A dataset provided by the European Space Agency

Name 072316
Title Characterizing Planck ESZ Clusters
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723160101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723160201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723160301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723160401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723160501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723160601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723160701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723160901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723161001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723161201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723161401
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723161601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723161701

DOI https://doi.org/10.5270/esa-srw9hy8
Author Dr Christine Jones
Description ESA.s Planck Mission has provided a large, statistically representative sample
of 189 clusters within z<0.55, detected over the full sky (|b| > 15deg) through
their SZ effect.The proposed XMM-Newton observations of 17 clusters will allow
us to complete the X-ray characterization of all ESZ clusters. We will determine
the dynamical state of each cluster, measure cluster masses and mass proxies,
and explore the origin of radio halos and relics. We will derive scaling
relations between X-ray and SZ properties, including cluster masses, which will
be used in future large SZ and X-ray surveys (e.g. eROSITA), where detailed
X-ray studies for each cluster will not be possible. This sample will become the
fundamental low redshift baseline for studies of cluster evolution.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-05-08T12:17:03Z/2014-04-26T18:53:40Z
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 2015-05-21T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Christine Jones, 2015, 072316, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-srw9hy8