A dataset provided by the European Space Agency

Name: XMM study of the interplay between the intra-group medium and galaxies
Published: 2013-02-18T00:00:00Z

Proposal ID	067448
Title	XMM study of the interplay between the intra-group medium and galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674480301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674480401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674480701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674480901
DOI	https://doi.org/10.5270/esa-p1ukq1t
Principal Investigator, PI	Dr Francesco Miniati
Abstract	Current models of galaxy evolution rely critically on AGN and SN feedbackprocesses. However, these ideas have not been fully tested, particularly in theintra-group medium (IGM), the environment most commonly experienced by galaxies.For this purpose we propose to use XMM-Newton to study the thermodynamicproperties of the IGM (via its diffuse X-ray emission), which retains a fossilrecord of the energy released by past star formation and AGN activity, for anunbiased sample of 23 groups with fully determined galaxy population and AGNproperties. The 23 target groups are selected from our Zurich ENvironmentalSurvey, for which we have optical spectroscopic, photometric and morphologicalinformation as well as HI mass content.
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 XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso E. Risaliti G. \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L 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 X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field \|Ota Naomi Mitsuishi Ikuyuki et al. \| PASJ \| 72-1 \| 2020 \| 2020PASJ...72....1O \| http://ui.adsabs.harvard.edu/#abs/2020PASJ...72....1O A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman Murray Ward Charlotte et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B 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 ESASky SSOSS: Solar System Object Search Service and the case of Psyche \|Racero E. Giordano F. et al. \| A&A \| 659-38 \| 2022 \| 2022A&A...659A..38R \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..38R X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf J. Nandra K. et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W 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
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 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	2013-02-18T00:00:00Z
Last Update	2025-01-27
Keywords	"hi mass content", "galaxy evolution rely", "xmm newton", "diffuse xray emission", "zurich environmental survey", "past star formation", "thermodynamic properties", "commonly experienced", "medium igm", "agn andsupernovafeedback processes", "unbiased sample", "igm via", "galaxy population", "XMM-Newton", "energy released", "agn properties", "fossil record", "agn activity", "XMM", "optical spectroscopic", "morphological information"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Francesco Miniati, 2013, 'XMM study of the interplay between the intra-group medium and galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-p1ukq1t