Results from the first engineering run of BOLOCAM and plans for the future

Details Results from the first engineering run of BOLOCAM and plans for the future Results from the first engineering run of BOLOCAM and plans for the future

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..616..107m&link_type=abstract

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

Physics

2

Photoconductors And Bolometers, Radio, Microwave, Submillimeter, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Galaxy Clusters

Scientific paper

We present results from the engineering run of the BOLOCAM receiver at the Caltech Submillimeter Observatory in May, 2000 and simulations of the sensitivity of the completed BOLOCAM receiver to astrophysical sources. BOLOCAM is a 144 element array of bolometers designed to operate in the millimeter wave atmospheric windows at 150, 220, and 280 GHz. These bands are well suited to studies of the Sunyaev-Zel'dovich effect in distant clusters of galaxies as well as measurements of the emission of interstellar dust. .

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