A dataset provided by the European Space Agency

Name: WARM AND HOT GASES IN AND AROUND CLUSTER GALAXIES
Published: 2015-01-09T23:00:00Z

Proposal ID	072188
Title	WARM AND HOT GASES IN AND AROUND CLUSTER GALAXIES
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721880101
DOI	https://doi.org/10.5270/esa-hqmdslb
Principal Investigator, PI	Prof Q. Daniel Wang
Abstract	We propose a pilot joint XMM-Newton/HST observing program to study both warm and hot gases in two optically-selected galaxy clusters at z=0.1-0.2. Eachcluster has a UV-bright background QSO projected within the expected strong accretion shock. We will measure the luminosity, temperature,and morphology of the hot gas component and observe UV absorption lines of the O VI doublet and other ion transitions of the clusters. These lines are sensitive to the thermal, kinetic, and chemical properties of warm gas, associated with the halos of individual galaxies and the intracluster medium.
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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda J. Guainazzi M. \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S 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 A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin \|Bhargava S. Giles P. A. et al. \| MNRAS \| 497-656 \| 2020 \| 2020MNRAS.497..656B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B 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 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	2013-12-17T08:25:05Z/2013-12-17T21:28:25Z
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	2015-01-09T23:00:00Z
Last Update	2025-01-27
Keywords	"individual galaxy", "warm gas", "ion transitions", "chemical properties", "uv absorption lines", "xmm newton", "hot gas component", "XMM-Newton", "hot gases", "vi doublet", "galaxy cluster", "cluster galaxy", "XMM", "accretion shock", "intracluster medium", "HST"
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', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hqmdslb