A dataset provided by the European Space Agency

Name 069366
Title Unveiling the most massive clusters at z>0.5 with Planck and XMM-Newton.
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693660101
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DOI https://doi.org/10.5270/esa-ngf0ztw
Author Dr monique arnaud
Description We propose to gather spatially resolved spectroscopy of a sample of 33 massive (M_{500}>5e+14 solar masses) clusters detected blindly by Planck and confirmed to-day to be in the redshift range 0.5
Publication No observations found associated with the current proposal
Instrument EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage 2012-05-19T04:12:10Z/2013-01-13T18:44:14Z
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 2014-02-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-02-05T00:00:00Z, 069366, 17.56_20190403_1200. https://doi.org/10.5270/esa-ngf0ztw