A dataset provided by the European Space Agency

Name: The Dark Matter and Baryon Content of a Sample of Isolated Elliptical Galaxies
Published: 2014-04-06T00:00:00Z

Proposal ID	069319
Title	The Dark Matter and Baryon Content of a Sample of Isolated Elliptical Galaxies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693190101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693190401
DOI	https://doi.org/10.5270/esa-647lut4
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 (< virgul10^{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	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 Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra \|Anderson, Michael E., Churazov, Eugene, \| MNRAS \| 452-3905 \| 2015 \| 2015MNRAS.452.3905A \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.452.3905A 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 Earth.s 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	2012-06-08T17:26:53Z/2013-03-27T21:29:30Z
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	2014-04-06T00:00:00Z
Keywords	"hot gas", "relaxed dynamical", "isolated elliptical galaxy", "XMM", "mass measurements", "mass profiles", "deep xmm", "quality xmm data", "elliptical galaxy", "galaxy formation", "galaxy scale", "total mass", "dark matter", "hydrostatic analysis", "sample lacking", "benchmark laboratory", "suitable targets", "baryon content"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof David Buote, 2014, 'The Dark Matter and Baryon Content of a Sample of Isolated Elliptical Galaxies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-647lut4