COSMOSOMAS: a circular scanning instrument to map the sky at centimetric wavelengths

We describe the first instrument of a cosmic microwave background experimen t for mapping cosmological structures on medium angular scales (the COSMOSO MAS experiment) and diffuse Galactic emission. The instrument is located at Teide Observatory (Tenerife) and is based on a circular scanning sky strat egy. It consists of a 1-Hz spinning flat mirror directing the sky radiation into a 1.8-m off-axis paraboloidal antenna, which focuses it on to a cryog enically cooled HEMT-based receiver operating in the frequency range 12-18 GHz. The signal is split by a set of three filters, allowing simultaneous o bservations at 13, 15 and 17 GHz, each with a 1-GHz bandpass. A 1 degrees - 5 degrees resolution sky map complete in right ascension and covering 20 de grees in declination is obtained each day at these frequencies. The observa tions presented here correspond to the first months of operation, which hav e provided a map of 9000 deg(2) on the sky centred at Dec. = +31 degrees wi th sensitivities of 140, 150 and 250 muK per beam area in the channels at 1 3, 15 and 17 GHz, respectively. We discuss the design and performance of th e instrument, the atmospheric effects, the reliability of the data obtained and prospects of achieving a sensitivity of 30 muK per beam in 2 years of operation.