Revised statistics of radio halos and the re-acceleration model

Details Revised statistics of radio halos and the re-acceleration model Revised statistics of radio halos and the re-acceleration model

2007-12-20

arxiv.org/abs/0712.3516v1

Astronomy and Astrophysics

Astrophysics

12 pages, 10 figures. Accepted by A&A

Scientific paper

10.1051/0004-6361:20078986

Aims. The statistical properties of radio halos can be used to discriminate among the possible models for their origin. Therefore an unbiased and exhaustive investigation in this direction is crucial. Methods. With this goal in mind in this paper we revise the occurrence of radio halos in the redshift range 0-0.4, combining the low redshift (z<0.2) statistical study of XBACs clusters with the NVSS (by Giovannini et al. 1999) with our recent results from the radio follow up of REFLEX and eBCS clusters, the GMRT radio halo survey, at higher redshift (0.2

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