A dataset provided by the European Space Agency

Name: Going Beyond COSMOS with the XMM-SERVS Survey of W-CDF-S comma XMM-LSS comma and ELAIS-S1
Published: 2017-01-23T23:00:00Z

Proposal ID	079358
Title	Going Beyond COSMOS with the XMM-SERVS Survey of W-CDF-S,XMM-LSS, and ELAIS-S1
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793580101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793580201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793580301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793580401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793580501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793580601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793580701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793580801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793580901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793581001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793581101 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793581201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793581301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793581401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793581501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0793581601
DOI	https://doi.org/10.5270/esa-32zx472
Principal Investigator, PI	Prof William Brandt
Abstract	We propose a 12 deg^2 XMM-Newton survey at 50 ks depth of three prime skyregions: the SERVS areas of W-CDF-S, XMM-LSS, and ELAIS-S1. This XMM-SERVSsurvey will allow outstanding studies of the newly detected 7800 AGNs and 760X-ray groups/clusters by powerfully leveraging multiple intensive radio-to-UVsurveys: ATLAS, HerMES, SERVS, VIDEO, DES, HSC, PS1MD, VOICE, CSI, and PRIMUS.We aim to dramatically advance studies of SMBH growth across the full range ofcosmic environments, links between SMBH accretion and star formation, excep-tional AGNs at high redshifts, protoclusters, and multiple other topics.The targeted XMM-SERVS fields will have extraordinary legacy value as MOONSmassive spectroscopy fields, prime ALMA fields, and DES/LSST deep-drilling fields.
Publications	The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field \|Chen, C.-T. J., Brandt, W. N., et al. \| MNRAS \| 478-2132 \| 2018 \| 2018MNRAS.478.2132C \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478.2132C The Evolution of the Quenching of Star Formation in Cluster Galaxies since z virgul 1 \|Pintos-Castro, I., Yee, H. K. C., et al. \| ApJ \| 876-40 \| 2019 \| 2019ApJ...876...40P \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...876...40P HSC-XD 52: An X-Ray Detected AGN in a Low-mass Galaxy at z \\u0303 0.56 \|Halevi, Goni, Goulding, Andy, et al. \| ApJ \| 885-3 \| 2019 \| 2019ApJ...885L...3H \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...885L...3H Implications of the Environments of Radio-detected Active Galactic Nuclei in a Complex Protostructure at z \\u223c 3.3 \|Shen, Lu, Lemaux, Brian C., et al. \| ApJ \| 912-60 \| 2021 \| 2021ApJ...912...60S \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...912...60S 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 Consistent Analysis of the AGN LF in X-Ray and MIR in the XMM-LSS Field \|Runburg, Jack, Farrah, Duncan, et al. \| ApJ \| 924-133 \| 2022 \| 2022ApJ...924..133R \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...924..133R The RapidXMM upper limit server: X-ray aperture photometry of the XMM-Newton archival observations \|Ruiz, A., Georgakakis, A., et al. \| MNRAS \| 511-4265 \| 2022 \| 2022MNRAS.511.4265R \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.511.4265R 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 A fresh look at AGN spectral energy distribution fitting with the XMM-SERVS AGN sample \|Marshall, Adam, Auger-Williams, Matthew W., et al. \| MNRAS \| 515-5617 \| 2022 \| 2022MNRAS.515.5617M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515.5617M The value-added catalogue of ASAS-SN eclipsing binaries: parameters of 30 000 detached systems \|Rowan, D. M., Jayasinghe, T., et al. \| MNRAS \| 517-2190 \| 2022 \| 2022MNRAS.517.2190R \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517.2190R The Obscured Fraction of Quasars at Cosmic Noon \|Vijarnwannaluk, Bovornpratch, Akiyama, Masayuki, et al. \| ApJ \| 941-97 \| 2022 \| 2022ApJ...941...97V \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...941...97V Detection of radio-AGN in dust-obscured galaxies using deep uGMRT radio continuum observations \|Kayal, Abhijit, Singh, Veeresh, et al. \| JApA \| 43-84 \| 2022 \| 2022JApA...43...84K \| http://ui.adsabs.harvard.edu/#abs/2022JApA...43...84K Search and Characterization of Remnant Radio Galaxies in the XMM-LSS Deep Field \|Dutta, Sushant, Singh, Veeresh, et al. \| ApJ \| 944-176 \| 2023 \| 2023ApJ...944..176D \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...944..176D Identification and Characterization of a Large Sample of Distant Active Dwarf Galaxies in XMM-SERVS \|Zou, Fan, Brandt, W. N., et al. \| ApJ \| 950-136 \| 2023 \| 2023ApJ...950..136Z \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...950..136Z The Most Obscured AGNs in the XMM-SERVS Fields \|Yan, Wei, Brandt, W. N., et al. \| ApJ \| 951-27 \| 2023 \| 2023ApJ...951...27Y \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...951...27Y The LSST AGN Data Challenge: Selection Methods \|Savi\\u0107, \\u0110or\\u0111e V., Jankov, Isidora, et al. \| ApJ \| 953-138 \| 2023 \| 2023ApJ...953..138S \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...953..138S 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 eUDS: the SRG/eROSITA X-ray survey of the UKIDSS Ultra Deep Survey field. Catalogue of sources \|Krivonos, R., Gilfanov, M., et al. \| MNRAS \| 528-1264 \| 2024 \| 2024MNRAS.528.1264K \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.528.1264K Observational properties of active galactic nucleus obscuration during the peak of accretion growth \|Vijarnwannaluk, Bovornpratch, Akiyama, Masayuki, et al. \| MNRAS \| 529-3610 \| 2024 \| 2024MNRAS.529.3610V \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.3610V X-ray spectral properties of dust-obscured galaxies in the XMM-SERVS coverage of the XMM-LSS field \|Kayal, Abhijit, Singh, Veeresh, \| MNRAS \| 531-830 \| 2024 \| 2024MNRAS.531..830K \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.531..830K 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	2017-01-01T03:59:38Z/2017-01-17T01:33:01Z
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	2017-01-23T23:00:00Z
Keywords	"star formation", "excep tional agns", "smbh accretion", "XMM", "760 xray", "xmm newton survey", "xmm servs survey", "XMM-Newton", "prime alma fields", "uv surveys", "elais s1", "cosmic environments", "7800 agns", "prime sky region", "xmm lss", "smbh growth"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof William Brandt, 2017, 'Going Beyond COSMOS with the XMM-SERVS Survey of W-CDF-S comma XMM-LSS comma and ELAIS-S1', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-32zx472