A dataset provided by the European Space Agency

Name 067448
Title XMM study of the interplay between the intra-group medium and galaxies
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674480301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674480401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674480701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674480901

DOI 10.5270/esa-p1ukq1t
Author Dr Francesco Miniati
Description Current models of galaxy evolution rely critically on AGN and SN feedback processes. However, these ideas have not been fully tested, particularly in the intra-group medium (IGM), the environment most commonly experienced by galaxies. For this purpose we propose to use XMM-Newton to study the thermodynamic properties of the IGM (via its diffuse X-ray emission), which retains a fossil record of the energy released by past star formation and AGN activity, for an unbiased sample of 23 groups with fully determined galaxy population and AGN properties. The 23 target groups are selected from our Zurich ENvironmental Survey, for which we have optical spectroscopic, photometric and morphological information as well as HI mass content.
Publication The X-Ray Zurich Environmental Study (X-ZENS). I. Chandra and XMM-Newton Observations of Active Galactic Nuclei in Galaxies in nearby Groups . Silverman, J. D., Miniati, F., et all. . ApJ . 780-67 . 2014 . 2014ApJ...780...67S ,
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 ,
The X-Ray Zurich Environmental Study (X-ZENS). II. X-Ray Observations of the Diffuse Intragroup Medium in Galaxy Groups . Miniati, Francesco, Finoguenov, Alexis, et all. . ApJ . 819-26 . 2016 . 2016ApJ...819...26M ,
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 ,
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 ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-11-01T19:31:00Z/2012-02-04T05:15:54Z
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 2013-02-18T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-02-18T00:00:00Z, 067448, 17.56_20190403_1200. https://doi.org/10.5270/esa-p1ukq1t