A dataset provided by the European Space Agency

Name: Studying X-ray cooling in a luminous cluster with feedback
Published: 2015-10-31T23:00:00Z

Proposal ID	074434
Title	Studying X-ray cooling in a luminous cluster with feedback
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744340101
DOI	https://doi.org/10.5270/esa-v2msqzb
Principal Investigator, PI	Dr Jeremy Sanders
Abstract	We propose a 130ks observation of the X-ray brightest cluster above z=0.1,PKS0745-191. In the absence of heating there should be cooling at 1000 Msun/yr.XMM shows the presence of central cool gas and Chandra the location of feedback.We will examine the central temperature distribution with RGS to study thefeedback-cooling connection. In addition, most of r_200 can be studied in asingle pointing to examine clumping. We will examine the surface brightnessfluctuation spectrum as a function of radius to connect to cluster-wide andAGN-related turbulence.
Publications	Probing the evolution of the substructure frequency in galaxy clusters up to z virgul 1 \|Weissmann, A., Bohringer, H., \| A&A \| 555-147 \| 2013 \| 2013A&A...555A.147W \| http://ui.adsabs.harvard.edu/#abs/2013A&A...555A.147W 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 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	2014-10-07T16:42:27Z/2014-10-09T07:34:07Z
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	2015-10-31T23:00:00Z
Keywords	"agn related turbulence", "XMM", "p0745 191", "xray brightest cluster", "central cool gas", "xray cooling", "examine clumping", "feedback cooling connection", "cluster wide", "luminous cluster", "central temperature distribution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jeremy Sanders, 2015, 'Studying X-ray cooling in a luminous cluster with feedback', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-v2msqzb