|Title||Going Beyond COSMOS with the XMM-SERVS Survey of W-CDF-S,XMM-LSS, and ELAIS-S1|
|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, excep-tional 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 ,
HSC-XD 52: An X-Ray Detected AGN in a Low-mass Galaxy at z u0303 0.56 . Halevi, Goni, Goulding, Andy, et all. . ApJ . 885-3 . 2019 . 2019ApJ...885L...3H ,
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 ,
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 all. . A&A . 640-124 . 2020 . 2020A&A...640A.124P ,
|Instrument||EPN, OM, RGS1, RGS2, EMOS1, EMOS2|
|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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2016-08-19T22:00:00Z, 078510, 17.56_20190403_1200. https://doi.org/10.5270/esa-ip6srta|