.48550/arXiv.2106.02672, arXiv e-prints, arXiv: 2106.02672 [astro-ph.CO].

[1620] O. Toomet, H. Andernach, J. Einasto, M. Einasto, E. Kasak, A.A. Starobinsky, E. Tago, The supercluster-void network v. alternative evidence for its regularity, Astron. Astrophys. 393 (2002) 1, arXiv:astro-ph/9907238.

[1621] J. Einasto, M. Einasto, S. Gottlöber, V. Müller, V. Saar, A.A. Starobinsky, E. Tago, D. Tucker, H. Andernach, P. Frisch, A 120 MPC periodicity in the three-dimensional distribution of galaxy superclusters, Nature 385 (1997) 139-141, arXiv:astro-ph/9701018.

[1622] J. Einasto, M. Einasto, P. Frisch, S. Gottlöber, V. Müller, V. Saar, A.A. Starobinsky, E. Tago, D. Tucker, H. Andernach, The supercluster-void network. 2. An oscillating cluster correlation function, Mon. Not. R. Astron. Soc. 289 (1997) 801-812, arXiv:astro-ph/9704127.

[1623] E. Tago, J. Einasto, M. Einasto, V. Müller, H. Andernach, Optical and x-ray clusters as tracers of the supercluster-void network. II the spatial correlation function, Astron. J. 123 (2002) 37, arXiv:astro-ph/0012537.

[1624] U. Lindner, J. Einasto, M. Einasto, W. Freudling, K. Fricke, E. Tago, The structure of supervoids - I: void hierarchy in the northern local supervoid, Astron. Astrophys. 301 (1995) 329, arXiv:astro-ph/9503044.

[1625] A. Kovács, J. García-Bellido, Cosmic troublemakers: the cold spot, the eridanus supervoid, and the great walls, Mon. Not. R. Astron. Soc. 462 (2) (2016) 1882-1893, arXiv:1511.09008 [astro-ph.CO].

[1626] M. Einasto, E. Tago, H. Lietzen, C. Park, P. Heinamaki, E. Saar, H. Song, L.J. Liivamägi, J. Einasto, Tracing a high redshift cosmic web with quasar systems, Astron. Astrophys. 568 (2014) A46, arXiv:1406.5578 [astro-ph.CO].

[1627] M. Einasto, P. Heinämäki, L.J. Liivamägi, V.J. Martinez, L. Hurtado-Gil, P. Arnalte-Mur, P. Nurmi, J. Einasto, E. Saar, Shell-like structures in our cosmic neighbourhood, Astron. Astrophys. 587 (2016) A116, arXiv:1506.05295 [astro-ph.CO].

[1628] M. Einasto, L.J. Liivamagi, E. Tago, E. Saar, E. Tempel, J. Einasto, V.J. Martinez, P. Heinamaki, SDSS DR7 superclusters, Morphology, Astron. Astrophys. 532 (2011) A5, arXiv:1105.2124 [astro-ph.CO].

[1629] C. R.B. Tully, C. Howlett, D. Pomarede, Ho'oleilana: an individual baryon acoustic oscillation? Astrophys. J. 954 (2) (2023) 169, arXiv:2309.00677 [astro-ph.CO].

[1630] P. Arnalte-Mur, A. Labatie, N. Clerc, V.J. Martinez, J.L. Starck, M. Lachieze-Rey, E. Saar, S. Paredes, Wavelet analysis of baryon acoustic structures in the galaxy distribution, Astron. Astrophys. 542 (2012) A34, arXiv:1101.1911 [astro-ph.CO].

[1631] M. Einasto, M. Gramann, E. Saar, L.J. Liivamagi, E. Tempel, J. Nevalainen, P. Heinamaki, C. Park, J. Einasto, Unusual A2142 supercluster with a collapsing core: distribution of light and mass, Astron. Astrophys. 580 (2015) A69, arXiv:1505.07233 [astro-ph.CO].

[1632] P. Heinämäki, P. Teerikorpi, M. Douspis, P. Nurmi, M. Einasto, M. Gramann, J. Nevalainen, E. Saar, Quasi-spherical superclusters, Astron. Astrophys. 668 (2022) A37, arXiv:2210.13294 [astro-ph.CO].

[1633] A. Vikhlinin, M. Markevitch, S.S. Murray, C. Jones, W. Forman, L. Van Speybroeck, Chandra temperature profiles for a sample of nearby relaxed galaxy clusters, Astrophys. J. 628 (2005) 655-672, arXiv:astro-ph/0412306.

[1634] E. Tempel, A. Tamm, M. Gramann, T. Tuvikene, L.J. Liivamägi, I. Suhonenko R. Kipper, M. Einasto, E. Saar, Flux- and volume-limited groups/clusters for the SDSS galaxies: catalogues and mass estimation, Astron. Astrophys. 566 (2014) A1, arXiv:1402.1350 [astro-ph.CO].

[1635] M.J. Rieke, D. Kelly, S. Horner, Overview of James Webb Space Telescope and NIRCam's Role, in: J.B. Heaney, L.G. Burriesci (Eds.), Cryogenic Optical Systems and Instruments XI, in: Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, vol. 5904, 2005, pp. 1-8.

[1636] P. Santini, A. Fontana, M. Castellano, N. Leethochawalit, M. Trenti, T. Treu, D. Belfiori, S. Birrer, A. Bonchi, E. Merlin, C. Mason, T. Morishita, M. Nonino, D. Paris, G. Polenta, P. Rosati, L. Yang, K. Boyett, M. Bradac, A. Calabrò, A. Dressler, K. Glazebrook, D. Marchesini, S. Mascia, T. Nanayakkara, L. Pentericci, G. Roberts-Borsani, C. Scarlata, B. Vulcani, X. Wang, Early results from GLASS-JWST. XI. Stellar masses and mass-to-light ratio of $z > 7$ galaxies, Astrophys. J. Lett. 942 (2) (2023) L27, arXiv:2207.11379 [astro-ph.GA].

[1637] M. Castellano, A. Fontana, T. Treu, P. Santini, E. Merlin, N. Leethochawalit, M. Trenti, E. Vanzella, U. Mestric, A. Bonchi, D. Belfiori, M. Nonino, D. Paris, G. Polenta, G. Roberts-Borsani, K. Boyett, M.S. Bradač, A. Calabrò, K. Glazebrook, C. Grillo, S. Mascia, C. Mason, A. Mercurio, T. Morishita, T. Nanayakkara, L. Pentericci, P. Rosati, B. Vulcani, X. Wang, L. Yang, Early results from GLASS-JWST. III. Galaxy candidates at $z > 9-15$, Astrophys. J. Lett. 938 (2) (2022) L15, arXiv:2207.09436 [astro-ph.GA].

[1638] S.L. Finkelstein, M.B. Bagley, H.C. Ferguson, S.M. Wilkins, J.S. Kartaltepe, et al., CEERS key paper. I. An early look into the first 500 Myr of galaxy formation with JWST, Astrophys. J. Lett. 946 (1) (2023) L13, arXiv:2211.05792 [astro-ph.GA].

[1639] R.P. Naidu, P.A. Oesch, P. van Dokkum, E.J. Nelson, K.A. Suess, G. Brammer, K.E. Whitaker, G. Illingworth, R. Bouwens, S. Tacchella, J. Matthee, N. Allen, R. Bezanson, C. Conroy, I. Labbe, J. Leja, E. Leonova, D. Magee, S.H. Price, D.J. Setton, V. Strait, M. Stefanon, S. Toft, J.R. Weaver, A. Weibel, Two remarkably luminous galaxy candidates at $z \approx 10-12$ revealed by JWST, Astrophys. J. Lett. 940 (1) (2022) L14, arXiv:2207.09434 [astro-ph.GA].

[1640] T. Treu, et al., The glass-jwst early release science program. I. Survey design and release plans, Astrophys. J. 935 (2) (2022) 110, arXiv:2206.07978 [astro-ph.GA].

[1641] Y. Harikane, M. Ouchi, M. Oguri, Y. Ono, K. Nakajima, Y. Isobe, H. Umeda, K. Mawatari, Y. Zhang, A comprehensive study of galaxies at $z \sim 9-16$ found in the early JWST data: ultraviolet luminosity functions and cosmic star formation history at the pre-reionization epoch, Astrophys. J. Suppl. 265 (1) (2023) arXiv:2208.01612 [astro-ph.GA].

[1642] P.G. Pérez-González, et al., CEERS key paper. IV. A triality in the nature of HST-dark galaxies, Astrophys. J. Lett. 946 (1) (2023) L16, arXiv:2211.00045 [astro-ph.GA].

[1643] C. Papovich, et al., CEERS key paper. V. Galaxies at $4 < z < 9$ are bluer than they appear-characterizing galaxy stellar populations from rest-frame $\sim 1 \mu$m imaging, Astrophys. J. Lett. 949 (2) (2023) L18, arXiv:2301.00027 [astro-ph.GA].

[1644] R.J. Bouwens, M. Stefanon, G. Brammer, P.A. Oesch, T. Herard-Demanche, G.D. Illingworth, J. Matthee, R.P. Naidu, P.G. van Dokkum, I.F. van Leeuwen, Evolution of the UV LF from $z 15$ to $z 8$ using new JWST/NIRCam medium-band observations over the HUDF/XDF, Mon. Not. R. Astron. Soc. 523 (1) (2023) 1036-1055, arXiv:2211.02607 [astro-ph.GA].

[1645] N.J. Adams, C.J. Conselice, L. Ferreira, D. Austin, J.A.A. Trussler, I. Juodžbalis, S.M. Wilkins, J. Caruana, P. Dayal, A. Verma, A.P. Vijayan, Discovery and properties of ultra-high redshift galaxies ($9 < z < 12$) in the JWST ERO SMACS 0723 Field, Mon. Not. R. Astron. Soc. 518 (3) (2023) 4755-4766, arXiv:2207.11217 [astro-ph.GA].

[1646] R. Bouwens, G. Illingworth, P. Oesch, M. Stefanon, R. Naidu, I. van Leeuwen, D. Magee, UV luminosity density results at $z > 8$ from the first JWST/NIRCam fields: limitations of early data sets and the need for spectroscopy, Mon. Not. R. Astron. Soc. 523 (1) (2023) 1009-1035, arXiv:2212.06683 [astro-ph.CO].

[1647] S.L. Finkelstein, et al., The complete CEERS early universe galaxy sample: a surprisingly slow evolution of the space density of bright galaxies at $z \sim 8.5-14.5$, Astrophys. J. Lett. 969 (1) (2024) L2, arXiv:2311.04279 [astro-ph.GA].

[1648] D.J. McLeod, C.T. Donnan, R.J. McLure, J.S. Dunlop, D. Magee, R. Begley, A.C. Carnall, F. Cullen, R.S. Ellis, M.L. Hamadouche, T.M. Stanton, The galaxy UV luminosity function at $z \approx 11$ from a suite of public JWST ERS, ERO, and Cycle-1 programs, Mon. Not. R. Astron. Soc. 527 (3) (2024) 5004-5022, arXiv:2304.14469 [astro-ph.GA].

[1649] L.Y.A. Yung, R.S. Somerville, S.L. Finkelstein, S.M. Wilkins, J.P. Gardner, Are the ultra-high-redshift galaxies at $z > 10$ surprising in the context of standard galaxy formation models? Mon. Not. R. Astron. Soc. 527 (3) (2024) 5929-5948, arXiv:2304.04348 [astro-ph.GA].

[1650] Y.-Y. Wang, L. Lei, S.-P. Tang, G.-W. Yuan, Y.-Z. Fan, Digging into the ultraviolet luminosity functions of galaxies at high redshifts: galaxies evolution, reionization, and cosmological parameters, Astrophys. J. 975 (2) (2024) 285, arXiv:2405.09350 [astro-ph.CO].

[1651] N. Sabti, J.B. Muñoz, M. Kamionkowski, Insights from HST into ultramassive galaxies and early-universe cosmology, Phys. Rev. Lett. 132 (6) (2024) 061002, arXiv:2305.07049 [astro-ph.CO].
[1652] C.T. Donnan, D.J. McLeod, J.S. Dunlop, R.J. McLure, A.C. Carnall, R. Begley, F. Cullen, M.L. Hamadouche, R.A.A. Bowler, D. Magee, H.J. McCracken, B. Milvang-Jensen, A. Moneti, T. Targett, The evolution of the galaxy UV luminosity function at redshifts $z \approx 8-15$ from deep JWST and ground-based near-infrared imaging, Mon. Not. R. Astron. Soc. 518 (4) (2023) 6011–6040, arXiv:2207.12356 [astro-ph.GA].

[1653] L.J. Furtak, M. Shuntov, H. Atek, A. Zitrin, J. Richard, M.D. Lehnert, J. Chevallard, Constraining the physical properties of the first lensed z 9-16 galaxy candidates with JWST, Mon. Not. R. Astron. Soc. 519 (2) (2023) 3064–3075, arXiv:2208.05473 [astro-ph.GA].

[1654] J.A. Zavala, et al., Dusty starbursts masquerading as ultra-high redshift galaxies in JWST CEERS observations, Astrophys. J. Lett. 943 (2) (2023) L9, arXiv:2208.01816 [astro-ph.GA].

[1655] H. Yan, Z. Ma, C. Ling, C. Cheng, J.-s. Huang, First batch of $z \approx 11-20$ candidate objects revealed by the James webb space telescope early release observations on SMACS 0723-73, Astrophys. J. Lett. 942 (1) (2023) L9, arXiv:2207.11558 [astro-ph.GA].

[1656] I. Labbe, et al., A population of red candidate massive galaxies ~600 Myr after the Big Bang, Nature 616 (7956) (2023) 266–269, arXiv:2207.12446 [astro-ph.GA].

[1657] M. Xiao, et al., Accelerated formation of ultra-massive galaxies in the first billion years, Nature 635 (8038) (2024) 311–315, arXiv:2309.02492 [astro-ph.GA].

[1658] C.M. Casey, H.B. Akins, M. Shuntov, O. Ilbert, L. Paquereau, M. Franco, C.C. Hayward, S.L. Finkelstein, M. Boylan-Kolchin, B.E. Robertson, N. Allen, M. Brinch, O.R. Cooper, X. Ding, N.E. Drakos, A.L. Faisst, S. Fujimoto, S. Gillman, S. Harish, M. Hirschmann, S. Jin, J.S. Kartaltepe, A.M. Koekemoer, V. Kokorev, D. Liu, A.S. Long, G. Magdis, C. Marastan, C.L. Martin, H.J. McCracken, J. McKinney, B. Mobasher, J. Rhodes, R.M. Rich, D.B. Sanders, J.D. Silverman, S. Toft, A.P. Vijayan, J.R. Weaver, S.M. Wilkins, L. Yang, J.A. Zavala, COSMOS-web: intrinsically luminous $z \ge 10$ galaxy candidates test early stellar mass assembly, Astrophys. J. 965 (1) (2024) 98, arXiv:2308.10932 [astro-ph.GA].

[1659] A. Weibel, P.A. Oesch, L. Barrufet, R. Gottumukkala, R.S. Ellis, P. Santini, J.R. Weaver, N. Allen, R. Bouwens, R.A.A. Bowler, G. Brammer, A.C. Carnall, F. Cullen, P. Dayal, M. Dickinson, C.T. Donnan, J.S. Dunlop, M. Giavalisco, N.A. Grogin, G.D. Illingworth, A.M. Koekemoer, I. Labbe, D. Marchesini, D.J. McLeod, R.J. McLure, R.P. Naidu, P.G. Pérez-González, M. Shuntov, M. Stefanon, S. Toft, M. Xiao, Galaxy build-up in the first 1.5 Gyr of cosmic history: insights from the stellar mass function at $z=4-9$ from JWST NIRCam observations, Mon. Not. R. Astron. Soc. 533 (2) (2024) 1808–1838, arXiv:2403.08872 [astro-ph.GA].

[1660] K. Chworowsky, S.L. Finkelstein, M. Boylan-Kolchin, E.J. McGrath, K.G. Iyer, C. Papovich, M. Dickinson, A.J. Taylor, L.Y.A. Yung, P. Arrabal Haro, M.B. Bagley, B.E. Backhaus, R. Bhatawdekar, Y. Cheng, N.J. Cleri, J.W. Cole, M.C. Cooper, L. Costantin, A. Dekel, M. Franco, S. Fujimoto, C.C. Hayward, B.W. Holwerda, M. Huertas-Company, M. Hirschmann, T.A. Hutchison, A.M. Koekemoer, R.L. Larson, Z. Li, A.S. Long, R.A. Lucas, N. Pirzkal, G. Rodighiero, R.S. Somerville, B.N. Vanderhoof, A. de la Vega, S. M. Wilkins, G. Yang, J.A. Zavala, Evidence for a shallow evolution in the volume densities of massive galaxies at $z=4-8$ from CEERS, Astron. J. 168 (3) (2024) 113, arXiv:2311.14804 [astro-ph.GA].

[1661] C.C. Lovell, I. Harrison, Y. Harikane, S. Tacchella, S.M. Wilkins, Extreme value statistics of the halo and stellar mass distributions at high redshift: are JWST results in tension with ΛCDM? Mon. Not. R. Astron. Soc. 518 (2) (2022) 2511–2520, arXiv:2208.10479 [astro-ph.GA].

[1662] M. Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nat. Astron. 7 (6) (2023) 731–735, arXiv:2208.01611 [astro-ph.CO].

[1663] M. Forconi, Ruchika, A. Melchiorri, O. Mena, N. Menci, Do the early galaxies observed by JWST disagree with Planck's CMB polarization measurements? J. Cosmol. Astropart. Phys. 10 (2023) 012, arXiv:2306.07781 [astro-ph.CO].

[1664] J. Lu, L. Wang, X. Chen, D. Rubin, S. Perlmutter, D. Baade, J. Mould, J. Vinko, E. Regós, A.M. Koekemoer, Constraints on cosmological parameters with a sample of type ia supernovae from JWST, Astrophys. J. 941 (1) (2022) 71, arXiv:2210.00746 [astro-ph.CO].

[1665] J.D.R. Pierel, et al., Testing for intrinsic type ia supernova luminosity evolution at $z > 2$ with JWST, Astrophys. J. Lett. 981 (1) (2025) L9, arXiv:2411.11953 [astro-ph.CO].

[1666] J. Vinko, E. Regos, SN 2023adsy – a normal Type Ia Supernova at $z=2.9$, discovered by JWST, 2024, arXiv:2411.10427 [astro-ph.HE].

[1667] D.A. Coulter, et al., Discovery of a likely Type II SN at $z=3.6$ with JWST, 2025, arXiv:2501.05513 [astro-ph.HE].

[1668] T.J. Moriya, et al., Properties of high-redshift Type II supernovae discovered by the JADES transient survey, 2025, arXiv:2501.08969 [astro-ph.HE].

[1669] T.J. Moriya, Y. Harikane, A.K. Inoue, Constraint on the event rate of general relativistic instability supernovae from the early JWST deep field data, Mon. Not. R. Astron. Soc. 526 (2) (2023) 2400–2402, arXiv:2309.12049 [astro-ph.HE].

[1670] M.G. Dainotti, et al., A New Master Supernovae Ia sample and the investigation of the $H_0$ tension, 2025, arXiv:2501.11772 [astro-ph.CO].

[1671] P.M.M. Alonso, C. Escamilla-Rivera, R. Sandoval-Orozco, Constraining dark energy cosmologies with spatial curvature using Supernovae JWST forecasting, J. Cosmol. Astropart. Phys. 04 (2024) 084, arXiv:2309.12292 [astro-ph.CO].

[1672] C.C. Williams, S. Alberts, Z. Ji, K.N. Hainline, J. Lyu, G. Rieke, R. Endsley, K.A. Suess, F. Sun, B.D. Johnson, M. Florian, I. Shivaei, W. Rujopakarn, W.M. Baker, R. Bhatawdekar, K. Boyett, A.J. Bunker, A.J. Cameron, S. Carniani, S. Charlot, E. Curtis-Lake, C. DeCoursey, A. de Graaff, E. Egami, D.J. Eisenstein, J.L. Gibson, R. Hausen, J.M. Helton, R. Maiolino, M.V. Maseda, E.J. Nelson, P.G. Pérez-González, M.J. Rieke, B.E. Robertson, A. Saxena, S. Tacchella, C.N.A. Willmer, C.J. Willott, The galaxies missed by hubble and ALMA: the contribution of extremely red galaxies to the cosmic census at $3 < z < 8$, Astrophys. J. 968 (1) (2024) 34, arXiv:2311.07483 [astro-ph.GA].

[1673] C.L. Steinhardt, V. Kokorev, V. Rusakov, E. Garcia, A. Sneppen, Templates for fitting photometry of ultra-high-redshift galaxies, Astrophys. J. Lett. 951 (2) (2023) L40, arXiv:2208.07879 [astro-ph.GA].

[1674] R. Endsley, D.P. Stark, L. Whitler, M.W. Topping, Z. Chen, A. Plat, J. Chisholm, S. Charlot, A JWST/NIRCam study of key contributors to reionization: the star-forming and ionizing properties of UV-faint z 7-8 galaxies, Mon. Not. R. Astron. Soc. 524 (2) (2023) 2312–2330, arXiv:2208.14999 [astro-ph.GA].

[1675] P. Arrabal Haro, M. Dickinson, S.L. Finkelstein, S. Fujimoto, V. Fernández, J.S. Kartaltepe, I. Jung, J.W. Cole, D. Burgarella, K. Chworowsky, T.A. Hutchison, A.M. Morales, C. Papovich, R.C. Simons, R.O. Amorín, B.E. Backhaus, M.B. Bagley, L. Bisigello, A. Calabrò, M. Castellano, N.J. Cleri, R. Davé, A. Dekel, H.C. Ferguson, A. Fontana, E. Gawiser, M. Giavalisco, S. Harish, N.P. Hathi, M. Hirschmann, B.W. Holwerda, M. Huertas-Company, A.M. Koekemoer, R.L. Larson, R.A. Lucas, B. Mobasher, P.G. Pérez-González, N. Pirzkal, C. Rose, P. Santini, J.R. Trump, A. de la Vega, X. Wang, B.J. Weiner, S.M. Wilkins, G. Yang, L.Y.A. Yung, J.A. Zavala, Spectroscopic confirmation of CEERS NIRCam-selected galaxies at $z \approx 8-10$, Astrophys. J. Lett. 951 (1) (2023) L22, arXiv:2304.05378 [astro-ph.GA].

[1676] B. Wang, S. Fujimoto, I. Labbé, L.J. Furtak, T.B. Miller, D.J. Setton, A. Zitrin, H. Atek, R. Bezanson, G. Brammer, J. Leja, P.A. Oesch, S.H. Price, I. Chemernyska, S.E. Cutler, P. Dayal, P. van Dokkum, A.D. Goulding, J.E. Greene, Y. Fudamoto, G. Khullar, V. Kokorev, D. Marchesini, R. Pan, J.R. Weaver, K.E. Whitaker, C.C. Williams, UNCOVER: illuminating the early universe JWST/NIRSpec confirmation of $z \ge 12$ galaxies, Astrophys. J. Lett. 957 (2) (2023) L34, arXiv:2308.03745 [astro-ph.GA].

[1677] B.E. Robertson, et al., Identification and properties of intense star-forming galaxies at redshifts $z \ge 10$, Nat. Astron. 7 (5) (2023) 611–621, arXiv:2212.04480 [astro-ph.GA].

[1678] E. Curtis-Lake, S. Carniani, A. Cameron, S. Charlot, P. Jakobsen, R. Maiolino, A. Bunker, J. Witstok, R. Smit, J. Chevallard, C. Willott, P. Ferruit, S. Arribas, N. Bonaventura, M. Curti, F. D'Eugenio, M. Franx, G. Giardino, T.J. Looser, N. Lützendorf, M.V. Maseda, T. Rawle, H.-W. Rix, R. Rodríguez del Pino, H. Übler, M. Sirianni, A. Dressler, E. Egami, D.J. Eisenstein, R. Endsley, K. Stark, S. Tacchella, C.C. Williams, C.N.A. Willmer, R. Bhatawdekar, R. Bowler, K. Boyett, Z. Chen, A. de Graaff, J.M. Helton, R.E. Hviding, G.C. Jones, N. Kumari, J. Lyu, E. Nelson, M. Perna, L. Sandles, A. Saxena, K.A. Suess, F. Sun, M.W. Topping, I.E.B. Wallace, L. Whitler, Spectroscopic confirmation of four metal-poor galaxies at $z=10.3-13.2$, Nat. Astron. 7 (2023) 622–632, arXiv:2212.04568 [astro-ph.GA].

[1679] S. Fujimoto, et al., CEERS spectroscopic confirmation of NIRCam-selected $z \ge 8$ galaxy candidates with JWST/NIRSpec: initial characterization of their properties, Astrophys. J. Lett. 949 (2) (2023) L25, arXiv:2301.09482 [astro-ph.GA].

[1680] S. Carniani, K. Hainline, F. D'Eugenio, D.J. Eisenstein, P. Jakobsen, J. Witstok, B.D. Johnson, J. Chevallard, M. Maiolino, J.M. Helton, C. Willott, B. Robertson, S. Alberts, S. Arribas, W.M. Baker, R. Bhatawdekar, K. Boyett, A.J. Bunker, A.J. Cameron, P.A. Cargile, S. Charlot, M. Curti, E. Curtis-Lake, E. Egami, G. Giardino, K. Isaak, Z. Ji, G.C. Jones, N. Kumari, M.V. Maseda, E. Parlanti, P.G. Pérez-González, T. Rawle, G. Rieke, M. Rieke, B.R. Del Pino, A. Saxena, J. Scholtz, R. Smit, F. Sun, S. Tacchella, H. Übler, G. Venturi, C.C. Williams, C.N.A. Willmer, Spectroscopic confirmation of two luminous galaxies at a redshift of 14, Nature 633 (8029) (2024) 318–322, arXiv:2405.18485 [astro-ph.GA].

[1681] M. Castellano, L. Napolitano, A. Fontana, G. Roberts-Borsani, T. Treu, E. Vanzella, J.A. Zavala, P. Arrabal Haro, A. Calabrò, M. Llerena, S. Mascia, E. Merlin, D. Paris, L. Pentericci, P. Santini, T.J.L.C. Bakx, P. Bergamini, G. Cupani, M. Dickinson, A.V. Filippenko, K. Glazebrook, C. Grillo, P.L. Kelly, M.A. Malkan, C.A. Mason, T. Morishita, T. Nanayakkara, P. Rosati, E. Sani, X. Wang, I. Yoon, JWST NIRSpec spectroscopy of the remarkable bright galaxy GHZ2/GLASS-z12 at redshift 12.34, Astrophys. J. 972 (2) (2024) 143, arXiv:2403.10238 [astro-ph.GA].

[1682] C. Giménez-Arteaga, et al., Spatially resolved properties of galaxies at $5 < z < 9$ in the SMACS 0723 JWST ERO field, Astrophys. J. 948 (2) (2023) 126, arXiv:2212.08670 [astro-ph.GA].

[1683] A. Ferrara, Super-early JWST galaxies, outflows, and $\Lambda\alpha$ visibility in the Epoch of Reionization, Astron. Astrophys. 684 (2024) A207, arXiv:2310.12197 [astro-ph.GA].
[1684] C.A. Mason, M. Trenti, T. Treu, The brightest galaxies at cosmic dawn, Mon. Not. R. Astron. Soc. 521 (1) (2023) 497–503, arXiv:2207.14808 [astro-ph.GA].

[1685] A. Kravtsov, V. Belokurov, Stochastic star formation and the abundance of $z > 10$ UV-bright galaxies, 2024, arXiv:2405.04578 [astro-ph.GA].

[1686] S. Hegde, M.M. Wyatt, S.R. Furlanetto, A hidden population of active galactic nuclei can explain the overabundance of luminous $z > 10$ objects observed by JWST, J. Cosmol. Astropart. Phys. 08 (2024) 025, arXiv:2405.01629 [astro-ph.GA].

[1687] V. Gelli, C. Mason, C.C. Hayward, The impact of mass-dependent stochasticity at cosmic dawn, Astrophys. J. 975 (2) (2024) 192, arXiv:2405.13108 [astro-ph.GA].

[1688] G. Desprez, et al., ΛCDM not dead yet: massive high-z Balmer break galaxies are less common than previously reported, Mon. Not. R. Astron. Soc. 530 (3) (2024) 2935–2952, arXiv:2310.03063 [astro-ph.GA].

[1689] A. Dekel, K.C. Sarkar, Y. Birnboim, N. Mandelker, Z. Li, Efficient formation of massive galaxies at cosmic dawn by feedback-free starbursts, Mon. Not. R. Astron. Soc. 523 (3) (2023) 3201–3218, arXiv:2303.04827 [astro-ph.GA].

[1690] A. Ferrara, A. Pallottini, P. Dayal, On the stunning abundance of super-early, luminous galaxies revealed by JWST, Mon. Not. R. Astron. Soc. 522 (3) (2023) 3986–3991, arXiv:2208.00720 [astro-ph.GA].

[1691] B. Wang, J. Leja, H. Atek, I. Labbé, Y. Li, R. Bezanson, G. Brammer, S.E. Cutler, P. Dayal, L.J. Furtak, J.E. Greene, V. Kokorev, R. Pan, S.H. Price, K.A. Suess, J.R. Weaver, K.E. Whitaker, C.C. Williams, Quantifying the effects of known unknowns on inferred high-redshift galaxy properties: burstiness, IMF, and nebular physics, Astrophys. J. 963 (1) (2024) 74, arXiv:2310.06781 [astro-ph.GA].

[1692] D. Narayanan, S. Lower, P. Torrey, G. Brammer, W. Cui, R. Davé, K.G. Iyer, Q. Li, C.C. Lovell, L.V. Sales, D.P. Stark, F. Marinacci, M. Vogelsberger, Outshining by recent star formation prevents the accurate measurement of high-z galaxy stellar masses, Astrophys. J. 961 (1) (2024) 73, arXiv:2306.10118 [astro-ph.GA].

[1693] R.K. Cochrane, H. Katz, R. Begley, C.C. Hayward, P.N. Best, High-z stellar masses can be recovered robustly with JWST photometry, Astrophys. J. 978 (2) (2025) L42, arXiv:2412.02622 [astro-ph.GA].

[1694] M. Haslbauer, P. Kroupa, A.H. Zonoozi, H. Haghi, Has JWST already falsified dark-matter-driven galaxy formation? Astrophys. J. Lett. 939 (2) (2022) L31, arXiv:2210.14915 [astro-ph.GA].

[1695] E.M. Ventura, Y. Qin, S. Balu, J.S.B. Wyithe, Semi-analytic modelling of Pop. III star formation and metallicity evolution – I. Impact on the UV luminosity functions at $z = 9–16$, Mon. Not. R. Astron. Soc. 529 (1) (2024) 628–646, arXiv:2401.07396 [astro-ph.GA].

[1696] A. Trinca, R. Schneider, R. Valiante, L. Graziani, A. Ferrotti, K. Omukai, S. Chon, Exploring the nature of UV-bright $z \ge 10$ galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF? Mon. Not. R. Astron. Soc. 529 (4) (2024) 3563–3581, arXiv:2305.04944 [astro-ph.GA].

[1697] E.E. Salpeter, The Luminosity function and stellar evolution, Astrophys. J. 121 (1955) 161–167.

[1698] E.R. Cueto, A. Hutter, P. Dayal, S. Gottlöber, K.E. Heintz, C. Mason, M. Trebitsch, G. Yepes, ASTRAEUS - IX. Impact of an evolving stellar initial mass function on early galaxies and reionisation, Astron. Astrophys. 686 (2024) A138, arXiv:2312.12109 [astro-ph.GA].

[1699] S. Tacchella, S.L. Finkelstein, M. Bagley, M. Dickinson, H.C. Ferguson, M. Giavalisco, L. Graziani, N.A. Grogin, N. Hathi, T.A. Hutchison, I. Jung, A.M. Koekemoer, R.L. Larson, C. Papovich, N. Pirzkal, S.a. Rojas-Ruiz, M. Song, R. Schneider, R.S. Somerville, S.M. Wilkins, L.Y.A. Yung, On the stellar populations of galaxies at $z=9-11$: the growth of metals and stellar mass at early times, Astrophys. J. 927 (2) (2022) 170, arXiv:2111.05351 [astro-ph.GA].

[1700] L. Whitler, D.P. Stark, R. Endsley, J. Leja, S. Charlot, J. Chevallard, Star formation histories of UV-luminous galaxies at $z \approx 6.8$: implications for stellar mass assembly at early cosmic times, Mon. Not. R. Astron. Soc. 519 (4) (2023) 5859–5881, arXiv:2206.05315 [astro-ph.GA].

[1701] F. Iocco, L. Visinelli, Compatibility of JWST results with exotic halos, Phys. Dark Univ. 44 (2024) 101496, arXiv:2403.13068 [astro-ph.CO].

[1702] A. Pallottini, A. Ferrara, Stochastic star formation in early galaxies: Implications for the James Webb Space Telescope, Astron. Astrophys. 677 (2023) L4, arXiv:2307.03219 [astro-ph.GA].

[1703] D. Ceverino, Y. Nakazato, N. Yoshida, R.S. Klessen, S.C.O. Glover, Redshift-dependent galaxy formation efficiency at $z=5–13$ in the First-Light Simulations, Astron. Astrophys. 689 (2024) A244, arXiv:2404.02537 [astro-ph.GA].

[1704] C. Turner, S. Tacchella, F. D'Eugenio, S. Carniani, M. Curti, K. Glazebrook, B.D. Johnson, S. Lim, T. Looser, R. Maiolino, T. Nanayakkara, J. Wan, Age-dating early quiescent galaxies: high star formation efficiency, but consistent with direct, higher-redshift observations, Mon. Not. R. Astron. Soc. 537 (2) (2025) 1826–1848, arXiv:2410.05377 [astro-ph.GA].

[1705] T. Harvey, C.J. Conselice, N.J. Adams, D. Austin, I. Juodžbalis, J. Trussler, Q. Li, K. Ormerod, L. Ferreira, C.C. Lovell, Q. Duan, L. Westcott, H. Harris, R. Bhatawdekar, D. Coe, S.H. Cohen, J. Caruana, C. Cheng, S.P. Driver, B. Frye, L.J. Furtak, N.A. Grogin, N.P. Hathi, B.W. Holwerda, R.A. Jansen, A.M. Koekemoer, M.A. Marshall, M. Nonino, A.P. Vijayan, S.M. Wilkins, R. Windhorst, C.N.A. Willmer, H. Yan, A. Zitrin, EPOCHS. IV. SED modeling assumptions and their impact on the stellar mass function at $6.5 \le z \le 13.5$ using PEARLS and public JWST observations, Astrophys. J. 978 (1) (2025) 89, arXiv:2403.03908 [astro-ph.GA].

[1706] Y. Chen, H.J. Mo, K. Wang, Massive dark matter haloes at high redshift: implications for observations in the JWST era, Mon. Not. R. Astron. Soc. 526 (2) (2023) 2542–2559, arXiv:2304.13890 [astro-ph.GA].

[1707] J. Wang, Z. Huang, L. Huang, J. Liu, Quantifying the tension between cosmological models and JWST red candidate massive galaxies, Res. Astron. Astrophys. 24 (4) (2024) 045001, arXiv:2311.02866 [astro-ph.CO].

[1708] Y. Qin, S. Balu, J.S.B. Wyithe, Implications of $z \ge 12$ JWST galaxies for galaxy formation at high redshift, Mon. Not. R. Astron. Soc. 526 (1) (2023) 1324–1342, arXiv:2305.17959 [astro-ph.GA].

[1709] H. Atek, M. Shuntov, L.J. Furtak, J. Richard, J.-P. Kneib, G. Mahler, A. Zitrin, H.J. McCracken, S. Charlot, J. Chevallard, I. Chemerynska, Revealing galaxy candidates out to $z 16$ with JWST observations of the lensing cluster SMACS0723, Mon. Not. R. Astron. Soc. 519 (1) (2023) 1201–1220, arXiv:2207.12338 [astro-ph.GA].

[1710] R. Navarro-Carrera, P. Rinaldi, K.I. Caputi, E. Iani, V. Kokorev, S.E. van Mierlo, Constraints on the faint end of the galaxy stellar mass function at $z \approx 4–8$ from deep JWST data, Astrophys. J. 961 (2) (2024) 207, arXiv:2305.16141 [astro-ph.GA].

[1711] M. Maggiore, A. Riotto, The Halo mass function from excursion set theory. II. The diffusing barrier, Astrophys. J. 717 (2010) 515–525, arXiv:0903.1250 [astro-ph.CO].

[1712] I.E. Achitouv, P.S. Corasaniti, Primordial bispectrum and trispectrum contributions to the non-gaussian excursion set halo mass function with diffusive drifting barrier, Phys. Rev. D 86 (2012) 083011, arXiv:1207.4796 [astro-ph.CO].

[1713] D. Reed, R. Bower, C. Frenk, A. Jenkins, T. Theuns, The halo mass function from the dark ages through the present day, Mon. Not. R. Astron. Soc. 374 (2007) 2–15, arXiv:astro-ph/0607150.

[1714] S. Basilakos, M. Plionis, J.A.S. Lima, Confronting dark energy models using galaxy cluster number counts, Phys. Rev. D 82 (2010) 083517, arXiv:1006.3418 [astro-ph.CO].

[1715] S. Bhattacharya, K. Heitmann, M. White, Z. Lukic, C. Wagner, S. Habib, Mass function predictions beyond LCDM, Astrophys. J. 732 (2011) 122, arXiv:1005.2239 [astro-ph.CO].

[1716] S. Tacchella, S. Bose, C. Conroy, D.J. Eisenstein, B.D. Johnson, A redshift-independent efficiency model: star formation and stellar masses in dark matter halos at $z \ge 4$, Astrophys. J. 868 (2) (2018) 92, arXiv:1806.03299 [astro-ph.GA].

[1717] S.W. Allen, R.W. Schmidt, H. Ebeling, A.C. Fabian, L. van Speybroeck, Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters, Mon. Not. R. Astron. Soc. 353 (2004) 457, arXiv:astro-ph/0405340.

[1718] A. Vikhlinin, A. Kravtsov, W. Forman, C. Jones, M. Markevitch, S.S. Murray, L. Van Speybroeck, Chandra sample of nearby relaxed galaxy clusters: Mass, gas fraction, and mass-temperature relation, Astrophys. J. 640 (2006) 691–709, arXiv:astro-ph/0507092.

[1719] A.V. Kravtsov, D. Nagai, A.A. Vikhlinin, Effects of cooling and star formation on the baryon fractions in clusters, Astrophys. J. 625 (2005) 588–598, arXiv:astro-ph/0501227.

[1720] S. Borgani, A. Kravtsov, Cosmological simulations of galaxy clusters, Adv. Sci. Lett. 4 (2011) 204, arXiv:0906.4370 [astro-ph.CO].

[1721] A.B. Mantz, S.W. Allen, R.G. Morris, D.A. Rapetti, D.E. Applegate, P.L. Kelly, A. von der Linden, R.W. Schmidt, Cosmology and astrophysics from relaxed galaxy clusters – II. Cosmological constraints, Mon. Not. R. Astron. Soc. 440 (3) (2014) 2077–2098, arXiv:1402.6212 [astro-ph.CO].

[1722] U. Maio, M. Viel, The first billion years of a warm dark matter universe, Mon. Not. R. Astron. Soc. 446 (2015) 2760–2775, arXiv:1409.6718 [astro-ph.CO].

[1723] K. Panchal, S. Desai, Comparison of ΛCDM and $Rh = ct$ with updated galaxy cluster fgas measurements using Bayesian inference, JHEAp 43 (2024) 15–19, arXiv:2401.11138 [astro-ph.CO].

[1724] H.-L. Huang, J.-Q. Jiang, Y.-S. Piao, High-redshift JWST massive galaxies and the initial clustering of supermassive primordial black holes, Phys. Rev. D 110 (10) (2024) 103540, arXiv:2407.15781 [astro-ph.CO].

[1725] G.-W. Yuan, L. Lei, Y.-Z. Wang, B. Wang, Y.-Y. Wang, C. Chen, Z.-Q. Shen, Y.-F. Cai, Y.-Z. Fan, Rapidly growing primordial black holes as seeds of the massive high-redshift JWST Galaxies, Sci. China Phys. Mech. Astron. 67 (10) (2024) 109512, arXiv:2303.09391 [astro-ph.CO].

[1726] B. Carr, S. Clesse, J. Garcia-Bellido, M. Hawkins, F. Kuhnel, Observational evidence for primordial black holes: A positivist perspective, Phys. Rep. 1054 (2024) 1–68, arXiv:2306.03903 [astro-ph.CO].

[1727] A.D. Dolgov, Tension between HST/JWST and ΛCDM cosmology, PBH, and antimatter in the galaxy, in: 14th Frascati workshop on Multifrequency Behaviour of High Energy Cosmic Sources, 2023, arXiv:2310.00671 [astro-ph.CO].

[1728] A. Trinca, R. Schneider, R. Maiolino, R. Valiante, L. Graziani, M. Volonteri, Seeking the growth of the first black hole seeds with JWST, Mon. Not. R. Astron. Soc. 519 (3) (2023) 4753–4764, arXiv:2211.01389 [astro-ph.GA].
[1729] F. Pacucci, B. Nguyen, S. Carniani, R. Maiolino, X. Fan, JWST CEERS and JADES active galaxies at z=4-7 violate the local M⁻M⁰ relation at >3σ: implications for low-mass black holes and seeding models, Astrophys. J. Lett. 957 (1) (2023) L3, arXiv:2308.12331 [astro-ph.GA].

[1730] R. Maiolino, et al., A small and vigorous black hole in the early Universe, Nature 627 (8002) (2024) 59–63, arXiv:2305.12492 [astro-ph.GA]; Nature 630 (2024) E2 (erratum).

[1731] H. Mo, Y. Chen, H. Wang, A two-phase model of galaxy formation: I. The growth of galaxies and supermassive black holes, Mon. Not. R. Astron. Soc. 532 (4) (2024) 3808–3838, arXiv:2311.05030 [astro-ph.GA].

[1732] CEERS Team Collaboration, R.L. Larson, et al., A CEERS discovery of an accreting supermassive black hole 570 Myr after the big bang: identifying a progenitor of massive z > 6 quasars, Astrophys. J. Lett. 953 (2) (2023) L29, arXiv:2303.08918 [astro-ph.GA].

[1733] A. Bogdan, et al., Evidence for heavy-seed origin of early supermassive black holes from a z≈10 X-ray quasar, Nat. Astron. 8 (1) (2024) 126–133, arXiv: 2305.15458 [astro-ph.GA].

[1734] R. Schneider, R. Valiante, A. Trinca, L. Graziani, M. Volonteri, R. Maiolino, Are we surprised to find SMBHs with JWST at z ≥ 9? Mon. Not. R. Astron. Soc. 526 (3) (2023) 3250–3261, arXiv:2305.12504 [astro-ph.GA].

[1735] H.-L. Huang, Y.-T. Wang, Y.-S. Piao, Supermassive primordial black holes for the GHZ9 and UHZ1 observed by the JWST, 2024, arXiv:2410.05891 [astro-ph.GA].

[1736] A. Trinca, R. Valiante, R. Schneider, I. Juodžbalis, R. Maiolino, L. Graziani, A. Lupi, P. Natarajan, M. Volonteri, T. Zana, Episodic super-eddington accretion as a clue to overmassive black holes in the early universe, 2024, arXiv: 2412.14248 [astro-ph.GA].

[1737] S. Kumar, N. Weiner, Early galaxies from rare inflationary processes and JWST observations, 2025, arXiv:2502.08701 [astro-ph.CO].

[1738] P. Parashari, R. Laha, Primordial power spectrum in light of JWST observations of high redshift galaxies, Mon. Not. R. Astron. Soc. 526 (1) (2023) L63–L69, arXiv:2305.00999 [astro-ph.CO].

[1739] S. Hirano, N. Yoshida, Early structure formation from primordial density fluctuations with a blue, tilted power spectrum: high-redshift galaxies, Astrophys. J. 963 (1) (2024) 2, arXiv:2306.11993 [astro-ph.GA].

[1740] H. Padmanabhan, A. Loeb, Alleviating the need for exponential evolution of JWST galaxies in 10¹⁰ M☉ haloes at z > 10 by a modified ΛCDM power spectrum, Astrophys. J. Lett. 953 (1) (2023) L4, arXiv:2306.04684 [astro-ph.CO].

[1741] M. Biagetti, G. Franciolini, A. Riotto, High-redshift JWST observations and primordial non-gaussianity, Astrophys. J. 944 (2) (2023) 113, arXiv:2210. 04812 [astro-ph.CO].

[1742] M. De Laurentis, P. Salucci, The accurate mass distribution of M87, the giant galaxy with imaged shadow of its supermassive black hole, as a portal to new physics, Astrophys. J. 929 (1) (2022) 17, arXiv:2206.01997 [astro-ph.CO].

[1743] S.-Y. Guo, M. Khlopov, X. Liu, L. Wu, Y. Wu, B. Zhu, Footprints of axion-like particle in pulsar timing array data and James Webb Space Telescope observations, Sci. China Phys. Mech. Astron. 67 (11) (2024) 111011, arXiv: 2306.17022 [hep-ph].

[1744] G. Hütsi, M. Raidal, J. Urrutia, V. Vaskonen, H. Veermäe, Did JWST observe imprints of axion miniclusters or primordial black holes? Phys. Rev. D 107 (4) (2023) 043502, arXiv:2211.02651 [astro-ph.CO].

[1745] S. Bird, C.-F. Chang, Y. Cui, D. Yang, Enhanced early galaxy formation in JWST from axion dark matter? Phys. Lett. B 858 (2024) 139062, arXiv:2307.10302 [hep-ph].

[1746] Y. Gong, B. Yue, Y. Cao, X. Chen, Fuzzy dark matter as a solution to reconcile the stellar mass density of high-z massive galaxies and reionization history, Astrophys. J. 947 (1) (2023) 28, arXiv:2209.13757 [astro-ph.CO].

[1747] A. Zhitnitsky, Structure formation paradigm and axion quark nugget dark matter model, Phys. Dark Univ. 40 (2023) 101217, arXiv:2302.00010 [hep-ph].

[1748] Q. Zhang, S. Li, X.-H. Tan, J.-Q. Xia, Constraints on primordial magnetic fields from high redshift stellar mass density, Astrophys. J. 972 (1) (2024) 117, arXiv:2408.03584 [astro-ph.CO].

[1749] H. Jiao, R. Brandenberger, A. Refregier, Early structure formation from cosmic string loops in light of early JWST observations, Phys. Rev. D 108 (4) (2023) 043510, arXiv:2304.06429 [astro-ph.CO].

[1750] H. Jiao, R. Brandenberger, A. Refregier, N-body simulation of early structure formation from cosmic string loops, Phys. Rev. D 109 (12) (2024) 123524, arXiv:2402.06235 [astro-ph.CO].

[1751] S.M. Koehler, H. Jiao, R. Kannan, Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies, 2024, arXiv:2412.00182 [astro-ph.CO].

[1752] P. Dayal, S.K. Giri, Warm dark matter constraints from the JWST, Mon. Not. R. Astron. Soc. 528 (2) (2024) 2784–2789, arXiv:2303.14239 [astro-ph.CO].

[1753] U. Maio, M. Viel, JWST high-redshift galaxy constraints on warm and cold dark matter models, Astron. Astrophys. 672 (2023) A71, arXiv:2211.03620 [astro-ph.CO].

[1754] G. Gandolfi, A. Lapi, T. Ronconi, L. Danese, Astroparticle constraints from the cosmic star formation rate density at high redshift: current status and forecasts for JWST, Universe 8 (11) (2022) 589, arXiv:2211.02840 [astro-ph.CO].

[1755] M. Forconi, W. Giarè, O. Mena, Ruchika, E. Di Valentino, A. Melchiorri, R.C. Nunes, A double take on early and interacting dark energy from JWST, J. Cosmol. Astropart. Phys. 05 (2024) 097, arXiv:2312.11074 [astro-ph.CO].

[1756] A. Klypin, V. Poulin, F. Prada, J. Primack, M. Kamionkowski, V. Avila-Reese, A. Rodriguez-Puebla, P. Behroozi, D. Hellinger, T.L. Smith, Clustering and halo abundances in early dark energy cosmological models, Mon. Not. R. Astron. Soc. 504 (1) (2021) 769–781, arXiv:2006.14910 [astro-ph.CO].

[1757] X. Shen, M. Vogelsberger, M. Boylan-Kolchin, S. Tacchella, R.P. Naidu, Early galaxies and early dark energy: a unified solution to the hubble tension and puzzles of massive bright galaxies revealed by JWST, Mon. Not. R. Astron. Soc. 533 (4) (2024) 3923–3936, arXiv:2406.15548 [astro-ph.GA].

[1758] J.-Q. Jiang, W. Liu, H. Zhan, B. Hu, Explanation of high redshift luminous galaxies from JWST by an early dark energy model, Phys. Rev. D 111 (2) (2025) 023519, arXiv:2409.19941 [astro-ph.CO].

[1759] N. Menci, M. Castellano, P. Santini, E. Merlin, A. Fontana, F. Shankar, High-redshift galaxies from early JWST observations: constraints on dark energy models, Astrophys. J. Lett. 938 (1) (2022) L5, arXiv:2208.11471 [astro-ph.CO].

[1760] N. Menci, A.A. Sen, M. Castellano, The excess of JWST bright galaxies: a possible origin in the ground state of dynamical dark energy in the light of DESI 2024 data, Astrophys. J. 976 (2) (2024) 227, arXiv:2410.22940 [astro-ph.CO].

[1761] N. Menci, S.A. Adil, U. Mukhopadhyay, A.A. Sen, S. Vagnozzi, Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies, J. Cosmol. Astropart. Phys. 07 (2024) 072, arXiv:2401.12659 [astro-ph.CO].

[1762] S.A. Adil, U. Mukhopadhyay, A.A. Sen, S. Vagnozzi, Dark energy in light of the early JWST observations: case for a negative cosmological constant? J. Cosmol. Astropart. Phys. 10 (2023) 072, arXiv:2307.12763 [astro-ph.CO].

[1763] E.A. Paraskevas, L. Perivolaropoulos, The density of virialized clusters as a probe of dark energy, Mon. Not. R. Astron. Soc. 531 (1) (2024) 1021–1033, arXiv:2308.07046 [astro-ph.CO].

[1764] P. Wang, B.-Y. Su, L. Zu, Y. Yang, L. Feng, Exploring the dark energy equation of state with JWST, Eur. Phys. J. Plus 139 (8) (2024) 711, arXiv:2307.11374 [astro-ph.CO].

[1765] M. Jöever, J. Einasto, E. Tago, Spatial distribution of galaxies and of clusters of galaxies in the southern galactic hemisphere, Mon. Not. R. Astro. Soc. 185 (1978) 357–370.

[1766] S.A. Gregory, L.A. Thompson, The Coma/A1367 supercluster and its environs, Astrophys. J. 222 (1978) 784–799.

[1767] R.P. Kirshner, A. Oemler Jr., P.L. Schechter, S.A. Shteman, A million cubic megaparsec void in Bootes, Astrophys. J. Lett. 248 (1981) L57–60.

[1768] V. de Lapparent, M.J. Geller, J.P. Huchra, A Slice of the universe, Astrophys. J. Lett. 302 (1986) L1–L5.

[1769] Y.B. Zeldovich, J. Einasto, S.F. Shandarin, Giant voids in the universe, Nature 300 (1982) 407–413.

[1770] P.J.E. Peebles, The void phenomenon, Astrophys. J. 557 (2001) 495–504, arXiv:astro-ph/0101127.

[1771] N. Padilla, D. Paz, M. Lares, L. Ceccarelli, D.G. Lambas, Y.-C. Cai, B. Li, Void dynamics, IAU Symp. 308 (2014) 530–537, arXiv:1410.8186 [astro-ph.CO].

[1772] A. Pisani, et al., Cosmic voids: a novel probe to shed light on our Universe, 2019, arXiv:1903.05161 [astro-ph.CO].

[1773] N. Hamaus, B.D. Wandelt, P.M. Sutter, G. Lavaux, M.S. Warren, Cosmology with void-galaxy correlations, Phys. Rev. Lett. 112 (4) (2014) 041304, arXiv: 1307.2571 [astro-ph.CO].

[1774] K.C. Chan, N. Hamaus, V. Desjacques, Large-scale clustering of cosmic voids, Phys. Rev. D 90 (10) (2014) 103521, arXiv:1409.3849 [astro-ph.CO].

[1775] G. Pollina, N. Hamaus, K. Dolag, J. Weller, M. Baldi, L. Moscardini, On the linearity of tracer bias around voids, Mon. Not. R. Astron. Soc. 469 (1) (2017) 787–799, arXiv:1610.06176 [astro-ph.CO].

[1776] S. Contarini, T. Ronconi, F. Marulli, L. Moscardini, A. Veropalumbo, M. Baldi, Cosmological exploitation of the size function of cosmic voids identified in the distribution of biased tracers, Mon. Not. R. Astron. Soc. 488 (3) (2019) 3526–3540, arXiv:1904.01022 [astro-ph.CO].

[1777] J. Einasto, L.J. Liivamägi, I. Suhonenko, M. Einasto, The biasing phenomenon, Astron. Astrophys. 630 (2019) A62, arXiv:1906.03617 [astro-ph.CO].

[1778] J.M. Colberg, et al., The aspen-amsterdam void finder comparison project, Mon. Not. R. Astron. Soc. 387 (2008) 933, arXiv:0803.0918 [astro-ph].

[1779] M.C. Neyrinck, ZOBOV: a parameter-free void-finding algorithm, Mon. Not. R. Astron. Soc. 386 (2008) 2101, arXiv:0712.3049 [astro-ph].

[1780] P.M. Sutter, G. Lavaux, N. Hamaus, A. Pisani, B.D. Wandelt, M.S. Warren, F. Villaescusa-Navarro, P. Zivick, Q. Mao, B.B. Thompson, VIDE: the void Identification and examination toolkit, Astron. Comput. 9 (2015) 1–9, arXiv: 1406.1191 [astro-ph.CO].

[1781] A. Elyiv, F. Marulli, G. Pollina, M. Baldi, E. Branchini, A. Cimatti, L. Moscardini, Cosmic voids detection without density measurements, Mon. Not. R. Astron. Soc. 448 (1) (2015) 642–653, arXiv:1410.4559 [astro-ph.CO].

[1782] D.J. Paz, C.M. Correa, S.R. Gualpa, A.N. Ruiz, C.S. Bederián, R.D. Graña, N.D. Padilla, Guess the cheese flavour by the size of its holes: a cosmological test using the abundance of popcorn voids, Mon. Not. R. Astron. Soc. 522 (2) (2023) 2553–2569, arXiv:2212.06849 [astro-ph.CO].
[1783] A.N. Ruiz, D.J. Paz, M. Lares, H.E. Luparello, L. Ceccarelli, D. Garcia Lambas, Clues on void evolution – III. Structure and dynamics in void shells, Mon. Not. R. Astron. Soc. 448 (2) (2015) 1471–1482, arXiv:1501.02120 [astro-ph.CO].

[1784] D.G. Lambas, M. Lares, L. Ceccarelli, A.N. Ruiz, D.J. Paz, V.E. Maldonado, H.E. Luparello, The sparkling Universe: the coherent motions of cosmic voids, Mon. Not. R. Astron. Soc. 455 (1) (2016) L99–L103, arXiv:1510.00712 [astro-ph.CO].

[1785] N. Schuster, N. Hamaus, K. Dolag, J. Weller, Why cosmic voids matter: mitigation of baryonic physics, J. Cosmol. Astropart. Phys. 08 (2024) 065, arXiv:2312.11241 [astro-ph.CO].

[1786] D. Paz, M. Lares, L. Ceccarelli, N. Padilla, D.G. Lambas, Clues on void evolution II: Measuring density and velocity profiles on SDSS galaxy redshift space distortions, Mon. Not. R. Astron. Soc. 436 (2013) 3480, arXiv:1306.5799 [astro-ph.CO].

[1787] N. Schuster, N. Hamaus, K. Dolag, J. Weller, Why cosmic voids matter: nonlinear structure & linear dynamics, J. Cosmol. Astropart. Phys. 05 (2023) 031, arXiv:2210.02457 [astro-ph.CO].

[1788] I. Szapudi, et al., The cold spot in the cosmic microwave background: the shadow of a supervoid, in: 49th Rencontres de Morion on Cosmology, 2014, pp. 33–41, arXiv:1406.3622 [astro-ph.CO].

[1789] R.K. Sheth, R. van de Weygaert, A. Hierarchy of voids: Much ado about nothing, Mon. Not. R. Astron. Soc. 350 (2004) 517, arXiv:astro-ph/0311260.

[1790] E. Jennings, Y. Li, W. Hu, The abundance of voids and the excursion set formalism, Mon. Not. R. Astron. Soc. 434 (2013) 2167, arXiv:1304.6087 [astro-ph.CO].

[1791] G. Verza, C. Carbone, A. Pisani, C. Porciani, S. Matarrese, The universal multiplicity function: counting haloes and voids, J. Cosmol. Astropart. Phys. 10 (2024) 079, arXiv:2401.14451 [astro-ph.CO].

[1792] G. Lavaux, B.D. Wandelt, Precision cosmology with stacked voids, Astrophys. J. 754 (2012) 109, arXiv:1110.0345 [astro-ph.CO].

[1793] N. Hamaus, A. Pisani, P.M. Sutter, G. Lavaux, S. Escoffier, B.D. Wandelt, J. Weller, Constraints on cosmology and gravity from the dynamics of voids, Phys. Rev. Lett. 117 (9) (2016) 091302, arXiv:1602.01784 [astro-ph.CO].

[1794] Y.-C. Cai, A. Taylor, J.A. Peacock, N. Padilla, Redshift-space distortions around voids, Mon. Not. R. Astron. Soc. 462 (3) (2016) 2465–2477, arXiv:1603.05184 [astro-ph.CO].

[1795] C.M. Correa, D.J. Paz, N.D. Padilla, A.N. Ruiz, R.E. Angulo, A.G. Sánchez, Non- fiducial cosmological test from geometrical and dynamical distortions around voids, Mon. Not. R. Astron. Soc. 485 (4) (2019) 5761–5772, arXiv:1811.12251 [astro-ph.CO].

[1796] C.M. Correa, D.J. Paz, A.G. Sánchez, A.N. Ruiz, N.D. Padilla, R.E. Angulo, Redshift-space effects in voids and their impact on cosmological tests. Part I: the void size function, Mon. Not. R. Astron. Soc. 500 (1) (2020) 911–925, arXiv:2007.12064 [astro-ph.CO].

[1797] C.M. Correa, D.J. Paz, N.D. Padilla, A.G. Sánchez, A.N. Ruiz, R.E. Angulo, Redshift-space effects in voids and their impact on cosmological tests – II. The void-galaxy cross-correlation function, Mon. Not. R. Astron. Soc. 509 (2) (2021) 1871–1884, arXiv:2107.01314 [astro-ph.CO].

[1798] S. Contarini, A. Pisani, N. Hamaus, F. Marulli, L. Moscardini, M. Baldi, The perspective of voids on rising cosmology tensions, Astron. Astrophys. 682 (2024) A20, arXiv:2212.07438 [astro-ph.CO].

[1799] N. Hamaus, A. Pisani, J.-A. Choi, G. Lavaux, B.D. Wandelt, J. Weller, Precision cosmology with voids in the final BOSS data, J. Cosmol. Astropart. Phys. 12 (2020) 023, arXiv:2007.07895 [astro-ph.CO].

[1800] Euclid Collaboration, N. Hamaus, et al., Euclid: Forecasts from redshift- space distortions and the Alcock–Paczynski test with cosmic voids, Astron. Astrophys. 658 (2022) A20, arXiv:2108.10347 [astro-ph.CO].

[1801] Euclid Collaboration, S. Contarini, et al., Euclid: Cosmological forecasts from the void size function, Astron. Astrophys. 667 (2022) A162, arXiv:2205.11525 [astro-ph.CO].

[1802] Euclid Collaboration, M. Bonici, et al., Euclid: Forecasts from the void- lensing cross-correlation, Astron. Astrophys. 670 (2023) A47, arXiv:2206. 14211 [astro-ph.CO].

[1803] S. Raghunathan, S. Nadathur, B.D. Sherwin, N. Whitehorn, The gravitational lensing signatures of BOSS voids in the cosmic microwave background, Astrophys. J. 890 (2) (2020) 168, arXiv:1911.08475 [astro-ph.CO].

[1804] DES Collaboration, U. Demirbozan, et al., The gravitational lensing imprints of DES Y3 superstructures on the CMB: a matched filtering approach, Mon. Not. R. Astron. Soc. 534 (3) (2024) 2328–2343, arXiv:2404.18278 [astro-ph.CO].

[1805] G. Camacho-Ciurana, P. Lee, N. Arsenal, A. Kovács, I. Szapudi, I. Csabai, The cosmic microwave background lensing imprint of cosmic voids detected in the WISE-Pan-STARRS luminous red galaxy catalog, Astron. Astrophys. 689 (2024) A171, arXiv:2312.08483 [astro-ph.CO].

[1806] S. Sartori, et al., The imprint of cosmic voids from the DESI Legacy Survey DR9 LRGs in the Planck 2018 lensing map through spectroscopically calibrated mocks, 2024, arXiv:2412.02761 [astro-ph.CO].

[1807] D.R. Lorimer, M. Bailes, M.A. McLaughlin, D.J. Narkevic, F. Crawford, A bright millisecond radio burst of extragalactic origin, Science 318 (2007) 777, arXiv:0709.4301 [astro-ph].

[1808] S.P. Tendulkar, et al., The host galaxy and redshift of the repeating fast radio burst FRB 121102, Astrophys. J. Lett. 834 (2) (2017) L7, arXiv:1701.01100 [astro-ph.HE].

[1809] A. Walters, A. Weltman, B.M. Gaensler, Y.-Z. Ma, A. Witzemann, Future cosmological constraints from fast radio bursts, Astrophys. J. 856 (1) (2018) 65, arXiv:1711.11277 [astro-ph.CO].

[1810] W. Deng, B. Zhang, Cosmological implications of fast radio burst/gamma- ray burst associations, Astrophys. J. Lett. 783 (2014) L35, arXiv:1401.0059 [astro-ph.HE].

[1811] A. Walters, Y.-Z. Ma, J. Sievers, A. Weltman, Probing diffuse gas with fast radio bursts, Phys. Rev. D 100 (10) (2019) 103519, arXiv:1909.02821 [astro-ph.CO].

[1812] J.P. Macquart, et al., A census of baryons in the Universe from localized fast radio bursts, Nature 581 (7809) (2020) 391–395, arXiv:2005.13161 [astro-ph.CO].

[1813] E. Platts, A. Weltman, A. Walters, S.P. Tendulkar, J.E.B. Gordin, S. Kandhai, A living theory catalogue for fast radio bursts, Phys. Rep. 821 (2019) 1–27, arXiv:1810.05836 [astro-ph.HE].

[1814] B. Zhang, The physical mechanisms of fast radio bursts, Nature 587 (2020) 45–53, arXiv:2011.03500 [astro-ph.HE].

[1815] B. Zhang, The physics of fast radio bursts, Rev. Modern Phys. 95 (3) (2023) 035005, arXiv:2212.03972 [astro-ph.HE].

[1816] S. Kalita, A. Weltman, Continuous gravitational wave detection to understand the generation mechanism of fast radio bursts, Mon. Not. R. Astron. Soc. 520 (3) (2023) 3742–3748, arXiv:2211.00940 [astro-ph.HE].

[1817] H.E.S.S. Collaboration, J.O. Chibueze, et al., A MeerKAT, e-MERLIN, H.E.S.S., and Swift search for persistent and transient emission associated with three localized FRBs, Mon. Not. R. Astron. Soc. 515 (1) (2022) 1365–1379, arXiv: 2201.00069 [astro-ph.HE].

[1818] B. Zhou, X. Li, T. Wang, Y.-Z. Fan, D.-M. Wei, Fast radio bursts as a cosmic probe? Phys. Rev. D 89 (10) (2014) 107303, arXiv:1401.2927 [astro-ph.CO].

[1819] H. Gao, Z. Li, B. Zhang, Fast radio burst/gamma-ray burst cosmography, Astrophys. J. 788 (2014) 189, arXiv:1402.2498 [astro-ph.CO].

[1820] Z. Pleunis, et al., LOFAR detection of 110–188 MHz emission and frequency- dependent activity from FRB 20180916B, Astrophys. J. Lett. 911 (1) (2021) L3, arXiv:2012.08372 [astro-ph.HE].

[1821] V. Gajjar, et al., Highest frequency detection of FRB 121102 at 4–8 GHz using the breakthrough listen digital backend at the green bank telescope, Astrophys. J. 863 (1) (2018) 2, arXiv:1804.04101 [astro-ph.HE].

[1822] L. Bonetti, J. Ellis, N.E. Mavromatos, A.S. Sakharov, E.K.G. Sarkisyan- Grinbaum, A.D.A.M. Spallucci, Photon mass limits from fast radio bursts, Phys. Lett. B 757 (2016) 548–552, arXiv:1602.09135 [astro-ph.HE].

[1823] H. Wang, X. Miao, L. Shao, Bounding the photon mass with cosmological propagation of fast radio bursts, Phys. Lett. B 820 (2021) 136596, arXiv: 2103.15299 [astro-ph.HE].

[1824] H.-N. Lin, L. Tang, R. Zou, Revised constraints on the photon mass from well-localized fast radio bursts, Mon. Not. R. Astron. Soc. 520 (1) (2023) 1324–1331, arXiv:2301.12103 [gr-qc].

[1825] R. Reischke, S. Hagstotz, Consistent constraints on the equivalence principle from localized fast radio bursts, Mon. Not. R. Astron. Soc. 523 (4) (2023) 6264–6271, arXiv:2302.10072 [astro-ph.CO].

[1826] S. Kalita, Constraining fundamental constants with fast radio bursts: unveiling the role of energy scale, Mon. Not. R. Astron. Soc. 533 (1) (2024) L57–L63, arXiv:2407.01736 [gr-qc].

[1827] T. Lemos, R. Gonçalves, J. Carvalho, J. Alcaniz, A search for the fine-structure constant evolution from fast radio bursts and type Ia supernovae data, J. Cosmol. Astropart. Phys. 01 (2025) 059, arXiv:2406.11691 [astro-ph.CO].

[1828] Z.-X. Li, H. Gao, X.-H. Ding, G.-J. Wang, B. Zhang, Strongly lensed repeating fast radio bursts as precision probes of the universe, Nat. Commun. 9 (1) (2018) 3833, arXiv:1708.06357 [astro-ph.CO].

[1829] S. Hagstotz, R. Reischke, R. Lilow, A new measurement of the Hubble constant using fast radio bursts, Mon. Not. R. Astron. Soc. 511 (1) (2022) 662–667, arXiv:2104.04538 [astro-ph.CO].

[1830] Q. Wu, G.-Q. Zhang, F.-Y. Wang, An 8 percent determination of the Hubble constant from localized fast radio bursts, Mon. Not. R. Astron. Soc. 515 (1) (2022) L1–L5, arXiv:2108.00581 [astro-ph.CO]; Mon. Not. Roy. Astron. Soc. 531 (2024) L8 (erratum).

[1831] C.W. James, et al., A measurement of hubble's constant using fast radio bursts, Mon. Not. R. Astron. Soc. 516 (4) (2022) 4862–4881, arXiv:2208.00819 [astro-ph.CO].

[1832] J. Baptista, J.X. Prochaska, A.G. Mannings, C.W. James, R.M. Shannon, S.D. Ryder, A.T. Deller, D.R. Scott, M. Glowacki, N. Tejos, Measuring the variance of the macquart relation in redshift–extragalactic dispersion measure modeling, Astrophys. J. 965 (1) (2024) 57, arXiv:2305.07022 [astro-ph.CO].

[1833] Y. Liu, H. Yu, P. Wu, Cosmological-model-independent determination of hubble constant from fast radio bursts and hubble parameter measurements, Astrophys. J. Lett. 946 (2) (2023) L49, arXiv:2210.05202 [astro-ph.CO].

[1834] J.-J. Wei, F. Melia, Investigating cosmological models and the hubble tension using localized fast radio bursts, Astrophys. J. 955 (2) (2023) 101, arXiv: 2308.05918 [astro-ph.CO].
[1835] Z.-W. Zhao, J.-G. Zhang, Y. Li, J.-F. Zhang, X. Zhang, FRB dark sirens: Measuring the Hubble constant with unlocalized fast radio bursts, 2022, arXiv:2212.13433 [astro-ph.CO].

[1836] J. Gao, Z. Zhou, M. Du, R. Zou, J. Hu, L. Xu, A measurement of hubble constant using cosmographic approach from fast radio bursts and SNe Ia, 2023, arXiv:2307.08285 [astro-ph.CO].

[1837] J.A.S. Fortunato, D.J. Bacon, W.S. Hipólito-Ricaldi, D. Wands, Fast Radio Bursts and Artificial Neural Networks: a cosmological-model-independent estimation of the Hubble constant, J. Cosmol. Astropart. Phys. 01 (2025) 018, arXiv:2407.03532 [astro-ph.CO].

[1838] S. Kalita, S. Bhatporia, A. Weltman, Fast Radio Bursts as probes of the late-time universe: A new insight on the Hubble tension, Phys. Dark Univ. 48 (2025) 101926, arXiv:2410.01972 [astro-ph.CO].

[1839] E.F. Piratova-Moreno, L.A. García, C.A. Benavides-Gallego, C. Cabrera, Fast Radio Bursts as cosmological proxies: estimating the Hubble constant, 2025, arXiv:2502.08509 [astro-ph.CO].

[1840] J.B. Muñoz, E.D. Kovetz, L. Dai, M. Kamionkowski, Lensing of fast radio bursts as a probe of compact dark matter, Phys. Rev. Lett. 117 (9) (2016) 091301, arXiv:1605.00008 [astro-ph.CO].

[1841] M.W. Sammons, J.-P. Macquart, R.D. Ekers, R.M. Shannon, H. Cho, J.X. Prochaska, A.T. Deller, C.K. Day, First constraints on compact dark matter from fast radio burst microstructure, Astrophys. J. 900 (2) (2020) 122, arXiv: 2002.12533 [astro-ph.CO].

[1842] R. Laha, Lensing of fast radio bursts: Future constraints on primordial black hole density with an extended mass function and a new probe of exotic compact fermion and boson stars, Phys. Rev. D 102 (2) (2020) 023016, arXiv:1812.11810 [astro-ph.CO].

[1843] K. Liao, S.B. Zhang, Z. Li, H. Gao, Constraints on compact dark matter with fast radio burst observations, Astrophys. J. 896 (1) (2020) L11, arXiv:2003.13349 [astro-ph.CO].

[1844] C. Leung, et al., Constraining primordial black holes using fast radio burst gravitational-lens interferometry with CHIME/FRB, Phys. Rev. D 106 (4) (2022) 043017, arXiv:2204.06001 [astro-ph.HE].

[1845] S. Kalita, S. Bhatporia, A. Weltman, Gravitational lensing in modified gravity: a case study for Fast Radio Bursts, J. Cosmol. Astropart. Phys. 11 (2023) 059, arXiv:2308.16604 [gr-qc].

[1846] D. Crichton, et al., Hydrogen intensity and real-time analysis experiment: 256-element array status and overview, J. Astron. Telesc. Instrum. Syst. 8 (2022) 011019, arXiv:2109.13755 [astro-ph.IM].

[1847] L. Connor, V. Ravi, Stellar prospects for FRB gravitational lensing, Mon. Not. R. Astron. Soc. 521 (3) (2023) 4024–4038, arXiv:2206.14310 [astro-ph.CO].

[1848] S.C.C. Ho, T. Hashimoto, T. Goto, Y.-W. Lin, S.J. Kim, Y. Uno, T.Y.Y. Hsiao, Future constraints on dark matter with gravitationally lensed fast radio bursts detected by BURSTT, Astrophys. J. 950 (1) (2023) 53, arXiv:2304.04990 [astro-ph.HE].

[1849] A. Weltman, et al., Fundamental physics with the square kilometre array, Publ. Astron. Soc. Austral. 37 (2020) e002, arXiv:1810.02680 [astro-ph.CO].

[1850] M.G. Hauser, E. Dwek, The cosmic infrared background: measurements and implications, Ann. Rev. Astron. Astrophys. 39 (2001) 249–307, arXiv:astro-ph/0105539.

[1851] R.C. Gilmore, P. Madau, J.R. Primack, R.S. Somerville, F. Haardt, GeV gamma-ray attenuation and the high-redshift UV background, Mon. Not. R. Astron. Soc. 399 (2009) 1694, arXiv:0905.1144 [astro-ph.CO].

[1852] N. Cappelluti, et al., The Chandra COSMOS legacy survey: Energy Spectrum of the Cosmic X-ray Background and constraints on undetected populations, Astrophys. J. 837 (1) (2017) 19, arXiv:1702.01660 [astro-ph.HE].

[1853] Fermi-LAT Collaboration, M. Ackermann, et al., Resolving the extragalactic γ-ray background above 50 GeV with the fermi large area telescope, Phys. Rev. Lett. 116 (15) (2016) 151105, arXiv:1511.00693 [astro-ph.CO].

[1854] J. Singal, et al., The second radio synchrotron background workshop: conference summary and report, Publ. Astron. Soc. Pac. 135 (1045) (2023) 036001, arXiv:2211.16547 [astro-ph.CO].

[1855] D.J. Fixsen, et al., ARCADE 2 measurement of the extra-galactic sky temperature at 3-90 GHz, Astrophys. J. 734 (2011) 5, arXiv:0901.0555 [astro-ph.CO].

[1856] J. Singal, et al., The ARCADE 2 instrument, Astrophys. J. 730 (2011) 138, arXiv:0901.0546 [astro-ph.IM].

[1857] J. Dowell, G.B. Taylor, The radio background below 100 MHz, Astrophys. J. Lett. 858 (1) (2018) L9, arXiv:1804.08581 [astro-ph.CO].

[1858] G. Jóhannesson, T.A. Porter, Signatures of recent cosmic-ray acceleration in the high-latitude gamma-ray sky, Astrophys. J. 917 (1) (2021) 30, arXiv: 2104.13708 [astro-ph.HE].

[1859] C.G.T. Haslam, C.J. Salter, H. Stoffel, W.E. Wilson, A 408 MHz all-sky continuum survey. II. The atlas of contour maps, Astron. Astrophys. Suppl. Ser. 47 (1982) 1–142.

[1860] K. Maeda, H. Alvarez, J. Aparici, J. May, P. Reich, A 45-MHz continuum survey of the northern hemisphere, Astron. Astrophys. Suppl. Ser. 140 (1999) 145–154.

[1861] R.S. Roger, C.H. Costain, T.L. Landecker, C.M. Swerdyk, The radio emission from the galaxy at 22 mhz, Astron. Astrophys. Suppl. Ser. 137 (1999) 7, arXiv:astro-ph/9902213.

[1862] J. Singal, et al., The radio synchrotron background: conference summary and report, Publ. Astron. Soc. Pac. 130 (985) (2018) 036001, arXiv:1711.09979 [astro-ph.HE].

[1863] J.J. Condon, W.D. Cotton, E.B. Fomalont, K.I. Kellermann, N. Miller, R.A. Perley, D. Scott, T. Vernstrom, J.V. Wall, Resolving the radio source background: deeper understanding through confusion, Astrophys. J. 758 (2012) 23, arXiv:1207.2439 [astro-ph.CO].

[1864] M.J. Hardcastle, T.W. Shimwell, C. Tasse, P.N. Best, A. Drabent, M.J. Jarvis, I. Prandoni, H.J.A. Röttgering, J. Sabater, D.J. Schwarz, The contribution of discrete sources to the sky temperature at 144 MHz, Astron. Astrophys. 648 (2021) A10, arXiv:2011.08294 [astro-ph.CO].

[1865] C.L. Hale, I.H. Whittam, M.J. Jarvis, P.N. Best, N.L. Thomas, I. Heywood, M. Prescott, N. Adams, J. Afonso, F. An, R.A.A. Bowler, J.D. Collier, R.H.W. Cook, R. Davé, B.S. Frank, M. Glowacki, P.W. Hatfield, S. Kolwa, C.C. Lovell, N. Maddox, L. Marchetti, L.K. Morabito, E. Murphy, I. Prandoni, Z. Randriamanakoto, A.R. Taylor, MIGHTEE: deep 1.4 GHz source counts and the sky temperature contribution of star-forming galaxies and active galactic nuclei, Mon. Not. R. Astro. Soc. 520 (2) (2023) 2668–2691, arXiv:2211.05741 [astro-ph.GA].

[1866] A. Kogut, et al., ARCADE 2 observations of galactic radio emission, Astrophys. J. 734 (2011) 4, arXiv:0901.0562 [astro-ph.GA].

[1867] J. Singal, A. Kogut, E. Jones, H. Dunlop, Axial ratio of edge-on spiral galaxies as a test for bright radio halos, Astrophys. J. Lett. 799 (1) (2015) L10, arXiv:1501.00499 [astro-ph.GA].

[1868] M.G.H. Krause, M.J. Hardcastle, Can the Local Bubble explain the radio background? Mon. Not. R. Astron. Soc. 502 (2) (2021) 2807–2814, arXiv: 2101.05255 [astro-ph.HE].

[1869] A.R. Offringa, J. Singal, S. Heston, S. Horiuchi, D.M. Lucero, Measurement of the anisotropy power spectrum of the radio synchrotron background, Mon. Not. R. Astron. Soc. 509 (1) (2021) 114–121, arXiv:2110.00499 [astro-ph.CO].

[1870] F.J. Cowie, A.R. Offringa, B.K. Gehlot, J. Singal, S. Heston, S. Horiuchi, D.M. Lucero, Diffuse sources, clustering, and the excess anisotropy of the radio synchrotron background, Mon. Not. R. Astron. Soc. 523 (4) (2023) 5034–5046, arXiv:2306.00829 [astro-ph.CO].

[1871] P.P. Ponente, Y. Ascasibar, J.M. Diego, The contribution of star-forming galaxies to the cosmic radio background, Mon. Not. R. Astron. Soc. 418 (2011) 691, arXiv:1104.3012 [astro-ph.CO].

[1872] J. Singal, L. Stawarz, A. Lawrence, V. Petrosian, Sources of the radio background considered, Mon. Not. R. Astron. Soc. 409 (2010) 1172, arXiv: 0909.1997 [astro-ph.CO].

[1873] E. Todarello, M. Regis, F. Bianchini, J. Singal, E. Branchini, F.J. Cowie, S. Heston, S. Horiuchi, D. Lucero, A. Offringa, Constraints on the origin of the radio synchrotron background via angular correlations, Mon. Not. R. Astron. Soc. 530 (3) (2024) 2994–3004, arXiv:2311.17641 [astro-ph.CO].

[1874] A. Fialkov, R. Barkana, Signature of excess radio background in the 21-cm global signal and power spectrum, Mon. Not. R. Astron. Soc. 486 (2) (2019) 1763–1773, arXiv:1902.02438 [astro-ph.CO].

[1875] P.L. Biermann, B.B. Nath, L.t.I. Caramete, B.C. Harms, T. Stanev, J. Becker Tjus, Cosmic backgrounds due to the formation of the first generation of supermassive black holes, Mon. Not. R. Astron. Soc. 441 (2) (2014) 1147–1156, arXiv:1403.3804 [astro-ph.CO].

[1876] K. Fang, T. Linden, Cluster mergers and the origin of the ARCADE-2 excess, J. Cosmol. Astropart. Phys. 10 (2016) 004, arXiv:1506.05807 [astro-ph.HE].

[1877] N. Fornengo, R. Lineros, M. Regis, M. Taoson, Possibility of a dark matter interpretation for the excess in isotropic radio emission reported by ARCADE, Phys. Rev. Lett. 107 (2011) 271302, arXiv:1108.0569 [hep-ph].

[1878] D. Hooper, A.V. Belikov, T.E. Jeltema, T. Linden, S. Profumo, T.R. Slatyer, The isotropic radio background and annihilating dark matter, Phys. Rev. D 86 (2012) 103003, arXiv:1203.3547 [astro-ph.CO].

[1879] K. Fang, T. Linden, Anisotropy of the extragalactic radio background from dark matter annihilation, Phys. Rev. D 91 (8) (2015) 083501, arXiv:1412.7545 [astro-ph.HE].

[1880] E.C.F.S. Fortes, O.D. Miranda, F.W. Stecker, C.A. Wuensche, Some implications of the leptonic annihilation of dark matter: possible galactic radio emission signatures and the excess radio flux of extragalactic origin, J. Cosmol. Astropart. Phys. 11 (2019) 047, arXiv:1907.13184 [hep-ph].

[1881] Y. Yang, G. Yang, X. Huang, X. Chen, T. Lu, H. Zong, Contribution of ultracompact dark matter minihalos to the isotropic radio background, Phys. Rev. D 87 (8) (2013) 083519, arXiv:1206.3750 [astro-ph.HE].

[1882] D. Spolyar, P. Bodenheimer, K. Freese, P. Gondolo, Dark stars: a new look at the first stars in the universe, Astrophys. J. 705 (2009) 1031–1042, arXiv: 0903.3070 [astro-ph.CO].

[1883] T. Rindler-Daller, K. Freese, R.H.D. Townsend, L. Visinelli, Stability and pulsation of the first dark stars, Mon. Not. R. Astron. Soc. 503 (3) (2021) 3677–3691, arXiv:2011.00231 [astro-ph.CO].

[1884] K. Lawson, A.R. Zhitnitsky, Isotropic radio background from quark nugget dark matter, Phys. Lett. B 724 (2013) 17–21, arXiv:1210.2400 [astro-ph.CO].

[1885] N. Cappelluti, G. Hasinger, P. Natarajan, Exploring the high-redshift PBH-ACDM universe: early black hole seeding, the first stars and cosmic radiation backgrounds, Astrophys. J. 926 (2) (2022) 205, arXiv:2109.08701 [astro-ph.CO].
[1886] S. Mittal, G. Kulkarni, Background of radio photons from primordial black holes, Mon. Not. R. Astron. Soc. 510 (4) (2022) 4992-4997, arXiv:2110.11975 [astro-ph.CO].

[1887] S.K. Acharya, J. Dhandha, J. Chluba, Can accreting primordial black holes explain the excess radio background? Mon. Not. R. Astron. Soc. 517 (2) (2022) 2454-2461, arXiv:2208.03816 [astro-ph.CO].

[1888] M. Pospelov, J. Pradler, J.T. Ruderman, A. Urbano, Room for new physics in the rayleigh-jeans tail of the cosmic microwave background, Phys. Rev. Lett. 121 (3) (2018) 031103, arXiv:1803.07048 [hep-ph].

[1889] A. Caputo, H. Liu, S. Mishra-Sharma, M. Pospelov, J.T. Ruderman, Radio excess from stimulated dark matter decay, Phys. Rev. D 107 (12) (2023) 123033, arXiv:2206.07713 [hep-ph].

[1890] S.K. Acharya, J. Chluba, A closer look at dark photon explanations of the excess radio background, Mon. Not. R. Astron. Soc. 521 (3) (2023) 3939-3950, arXiv:2209.09063 [astro-ph.CO].

[1891] S.K. Acharya, B. Cyr, J. Chluba, Constraining broad photon spectrum injections from exotic and astrophysical sources, Mon. Not. R. Astron. Soc. 527 (2023) 2024, arXiv:2309.00975 [astro-ph.CO].

[1892] B. Cyr, J. Chluba, S.K. Acharya, Cosmic string solution to the radio synchrotron background, Phys. Rev. D 109 (12) (2024) L121301, arXiv:2308.03512 [astro-ph.CO].

[1893] P.S.B. Dev, P. Di Bari, I. Martínez-Soler, R. Roshan, Relic neutrino decay solution to the excess radio background, J. Cosmol. Astropart. Phys. 04 (2024) 046, arXiv:2312.03082 [hep-ph].

[1894] S.D. Bale, N. Bassett, J.O. Burns, J. Dorigo Jones, K. Goetz, C. Hellum-Bye, S. Hermann, J. Hibbard, M. Maksimovic, R. McLean, R. Monsalve, P. O'Connor, A. Parsons, M. Pulupa, R. Kund, D. Rapetti, K.M. Rotermund, B. Saliwanchik, A. Slosar, D. Sundkvist, A. Suzuki, LuSEE 'night': the lunar surface electromagnetics experiment, 2023, http://dx.doi.org/10.48550/arXiv.2301.10345, arXiv e-prints, arXiv:2301.10345 [astro-ph.IM].

[1895] E. Lee, J. Chluba, G.P. Holder, Refined modeling of the radio SZ signal: kinematic terms, relativistic temperature corrections, and anisotropies in the radio background, Mon. Not. R. Astron. Soc. 512 (4) (2022) 5153-5164, arXiv:2112.10666 [astro-ph.CO].

[1896] G. Holder, J. Chluba, The radio SZ effect as a probe of the cosmological radio background, 2021, arXiv:2110.08373 [astro-ph.CO].

[1897] R. Watkins, H.A. Feldman, M.J. Hudson, Consistently large cosmic flows on scales of 100 Mpc/h: a challenge for the standard LCDM cosmology, Mon. Not. R. Astron. Soc. 392 (2009) 743-756, arXiv:0809.4041 [astro-ph].

[1898] H.A. Feldman, R. Watkins, M.J. Hudson, Cosmic flows on 100 Mpc/h scales: standardized minimum variance bulk flow, shear and octupole moments, Mon. Not. R. Astron. Soc. 407 (2010) 2328-2338, arXiv:0911.5516 [astro-ph.CO].

[1899] J.C. Bird, K.Z. Stanek, J.L. Prieto, Using ultra long period cepheids to extend the cosmic distance ladder to 100 Mpc and beyond, Astrophys. J. 695 (2009) 874-882, arXiv:0807.4933 [astro-ph].

[1900] G. Fiorentino, R.C. Ramos, G. Clementini, M. Marconi, I. Musella, A. Aloisi, F. Annibali, A. Saha, M. Tosi, R.P. van der Marel, Multi-epoch HST observations of IZW18: characterization of variable stars at ultra-low metallicities, Astrophys. J. 711 (2010) 808-817, arXiv:1001.4044 [astro-ph.SR].

[1901] M. Marconi, I. Musella, G. Fiorentino, G. Clementini, A. Aloisi, F. Annibali, R.C. Ramos, A. Saha, M. Tosi, R.P. van der Marel, Pulsation models for ultra-low (Z=0.0004) metallicity classical cepheids, Astrophys. J. 713 (2010) 615-625, arXiv:1002.4752 [astro-ph.SR].

[1902] I. Musella, M. Marconi, R. Molinaro, G. Fiorentino, V. Ripepi, G. De Somma, M.I. Moretti, New insights into the use of Ultra Long Period Cepheids as cosmological standard candles, Mon. Not. R. Astro. Soc. 501 (1) (2021) 866-874, arXiv:2011.10533 [astro-ph.SR].

[1903] I. Musella, Ultra long period cepheids: observation and theory, Universe 8 (6) (2022) 335.

[1904] C.-C. Ngeow, C.-H. Lee, M.T.-C. Yang, C.-S. Lin, H.-Y. Hsiao, Y.-C. Cheng, Z.-Y. Lin, I.L. Lin, S.M. Kanbur, W.-H. Ip, VI-band follow-up observations of ultra-long-period cepheid candidates in M31, Astron. J. 149 (2) (2015) 66, arXiv:1501.02456 [astro-ph.SR].

[1905] I. Musella, S. Leccia, R. Molinaro, M. Marconi, F. Cusano, M. Di Criscienzo, G. Fiorentino, V. Braga, V. Ripepi, G. De Somma, M. Gatto, E. Luongo, T. Sicignano, Ultra-long-period cepheids as standard candles from gaia to rubin-LSST, Astrophys. J. Suppl. 275 (2) (2024) 26, arXiv:2410.12017 [astro-ph.GA].

[1906] DESI Collaboration, A.G. Adame, et al., The early data release of the dark energy spectroscopic instrument, Astron. J. 168 (2) (2024) 58, arXiv:2306.06308 [astro-ph.CO].

[1907] DESI Collaboration, M. Abdul Karim, et al., Data release 1 of the dark energy spectroscopic instrument, 2025, arXiv:2503.14745 [astro-ph.CO].

[1908] DESI Collaboration, W. Elbers, et al., Constraints on neutrino physics from DESI DR2 BAO and DR1 full shape, 2025, arXiv:2503.14744 [astro-ph.CO].

[1909] DES Collaboration, B. Flaugher, et al., The dark energy camera, Astron. J. 150 (2015) 150, arXiv:1504.02900 [astro-ph.IM].

[1910] Linea Science Server, DES Collaboration, T.M.C. Abbott, et al., The dark energy survey data release 2, Astrophys. J. Supp. 255 (2) (2021) 20, arXiv: 2101.05765 [astro-ph.IM].

[1911] S. Miyazaki, et al., Hyper Suprime-Cam: System design and verification of image quality, Publ. Astron. Soc. Japan 70 (2018) S1.

[1912] H. Aihara, et al., First data release of the hyper suprime-cam subaru strategic program, Publ. Astron. Soc. Jap. 70 (2018) S8, arXiv:1702.08449 [astro-ph.IM].

[1913] H. Aihara, et al., Third data release of the hyper suprime-cam subaru strategic program, Publ. Astron. Soc. Jap. 74 (2) (2022) 247-272-272, arXiv:2108.13045 [astro-ph.IM].

[1914] K. Moriwaki, T. Nishimichi, N. Yoshida, Machine learning for observational cosmology, Rep. Progr. Phys. 86 (7) (2023) 076901, arXiv:2303.15794 [astro-ph.IM].

[1915] A. Lewis, Efficient sampling of fast and slow cosmological parameters, Phys. Rev. D 87 (10) (2013) 103529, arXiv:1304.4473 [astro-ph.CO].

[1916] B. Audren, J. Lesgourgues, K. Benabed, S. Prunet, Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code, J. Cosmol. Astropart. Phys. 02 (2013) 001, arXiv:1210.7183 [astro-ph.CO].

[1917] T. Brinckmann, J. Lesgourgues, MontePython 3: boosted MCMC sampler and other features, Phys. Dark Univ. 24 (2019) 100260, arXiv:1804.07261 [astro-ph.CO].

[1918] J. Torrado, A. Lewis, Cobaya: Code for Bayesian Analysis of hierarchical physical models, J. Cosmol. Astropart. Phys. 05 (2021) 057, arXiv:2005.05290 [astro-ph.IM].

[1919] D. Foreman-Mackey, D.W. Hogg, D. Lang, J. Goodman, emcee: The MCMC Hammer, Publ. Astron. Soc. Pac. 125 (2013) 306-312, arXiv:1202.3665 [astro-ph.IM].

[1920] M. Karamanis, F. Beutler, J.A. Peacock, D. Nabergoj, U. Seljak, Accelerating astronomical and cosmological inference with preconditioned Monte Carlo, Mon. Not. R. Astron. Soc. 516 (2) (2022) 1644-1653, arXiv:2207.05652 [astro-ph.IM].

[1921] G. Papamakarios, E. Nalisnick, D.J. Rezende, S. Mohamed, B. Lakshmi-narayanan, Normalizing flows for probabilistic modeling and inference, J. Mach. Learn. Res. 22 (57) (2021) 1-64, arXiv:1912.02762 [stat.ML], http://jmlr.org/papers/v22/19-1028.html.

[1922] R.M. Neal, Slice sampling, Ann. Statist. 31 (3) (2003) 705-767.

[1923] M. Karamanis, F. Beutler, J.A. Peacock, zeus: a python implementation of ensemble slice sampling for efficient Bayesian parameter inference, Mon. Not. R. Astron. Soc. 508 (3) (2021) 3589-3603, arXiv:2105.03468 [astro-ph.IM].

[1924] M.D. Hoffman, A. Gelman, The No-U-turn sampler: adaptively setting path lengths in Hamiltonian Monte Carlo, J. Mach. Learn. Res. 15 (47) (2014) 1593-1623, arXiv:1111.4246 [stat.CO], http://jmlr.org/papers/v15/ hoffman14a.html.

[1925] J. Bradbury, R. Frostig, P. Hawkins, M.J. Johnson, C. Leary, D. Maclaurin, G. Necula, A. Paszke, J. VanderPlas, S. Wanderman-Milne, Q. Zhang, JAX: composable transformations of Python+NumPy programs, 2018, http://github.com/jax-ml/jax.

[1926] J.-E. Campagne, F. Lanusse, J. Zuntz, A. Boucaud, S. Casas, M. Karamanis, D. Kirkby, D. Lanzieri, Y. Li, A. Peel, JAX-COSMO: an end-to-end differentiable and GPU accelerated cosmology library, Open J. Astrophys. 6 (2023) 1-15, arXiv:2302.05163 [astro-ph.CO].

[1927] O. Hahn, F. List, N. Porqueres, DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology, J. Cosmol. Astropart. Phys. 06 (2024) 063, arXiv: 2311.03291 [astro-ph.CO].

[1928] L. Balkenhol, C. Trendafilova, K. Benabed, S. Galli, candl: cosmic microwave background analysis with a differentiable likelihood, Astron. Astrophys. 686 (2024) A10, arXiv:2401.13433 [astro-ph.CO].

[1929] D. Piras, A. Spurio Mancini, CosmoPower-JAX: high-dimensional Bayesian inference with differentiable cosmological emulators, 2023, http://dx.doi.org/10.21105/astro.2305.06347, arXiv:2305.06347 [astro-ph.CO].

[1930] J. Ruiz-Zapatero, D. Alonso, C. García-García, A. Nicola, A. Mootoovaloo, J.M. Sullivan, M. Bonici, P.G. Ferreira, LimberJack.jl: auto-differentiable methods for angular power spectra analyses, 2023, http://dx.doi.org/10.21105/astro.2310.08306, arXiv:2310.08306 [astro-ph.CO].

[1931] M. Bonici, F. Bianchini, J. Ruiz-Zapatero, Capse.jl: efficient and auto-differentiable CMB power spectra emulation, 2023, http://dx.doi.org/10.21105/astro.2307.14339, arXiv:2307.14339 [astro-ph.CO].

[1932] M. Bonici, G. D'Amico, J. Bel, C. Carbone, Effort: a fast and differentiable emulator for the effective field theory of the large scale structure of the universe, 2025, arXiv:2501.04639 [astro-ph.CO].

[1933] E. Bingham, J.P. Chen, M. Jankowiak, F. Obermeyer, N. Pradhan, T. Karateksos, R. Singh, P. Szerlip, P. Horsfall, N.D. Goodman, Pyro: deep universal probabilistic programming, 2018, http://dx.doi.org/10.48550/arXiv.1810.09538, arXiv e-prints, arXiv:1810.09538 [cs.LG].

[1934] D. Piras, A. Polanska, A. Spurio Mancini, M.A. Price, J.D. McEwen, The future of cosmological likelihood-based inference: accelerated high-dimensional parameter estimation and model comparison, Open J. Astrophys. 7 (2024) arXiv:2405.12965 [astro-ph.CO].

[1935] A. Mootoovaloo, J. Ruiz-Zapatero, C. García-García, D. Alonso, Assessment of gradient-based samplers in standard cosmological likelihoods, Mon. Not. R. Astron. Soc. 534 (3) (2024) 1668-1681, arXiv:2406.04725 [astro-ph.IM].
[1936] J. Skilling, Nested sampling for general Bayesian computation, Bayesian Anal. 1 (4) (2006) 833–859, https://doi.org/10.1214/06-BA127.

[1937] J. Buchner, UltraNest - a robust, general purpose Bayesian inference engine, J. Open Source Softw. 6 (60) (2021) 3001, https://doi.org/10.21105/joss.03001.

[1938] W.J. Handley, M.P. Hobson, A.N. Lasenby, PolyChord: nested sampling for cosmology, Mon. Not. R. Astron. Soc. 450 (1) (2015) L61–L65, arXiv:1502.01856 [astro-ph.CO].

[1939] J.S. Speagle, dynasty: a dynamic nested sampling package for estimating Bayesian posteriors and evidences, Mon. Not. R. Astron. Soc. 493 (3) (2020) 3132–3158, arXiv:1904.02180 [astro-ph.IM].

[1940] J.U. Lange, nautilus: boosting Bayesian importance nested sampling with deep learning, Mon. Not. R. Astron. Soc. 525 (2) (2023) 3181–3194, arXiv:2306.16923 [astro-ph.IM].

[1941] I. Gómez-Vargas, J.A. Vázquez, Deep learning and genetic algorithms for cosmological Bayesian inference speed-up, Phys. Rev. D 110 (8) (2024) 083518, arXiv:2405.03293 [astro-ph.IM].

[1942] M.J. Williams, J. Veitch, C. Messenger, Importance nested sampling with normalising flows, Mach. Learn. Sci. Tech. 4 (3) (2023) 035011, arXiv:2302.08526 [astro-ph.IM].

[1943] J. Buchner, Nested sampling methods, Stat. Surv. (2021) arXiv:2101.09675 [stat.CO].

[1944] E.O. Colgáin, S. Pourojaghi, M.M. Sheikh-Jabbari, D. Sherwin, A comparison of Bayesian and frequentist confidence intervals in the presence of a late Universe degeneracy, Eur. Phys. J. C 85 (2) (2025) 124, arXiv:2307.16349 [astro-ph.CO].

[1945] J. Albert, C. Balazs, A. Fowlie, W. Handley, N. Hunt-Smith, R.R. de Aus- tri, M. White, A comparison of Bayesian sampling algorithms for high- dimensional particle physics and cosmology applications, 2024, arXiv:2409. 18464 [hep-ph].

[1946] D. Staicova, Modern Bayesian sampling methods for cosmological infer- ence: a comparative study, Universe 11 (2) (2025) 68, arXiv:2501.06022 [astro-ph.CO].

[1947] S. Raghvendra, P. Shirzadian, K. Zhang, A new robust partial *p*-wasserstein- based metric for comparing distributions, 2024, http://dx.doi.org/10.48550/ arXiv.2405.03664, arXiv e-prints, arXiv:2405.03664 [cs.LG].

[1948] A. Lewis, A. Challinor, A. Lasenby, Efficient computation of CMB anisotropies in closed FRW models, Astrophys. J. 538 (2000) 473–476, arXiv:astro-ph/ 9911177.

[1949] D. Blas, J. Lesgourgues, T. Tram, The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes, J. Cosmol. Astropart. Phys. 07 (2011) 034, arXiv:1104.2933 [astro-ph.CO].

[1950] B. Moser, C.S. Lorenz, U. Schmitt, A. Refregier, J. Fluri, R. Sgier, F. Tarsitano, L. Heisenberg, Symbolic implementation of extensions of the PyCosmo Boltzmann solver, Astron. Comput. 40 (2022) 100603, arXiv:2112. 08395 [astro-ph.CO].

[1951] J. Zuntz, M. Paterno, E. Jennings, D. Rudd, A. Manzotti, S. Dodelson, S. Bridle, S. Sehrish, J. Kowalkowski, CosmoSIS: modular cosmological parameter estimation, Astron. Comput. 12 (2015) 45–59, arXiv:1409.3409 [astro-ph.CO].

[1952] A. Lewis, GetDist: a Python package for analysing Monte Carlo samples, 2019, arXiv:1910.13970 [astro-ph.IM].

[1953] L. Senatore, M. Zaldarriaga, The IR-resummed effective field theory of large scale structures, J. Cosmol. Astropart. Phys. 02 (2015) 013, arXiv:1404.5954 [astro-ph.CO].

[1954] L. Senatore, Bias in the effective field theory of large scale structures, J. Cosmol. Astropart. Phys. 11 (2015) 007, arXiv:1406.7843 [astro-ph.CO].

[1955] L. Senatore, M. Zaldarriaga, Redshift-space distortions in the effective field theory of large scale structures, 2014, arXiv:1409.1225 [astro-ph.CO].

[1956] P. Carrilho, C. Moretti, A. Pourtsidou, Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors, J. Cosmol. Astropart. Phys. 01 (2023) 028, arXiv:2207.14784 [astro-ph.CO].

[1957] T. Simon, P. Zhang, V. Poulin, T.L. Smith, Consistency of effective field theory analyses of the BOSS power spectrum, Phys. Rev. D 107 (12) (2023) 123530, arXiv:2208.05929 [astro-ph.CO].

[1958] M. Maus, S.-F. Chen, M. White, A comparison of template vs. direct model fitting for redshift-space distortions in BOSS, J. Cosmol. Astropart. Phys. 06 (2023) 005, arXiv:2302.07430 [astro-ph.CO].

[1959] E.B. Holm, L. Herold, T. Simon, E.G.M. Ferreira, S. Hannestad, V. Poulin, T. Tram, Bayesian and frequentist investigation of prior effects in EFT of LSS analyses of full-shape BOSS and eBOSS data, Phys. Rev. D 108 (12) (2023) 123514, arXiv:2309.04468 [astro-ph.CO].

[1960] J. Donald-McCann, R. Gsponer, R. Zhao, K. Koyama, F. Beutler, Analysis of unified galaxy power spectrum multipole measurements, Mon. Not. R. Astron. Soc. 526 (3) (2023) 3461–3481, arXiv:2307.07475 [astro-ph.CO].

[1961] M.M. Ivanov, A. Obuljen, C. Cuesta-Lazaro, M.W. Toomey, Full-shape analysis with simulation-based priors: Cosmological parameters and the structure growth anomaly, Phys. Rev. D 111 (6) (2025) 063548, arXiv:2409.10609 [astro-ph.CO].

[1962] A. Chudaykin, M.M. Ivanov, T. Nishimichi, On priors and scale cuts in EFT-based full-shape analyses, 2024, arXiv:2410.16358 [astro-ph.CO].

[1963] H. Zhang, M. Bonici, G. D'Amico, S. Paradiso, W.J. Percival, HOD-informed prior for EFT-based full-shape analyses of LSS, J. Cosmol. Astropart. Phys. 04 (2025) 041, arXiv:2409.12937 [astro-ph.CO].

[1964] T.L. Smith, V. Poulin, Current small-scale CMB constraints to axionlike early dark energy, Phys. Rev. D 109 (10) (2024) 103506, arXiv:2309.03265 [astro-ph.CO].

[1965] R. Murgia, G.F. Abellán, V. Poulin, Early dark energy resolution to the Hubble tension in light of weak lensing surveys and lensing anomalies, Phys. Rev. D 103 (6) (2021) 063502, arXiv:2009.10733 [astro-ph.CO].

[1966] T.L. Smith, V. Poulin, J.L. Bernal, K.K. Boddy, M. Kamionkowski, R. Murgia, Early dark energy is not excluded by current large-scale structure data, Phys. Rev. D 103 (12) (2021) 123542, arXiv:2009.10740 [astro-ph.CO].

[1967] L. Herold, E.G.M. Ferreira, E. Komatsu, New constraint on early dark energy from planck and BOSS data using the profile likelihood, Astrophys. J. Lett. 929 (1) (2022) L16, arXiv:2112.12140 [astro-ph.CO].

[1968] L. Herold, E.G.M. Ferreira, Resolving the Hubble tension with early dark energy, Phys. Rev. D 108 (4) (2023) 043513, arXiv:2210.16296 [astro-ph.CO].

[1969] A. Reeves, L. Herold, S. Vagnozzi, B.D. Sherwin, E.G.M. Ferreira, Restoring cosmological concordance with early dark energy and massive neutr- nos? Mon. Not. R. Astron. Soc. 520 (3) (2023) 3688–3695, arXiv:2207.01501 [astro-ph.CO].

[1970] G. Efstathiou, E. Rosenberg, V. Poulin, Improved planck constraints on axionlike early dark energy as a resolution of the hubble tension, Phys. Rev. Lett. 132 (22) (2024) 221002, arXiv:2311.00524 [astro-ph.CO].

[1971] F. Niedermann, M.S. Sloth, Resolving the Hubble tension with new early dark energy, Phys. Rev. D 102 (6) (2020) 063527, arXiv:2006.06686 [astro-ph.CO].

[1972] J.S. Cruz, S. Hannestad, E.B. Holm, F. Niedermann, M.S. Sloth, T. Tram, Profiling cold new early dark energy, Phys. Rev. D 108 (2) (2023) 023518, arXiv:2302.07934 [astro-ph.CO].

[1973] J. Hamann, S. Hannestad, G.G. Raffelt, Y.Y.Y. Wong, Observational bounds on the cosmic radiation density, J. Cosmol. Astropart. Phys. 08 (2007) 021, arXiv:0705.0440 [astro-ph].

[1974] J. Hamann, Evidence for extra radiation? Profile likelihood versus Bayesian posterior, J. Cosmol. Astropart. Phys. 03 (2012) 021, arXiv:1110.4271 [astro-ph.CO].

[1975] S. Henrot-Versillé, F. Couchot, X. Garrido, H. Imada, T. Louis, M. Tristram, S. Vanasse, Comparison of results on N\_eff from various Planck likelihoods, Astron. Astrophys. 623 (2019) A9, arXiv:1807.05003 [astro-ph.CO].

[1976] A. Gómez-Valent, Fast test to assess the impact of marginalization in Monte Carlo analyses and its application to cosmology, Phys. Rev. D 106 (6) (2022) 063506, arXiv:2203.16285 [astro-ph.CO].

[1977] E.B. Holm, L. Herold, S. Hannestad, A. Nygaard, T. Tram, Decaying dark matter with profile likelihoods, Phys. Rev. D 107 (2) (2023) L021303, arXiv: 2211.01935 [astro-ph.CO].

[1978] A.R. Liddle, Information criteria for astrophysical model selection, Mon. Not. R. Astron. Soc. 377 (2007) L74–L78, arXiv:astro-ph/0701113.

[1979] H. Jeffreys, The theory of probability, in: Oxford Classic Texts in the Physical Sciences, Oxford University Press, 1939.

[1980] D.J. Spiegelhalter, N.G. Best, B.P. Carlin, A. van der Linde, Bayesian measures of model complexity and fit, J. Roy. Stat. Soc. B 64 (4) (2002) 583–639.

[1981] R. Trotta, Bayes in the sky: Bayesian inference and model selection in cosmology, Contemp. Phys. 49 (2008) 71–104, arXiv:0803.4089 [astro-ph].

[1982] P. Marshall, N. Rajguru, A.Z. Slosar, Bayesian evidence as a tool for com- paring datasets, Phys. Rev. D 73 (6) (2006) 067302, arXiv:astro-ph/0412535 [astro-ph].

[1983] W. Handley, P. Lemos, Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio, Phys. Rev. D 100 (4) (2019) 043504, arXiv:1902.04029 [astro-ph.CO].

[1984] M. Raveri, W. Hu, Concordance and discordance in cosmology, Phys. Rev. D 99 (2019) 043506, https://link.aps.org/doi/10.1103/PhysRevD.99.043506.

[1985] M. Raveri, G. Zacharegkas, W. Hu, Quantifying concordance of correlated cosmological data sets, Phys. Rev. D 101 (2020) 103527, https://link.aps.org/ doi/10.1103/PhysRevD.101.103527.

[1986] M. Raveri, C. Doux, Non-Gaussian estimates of tensions in cosmological parameters, Phys. Rev. D 104 (2021) 043504, https://link.aps.org/doi/10. 1103/PhysRevD.104.043504.

[1987] M.a. Leizerovich, S.J. Landau, C.G. Scóccola, Tensions in cosmology: A discussion of statistical tools to determine inconsistencies, Phys. Lett. B 855 (2024) 138844, arXiv:2312.08542 [astro-ph.CO].

[1988] P. Lemos, M. Raveri, A. Campos, et al., DES Collaboration, Assessing tension metrics with dark energy survey and Planck data, Mon. Not. R. Astro. Soc. 505 (4) (2021) 6179–6194, arXiv:2012.09554 [astro-ph.CO].

[1989] M. Ho, M.M. Rau, M. Ntampaka, A. Farahi, H. Trac, B. Poczos, A robust and efficient deep learning method for dynamical mass measurements of galaxy clusters, Astrophys. J. 887 (2019) 25, arXiv:1902.05950 [astro-ph.CO].

[1990] A. Peel, F. Lalande, J.-L. Starck, V. Pettorino, J. Merten, C. Giocoli, M. Meneghetti, M. Baldi, Distinguishing standard and modified gravity cosmolо- gies with machine learning, Phys. Rev. D 100 (2) (2019) 023508, arXiv: 1810.11030 [astro-ph.CO].