Search for the Sunyaev-Zeldovich effect in the coma cluster with the MITO experiment

Physics

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Background Radiations, Galaxy Clusters, Radio, Microwave

Scientific paper

We report the strategy for observing the Sunyaev-Zeldovich effect towards the Coma cluster of galaxies with the MITO telescope. The instrument has a 17 arcminutes FWHM field of view and uses a 3-field square wave mechanical modulation with a beamthrow of 41 arcminutes. The channels centered at 2.1, 1.4, 1.1 and 0.85 mm allow for matching the Sunyaev-Zeldovich effect spectral range and monitoring atmospheric fluctuations for spectral decorrelation. In this paper we describe both the analysis procedure and the preliminary results of our observations. We also make a first comparison with the available X-ray data. .

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