A dataset provided by the European Space Agency

Name 020302
Title A FIRST COMPARISON OF X-RAY AND OPTICAL INTRACLUSTER LIGHT
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203020101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203020201

DOI 10.5270/esa-3v5li5f
Author Prof ANN ZABLUDOFF
Description We propose to make the first comparison of intracluster light in the X-ray and optical bands for four clusters of galaxies. We have developed a new approach that constrains the stellar light profile out to at least 0.5 Mpc. The sensitivity, wide field, and spectral capabilities of XMM-Newton will allow us to derive the total mass and gas mass profiles out to a similar radius and to answer 1] whether the observed variations in the stellar light profiles of similar clusters reflect differences in the mass profiles or in the evolution of the stellar intracluster medium? and 2] what are the relative contributions of gas and stars to the overall baryon fraction?
Publication Metal abundances in the cool cores of galaxy clusters . de Grandi, S., Molendi, S., . A&A . 508-565 . 2009 . 2009A&A...508..565D ,
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The XMM-Newton serendipitous ultraviolet source survey catalogue . Page, M. J., Brindle, C., et all. . MNRAS . 426-903 . 2012 . 2012MNRAS.426..903P ,
The cool-core bias in X-ray galaxy cluster samples. I. Method and application to HIFLUGCS . Eckert, D., Molendi, S., . A&A . 526-79 . 2011 . 2011A&A...526A..79E ,
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Galaxy Cluster Baryon Fractions Revisited . Gonzalez, Anthony H., Sivanandam, Suresh, et all. . ApJ . 778-14 . 2013 . 2013ApJ...778...14G ,
A Good Mass Proxy for Galaxy Clusters with XMM-Newton . Zhao, Hai-Hui, Jia, Shu-Mei, et all. . ApJ . 778-124 . 2013 . 2013ApJ...778..124Z ,
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Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
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SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release . Clerc, N., Kirkpatrick, C. C., et all. . MNRAS . 497-3976 . 2020 . 2020MNRAS.497.3976C ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-07-01T14:28:14Z/2004-10-06T14:17:41Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2005-11-11T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-11-11T00:00:00Z, 020302, 17.56_20190403_1200. https://doi.org/10.5270/esa-3v5li5f