A dataset provided by the European Space Agency

Name 067449
Title Cosmological Constraints from X-ray Observations of SZ Discovered Clusters
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674490101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674490201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674490301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674490401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674490501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674490601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674490701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674490801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674490901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674491001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674491101
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674491201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674491301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674491401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674491501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674491601

DOI https://doi.org/10.5270/esa-vm1vapf
Author European Space Agency
Description We propose to observe 14 intermediate redshift massive clusters of galaxies
discovered via the Sunyaev-Zel.dovich (SZ) effect by the South Pole Telescope
(SPT). Currently the SPT survey has measured redshifts for 194 clusters, the
majority of which are newly discovered clusters at z > 0.5. We propose to
observe a sub-sample of SPT clusters at redshifts between 0.3 < z < 0.5 to
obtain well calibrated Yx-derived mass estimates. With these mass estimates and
the WMAP 7-year results, we expect that the SPT survey will allow a 7%
constraint on w, the dark energy equation of state, a factor of 2 improvement
over comparable constraints using cluster evolution and WMAP from Vikhlinin et
al.(2009).
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-05-03T09:39:42Z/2012-04-26T19:19:39Z
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 2013-05-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, Cosmological Constraints From X-Ray Observations Of Sz Discovered Clusters, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vm1vapf