A dataset provided by the European Space Agency

Name 020567
Title COSMOLOGY WITH A SECOND SUNYAEV-ZEL.DOVICH EFFECT CLUSTER AT Z
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0205670101

DOI 10.5270/esa-ndofawr
Author Dr DIANA WORRALL
Description Sensitive XMM-Newton observations of the luminous Sunyaev-Zel.dovich effect cluster CL 0016+16 (z=0.55) have led to considerably improved measurements of distance, gas-mass fraction, and Hubble constant, for a cluster at a redshift where curvature of the angular-diameter-redshift relation is particularly evident. We propose a deep observation of the cluster.s twin, MS 0451.6-0305, to allow similar measurements for this second cluster. Averaging results for the two clusters will alleviate the potential problem of systematic errors in the distance estimate arising from projection effects. The results will also test the suggestion that the baryonic mass fraction in MS 0451.6-0305 is anomalously low, at only about a third the value seen in CL 0016+16.
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Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 . Ballo, L., Heras, F. J. H., et all. . A&A . 545-66 . 2012 . 2012A&A...545A..66B ,
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Structure and substructure analysis of DAFT-FADA galaxy clusters in the [0.4-0.9] redshift range . Guennou, L., Adami, C., et all. . A&A . 561-112 . 2014 . 2014A&A...561A.112G ,
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Revisiting the relationship between 6 mum and 2-10 keV continuum luminosities of AGN . Mateos, S., Carrera, F. J., et all. . MNRAS . 449-1422 . 2015 . 2015MNRAS.449.1422M ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
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The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
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A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). II. Physical Properties Derived from the SED Fitting with Optical, Infrared, and Radio Data . Toba, Yoshiki, Yamashita, Takuji, et all. . ApJS . 243-15 . 2019 . 2019ApJS..243...15T ,
Testing emergent gravity on galaxy cluster scales . Tamosiunas, Andrius, Bacon, David, et all. . JCAP . 5-53 . 2019 . 2019JCAP...05..053T ,
Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline . Hollowood, Devon L., Jeltema, Tesla, et all. . ApJS . 244-22 . 2019 . 2019ApJS..244...22H ,
The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state . Bartalucci, I., Arnaud, M., et all. . A&A . 628-86 . 2019 . 2019A&A...628A..86B ,
Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters . Palmese, A., Annis, J., et all. . MNRAS . 493-4591 . 2020 . 2020MNRAS.493.4591P ,
X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation . Molham, Mona, Clerc, Nicolas, et all. . MNRAS . 494-161 . 2020 . 2020MNRAS.494..161M ,
The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451u221203 . Tam, Sut-Ieng, Jauzac, Mathilde, et all. . MNRAS . 496-4032 . 2020 . 2020MNRAS.496.4032T ,
Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks . Kosiba, Matej, Lieu, Maggie, et all. . MNRAS . 496-4141 . 2020 . 2020MNRAS.496.4141K ,
SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release . Clerc, N., Kirkpatrick, C. C., et all. . MNRAS . 497-3976 . 2020 . 2020MNRAS.497.3976C ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-09-16T23:52:02Z/2004-09-17T12:13:48Z
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 2005-10-08T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-10-08T00:00:00Z, 020567, 17.56_20190403_1200. https://doi.org/10.5270/esa-ndofawr