A dataset provided by the European Space Agency

Name 090183
Title Measuring Projection Effects in Optical Cluster Catalogues
URL

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
Author European Space Agency
Description The impact of projection effects on optical, photometric galaxy cluster
selection has recently been clarified at z virgul 0.1 using extensive spectroscopy of
putative member galaxies. The projected fraction of photometrically associated
galaxies has been constrained as a function of richness, along with the
relations between photometric and spectroscopically-corrected richness and
velocity dispersion. We propose XMM-Newton observations of a complete sub-sample
of these clusters at high richness to obtain low-scatter X-ray mass proxies.
These measurements will provide independent, complementary information on
projection effects and, crucially, will allow the scatter of
spectroscopically-corrected richness with mass to be quantified.
Publication No observations found associated with the 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 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 2023-11-30T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, Measuring Projection Effects In Optical Cluster Catalogues, 20.09_20221024_1724, European Space Agency, https://doi.org/10.57780/esa-70k0l4c