Proposal ID | 011225 |
Title | High Redshift Galaxy Clusters and the Value of Omega |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112250101 |
DOI | https://doi.org/10.5270/esa-6cxr9z4 |
Principal Investigator, PI | Dr Martin Turner |
Abstract | The goal of our project is to quantify the number of massive, high-redshiftgalaxy clusters, with the aim of constraining the density parameter of theUniverse by employing the extreme sensitivity of the high-mass end of thecosmological mass function to Omega. For that purpose, we propose a two-foldapproach: 1) measure the temperature of a sample of known high-z (0.4 |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2001-06-06T04:49:47Z/2002-08-03T05:44:57Z |
Version | 17.56_20190403_1200 |
Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 | 2003-09-07T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "redshift galaxy clusters", "fold approach", "dovich signal", "optical loading proves", "soc enhance", "density parameter", "redshift galaxy cluster", "xray emission", "cosmological mass function", "relatively massive", "sharc xray survey", "lensing effects", "sunyaev zel" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Martin Turner, 2003, 'High Redshift Galaxy Clusters and the Value of Omega', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6cxr9z4 |