@article{10902/26546,
year = {2012},
url = {https://hdl.handle.net/10902/26546},
abstract = {We describe the state-of-the art status of multifrequency detection techniques for compact sources in microwave astronomy. From the simplest cases where the spectral behaviour is well known (i.e., thermal SZ clusters) to the more complex cases where there is little a priori information (i.e., polarized radio sources) we will review the main advances and the most recent results in the detection problem.},
organization = {The authors would like to thank the editors of this special Issue for their invitation to submit a contribution. The author also thank Prof. Gianfranco De Zotti for his useful advice. D. Herranz and F. Argüeso acknowledge partial financial support from the Spanish Ministerio de Ciencia e Innovación project AYA2010-21766-C03-01. D. Herranz also acknowledges the Spanish Ministerio de Educación for a José Castillejo’ mobility grant with reference JC2010-0096and the Astronomy Department at the Cavendish Laboratory for their hospitality during the elaboration of this paper. F.Argüeso also wants to thank the Astronomy Department at the Cavendish Laboratory for their hospitality during two short stays in the summer of 2011. The authors would like to thank Mike Hobson for his very useful contributions and for the wonderful, although very sharp and clear, descriptions.P. Carvalho is supported by a Portuguese fellowship (ref:SFRH/BD/42366/2007) from the Fundação para a Ciência eTecnologia (FCT)},
publisher = {Hindawi},
publisher = {Advances in Astronomy, 2012. 410965, 1-14},
title = {Compact source detection in multichannel microwave surveys: From SZ clusters to polarized sources},
author = {Herranz Muñoz, Diego and Argüeso, Framcisco and Carvalho, Pedro},
}