A dataset provided by the European Space Agency

Name: Warm And Hot Gases In And Around Cluster Galaxies At Z=0.1-0.2
Published: 2015-01-24T23:00:00Z

Proposal ID	072817
Title	Warm And Hot Gases In And Around Cluster Galaxies At Z=0.1-0.2
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728170101
DOI	https://doi.org/10.5270/esa-m6uw63l
Principal Investigator, PI	Prof Q. Daniel Wang
Abstract	We propose a joint HST/XMM-Newton observing program to study both warm and hotgases in three optically-selected galaxy clusters at z=0.117-0.2108. Eachcluster has a UV-bright background QSO projected within the expected strongaccretion shock (< 2r_200). We will observe UV absorption lines of the O VIdoublet, HI Ly-alpha and Ly-beta, and other ion transitions in the rest frame ofthe clusters, using the HST/COS G130M grating. These absorption lines aresensitive to the thermal, kinetic, and chemical properties of warm (T < 10^6K) gas, associated with the halos of individual galaxies and the intraclustermedium. Chandra/ACIS observations will be used to measure the luminosity,temperature, and morphology of the hot gas component of the clusters.
Publications	XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N Baryon content and dynamic state of galaxy clusters: XMM-Newton observations of A1095 and A1926 \|Ge Chong Wang Q. Daniel et al. \| MNRAS \| 459-366 \| 2016 \| 2016MNRAS.459..366G \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.459..366G 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 Warm-hot gas in X-ray bright galaxy clusters and the H I-deficient circumgalactic medium in dense environments \|Burchett Joseph N. Tripp Todd M. et al. \| MNRAS \| 475-2067 \| 2018 \| 2018MNRAS.475.2067B \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.2067B The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou Min-Hua Gu Min-Feng \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z 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 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	2014-01-05T21:45:41Z/2014-01-06T10:57:21Z
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	2015-01-24T23:00:00Z
Last Update	2025-01-27
Keywords	"xmm newton", "accretion shock", "ly beta", "absorption lines", "hot gases", "vi doublet", "rest frame", "cluster galaxy", "individual galaxy", "intracluster medium", "uv absorption lines", "XMM-Newton", "HST", "ion transitions", "chemical properties", "hi ly alpha", "cos g130m grating", "hot gas component", "galaxy cluster", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Q. Daniel Wang, 2015, 'Warm And Hot Gases In And Around Cluster Galaxies At Z=0.1-0.2', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-m6uw63l