A dataset provided by the European Space Agency

Name 080305
Title Deep X-ray Spectroscopy of the Most Distant, Massive Clusters Known
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803050101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803050201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803050301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803050401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803050501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803050601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803050701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803050801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803050901

DOI https://doi.org/10.5270/esa-qvo82wi
Author European Space Agency
Description We propose to observe the six most massive clusters at z>1.2, discovered via the
Sunyaev-Zel.dovich (SZ) effect by the South Pole Telescope (SPT). The proposed
700 ks program will provide deep X-ray spectroscopy for a sample that is already
rich in multi-wavelength data from a variety of telescopes, including Spitzer,
Hubble, and Chandra. These new data, coupled with spatially-resolved X-ray
imaging from Chandra, will provide the first constraints on the thermodynamic
profiles for a complete sample of galaxy clusters at z>1.2, allowing us to study
a variety of physical processes in clusters cores and outskirts, and test
predictions of self similarity and AGN feedback models, at a time shortly after
these systems formed.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2017-04-08T23:46:53Z/2017-07-10T05:54:35Z
Version PPS_NOT_AVAILABLE
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 2018-08-01T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2018, Deep X-Ray Spectroscopy Of The Most Distant Comma Massive Clusters Known, PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-qvo82wi