A dataset provided by the European Space Agency

Proposal ID 069293
Title Characterizing Planck ESZ Clusters
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DOI https://doi.org/10.5270/esa-oc24dji
Principal Investigator, PI Dr Christine Jones
Abstract XMM-Newton observations of 44 Planck ESZ clusters will allow us to characterizethe 156 0.02
Publications
Instrument RGS1, EPN, RGS2, EMOS1, OM, EMOS2
Temporal Coverage 2012-07-09T07:48:24Z/2013-04-23T08:40:27Z
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 2014-05-09T00:00:00Z
Last Update 2025-01-27
Keywords "planck clusters", "radio halos", "planck esz clusters", "scaling relations", "xmm newton", "calibrate mass proxies", "planck esz cluster", "XMM-Newton", "structure formation", "cluster sample", "sz properties", "weak lensing analysis", "weak lensing", "cluster evolution", "XMM", "cluster dynamical", "total mass"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Christine Jones, 2014, 'Characterizing Planck ESZ Clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-oc24dji