adsabs/WIESP2022-NER huggingface dataset:
Paper: 2017MNRAS.470.3250J (acknowledgments)
Acknowledgements We would like to thank J. D. Long for Python advice and the referee for comments that improved this paper. OCJ and MM acknowledge support from NASA grant, NNX14AN06G, for this work. The authors also acknowledge financial support from the Ministry of Science and Technology (MoST) Taiwan under grant MOST104-2628-M-001-004-MY3. IM and AAZ were funded by the Science and Technology Facilities Council under grant ST/L000768/1. The NASA Astrophysics and Data Analysis Program (Grant NNX13AE66G) supported GCS and the addition of high-resolution IRS spectra to CASSIS, the Combined Atlas of Sources with Spitzer IRS Spectra. Readers are referred to ApJS, 196, 8 (2011). BAS acknowledges support from NASA grants NNX13AD54G and NNX15AF15G. The work of MS was supported by the appointment to the NASA Postdoctoral Program at Goddard Space Flight Center. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. The original description of the VizieR service was published in AAS, 143, 23 (2000). Facilities: Spitzer (IRS), Spitzer (MIPS), Spitzer (IRAC).
Paper: 2018MNRAS.476.4725S (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for their constructive comments that helped us improve the manuscript. DS acknowledges the hospitality of the IAC and a Severo Ochoa visiting grant. SS and JC acknowledge studentships from the Lancaster University. JM acknowledges a Huygens PhD fellowship from Leiden University. APA acknowledges financial support from the Science and Technology Foundation (FCT, Portugal) through research grants UID/FIS/04434/2013 and fellowship PD/BD/52706/2014. The authors thank Alyssa Drake, Kimihiko Nakajima, Yuichi Harikane, Max Gronke, Irene Shivaei, Helmut Dannerbauer, Huub Röttgering, Marius Eide, and Masami Ouchi for many engaging and stimulating discussions. We also thank Sara Perez, Alex Bennett, and Tom Rose for their involvement in the early stages of this project. Based on data products from observations made with European Southern Observatory (ESO) Telescopes at the La Silla Paranal Observatory under ESO programme IDs 294.A-5018, 097.A-0943, 098.A-0819, 099.A-0254, and 179.A-2005 and on data products produced by terapix and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium. Based on observations using the WFC on the 2.5 m INT, as part of programmes 2013AN002, 2013BN008, 2014AC88, 2014AN002, 2014BN006, 2014BC118, and 2016AN001. The INT is operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. This work is based in part on data products produced at terapix available at the Canadian Astronomy Data Centre as part of the Canada–France–Hawaii Telescope Legacy Survey (CFHTLS), a collaborative project of NRC and CNRS. We are grateful to the CFHTLS, COSMOS-UltraVISTA, and COSMOS survey teams. We are also unmeasurably thankful to the pioneering and continuous work from previous Ly α surveys’ teams. Without these previous Ly α and the wider reach legacy surveys, this research would have been impossible. We also thank the VUDS team for making available spectroscopic redshifts from data obtained with VIMOS at the European Southern Observatory Very Large Telescope, Paranal, Chile, under Large Programme 185.A-0791. Finally, the authors acknowledge the unique value of the publicly available programming language python , including the numpy and scipy (Van Der Walt, Colbert Varoquaux 2011 ; Jones et al. 2001 ), matplotlib (Hunter 2007 ), astropy (Astropy Collaboration et al. 2013 ), and the topcat analysis program (Taylor 2005 ). We publicly release a catalogue with all LAEs used in this paper (SC4K), so it can be freely explored by the community (see five example entries in Table A1 ).
Paper: 2015ApJ...808..194L (acknowledgments)
The authors would like to sincerely thank an anonymous referee whose comments led to substantial improvements in the manuscript, Luc Arnold for discussions on the E-ELT capabilities, Franck Selsis for discussions on the thermal-IR emission of planets with an atmosphere during their day–night cycle, and Antoine Crouzier for different comments. A.L. and F.M. thank CNES for their continuous technical support regarding space interferometry, free flying, and high-precision astrometry, and the French POLCA project (ANR-10-BLAN-0511). O.A. acknowledges support from the European Research Council under the European Union's Seventh Framework Program (ERC grant agreement No. 337569) and from the French Community of Belgium through an ARC grant for Concerted Research Action.
Paper: 2017MNRAS.465..492M (acknowledgments)
This work is based on the observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under ESO programme 095.D-0343(A). We thank the anonymous referee for his/her very constructive comments to our manuscript. RPM acknowledges financial support from the project TElescopi CHErenkov made in Italy (TECHE).it. CRA 1.05.06.04.01 cap 1.05.08 for the project ‘Studio multi-lunghezze d'onda da stelle di neutroni con particolare riguardo alla emissione di altissima energia’. DGC acknowledges the financial support by CONICYT through a ‘Becas Chile’ fellowship no. 72150555.
Paper: 2018MNRAS.479.2853N (acknowledgments)
ACKNOWLEDGEMENTS The authors would like to thank the anonymous referee for detailed, insightful, and thorough feedback that improved the quality of the manuscript. We would also like to thank Till Sawala for useful discussions and for providing the raw data used in Appendix C , and Roan Haggar for code-testing the public software. This research made use of numpy (van der Walt, Colbert Varoquaux 2011 ), scipy (Jones, Oliphant Peterson 2011 ) and matplotlib (Hunter 2007 ) and we thank their developers for making them freely available. ON was supported by the Science and Technology Facilities Council (STFC) through grant ST/N50404X/1 and MC, ARJ, and CSF were supported by STFC grant ST/L00075X/1. This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility ( www.dirac.ac.uk ). This equipment was funded by BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grants ST/H008539/1 and ST/K00087X/1, STFC DiRAC Operations grant ST/K003267/1, and Durham University. DiRAC is part of the National E-Infrastructure.
Paper: 2018MNRAS.473..909B (acknowledgments)
Acknowledgements SB is thankful to the anonymous referee for helpful comments that helped us improve some of the descriptions in this paper. SB is indebted to Sverre Aarseth of the Institute of Astronomy, Cambridge, for his efforts in improving nbody6/7 , without which this study would not have been possible. SB is thankful to Sverre Aarseth also for reading the manuscript and providing improvement suggestions. SB is thankful to the computing team of the Argelander-Institut fr Astronomie, University of Bonn, for their efficient maintenance of the workstations on which all the computations have been performed.
Paper: 2018MNRAS.474.5300D (acknowledgments)
ACKNOWLEDGEMENTS We thank Alis Deason for providing the properties of her modelled stellar haloes in electronic form. We acknowledge useful discussions with Antonela Monachesi, Kohei Hattori, Sarah Loebman, Monica Valluri, Ian Roederer, and Adam Smercina. We also would like to thank the Illustris simulations team, in particular Annalisa Pillepich, Vincent Rodrigues-Gomez, and Dylan Nelson.
Paper: 2018ApJ...863....4L (acknowledgments)
We thank Bharat Kumar Yerra, Li Haining, Tan Kefeng, and Liu Yujuan for their constructive suggestions and discussions. This work is supported by the Astronomical Big Data Joint Research Center, co-founded by the National Astronomical Observatories, Chinese Academy of Sciences, and the Alibaba Cloud. This study is supported by the National Natural Science Foundation of China under grant Nos. 11390371, 11233004, U1431106, 11573035, 11625313, and 11603033, the National Key Basic Research Program of China (973 program), 2014CB845701 and 2014CB845703, and JSPS—CAS Joint Research Program. W.A. is partially supported by JSPS KAKENHI grant No. 16H02168.
Paper: 2019MNRAS.483L..42K (acknowledgments)
ACKNOWLEDGEMENTS We would like to thank the referee for valuable comments. EK thanks K. É. Gabányi and S. Frey for discussions on the topic. This work was supported by the Hungarian National Research Development and Innovation Office (NKFIH) in the form of the grant 123996, and it was based upon work from the COST action CA15117 (CANTATA), supported by COST (European Cooperation in Science and Technology). This research has made use of data from the OVRO 40-m monitoring programme (Richards et al. 2011 ), which is supported in part by NASA grants NNX08AW31G, NNX11A043G and NNX14AQ89G and NSF grants AST-0808050 and AST-1109911. This research has made use of data from the MOJAVE data base, which is maintained by the MOJAVE team (Lister et al. 2009a ). The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Paper: 2016MNRAS.457.4012A (acknowledgments)
We thank the anonymous referee for the comments and suggestions that improved this paper. We acknowledge Vladimir Avila-Reese, Xavier Hernandez, Manuel Peimbert and Liliana Hernández-Martínez, for helpful suggestions. LC thanks for the financial supports provided by CONACyT of México (grant 241732), by PAPIIT of México (IG110115, IA100815, IA101315) and by MINECO of Spain (AYA2010-16717). NA-V thanks for the financial support provided by Universidad Iberoamericana.
Paper: 2019MNRAS.482.2950T (acknowledgments)
ACKNOWLEDGEMENTS The authors thank the anonymous referee for constructive feedback that improved the manuscript. We wish to sincerely thank all the National Radio Astronomy Observatory, SMA, JCMT, and IRAM NOEMA staff that supported us during this observing campaign. The authors also offer a special thanks to the IRAM NOEMA Director, Karl-Fredrich Schuster, for granting our NOEMA DDT request. AJT thanks Craig Heinke and Bailey Tetarenko for useful discussions on accretion disc contributions in broad-band spectra of X-ray binaries. AJT is supported by an Natural Sciences and Engineering Research Council of Canada (NSERC) Post-Graduate Doctoral Scholarship (PGSD2-490318-2016). AJT and GRS are supported by NSERC Discovery Grants. JCAMJ is the recipient of an Australian Research Council Future Fellowship (FT140101082). SBM acknowledges support from VICI grant Nr. 639.043.513/520, funded by the Netherlands Organisation for Scientific Research (NWO). TDR acknowledges support from the NWO Veni Fellowship, grant number 639.041.646. DA acknowledges support from the Royal Society. This work is based on observations carried out under project numbers S15DE and D15AB with the IRAM NOEMA Interferometer. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain). The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. We thank the engineers and staff of the Mullard Radio Astronomy Observatory for maintenance and operation of AMI, which is supported by the Universities of Cambridge and Oxford. The AMI telescope acknowledges support from the European Research Council under grant ERC-2012-StG-307215 LODESTONE. The SMA is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics, and is funded by the Smithsonian Institution and the Academia Sinica. The JCMT is operated by the East Asian Observatory on behalf of The National Astronomical Observatory of Japan; Academia Sinica Institute of Astronomy and Astrophysics; the Korea Astronomy and Space Science Institute; the Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments, budgeted from the Ministry of Finance (MoF) of China and administrated by the Chinese Academy of Sciences (CAS), as well as the National Key RD Program of China (No. 2017YFA0402700). Additional funding support is provided by the Science and Technology Facilities Council of the United Kingdom and participating universities in the United Kingdom and Canada. The authors also wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. We acknowledge with thanks the variable star observations from the AAVSO International Database contributed by observers worldwide and used in this research.
Paper: 2016MNRAS.459.3059S (acknowledgments)
The authors thank Prateek Sharma for useful discussions. SC gratefully acknowledges financial support received through the INSPIRE faculty fellowship (DST/INSPIRE/04/2013/000365) awarded by Department of Science and Technology (Government of India).
Paper: 2017ApJ...849..161F (acknowledgments)
We are grateful to the anonymous referee for constructive comments leading to significant improvement of this paper. We thank the financial support of the Key Research Program of the CAS (grant No. KJZD-EW-M06), the National Natural Science Foundation of China (NSFC; grant No. 11433004), and the Ministry of Science and Technology of China (2016YFA0400700). We also thank the financial support of the NSFC (grant No. 11273052), and the Youth Innovation Promotion Association, CAS. We also acknowledge the support of the staff of the Lijiang 2.4 m telescope. Funding for this telescope has been provided by the CAS and the People’s Government of Yunnan Province.
Paper: 2019A&A...626A..50D (acknowledgments)
Based on observations at the European Southern Observatory in programme 074D.0011 and 171.D-0237. This work has made use of data from the European Space Agency (ESA) mission Gaia ( https://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium ). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. CJE and DJL acknowledge the OWC. CJE thanks Linda Smith for obtaining the AAT spectra, and is grateful for the past hospitality of the Space Telescope Science Institute and travel funding from its Director’s Discretionary Research Fund (DDRF).
Paper: 2017ApJ...849..105L (acknowledgments)
We thank everyone who offered their help to this work, including Matthew Miller, Edmund Hodges-Kluck, Zhijie Qu, and our anonymous referee, whose comments helped to improve this work. Special thanks also go to Eric Peng for the computational resources he provided. This research is funded by the China Scholarship Council, NASA ADAP grant NNX16AF23G, and the Department of Astronomy at the University of Michigan, who we also thank for their hospitality. Software: AtomDB (Foster et al. 2012 ), emcee (Foreman-Mackey et al. 2013 ).
Paper: 2019ApJ...887..107F (acknowledgments)
We are grateful to Ivan Marti-Vidal and the Nordic ALMA Regional Center for providing us with helpful CASA software tools and advice on analyzing the data. We appreciate Tohru Nagao, Jeremy Blaizot, Peter Mitchell, Takashi Kojima, Shiro Mukae, Yuichi Harikane, Akio Inoue, and Rieko Momose for useful comments and suggestions. We are indebted for the support of the staff at the ALMA Regional Center. This paper makes use of the following ALMA data: ADS/JAO, ALMA #2013.1.00815.S, #2015.1.00834.S, #2015.1.01111.S, #2015.1.01105, #2016.1.01240.S, #2012.1.00523.S, and #2012.1.00602.S. ALMA is a partnership of the ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by the ESO, AUI/NRAO, and NAOJ. This study is supported by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan, and KAKENHI (15H02064, 16J02344, 17H01110, 17H01111, and 17H01114) Grant-in-Aid for Scientific Research (A) through the Japan Society for the Promotion of Science (JSPS), the Grant-in-Aid for JSPS Research Fellow, the NAOJ ALMA Scientific Research grant No. 2017-06B, and the Munich Institute for Astro- and Particle Physics (MIAPP) of the DFG cluster of excellence “Origin and Structure of the Universe.” S.F. is supported by the ALMA Japan Research Grant of NAOJ Chile Observatory NAOJ-ALMA-197, The 2018 Graduate Research Abroad in Science Program Grant (GRASP2018), and the Hayakawa Satio Fund awarded by the Astronomical Society of Japan. A.F. and R.J.I. acknowledge support from the ERC Advanced Grant INTERSTELLAR H2020/740120 and COSMIC ISM 321302, respectively.
Paper: 2019ApJ...871...14B (acknowledgments)
We thank the referee for the comments and suggestions to improve the presentation of our results. The work of L.B., C.E., and C.F. was partially funded under the auspices of the U.S. Dept. of Energy and supported by contract W-7405-ENG-36 to Los Alamos National Laboratory. Simulations at LANL were performed on HPC resources provided under the Institutional Computing program.
Paper: 2020MNRAS.491.4509B (acknowledgments)
ACKNOWLEDGEMENTS This work was supported by XSEDE computing grants TG-AST190001 and TG-AST180052 and the Stampede2 supercomputer at the Texas Advanced Computing Center. KSSB was supported by a Porat Postdoctoral Fellowship at Stanford University.
Paper: 2018MNRAS.478.1660G (acknowledgments)
Acknowledgements We are grateful to Ski Antonucci, Edi Bon, Xiao-Bo Dong, Wen-Juan Liu, Bill Mathews, and Victor Oknyansky for extensive comments on the paper. We also wish to thank the anonymous referee for numerous helpful comments that have improved the paper.
Paper: 2016ApJ...816...16J (acknowledgments)
We acknowledge the support from a 985 project at Peking University. L.J., S.C., and E.E. also acknowledge the support from NASA through awards issued by STScI ( HST PID: 11149,12329,12616) and by JPL/Caltech ( Spitzer PID: 40026,70094). We would like to thank R. Ryan for his advice on IRAC photometry and using iGALFIT . We also thank J. Rhoads and Z. Zheng for their insightful comments, and thank P. Madau and P. A. Oesch for providing us with the data used for Figures 10 and 12 . Facilities: HST (NICMOS,WFC3) , Spitzer (IRAC) , Subaru (Suprime-Cam) .
Paper: 2015MNRAS.449.2250K (acknowledgments)
I would like to thank Frank Postberg, Nicolas Altobelli, and Mario Trieloff for stimulating discussions on the composition of dust in the Local Cloud. I also thank Martin Hilchenbach, Harald Krüger, and Thomas Albin for their hospitality during my stay at Max Planck Institute for Solar System Research (MPS), where much of the writing was performed. Special thanks go to an anonymous reviewer who made careful reading and provided useful comments and suggestions. I am grateful to MPS's research fellowship and financial support for my travel expense to MPS as well as to JSPS's Grants-in-Aid for Scientific Research (#26400230). This research has made use of the SIMBAD data base, operated at CDS, Strasbourg, France.
Paper: 2018A&A...619A.164G (acknowledgments)
MG and PKB are funded by Science and Technology Facilities Council (UK), grant ST/P000428/1. Simulations have been performed using the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility.
Paper: 2018ApJ...864..170G (acknowledgments)
V.V.G. and J.C. acknowledge support from the National Aeronautics and Space Administration under grant No. 15XRP15_20140 issued through the Exoplanets Research Program. This paper makes use of the following ALMA data: ADS/JAO.ALMA# 2012.1.00681.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ.
Paper: 2017A&A...600A..52D (acknowledgments)
Authors thank the anonymous referee for the helpful comments. This work is partially supported by the Bundesministerium für Wirtschaft und Technologie through the Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR) under the grant numbers 50 OG 1301, 50 OR 1310.
Paper: 2020MNRAS.492.4080G (acknowledgments)
ACKNOWLEDGEMENTS We are sincerely grateful to the referee for constructive and valuable suggestions and comments, which help us improve the manuscript. We thank the Square Kilometre Array Regional Center prototype developed by Shanghai Astronomical Observatory for providing us with computing resources. We acknowledge the support of Astronomical Information Technology Group and Public Technology Service Center, National Astronomical Observatories, Chinese Academy of Sciences (NAOC); this work was supported by High Performance Computing Cluster of NAOC. This work was supported by the National Key RD Programme of China (grant no. 2018YFA0404600), the Strategic Priority Research Program of Chinese Academy of Sciences (grant no. XDB23010300), and the Key Projects of Frontier Science of Chinese Academy of Sciences (grant no. QYZDY-SSW-SLH022).
Paper: 2019MNRAS.485.1435H (acknowledgments)
ACKNOWLEDGEMENTS Parts of this research were conducted by the Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav), through project number CE170100004. EJH acknowledges support from an Australian Research Council DECRA Fellowship (DE170100891). The authors gratefully thank Raymond Frey (University of Oregon), the assigned reviewer for the LIGO Scientific Collaboration, for conducting a thorough review of the manuscript that included a number of insightful suggestions. We are also particularly grateful to Giulia Stratta (INAF/OAS), who provided some useful comments to improve the manuscript. We also thank Aaron Tohuvavohu of the Neil Gehrels Swift Observatory ( Swift ) for useful discussions on the follow-up capabilities of Swift . Finally, we thank the anonymous referee for a thorough reading of the manuscript and for providing a number of erudite suggestions that have enriched the paper. This paper has LIGO document ID P1800322.
Paper: 2017MNRAS.471.4917J (acknowledgments)
Acknowledgements The authors thank Elena Lega and Bertram Bitsch for an extremely careful reading of a first draft of this manuscript, and for constructive feedback. MAJ acknowledges financial support from a UNAM DGAPA fellowship. The simulations presented in this work were run on a GPU cluster acquired with CONACyT's grant 178377. The authors acknowledge support from UNAM's grant PAPIIT IN101616.
Paper: 2015ApJ...809..137K (acknowledgments)
We thank K. Dalmasse, S. Guidoni, A. Higginson, S. Masson, and K. Muglach for illuminating discussions and helpful suggestions, and we greatly appreciate J. Karpen's contribution of the artwork shown in Figure 1 . K.J.K. acknowledges support for this work by a cooperative agreement between the Catholic University of America and the NASA Goddard Space Flight Center, as well as additional funding received through the NASA Earth and Space Science Fellowship program. The participation of S.KA. and C.R.D. was sponsored by NASA's Heliophysics Theory and Supporting Research programs. The numerical simulations were supported by a grant of NASA High End Computing resources to C.R.D.
Paper: 2016ApJ...821...77K (acknowledgments)
The authors are grateful to the anonymous referee who provided a variety of insightful comments that helped to strengthen and clarify the results presented here.