A dataset provided by the European Space Agency

Name: AGN Feedback and Star Formation in the Cooling Flow Cluster RBS797
Published: 2009-06-06T00:00:00Z

Proposal ID	050294
Title	AGN Feedback and Star Formation in the Cooling Flow Cluster RBS797
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502940301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502940401
DOI	https://doi.org/10.5270/esa-68m5b1c
Principal Investigator, PI	Dr Myriam Gitti
Abstract	We propose to observe the X-ray cavity cluster RBS797, in which radio emissionis seen on three different scales and orientations and a massive starburst isfound at its center. With the requested observation we aim to: 1) determine theglobal properties of the cluster (temperature, mass, luminosity) and assess itsconformity to scaling relations in order to investigate the potential impact ofAGN feedback; 2) compare cooling rate or limits with the star formation rate; 3)investigate the nature of the large-scale radio emission by using the X-rayproperties as input to test the electron reacceleration model for the origin ofradio mini-halos; 4) study the ICM enrichment process by means of a metallicitymap.
Publications	A Powerful AGN Outburst in RBS 797 \|Cavagnolo K. W. McNamara B. R. et al. \| ApJ \| 732-71 \| 2011 \| 2011ApJ...732...71C \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...732...71C Constraints on turbulent velocity broadening for a sample of clusters groups and elliptical galaxies using XMM-Newton \|Sanders J. S. Fabian A. C. \| MNRAS \| 410-1797 \| 2011 \| 2011MNRAS.410.1797S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.410.1797S Revealing O VII from stacked X-ray grating spectra of clusters groups and elliptical galaxies \|Sanders J. S. Fabian A. C. \| MNRAS \| 412-35 \| 2011 \| 2011MNRAS.412L..35S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.412L..35S Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc N. Sadibekova T. et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H Velocity width measurements of the coolest X-ray emitting material in the cores of clusters groups and elliptical galaxies \|Sanders J. S. Fabian A. C. \| MNRAS \| 429-2727 \| 2013 \| 2013MNRAS.429.2727S \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.429.2727S An XMM-Newton Survey of the Soft X-Ray Background. III. The Galactic Halo X-Ray Emission \|Henley David B. Shelton Robin L. \| ApJ \| 773-92 \| 2013 \| 2013ApJ...773...92H \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...773...92H Probing of the Interactions between the Hot Plasmas and Galaxies in Clusters from z = 0.1 to 0.9 \|Gu Liyi Gandhi Poshak et al. \| ApJ \| 767-157 \| 2013 \| 2013ApJ...767..157G \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...767..157G 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 Origin of the Hot Gas in the Galactic Halo: Testing Galactic Fountain Models X-Ray Emission \|Henley David B. Shelton Robin L. et al. \| ApJ \| 800-102 \| 2015 \| 2015ApJ...800..102H \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...800..102H The Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc N. Merloni A. et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham Mona Clerc Nicolas et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba Matej Lieu Maggie et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc N. Kirkpatrick C. C. et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C Constraining the Milky Way Mass with Its Hot Gaseous Halo \|Guo Fulai Zhang Ruiyu \| ApJ \| 904-14 \| 2020 \| 2020ApJ...904L..14G \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904L..14G An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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	2008-04-15T13:13:24Z/2008-04-16T01:05:29Z
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	2009-06-06T00:00:00Z
Last Update	2025-01-27
Keywords	"potential impact", "metallicity map", "star formation", "scaling relations", "massive starburst", "radio mini halos", "global properties", "icm enrichment process", "scale radio emission", "star formation rate", "radio emission", "xray properties", "cluster temperature", "electron reacceleration model", "compare cooling rate", "agn feedback"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Myriam Gitti, 2009, 'AGN Feedback and Star Formation in the Cooling Flow Cluster RBS797', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-68m5b1c