A dataset provided by the European Space Agency

Name 072531
Title The XMM-ATLAS survey: AGN - star-formation co-evolution
URL

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DOI 10.5270/esa-c20emuv
Author Dr Ioannis Georgantopoulos
Description We propose to observe the 16 sq. deg. of the Herschel-ATLAS Science Demonstration Phase (SDP) in mosaic mode (total requested exposure 700 ks). The H-ATLAS (PACS+SPIRE) survey covers regions with excellent quality multi-wavelength data, including the GAMA AAT spectroscopic survey and near- and mid-IR data from the UKIDSS and WISE surveys. The proposed observations will provide the largest contiguous area far-IR-sub-mm survey with X-ray follow-up. This area will contain about 6000 250um and 2000 X-ray sources. The major scientific goals are to place strong constrains on the link between AGN and star-formation activity in the low-redshift (z<0.5) Universe, and to investigate the effect of very luminous AGN on their hosts.
Publication The XMM-Newton survey in the H-ATLAS field . Ranalli, P., Georgantopoulos, I., et all. . A&A . 577-121 . 2015 . 2015A&A...577A.121R ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Estimating photometric redshifts for X-ray sources in the X-ATLAS field using machine-learning techniques . Mountrichas, G., Corral, A., et all. . A&A . 608-39 . 2017 . 2017A&A...608A..39M ,
X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field . Ota, Naomi, Mitsuishi, Ikuyuki, et all. . PASJ . 72-1 . 2020 . 2020PASJ...72....1O ,
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 2013-05-21T02:29:42Z/2013-05-22T11:41:58Z
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 2014-06-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-06-01T00:00:00Z, 072531, 17.56_20190403_1200. https://doi.org/10.5270/esa-c20emuv