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The XXL Survey. V. ...
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Mantz, A. B.University of Chicago
(author)
The XXL Survey. V. Detection of the Sunyaev-Zel'Dovich Effect of the Redshift 1.9 Galaxy Cluster XLSSU J021744.1-034536 With Carma
- Article/chapterEnglish2014
Publisher, publication year, extent ...
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2014-10-07
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American Astronomical Society,2014
Numbers
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LIBRIS-ID:oai:research.chalmers.se:8ee0f81b-c3d3-475c-848c-fd936a5788af
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https://doi.org/10.1088/0004-637x/794/2/157DOI
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https://research.chalmers.se/publication/205934URI
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Language:English
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Summary in:English
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Subject category:art swepub-publicationtype
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Subject category:ref swepub-contenttype
Notes
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We report the detection of the Sunyaev-Zel'dovich (SZ) effect of galaxy cluster XLSSU J021744.1-034536, using 30 GHz Combined Array for Research in Millimeter-wave Astronomy (CARMA) data. This cluster was discovered via its extended X-ray emission in the XMM-Newton Large Scale Structure survey, the precursor to the XXL survey. It has a photometrically determined redshift z = 1.91(-0.21)(+0.19), making it among the most distant clusters known, and nominally the most distant for which the SZ effect has been measured. The spherically integrated Comptonization is Y-500 = (3.0 +/- 0.4) x 10(-12), a measurement that is relatively insensitive to assumptions regarding the size and redshift of the cluster, as well as the background cosmology. Using a variety of locally calibrated cluster scaling relations extrapolated to z similar to 2, we estimate a mass M-500 similar to (1-2) x 10(14) M-circle dot from the X-ray flux and SZ signal. The measured properties of this cluster are in good agreement with the extrapolation of an X-ray luminosity-SZ effect scaling relation calibrated from clusters discovered by the South Pole Telescope at higher masses and lower redshifts. The full XXL-CARMA sample will provide a more complete, multi-wavelength census of distant clusters in order to robustly extend the calibration of cluster scaling relations to these high redshifts.
Subject headings and genre
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Abdulla, Z.University of Chicago
(author)
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Carlstrom, J. E.University of Chicago
(author)
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Greer, C. H.University of Arizona
(author)
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Leitch, E. M.University of Chicago
(author)
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Marrone, D. P.University of Arizona
(author)
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Muchovej, S.California Institute of Technology (Caltech)
(author)
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Adami, C.Laboratoire d'Astrophysique de Marseille
(author)
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Birkinshaw, M.University of Bristol
(author)
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Bremer, M.University of Bristol
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Clerc, N.Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
(author)
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Giles, P.University of Bristol
(author)
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Horellou, Cathy,1967Chalmers tekniska högskola,Chalmers University of Technology(Swepub:cth)horellou
(author)
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Maughan, B.University of Bristol
(author)
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Pacaud, F.
(author)
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Pierre, M.Le Commissariat à l’Énergie Atomique et aux Énergies Alternatives (CEA),The French Alternative Energies and Atomic Energy Commission (CEA)
(author)
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Willis, J.University of Victoria
(author)
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University of ChicagoUniversity of Arizona
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In:Astrophysical Journal: American Astronomical Society794:21538-43570004-637X
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Mantz, A. B.
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Abdulla, Z.
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Carlstrom, J. E.
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Greer, C. H.
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Leitch, E. M.
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Marrone, D. P.
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Muchovej, S.
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Adami, C.
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Birkinshaw, M.
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Bremer, M.
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Clerc, N.
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Giles, P.
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Horellou, Cathy, ...
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Maughan, B.
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Pacaud, F.
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Pierre, M.
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Willis, J.
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Chalmers University of Technology