Bolometer arrays for Mm/Submm astronomy

Details Bolometer arrays for Mm/Submm astronomy Bolometer arrays for Mm/Submm astronomy

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..616..262k&link_type=abstract

EXPERIMENTAL COSMOLOGY AT MILLIMETRE WAVELENGTHS: 2K1BC Workshop. Breuil-Cervinia, Valle d'Aosta, Italy, 9-13 July, 2001. Edit

Physics

11

Photoconductors And Bolometers, Radio, Microwave, Submillimeter

Scientific paper

Arrays consisting of large numbers of sensitive bolometers have become powerful tools for Mm/Submm Astronomy. On large ground-based telescopes for example they were essential in the discovery of a population of faint, highly redshifted point sources which provide important clues to the star-formation history of the universe. The Bolometer group at the Max-Planck-Institut für Radioastronomie has been developing bolometer arrays since 1980. This paper is meant to give an overview of the state and future of this effort. .

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