A dataset provided by the European Space Agency

Name: AGN-ICM interaction and peculiar radio emission in the cool core cluster RBS 797
Published: 2013-05-09T00:00:00Z

Proposal ID	067140
Title	AGN-ICM interaction and peculiar radio emission in the cool core cluster RBS 797
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671400101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671400201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671400301
DOI	https://doi.org/10.5270/esa-7jbev9t
Principal Investigator, PI	Dr Myriam Gitti
Abstract	We propose to observe the X-ray cavity cluster RBS797, which has a massivecentral starburst and a unique radio source that exhibits large changes inorientation with scale. With the requested observation we aim at: 1) determiningthe global properties of the cluster (temperature, metallicity, mass, gas massfraction) up to ~1.3 Mpc (~0.5 r_vir), and investigating the potential impact ofAGN feedback on scaling relations; 2) characterizing the AGN/ICM interaction byinvestigating the nature of the extended radio emission; 3) comparing thecooling rate or limits with the star formation rate.
Publications	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 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda J. Guainazzi M. \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S 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 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	2012-04-06T16:14:51Z/2012-04-18T20:41:24Z
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	2013-05-09T00:00:00Z
Keywords	"star formation rate", "potential impact", "icm interaction", "cluster temperature", "cooling rate", "agn icm interaction", "radio emission", "agn feedback", "scaling relations", "global properties", "gas mass fraction", "massive central starburst", "radio source"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Myriam Gitti, 2013, 'AGN-ICM interaction and peculiar radio emission in the cool core cluster RBS 797', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7jbev9t