Blazar surveys with WMAP and Swift

P. Giommi; M. Capalbi; E. Cavazzuti; S. Colafrancesco; S. Cutini; D. Gasparrini; E. Massaro; P. Padovani; M. Perri; S. Puccetti

doi:10.1063/1.2757262

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arXiv · 0704.1744

Blazar surveys with WMAP and Swift

P. Giommi·M. Capalbi·E. Cavazzuti·S. Colafrancesco·S. Cutini·D. Gasparrini·E. Massaro·P. Padovani·M. Perri·S. Puccetti

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Abstract

We present the preliminary results from two new surveys of blazars that have direct implications on the GLAST detection of extragalactic sources from two different perspectives: microwave selection and a combined deep X-ray/radio selection. The first one is a 41 GHz flux-limited sample extracted from the WMAP 3-yr catalog of microwave point sources. This is a statistically well defined sample of about 200 blazars and radio galaxies, most of which are expected to be detected by GLAST. The second one is a new deep survey of Blazars selected among the radio sources that are spatially coincident with serendipitous sources detected in deep X-ray images (0.3-10 keV) centered on the Gamma Ray Bursts (GRB) discovered by the Swift satellite. This sample is particularly interesting from a statistical viewpoint since a) it is unbiased as GRBs explode at random positions in the sky, b) it is very deep in the X-ray band (\fx \simgt $10^{-15}$ \ergs) with a position accuracy of a few arc-seconds, c) it will cover a fairly large (20-30 square deg.) area of sky, d) it includes all blazars with radio flux (1.4 GHz) larger than 10 mJy, making it approximately two orders of magnitude deeper than the WMAP sample and about one order of magnitude deeper than the deepest existing complete samples of radio selected blazars, and e) it can be used to estimate the amount of unresolved GLAST high latitude gamma-ray background and its anisotropy spectrum.

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P. Giommi, M. Capalbi, E. Cavazzuti, S. Colafrancesco, S. Cutini, D. Gasparrini, E. Massaro, P. Padovani, M. Perri, S. Puccetti. 2007-04-13. Blazar surveys with WMAP and Swift. https://doi.org/10.1063/1.2757262

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