Diese Webseite wird nicht länger aktualisiert. Für Inhalte und Links wird keine Haftung übernommen. Bitte besuchen Sie die Seite des Nachfolgeclusters ORIGINS.
This website is no longer maintained. We assume no liability for content and links. Please visit the webpage of the successive cluster ORIGINS.

South Pole Telescope Detections of the Previously Unconfirmed Planck Early Sunyaev-Zel_s14dovich Clusters in the Southern Hemisphere

Story, K. and Aird, K.~A. and Andersson, K. and Armstrong, R. and Bazin, G. and Benson, B.~A. and Bleem, L.~E. and Bonamente, M. and Brodwin, M. and C

Keywords

cosmology: observations, galaxies: clusters: individual: PLCKESZ G255.62-46.16 PLCKESZ G225.92-19.99 PLCKESZ G264.41_s1619.48 PLCKESZ G283.16-29.93 PLCKESZ G304.84-41.42

Abstract

We present South Pole Telescope (SPT) observations of the five galaxy cluster candidates in the southern hemisphere which were reported as unconfirmed in the Planck Early Sunyaev-Zel_s14dovich (ESZ) sample. One cluster candidate, PLCKESZ G255.62-46.16, is located in the 2500-square-degree SPT SZ survey region and was reported previously as SPT-CL J0411-4819. For the remaining four candidates, which are located outside of the SPT SZ survey region, we performed short, dedicated SPT observations. Each of these four candidates was strongly detected in maps made from these observations, with signal-to-noise ratios ranging from 6.3 to 13.8. We have observed these four candidates on the Magellan-Baade telescope and used these data to estimate cluster redshifts from the red sequence. Resulting redshifts range from 0.24 to 0.46. We report measurements of Y_0.75_s14, the integrated Comptonization within a 0.75_s14 radius, for all five candidates. We also report X-ray luminosities calculated from ROSAT All-Sky Survey catalog counts, as well as optical and improved SZ coordinates for each candidate. The combination of SPT SZ measurements, optical red-sequence measurements, and X-ray luminosity estimates demonstrates that these five Planck ESZ cluster candidates do indeed correspond to real galaxy clusters with redshifts and observable properties consistent with the rest of the ESZ sample.

Information

Published
2011 as article
735 - page(s): L36
Contact
Dr. Alexandro Saro
Type
theoretical work
Links
pdf
ads
adsabs.harvard.edu/a…
Related to the research area(s):
E
e-Print
1102.2189

Technische Universitaet Muenchen
Exzellenzcluster Universe

Boltzmannstr. 2
D-85748 Garching

Tel. + 49 89 35831 - 7100
Fax + 49 89 3299 - 4002
info@universe-cluster.de