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 ~1200 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
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
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 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
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 > 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
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 |Wou0142owska Aleksandra Kunert-Bajraszewska Magdalena et al. | ApJ | 914-22 | 2021 | 2021ApJ...914...22W | http://ui.adsabs.harvard.edu/#abs/2021ApJ...914...22W
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 deg2 Stripe 82X |Peca Alessandro Cappelluti Nico et al. | ApJ | 943-162 | 2023 | 2023ApJ...943..162P | http://ui.adsabs.harvard.edu/#abs/2023ApJ...943..162P
Xu2011HESS: A large sample of highly accreting serendipitous AGN under the XMMu2011Newton 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
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
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.
