MITO: a procedure for CBA measurements and a search for cosmic strings.

Details MITO: a procedure for CBA measurements and a search for cosmic strings. MITO: a procedure for CBA measurements and a search for cosmic strings.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ncimc..18..305d&link_type=abstract

Nuovo Cimento C, Vol. 18C, N. 3, p. 305 - 324

Mathematics

Logic

Background Radiation: Cosmic, Background Radiation: Anisotropy

Scientific paper

MITO (Millimetric and Infrared Testa Grigia Observatory) is a 3-m telescope dedicated to the study of the cosmic background anisotropies. It is located at 3500 m above sea-level at Plateau Rosa, Cervinia, Italy. The authors describe the observatory and discuss two on-going research programs: a cleaning procedure in order to remove Galactic dust signals from cosmological data and a search for cosmic strings toward double-lensed quasars. Both programs will be carried out by means of a He-3 photometer operating at the frequencies of 5, 10, 12, and 30 cm-1.

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