A dataset provided by the European Space Agency

Name 067718
Title A new Cosmological Study Approach with a Volume Limited X-ray Cluster Sample
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677180101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677180201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677180301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677180401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677180501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677180601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677180701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677180801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677180901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677181001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677181101
...
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677181201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677181301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677181401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677181501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677181601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677181701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677181801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677181901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677182001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677182101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677182201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677182301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677182401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677182501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677182701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677182801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677183001

DOI 10.5270/esa-fpyn31i
Author Prof Hans Boehringer
Description The application of galaxy clusters in constraining cosmological models is currently mostly limited by our uncertain knowledge of scaling relations of easy observables and cluster mass. Most of the scaling relation studies are based on X-ray flux limited samples. Here we propose to take a new approach to study galaxy cluster properties in a volume-limited sample. From the comparison of flux and volume-limited samples we would be able to determine the intrinsic scatter of scaling relations in an unambiguous way, providing an important advance in cluster cosmology studies. Apart from the cosmological application, the volume-limited survey of nearby clusters will also provide a great benchmark sample for all aspects of characterizing the properties of the cluster population.
Publication Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Witnessing a merging bullet being stripped in the galaxy cluster RXCJ2359.3-6042 . Chon, Gayoung, Bohringer, Hans, . A&A . 574-132 . 2015 . 2015A&A...574A.132C ,
Suzaku and XMM-Newton observations of the newly discovered early-stage cluster merger of 1E2216.0-0401 and 1E2215.7-0404 . Akamatsu, H., Gu, L., et all. . A&A . 593-7 . 2016 . 2016A&A...593L...7A ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
X-Ray Morphological Analysis of the Planck ESZ Clusters . Lovisari, Lorenzo, Forman, William R., et all. . ApJ . 846-51 . 2017 . 2017ApJ...846...51L ,
The non-uniformity of galaxy cluster metallicity profiles . Lovisari, L., Reiprich, T. H., . MNRAS . 483-540 . 2019 . 2019MNRAS.483..540L ,
Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers . Golovich, N., Dawson, W. A., et all. . ApJ . 882-69 . 2019 . 2019ApJ...882...69G ,
X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton . Lovisari, Lorenzo, Schellenberger, Gerrit, et all. . ApJ . 892-102 . 2020 . 2020ApJ...892..102L ,
Probing cosmic isotro...
Instrument EPN, OM, RGS1, RGS2, EMOS1, EMOS2
Temporal Coverage 2011-06-13T04:33:27Z/2012-06-11T16:41:27Z
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 2013-06-26T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-06-26T00:00:00Z, 067718, 17.56_20190403_1200. https://doi.org/10.5270/esa-fpyn31i