A dataset provided by the European Space Agency

Name: XMM tests galaxy evolutions models
Published: 2014-05-09T00:00:00Z

Proposal ID	069374
Title	XMM tests galaxy evolutions models
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693741001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693741101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693741601
DOI	https://doi.org/10.5270/esa-77pzm91
Principal Investigator, PI	Dr Francesco Miniati
Abstract	Current models of galaxy evolution rely critically on feedback supernova and AGNfeedback processes. The energy released by past star formation and AGN activityimprints a fossil record on the thermodynamic properties of theintra-group-medium (IGM). This can be decoded by studying the X-ray emission.for an unbiased sample of groups with known galaxy and AGN properties. Thereforewe propose an X-ray survey with XMM-Newton for 255 ksec to observe 17 galaxygroups with $Msim10^{13} M_odot$ selected from our Zurich ENvironmental Surveythat host $>8$ members.
Publications	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 al. \| ApJ \| 780-67 \| 2014 \| 2014ApJ...780...67S \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/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 al. \| ApJ \| 819-26 \| 2016 \| 2016ApJ...819...26M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819...26M The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-06-29T09:03:52Z/2013-04-26T19:28:11Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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	2014-05-09T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "feedback supernova", "XMM-Newton", "agn properties", "zurich environmental survey", "agn feedback processes", "past star formation", "energy released", "fossil record", "galaxy evolution rely", "xmm newton", "unbiased sample", "xray survey", "medium igm", "agn activity imprints", "xray emission", "thermodynamic properties", "msim10 ^{"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Francesco Miniati, 2014, 'XMM tests galaxy evolutions models', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-77pzm91