A dataset provided by the European Space Agency

Name 086408
Title Enhancing DES cosmology with a complete sample of RedMaPPer selected clusters
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864080401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864080701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864080901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864081201

DOI https://doi.org/10.5270/esa-[xxxxxxx]
Author Dr Paul Giles
Description The Dark Energy Survey (DES) is currently the pre-eminent optical-near-IR survey for cosmology. DES uses four probes to study the physical nature of dark energy, including clusters of galaxies. To unlock the full potential of DES clusters, we require precise information of the galaxy-richness to halo-mass scaling relation, i.e. its slope, normalisation, and scatter. Of these, the least well known is the scatter. Therefore, one of the highest priorities for DES is to improve measurements of the scatter (and its evolution). For this, X-ray observations of a statistically complete sample are essential (archival, including serendipitous, observations are insufficient). We propose XMM observations of 14 DES clusters, to complete a sample of 40 of the richest clusters in DES.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2020-08-07T19:17:25Z/2021-02-14T17:14:43Z
Version 18.02_20200221_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 2022-03-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2022-03-04T00:00:00Z, 086408, 18.02_20200221_1200. https://doi.org/10.5270/esa-[xxxxxxx]