A dataset provided by the European Space Agency

Name: Testing the effect of quasar-mode feedback on the intracluster medium
Published: 2017-09-09T22:00:00Z

Proposal ID	078104
Title	Testing the effect of quasar-mode feedback on the intracluster medium
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0781040101
DOI	https://doi.org/10.5270/esa-jdu55kd
Principal Investigator, PI	Dr Matt Hilton
Abstract	We propose to obtain XMM-Newton EPIC observations of the massive galaxy clusterACT-CL J0320.4+0032 at z=0.384. We have recently identified that the Brightest Cluster Galaxy hosts a Type II quasar - one of only a handful of such systems to be discovered. This presents a rare opportunity to study the effect of quasar-mode feedback on the intracluster medium (ICM). We will address this by using the XMM observations to measure the temperature, entropy, and metallicityprofiles of the cluster, and compare these to well-studied representative cluster samples and the results of numerical simulations. These observations will complement our 50 ksec Cycle 17 Chandra observation, the goal of which is to search for cavities in the X-ray emission.
Publications	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 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	2016-08-27T22:03:30Z/2016-08-28T23:36:50Z
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	2017-09-09T22:00:00Z
Keywords	"xmm newton epic", "intracluster medium", "XMM", "numerical simulations", "intracluster medium icm", "J0320.4", "quasar mode feedback", "type ii quasar", "XMM-Newton", "xray emission", "EPIC", "cluster samples", "metallicity profiles"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Matt Hilton, 2017, 'Testing the effect of quasar-mode feedback on the intracluster medium', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jdu55kd