Abstract
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(This patch is compatible with Halo PC version 1.09) Download english universal binary patch 2.0.4 (4MB) Download french universal binary patch 2.0.4 (4MB) Download german universal binary patch 2.0.4. Mar 01, 2007 Aims:We present the first results of an ongoing project devoted to the search of giant radio halos in galaxy clusters located in the redshift range z=0.2-0.4. One of the main goals of our study is to measure the fraction of massive galaxy clusters in this redshift interval hosting a radio halo, and to constrain the expectations of the particle re-acceleration model for the origin of non. Sep 04, 2014 Important Note: OS X 10.7 Lion has been replaced by OS X 10.8 Mountain Lion. The 10.7.4 update is recommended for all OS X Lion users and includes general operating system fixes that improve the stability, compatibility, and security of your Mac. The missions such as Noble Actual, Epilogue and Lone Wolf are not required for this achievement. Halo Reach Par Times Easy Difficulty Winter Contingency – Time Required 00:15:00 / My Time 00:10.
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Aims. We present the results of the GMRT cluster radio halo survey. The main purposes of our observational project are to measure which fraction of massive galaxy clusters in the redshift range z=0.2–0.4 hosts a radio halo, and to constrain the expectations of the particle re–acceleration model for the origin of the non–thermal radio emission. Methods. We selected a complete sample of 50 clusters in the X–ray band from the REFLEX (27) and the eBCS (23) catalogues. In this paper we present Giant Metrewave Radio Telescope (GMRT) observations at 610 MHz for all clusters still lacking high sensitivity radio information, i.e. 16 eBCS and 7 REFLEX clusters, thus completing the radio information for the whole sample. The typical sensitivity in our images is in the range 1σ ∼ 35 − 100 µJy b −1. Results. We found a radio halo in A697, a diffuse peripheral source of unclear nature in A 781, a core–halo source in Z 7160, a candidate radio halo in A1682 and “suspect ” central emission in Z 2661. Including the literature information, a total of 10 clusters in the sample host a radio halo. A very important result of our work is that 25 out of the 34 clusters observed with the GMRT do not host extended central emission at the sensitivity level of our observations, and for 20 of them firm upper limits to the radio power of a giant radio halo were derived. The GMRT Radio Halo Survey shows that radio halos are not common, and our findings on the fraction of giant radio halos in massive clusters are consistent with the statistical expectations based on the re–acceleration model. Our results favour primary to secondary electron