A dataset provided by the European Space Agency

Name: Stripe 82 X
Published: 2013-06-15T00:00:00Z

Proposal ID	067300
Title	Stripe 82 X
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000131 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000132 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000133 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000134 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000135 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000136 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000137 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000138 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000139 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000140 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000141 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000142 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000143 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000144 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000145 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000146 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000147 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000148 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000149 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000150 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000151 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673000152 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002331 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002332 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002333 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002334 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002335 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002336 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002337 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002338 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002339 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002340 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002341 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002342 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002343 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002344 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002345 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002346 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002347 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002348 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002349 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002350 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002351 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673002352 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673004501
DOI	https://doi.org/10.5270/esa-vaebffc
Principal Investigator, PI	Prof C. Megan Urry
Abstract	We propose to survey 100 deg2 with XMM-Newton in SDSS Stripe 82, the location ofan unsurpassed collection of publicly available deep multi-wavelength data. Thekey science goals address supermassive black hole growth and clusters ofgalaxies, for which XMMs hard X-ray response and high throughput are essential.This survey will fill a major gap in the spectral coverage over this large aregion of the sky. The survey requires virgul1200 overlapping 3.5ks pointings inMosaic mode, averaging 10ks across most of the field for a flux limit of F=2e-15erg/s/cm2 for point sources. This public Stripe 82 X survey represents aninvestment similar to the CDFS but for an area-flux choice that capitalizes onXMMs unique capabilites and will constitute a major legacy for XMM.
Publications	Finding rare AGN: XMM-Newton and Chandra observations of SDSS Stripe 82 \|LaMassa, Stephanie M., Urry, C. Megan, et al. \| MNRAS \| 436-3581 \| 2013 \| 2013MNRAS.436.3581L \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.436.3581L 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 Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso, E., Risaliti, G., \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti, F., Middei, R., et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey. I. Cluster catalogue and discovery of two merging cluster candidates \|Takey, A., Durret, F., et al. \| A&A \| 594-32 \| 2016 \| 2016A&A...594A..32T \| http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..32T 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 A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 \|Pons, E., Watson, M. G., \| A&A \| 594-72 \| 2016 \| 2016A&A...594A..72P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..72P M Dwarf Activity in the Pan-STARRS1 Medium-Deep Survey: First Catalog and Rotation Periods \|Kado-Fong, E., Williams, P. K. G., et al. \| ApJ \| 833-281 \| 2016 \| 2016ApJ...833..281K \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...833..281K The X-ray properties of z 6 luminous quasars \|Nanni, R., Vignali, C., et al. \| A&A \| 603-128 \| 2017 \| 2017A&A...603A.128N \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.128N The Hunt for Red Quasars: Luminous Obscured Black Hole Growth Unveiled in the Stripe 82 X-Ray Survey \|LaMassa, Stephanie M., Glikman, Eilat, et al. \| ApJ \| 847-100 \| 2017 \| 2017ApJ...847..100L \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...847..100L 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 Luminous WISE-selected Obscured, Unobscured, and Red Quasars in Stripe 82 \|Glikman, E., Lacy, M., et al. \| ApJ \| 861-37 \| 2018 \| 2018ApJ...861...37G \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...861...37G 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 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 The X-ray properties of z &gt; 6 quasars: no evident evolution of accretion physics in the first Gyr of the Universe \|Vito, F., Brandt, W. N., et al. \| A&A \| 630-118 \| 2019 \| 2019A&A...630A.118V \| http://ui.adsabs.harvard.edu/#abs/2019A&A...630A.118V X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field \|Ota, Naomi, Mitsuishi, Ikuyuki, et al. \| PASJ \| 72-1 \| 2020 \| 2020PASJ...72....1O \| http://ui.adsabs.harvard.edu/#abs/2020PASJ...72....1O 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 The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters \|Pastor-Marazuela, I., Webb, N. A., et al. \| A&A \| 640-124 \| 2020 \| 2020A&A...640A.124P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...640A.124P 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 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 A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman, Murray, Ward, Charlotte, et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B 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 An XMM-Newton study of active-inactive galaxy pairs \|Guainazzi, Matteo, De Rosa, Alessandra, et al. \| MNRAS \| 504-393 \| 2021 \| 2021MNRAS.504..393G \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.504..393G Probing the Disk-Corona Systems and Broad-line Regions of Changing-look Quasars with X-Ray and Optical Observations \|Jin, Xiangyu, Ruan, John J., et al. \| ApJ \| 912-20 \| 2021 \| 2021ApJ...912...20J \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...912...20J Caltech-NRAO Stripe 82 Survey (CNSS). V. AGNs That Transitioned to Radio-loud State \|Wo\\u0142owska, Aleksandra, Kunert-Bajraszewska, Magdalena, et al. \| ApJ \| 914-22 \| 2021 \| 2021ApJ...914...22W \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...914...22W An XMM-Newton catalogue of BL Lacs \|de la Calle P\\u00e9rez, I., \\u00c1lvarez Crespo, N., et al. \| A&A \| 655-48 \| 2021 \| 2021A&A...655A..48D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...655A..48D Do blue galaxy-clusters have hot intracluster gas? \|Misato, Rana, Toba, Yoshiki, et al. \| PASJ \| 74-398 \| 2022 \| 2022PASJ...74..398M \| http://ui.adsabs.harvard.edu/#abs/2022PASJ...74..398M 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 The X-ray view of optically selected dual AGN \|De Rosa, Alessandra, Vignali, Cristian, et al. \| MNRAS \| 519-5149 \| 2023 \| 2023MNRAS.519.5149D \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.519.5149D X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf, J., Nandra, K., et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W 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 X\\u2011HESS: A large sample of highly accreting serendipitous AGN under the XMM\\u2011Newton microscope \|Laurenti, M., Tombesi, F., et al. \| AN \| 344-20230053 \| 2023 \| 2023AN....34430053L \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L 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 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	RGS1, EPN, RGS2, EMOS1, OM, EMOS2
Temporal Coverage	2011-12-07T16:01:55Z/2012-05-26T17:50:29Z
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	2013-06-15T00:00:00Z
Keywords	"spectral coverage", "stripe 82 x", "SDSS", "unsurpassed collection", "XMM", "supermassive blackhole growth", "1200 overlapping", "flux choice", "XMM-Newton", "mosaic mode", "major gap", "flux limit", "key science", "sdss stripe 82", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof C. Megan Urry, 2013, 'Stripe 82 X', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vaebffc