A dataset provided by the European Space Agency

Name 088107
Title eeHIFLUGCS\: Cosmology with virgul400 Galaxy Clusters
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881070301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881070701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881070901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881071101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881071201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881071301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881071401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881071701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881071801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881072701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881072801
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881073301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881073401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0881073501

DOI https://doi.org/10.57780/esa-ktq9tpv
Author European Space Agency
Description We propose to complete the last 10% of high-quality observations for the
eeHIFLUGCS galaxy cluster sample (31 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 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 2021-06-07T03:27:08Z/2022-04-10T11:30:18Z
Version 19.17_20220121_1250
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 2023-04-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, Eehiflugcs\: Cosmology With Virgul400 Galaxy Clusters, 19.17_20220121_1250, European Space Agency, https://doi.org/10.57780/esa-ktq9tpv