A dataset provided by the European Space Agency

Name 080076
Title Scaling Properties and the Effects of Feedback for a Complete Sample of Groups
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800760101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800760201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800760301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800760501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800760601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800760701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800760801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800760901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800761001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800761301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800761501
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800761701

DOI https://doi.org/10.5270/esa-t0bl41r
Author European Space Agency
Description The largest fraction of matter content in the Universe is attributed to galaxy
groups, therefore they play a key role in astrophysics and cosmology. Upcoming
X-ray surveys like eROSITA, require precise calibration between X-ray
observables and mass, down to the low mass regime to set tight constraints on
the fundamental cosmological parameters. We propose to observe 14 galaxy groups
with a total exposure time of 137 ks to complete observations for a flux limited
sample consisting of 69 objects. The requested data will allow to precisely
correct for selection effects the scaling relations, with an improvement on the
corrected scaling relations by a factor of 2 with respect to what can be done
with the current data.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2017-06-10T07:17:04Z/2018-04-20T02:52:14Z
Version 17.56_20190403_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 2019-05-14T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2019, Scaling Properties And The Effects Of Feedback For A Complete Sample Of Groups, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-t0bl41r