A dataset provided by the European Space Agency

Name: Black Hole Growth in Luminous Quasars with XMM-Newton Legacy Stripe 82X Survey
Published: 2015-08-27T22:00:00Z

Proposal ID	074744
Title	Black Hole Growth in Luminous Quasars with XMM-Newton Legacy Stripe 82X Survey
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440131 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440132 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440133 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440134 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440135 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440136 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440137 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440138 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440139 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440140 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440141 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440142 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440143 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440144 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440145 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440146 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440147 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440148 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440149 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440150 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440151 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747440152
DOI	https://doi.org/10.5270/esa-rxwrvia
Principal Investigator, PI	Prof C. Megan Urry
Abstract	We propose an XMM-Newton survey overlapping 20 deg^2 in legacy field SDSS Stripe82, the location of an unsurpassed collection of publicly available deepmulti-wavelength data, including >800 optical spectra per deg^2. The addition ofwide-field hard X-ray coverage addresses our key science goal to determinesupermassive black hole growth in quasars, which likely dominate the total blackhole mass accreted over cosmic time. The survey area and depth are designed toprobe luminosities and redshifts that have been poorly explored in hard X-rays,capitalizing on XMM-Newton.s hard X-ray response, large effective area and fieldof view. Stripe 82X.. requires 185 overlapping 4.5-ks pointings in mosaic mode,with limiting flux F_(0.5-2keV) virgul 5e-15 erg/s/cm^2 over most of the field.
Publications	The 31 Deg2 Release of the Stripe 82 X-Ray Survey: The Point Source Catalog \|LaMassa, Stephanie M., Urry, C. Megan, et al. \| ApJ \| 817-172 \| 2016 \| 2016ApJ...817..172L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...817..172L XMM-Newton publication statistics \|Ness, J.-U., Parmar, A. N., et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The legacy of Stripe 82X in the next decade of XMM-Newton \|LaMassa, S. M., \| AN \| 338-323 \| 2017 \| 2017AN....338..323L \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..323L AGN Populations in Large-volume X-Ray Surveys: Photometric Redshifts and Population Types Found in the Stripe 82X Survey \|Ananna, Tonima Tasnin, Salvato, Mara, et al. \| ApJ \| 850-66 \| 2017 \| 2017ApJ...850...66A \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...850...66A An Intrinsic Link between Long-term UV/Optical Variations and X-Ray Loudness in Quasars \|Kang, Wen-yong, Wang, Jun-Xian, et al. \| ApJ \| 868-58 \| 2018 \| 2018ApJ...868...58K \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...868...58K SDSS-IV eBOSS Spectroscopy of X-Ray and WISE AGNs in Stripe 82X: Overview of the Demographics of X-Ray- and Mid-infrared-selected Active Galactic Nuclei \|LaMassa, Stephanie M., Georgakakis, Antonis, et al. \| ApJ \| 876-50 \| 2019 \| 2019ApJ...876...50L \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...876...50L Photometric redshifts for X-ray-selected active galactic nuclei in the eROSITA era \|Brescia, M., Salvato, M., et al. \| MNRAS \| 489-663 \| 2019 \| 2019MNRAS.489..663B \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489..663B X-ray observations of luminous dusty quasars at z &gt; 2 \|Lansbury, G. B., Banerji, M., et al. \| MNRAS \| 495-2652 \| 2020 \| 2020MNRAS.495.2652L \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.495.2652L A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O Exploring AGN and star formation activity of massive galaxies at cosmic noon \|Florez, Jonathan, Jogee, Shardha, et al. \| MNRAS \| 497-3273 \| 2020 \| 2020MNRAS.497.3273F \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3273F Forward modelling the multiwavelength properties of active galactic nuclei: application to X-ray and WISE mid-infrared samples \|Georgakakis, Antonis, Ruiz, Angel, \| MNRAS \| 499-710 \| 2020 \| 2020MNRAS.499..710G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.499..710G Dying of the Light: An X-Ray Fading Cold Quasar at z \\u223c 0.405 \|Cooke, Kevin C., Kirkpatrick, Allison, et al. \| ApJ \| 903-106 \| 2020 \| 2020ApJ...903..106C \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...903..106C The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou, Min-Hua, Gu, Min-Feng, \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z AGN and star formation at cosmic noon: comparison of data to theoretical models \|Florez, Jonathan, Jogee, Shardha, et al. \| MNRAS \| 508-762 \| 2021 \| 2021MNRAS.508..762F \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.508..762F Accretion history of AGN: Estimating the host galaxy properties in X-ray luminous AGN from z = 0-3 \|Coleman, Brandon, Kirkpatrick, Allison, et al. \| MNRAS \| 515-82 \| 2022 \| 2022MNRAS.515...82C \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515...82C On the Cosmic Evolution of AGN Obscuration and the X-Ray Luminosity Function: XMM-Newton and Chandra Spectral Analysis of the 31.3 degSUP_OPEN2SUP_CLOSE Stripe 82X \|Peca, Alessandro, Cappelluti, Nico, et al. \| ApJ \| 943-162 \| 2023 \| 2023ApJ...943..162P \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...943..162P The Accretion History of AGN: The Spectral Energy Distributions of X-Ray-luminous Active Galactic Nuclei \|Auge, Connor, Sanders, David, et al. \| ApJ \| 957-19 \| 2023 \| 2023ApJ...957...19A \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...957...19A The intrinsic X-ray luminosity distribution of an optically selected SDSS quasar population \|Rankine, Amy L., Aird, James, et al. \| MNRAS \| 527-9004 \| 2024 \| 2024MNRAS.527.9004R \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.527.9004R Exploring X-Ray Properties of Low-metallicity Dwarf Galaxies \|Cann, Jenna M., Weaver, Kimberly A., et al. \| ApJ \| 961-178 \| 2024 \| 2024ApJ...961..178C \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..178C The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2014-08-04T20:17:02Z/2014-08-06T12:11:43Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2015-08-27T22:00:00Z
Keywords	"hard xray", "XMM-Newton", "key science", "unsurpassed collection", "xmm newton", "stripe 82x survey", "optical spectra", "luminous quasars", "limiting flux f_0", "hard xray response", "SDSS", "XMM", "stripe 82x ''", "black hole growth", "mosaic mode", "185 overlapping", "poorly explored", "supermassive blackhole growth", "probe luminosities", "cosmic time"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof C. Megan Urry, 2015, 'Black Hole Growth in Luminous Quasars with XMM-Newton Legacy Stripe 82X Survey', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rxwrvia