Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Farina EP"'
Autor:
Bischetti, M, Feruglio, C, D'Odorico, V, Arav, N, Bañados, E, Becker, G, Bosman, SEI, Carniani, S, Cristiani, S, Cupani, G, Davies, R, Eilers, AC, Farina, EP, Ferrara, A, Maiolino, R, Mazzucchelli, C, Mesinger, A, Meyer, RA, Onoue, M, Piconcelli, E, Ryan-Weber, E, Schindler, J-T, Wang, F, Yang, J, Zhu, Y, Fiore, F
Publikováno v:
Nature, 605(7909), 244-247. NATURE PORTFOLIO
Bright quasars, powered by accretion onto billion-solar-mass black holes, already existed at the epoch of reionization, when the Universe was 0.5-1 billion years old(1). How these black holes formed in such a short time isthe subject of debate, parti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::01af10b1662210bf8ad9236ca100bd41
https://www.repository.cam.ac.uk/handle/1810/337919
https://www.repository.cam.ac.uk/handle/1810/337919
Autor:
Bischetti M; INAF - Osservatorio Astronomico di Trieste, Trieste, Italy. manuela.bischetti@inaf.it., Feruglio C; INAF - Osservatorio Astronomico di Trieste, Trieste, Italy.; IFPU - Institute for Fundamental Physics of the Universe, Trieste, Italy., D'Odorico V; INAF - Osservatorio Astronomico di Trieste, Trieste, Italy.; IFPU - Institute for Fundamental Physics of the Universe, Trieste, Italy.; Scuola Normale Superiore, Pisa, Italy., Arav N; Department of Physics, Virginia Tech, Blacksburg, VA, USA., Bañados E; Max-Planck-Institut für Astronomie, Heidelberg, Germany., Becker G; Department of Physics & Astronomy, University of California, Riverside, CA, USA., Bosman SEI; Max-Planck-Institut für Astronomie, Heidelberg, Germany., Carniani S; Scuola Normale Superiore, Pisa, Italy., Cristiani S; INAF - Osservatorio Astronomico di Trieste, Trieste, Italy., Cupani G; INAF - Osservatorio Astronomico di Trieste, Trieste, Italy., Davies R; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia.; ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Canberra, Australian Capital Territory, Australia., Eilers AC; MIT Kavli Institute for Astrophysics and Space Research, Cambridge, MA, USA., Farina EP; Max Planck Institut für Astrophysik, Garching bei München, Germany., Ferrara A; Scuola Normale Superiore, Pisa, Italy., Maiolino R; Kavli Institute for Cosmology, University of Cambridge, Cambridge, UK., Mazzucchelli C; European Southern Observatory, Vitacura, Chile., Mesinger A; Scuola Normale Superiore, Pisa, Italy., Meyer RA; Max-Planck-Institut für Astronomie, Heidelberg, Germany., Onoue M; Max-Planck-Institut für Astronomie, Heidelberg, Germany., Piconcelli E; INAF - Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy., Ryan-Weber E; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, Australia.; ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Canberra, Australian Capital Territory, Australia., Schindler JT; Max-Planck-Institut für Astronomie, Heidelberg, Germany., Wang F; Department of Astronomy, University of Arizona, Tucson, AZ, USA., Yang J; Steward Observatory, University of Arizona, Tucson, AZ, USA., Zhu Y; Department of Physics & Astronomy, University of California, Riverside, CA, USA., Fiore F; INAF - Osservatorio Astronomico di Trieste, Trieste, Italy.; IFPU - Institute for Fundamental Physics of the Universe, Trieste, Italy.
Publikováno v:
Nature [Nature] 2022 May; Vol. 605 (7909), pp. 244-247. Date of Electronic Publication: 2022 May 11.
Autor:
Bañados E; The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, California 91101, USA., Venemans BP; Max Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany., Mazzucchelli C; Max Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany., Farina EP; Max Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany., Walter F; Max Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany., Wang F; Department of Astronomy, School of Physics, Peking University, Beijing 100871, China.; Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China., Decarli R; Max Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany.; INAF-Osservatorio Astronomico di Bologna, via Gobetti 93/3, 40129 Bologna, Italy., Stern D; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA., Fan X; Steward Observatory, The University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA., Davies FB; Department of Physics, Broida Hall, University of California, Santa Barbara, California 93106-9530, USA., Hennawi JF; Department of Physics, Broida Hall, University of California, Santa Barbara, California 93106-9530, USA., Simcoe RA; MIT-Kavli Center for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, Massachusetts 02139, USA., Turner ML; MIT-Kavli Center for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, Massachusetts 02139, USA.; Las Cumbres Observatory, 6740 Cortona Drive, Goleta, California 93117, USA., Rix HW; Max Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany., Yang J; Department of Astronomy, School of Physics, Peking University, Beijing 100871, China.; Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China., Kelson DD; The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, California 91101, USA., Rudie GC; The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, California 91101, USA., Winters JM; Institut de Radioastronomie Millimétrique (IRAM), 300 rue de la Piscine, 38406 Saint Martin d'Hères, France.
Publikováno v:
Nature [Nature] 2018 Jan 25; Vol. 553 (7689), pp. 473-476. Date of Electronic Publication: 2017 Dec 06.
Autor:
Decarli R; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany., Walter F; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany.; National Radio Astronomy Observatory, Pete V. Domenici Array Science Center, PO Box O, Socorro, New Mexico 87801, USA.; Astronomy Department, California Institute of Technology, MC105-24, Pasadena, California 91125, USA., Venemans BP; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany., Bañados E; The Observatories of the Carnegie Institute of Washington, 813 Santa Barbara Street, Pasadena, California 91101, USA., Bertoldi F; Argelander Institute for Astronomy, University of Bonn, Auf dem Hügel 71, Bonn 53121, Germany., Carilli C; National Radio Astronomy Observatory, Pete V. Domenici Array Science Center, PO Box O, Socorro, New Mexico 87801, USA.; Battcock Centre for Experimental Astrophysics, Cavendish Laboratory, Cambridge CB3 0HE, UK., Fan X; Steward Observatory, The University of Arizona, 933 North Cherry Avenue, Tucson, Arizona 85721-0065, USA., Farina EP; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany., Mazzucchelli C; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany., Riechers D; Cornell University, 220 Space Sciences Building, Ithaca, New York 14853, USA., Rix HW; Max Planck Institut für Astronomie, Königstuhl 17, Heidelberg 69117, Germany., Strauss MA; Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08533, USA., Wang R; Kavli Institute of Astronomy and Astrophysics at Peking University, 5 Yiheyuan Road, Haidian District, Beijing 100871, China., Yang Y; Korea Astronomy and Space Science Institute, Daedeokdae-ro 776, Yuseong-gu Daejeon 34055, South Korea.
Publikováno v:
Nature [Nature] 2017 May 24; Vol. 545 (7655), pp. 457-461.