The Viper Telescope : an Instrument to Measure Primary and Secondary CMB Anisotropy at Small Scales

Details The Viper Telescope : an Instrument to Measure Primary and Secondary CMB Anisotropy at Small Scales The Viper Telescope : an Instrument to Measure Primary and Secondary CMB Anisotropy at Small Scales

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.5803g&link_type=abstract

American Astronomical Society, 192nd AAS Meeting, #58.03; Bulletin of the American Astronomical Society, Vol. 30, p.904

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Viper is a 2-meter off-axis telescope designed to measure small-scale anisotropy in the Cosmic Microwave Background Radiation. It is currently deployed at the South Pole, operating with a 40 GHz HEMT receiver. We are attempting to measure primary anisotropy in addition to secondary anistropy from the Sunyaev-Zeldovich (S-Z) effect. Preliminary data will be presented, along with a description of plans for future cosmological and non-cosmological observations.

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