A dataset provided by the European Space Agency

Name 9777
Title The environment of QSOs at the reionization epoch
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9777;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-q4jp02k
Author European Space Agency
Description This is a scientific proposal for HST mission. For specific information please visit https:\\archive.stsci.edu\proposal_search.php?id=9777&mission=hst
Publication A deep 1.4 GHz survey of the J1030 equatorial field: A new window on radio source populations across cosmic time, D'Amato, Quirino,Prandoni, I.,Gilli, R., Astronomy and Astrophysics, 668, 2022-12-01 00:00:00, 2022A&A...668A.133D||A galaxy as the source of a C IV absorption system close to the epoch of reionization, Díaz, C. Gonzalo,Ryan-Weber, Emma V.,Cooke, Jeff, Monthly Notices of the Royal Astronomical Society, 418, 2011-12-01 00:00:00, 2011MNRAS.418..820D||Discovery of molecular gas fueling galaxy growth in a protocluster at z = 1.7, D'Amato, Q.,Gilli, R.,Prandoni, I., Astronomy and Astrophysics, 641, 2020-09-01 00:00:00, 2020A&A...641L...6D||Evidence of Primordial Clustering around the QSO SDSS J1030+0524 at z=6.28, Stiavelli, M.,Djorgovski, S. G.,Pavlovsky, C., The Astrophysical Journal, 622, 2005-03-01 00:00:00, 2005ApJ...622L...1S||Faint LAEs near z > 4.7 C IV absorbers revealed by MUSE, Díaz, C. G.,Ryan-Weber, E. V.,Karman, W., Monthly Notices of the Royal Astronomical Society, 502, 2021-04-01 00:00:00, 2021MNRAS.502.2645D||Large-scale environment of z ∼ 5.7 C IV absorption systems -II. Spectroscopy of Lyman α emitters, Díaz, C. Gonzalo,Ryan-Weber, Emma V.,Cooke, Jeff, Monthly Notices of the Royal Astronomical Society, 448, 2015-04-01 00:00:00, 2015MNRAS.448.1240D||Multi-Wavelength Study of a Proto-BCG at z = 1.7, D'Amato, Quirino,Prandoni, I.,Brienza, Marisa, Galaxies, 9, 2021-12-01 00:00:00, 2021Galax...9..115D||No Overdensity of Lyman-Alpha Emitting Galaxies around a Quasar at z ∼ 5.7, Mazzucchelli, C.,Bañados, E.,Decarli, R., The Astrophysical Journal, 834, 2017-01-01 00:00:00, 2017ApJ...834...83M||Redshift identification of X-ray-selected active galactic nuclei in the J1030 field: searching for large-scale structures and high-redshift sources, Marchesi, S.,Mignoli, M.,Gilli, R., Astronomy and Astrophysics, 656, 2021-12-01 00:00:00, 2021A&A...656A.117M||Stellar Masses of Lyman Break Galaxies, Lyα Emit...ters, and Radio Galaxies in Overdense Regions at z = 4-6, Overzier, Roderik A.,Shu, Xinwen,Zheng, Wei, The Astrophysical Journal, 704, 2009-10-01 00:00:00, 2009ApJ...704..548O||The Dark Side of QSO Formation at High Redshifts, Romano-Diaz, Emilio,Shlosman, Isaac,Trenti, Michele, The Astrophysical Journal, 736, 2011-07-01 00:00:00, 2011ApJ...736...66R||The diverse galaxy counts in the environment of high-redshift massive black holes in Horizon-AGN, Habouzit, Mélanie,Volonteri, Marta,Somerville, Rachel S., Monthly Notices of the Royal Astronomical Society, 489, 2019-10-01 00:00:00, 2019MNRAS.489.1206H||The realm of the galaxy protoclusters. A review, Overzier, Roderik A., Astronomy and Astrophysics Review, 24, 2016-11-01 00:00:00, 2016A&ARv..24...14O||Web of the giant: Spectroscopic confirmation of a large-scale structure around the z = 6.31 quasar SDSS J1030+0524, Mignoli, Marco,Gilli, R.,Decarli, Roberto, Astronomy and Astrophysics, 642, 2020-10-01 00:00:00, 2020A&A...642L...1M
Instrument ACS, ACS/WFC
Temporal Coverage 2003-11-15T18:54:47Z/2004-07-06T11:06:09Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2005-07-07T12:40:29Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005, The Environment Of Qsos At The Reionization Epoch, 1.0, European Space Agency, https://doi.org/10.5270/esa-q4jp02k