A dataset provided by the European Space Agency

Name: DETERMINING THE TEMPERATURE OF HOT GAS IN X-RAY FAINT EARLY-TYPE GALAXIES
Published: 2006-01-27T00:00:00Z

Proposal ID	020509
Title	DETERMINING THE TEMPERATURE OF HOT GAS IN X-RAY FAINT EARLY-TYPE GALAXIES
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205090101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205090201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205090401
DOI	https://doi.org/10.5270/esa-1drvvj1
Principal Investigator, PI	Dr JIMMY IRWIN
Abstract	The temperature of the hot X-ray gas contained within early-type galaxies is animportant diagnostic of the hydrodynamical processes that affect the gas.Previous studies of X-ray bright ellipticals indicate that they are all hotterthan the kinetic motion of the stars, and it has been suggested that the gas isin the potential well of a massive dark matter halo that is dynamically hotterthan the stars. X-ray faint galaxies have lost most of their gas, possiblybecause of a shallower dark matter potential well. If this is true, then the gasthat does remain in these galaxies should have a temperature that more closelyreflects the stellar kinetic temperature. We propose to observe three X-rayfaint galaxies to determine their temperature and test this prediction.
Publications	The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson M. G. Schroder A. C. et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy \|Levan A. J. Tanvir N. R. et al. \| Sci \| 333-199 \| 2011 \| 2011Sci...333..199L \| http://ui.adsabs.harvard.edu/#abs/2011Sci...333..199L Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos S. Saxton R. D. et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. 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Clusters associated with spectroscopically targeted luminous red galaxies in SDSS-DR10 \|Takey A. Schwope A. \| A&A \| 564-54 \| 2014 \| 2014A&A...564A..54T \| http://ui.adsabs.harvard.edu/#abs/2014A&A...564A..54T The diversity of quasars unified by accretion and orientation \|Shen Yue Ho Luis C. \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S Confirming the thermal Comptonization model for black hole X-ray emission in the low-hard state \|Castro M. DAmico F. et al. \| A&A \| 569-82 \| 2014 \| 2014A&A...569A..82C \| http://ui.adsabs.harvard.edu/#abs/2014A&A...569A..82C Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. 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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 Investigations of AGN populations through X-ray and optical surveys \|Pons Estelle \| PhDT \| 0-235 \| 2016 \| 2016PhDT.......235P \| http://ui.adsabs.harvard.edu/#abs/2016PhDT.......235P Probing the inner Galactic halo with blue horizontal-branch stars. 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Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2004-01-06T00:23:24Z/2004-12-23T19:27:21Z
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	2006-01-27T00:00:00Z
Last Update	2025-08-04
Keywords	"closely reflects", "dynamically hotter", "xray bright ellipticals", "hydrodynamical processes", "xray faint galaxy", "stellar kinetic temperature", "hot gas", "type galaxy", "xray faint", "hot xray gas", "kinetic motion"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr JIMMY IRWIN, 2006, 'DETERMINING THE TEMPERATURE OF HOT GAS IN X-RAY FAINT EARLY-TYPE GALAXIES', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-1drvvj1