A dataset provided by the European Space Agency

Name 030382
Title Determining Temperatures of DLS Shear-Selected Galaxy Clusters
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303820101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303820201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303820301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0303820601

DOI https://doi.org/10.5270/esa-bzi7uvi
Author European Space Agency
Description The Deep Lens Survey (DLS) is a deep, multicolor (BVRz.), wide area, optical
imaging survey that is producing a new sample of massive galaxy clusters,
selected purely based on their weak lensing shear. The main goal of these
XMM-Newton observations is to measure the intracluster gas temperatures of X-ray
clusters in the DLS sample that we have identified using Chandra. The new
observations will allow us to construct an X-ray luminosity-temperature
correlation from the mass-selected DLS clusters for comparison with the known
correlation from purely X-ray selected samples. This is a critical test of the
fair sample hypothesis, which underlies several cosmological tests using galaxy
clusters.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-08-27T08:05:03Z/2006-04-16T07:46:59Z
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 2007-05-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007, Determining Temperatures Of Dls Shear-Selected Galaxy Clusters, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-bzi7uvi