A dataset provided by the European Space Agency

Name 086405
Title eeHIFLUGCS: Cosmology with virgul400 Galaxy Clusters
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864050101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864050201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864050401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864050501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864050601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864051201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864051301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864052301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864052401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864052501
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864052801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864053001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864053101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864053201
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864053601

DOI https://doi.org/10.57780/esa-jqn3k9h
Author Prof Thomas Reiprich
Description We propose to complete the last 10% of high-quality observations for the
eeHIFLUGCS galaxy cluster sample (36 of 376 clusters). The sample is based on
ROSAT with completely and homogeneously redetermined fluxes as well as updated
redshifts. For the already observed clusters we have also identified >10
double/triple clusters and clusters dominated by AGN emission, which then fall
below the flux limit of 5e- 12 erg/s/cm2. With the completed follow-up
observations we will decrease the uncertainties in OmegaM by a factor of 2.8
compared to those obtained with the HIFLUGCS sample. If these 10% do not get
observed, the flux-limited sample drops by almost a factor of 3 to a
disappointing 137 clusters. The observations will also have long lasting legacy value for a range of astrophysical studies
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2020-07-30T19:22:36Z/2021-04-26T11:20:28Z
Version 19.16_20210326_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 2022-06-08T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Thomas Reiprich, 2022, 086405, 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-jqn3k9h