A dataset provided by the European Space Agency

Name: The Profiles of Dark Matter and Baryons of a Sample of Isolated Elliptical Galax
Published: 2015-02-05T23:00:00Z

Proposal ID	072236
Title	The Profiles of Dark Matter and Baryons of a Sample of Isolated Elliptical Galax
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722360201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722360301
DOI	https://doi.org/10.5270/esa-t5hxdhj
Principal Investigator, PI	Prof David Buote
Abstract	The mass profiles of elliptical galaxies are important probes of galaxyformation and cosmology. Only a few elliptical galaxies have detailed massmeasurements from X-rays because of the lack of suitable targets in terms oftotal mass (< ~10^{13} m_sun) and relaxed dynamical states appropriate forhydrostatic analysis. We have identified a sample of 10 (hot) gas-rich isolatedelliptical galaxies well-suited for X-ray studies of mass profiles on the galaxyscale. We request deep XMM observations to map the detailed profiles of stars,dark matter, and hot gas for the 5 systems in the sample lacking high-qualityXMM data. This sample will serve as a benchmark laboratory for hydrostaticstudies of the hot gas in isolated elliptical galaxies.
Publications	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 X-ray shapes of elliptical galaxies and implications for self-interacting dark matter \|McDaniel A. Jeltema T. \| JCAP \| 5-20 \| 2021 \| 2021JCAP...05..020M \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...05..020M Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earths Magnetosphere to the Solar Wind Proton Flux \|Zhang Yingjie Sun Tianran et al. \| ApJ \| 948-69 \| 2023 \| 2023ApJ...948...69Z \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z 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	2013-11-26T15:10:20Z/2014-01-17T01:32:37Z
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	2015-02-05T23:00:00Z
Last Update	2025-01-27
Keywords	"relaxed dynamical", "elliptical galaxy", "isolated elliptical galax", "suitable targets", "mass profiles", "galaxy formation", "hydrostatic analysis", "dark matter", "isolated elliptical galaxy", "sample lacking", "galaxy scale", "quality xmm data", "deep xmm", "XMM", "benchmark laboratory", "hot gas", "mass measurements", "total mass"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof David Buote, 2015, 'The Profiles of Dark Matter and Baryons of a Sample of Isolated Elliptical Galax', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-t5hxdhj