Name | 067466 |
Title | THE X-RAY PROPERTIES OF HIGH REDSHIFT WEAK-LENSING SELECTED GALAXY CLUSTERS |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674660201 |
DOI | https://doi.org/10.5270/esa-kj2i2z4 |
Author | European Space Agency |
Description | We propose XMM observations (totaling 107 ks) of 6 galaxy clusters in the redshift range 0.3 < z < 0.6 selected in a Subaru weak lensing (WL) survey. This will complete a sample of 8 clusters that will be used to study systematically the X-ray properties of clusters detected independently of their baryonic content. We will investigate biases in cluster selection techniques for high-z clusters, compare the high-z scaling relations of the X-ray properties (e.g. Lx, kT, Mgas, Yx) of WL selected clusters to those of X-ray selected clusters, investigate the evolution of the properties of WL selected clusters from the local to high redshift universe and study their morphology/structure. |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2012-01-06T14:35:14Z/2012-01-07T00:01:23Z |
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 | 2013-02-04T00:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2013, The X-Ray Properties Of High Redshift Weak-Lensing Selected Galaxy Clusters, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kj2i2z4 |