A dataset provided by the European Space Agency

Name 078045
Title Going Beyond COSMOS with the XMM-SERVS Survey of W-CDF-S, XMM-LSS, and ELAIS-S1
URL

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DOI 10.5270/esa-dz4rqtv
Author Prof William Brandt
Description We propose a 12 deg^2 XMM-Newton survey at 50 ks depth of three prime sky regions: the SERVS areas of W-CDF-S, XMM-LSS, and ELAIS-S1. This XMM-SERVS survey will allow outstanding studies of the newly detected 7800 AGNs and 760 X-ray groups-clusters by powerfully leveraging multiple intensive radio-to-UV surveys: ATLAS, HerMES, SERVS, VIDEO, DES, HSC, PS1MD, VOICE, CSI, and PRIMUS. We aim to dramatically advance studies of SMBH growth across the full range of cosmic environments, links between SMBH accretion and star formation, exceptional AGNs at high redshifts, protoclusters, and multiple other topics. The targeted XMM-SERVS fields will have extraordinary legacy value as MOONS massive spectroscopy fields, prime ALMA fields, and DES-LSST deep-drilling fields.
Publication The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field . Chen, C.-T. J., Brandt, W. N., et all. . MNRAS . 478-2132 . 2018 . 2018MNRAS.478.2132C ,
Constraining the Dark-matter Halo Mass of Isolated Low-surface-brightness Galaxies . Kovacs, Orsolya E., Bogdan, Akos, . ApJ . 879-12 . 2019 . 2019ApJ...879L..12K ,
The Evolution of the Quenching of Star Formation in Cluster Galaxies since zxa0~xa01 . Pintos-Castro, I., Yee, H. K. C., et all. . ApJ . 876-40 . 2019 . 2019ApJ...876...40P ,
A Tidal Disruption Event Candidate Discovered in the Active Galactic Nucleus SDSS J022700.77-042020.6 . Liu, Zhu, Li, Dongyue, et all. . ApJ . 894-93 . 2020 . 2020ApJ...894...93L ,
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies . Ojha, Vineet, Chand, Hum, et all. . ApJ . 896-95 . 2020 . 2020ApJ...896...95O ,
Instrument EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage 2016-08-13T01:16:31Z/2017-02-10T10:05:08Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2017-02-22T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017-02-22T23:00:00Z, 078045, 17.56_20190403_1200. https://doi.org/10.5270/esa-dz4rqtv