HYPERION: Coevolution of supermassive black holes and galaxies at z > 6 and the build-up of massive galaxies

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作者
Tripodi, R. [1 ,2 ,3 ,4 ]
Feruglio, C. [2 ,3 ]
Fiore, F. [1 ,2 ,3 ]
Zappacosta, L. [5 ]
Piconcelli, E. [5 ]
Bischetti, M. [1 ]
Bongiorno, A. [5 ]
Carniani, S. [6 ]
Civano, F. [7 ]
Chen, C.-C. [8 ]
Cristiani, S. [2 ,3 ]
Cupani, G. [2 ,3 ]
Di Mascia, F. [6 ]
D'Odorico, V. [1 ,3 ,6 ]
Fan, X. [9 ]
Ferrara, A. [6 ]
Gallerani, S. [6 ]
Ginolfi, M. [10 ,11 ]
Maiolino, R. [12 ,13 ,14 ]
Mainieri, V. [15 ]
Marconi, A. [10 ]
Saccheo, I. [5 ]
Salvestrini, F. [2 ]
Tortosa, A. [5 ]
Valiante, R. [5 ]
机构
[1] Dipartimento di Fisica, Università di Trieste, Sezione di Astronomia, Via G. B. Tiepolo 11, Trieste,34131, Italy
[2] INAF - Osservatorio Astronomico di Trieste, Via G. Tiepolo 11, Trieste,34143, Italy
[3] IFPU - Institute for Fundamental Physics of the Universe, Via Beirut 2, Trieste,34151, Italy
[4] University of Ljubljana, Department of Mathematics and Physics, Jadranska ulica 19, Ljubljana,1000, Slovenia
[5] INAF - Osservatorio Astronomico di Roma, Via Frascati 33, Monte Porzio Catone,00040, Italy
[6] Scuola Normale Superiore, Piazza dei Cavalieri 7, Pisa,56126, Italy
[7] NASA Goddard Space Flight Center, Greenbelt,MD,20771, United States
[8] Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), No. 1, Sec. 4, Roosevelt Road, Taipei,10617, Taiwan
[9] Steward Observatory, University of Arizona, Tucson,AZ, United States
[10] Università di Firenze, Dipartimento di Fisica e Astronomia, Via G. Sansone 1, Firenze, Sesto Fiorentino,50019, Italy
[11] INAF - Osservatorio Astrofisico di Arcetri, Via Largo E. Fermi 5, Firenze,50125, Italy
[12] Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge,CB3 0HA, United Kingdom
[13] Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge,CB3 0HA, United Kingdom
[14] Department of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom
[15] European Southern Observatory, Karl- Schwarzschild- Straße 2, Garching bei München,85748, Germany
来源
Astronomy and Astrophysics | 2024年 / 689卷
关键词
We thank the referee for providing insightful comments that helped the clarity and robustness of this work. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2019.1.01633.S; 2015.1.00399.S; 2018.1.01790.S; 2021.2.00151.S; 2017.1.01472.S; 2018.1.01188.S; 2021.1.00934.S; 2021.2.00064.S; 2018.1.01289.S; 2019.1.00672.S; 2017.1.01195.S; 2016.1.01063.S. ALMA is a partnership of ESO (representing its member states); NFS (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 ESO; AUI/NRAO and NAOJ. The project leading to this publication has received support from ORP; that is funded by the European Unionu2019s Horizon 2020 research and innovation programme under grant agreement No. 101004719 [ORP]. RT acknowledges financial support from the University of Trieste. RT; CF; FF; MB; EP acknowledge support from PRIN MIUR project u201CBlack Hole winds and the Baryon Life Cycle of Galaxies: the stone-guest at the galaxy evolution supperu201D; contract #2017PH3WAT. C.-C.C. acknowledges support from the National Science and Technology Council of Taiwan (NSTC 111-2112M-001-045-MY3); as well as Academia Sinica through the Career Development Award (AS-CDA-112-M02). EP; LZ and CF acknowledge financial support from the Bando Ricerca Fondamentale INAF 2022 Large Grant u201CToward a holistic view of the Titans: multi-band observations of zu2004>u20046 QSOs powered by greedy supermassive black-holesu201D. RM acknowledges ERC Advanced Grant 695671 QUENCH; and support from the UK Science and Technology Facilities Council (STFC). RM also acknowledges funding from a research professorship from the Royal Society. SC acknowledges support from the European Union (ERC; WINGS; 101040227). Facilities: ALMA. Software: astropy (Astropy Collaboration 2022); Matplotlib; (Hunter; 2007); SciPy (Gommers et al. 2023); CASA; (v5.1.1-5; CASA Team 2022);
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