A dataset provided by the European Space Agency

Proposal ID 090183
Title Measuring Projection Effects in Optical Cluster Catalogues
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0901830301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0901830501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0901830601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0901830701

DOI https://doi.org/10.57780/esa-70k0l4c
Principal Investigator, PI Mr Justin Myles
Abstract The impact of projection effects on optical, photometric galaxy clusterselection has recently been clarified at z virgul 0.1 using extensive spectroscopy ofputative member galaxies. The projected fraction of photometrically associatedgalaxies has been constrained as a function of richness, along with therelations between photometric and spectroscopically-corrected richness andvelocity dispersion. We propose XMM-Newton observations of a complete sub-sampleof these clusters at high richness to obtain low-scatter X-ray mass proxies.These measurements will provide independent, complementary information onprojection effects and, crucially, will allow the scatter ofspectroscopically-corrected richness with mass to be quantified.
Publications No publications found for current proposal!
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-06-05T03:38:43Z/2022-11-07T21:15:40Z
Version 20.09_20221024_1724
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 2023-11-30T00:00:00Z
Keywords "XMM", "projected fraction", "complete sub sample", "velocity dispersion", "optical cluster catalogues", "XMM-Newton", "extensive spectroscopy", "projection effects", "complementary information", "spectroscopically corrected richness", "xmm newton"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Mr Justin Myles, 2023, 'Measuring Projection Effects in Optical Cluster Catalogues', 20.09_20221024_1724, European Space Agency, https://doi.org/10.57780/esa-70k0l4c