A dataset provided by the European Space Agency

Name 065358
Title X-Ray Luminosity--Mass Relation and AGN Feedback in Galaxy Groups
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653580101

DOI 10.5270/esa-nu96n8s
Author Dr Thomas Reiprich
Description Most of the mass, most of the baryons, and most of the galaxies in the Universe are in galaxy groups. The processes connecting cooling gas in the hot inter- galactic medium and feedback from AGN are more easily observed in groups than in clusters because of their shallower potential wells. A precise characterization of the X-ray luminosity-mass relation over a large mass range is today.s single most important task to ensure that the full cosmological power from the 100000 groups and clusters to be detected with eROSITA can be exploited. We will use a complete sample of almost 90 galaxy groups and clusters to constrain cooling and feedback mechanisms as well as the Lx-M relation. Observations for all clusters are available. With this short proposal we aim to complete observations for the group sample.
Publication Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Scaling properties of a complete X-ray selected galaxy group sample . Lovisari, L., Reiprich, T. H., . A&A . 573-118 . 2015 . 2015A&A...573A.118L ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
The non-uniformity of galaxy cluster metallicity profiles . Lovisari, L., Reiprich, T. H., . MNRAS . 483-540 . 2019 . 2019MNRAS.483..540L ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-10-02T00:54:35Z/2010-10-02T11:22:24Z
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 2011-10-27T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-10-27T00:00:00Z, 065358, 17.56_20190403_1200. https://doi.org/10.5270/esa-nu96n8s