Detector Technologies for a New Generation of CMB Cosmology Experiments

Details Detector Technologies for a New Generation of CMB Cosmology Experiments Detector Technologies for a New Generation of CMB Cosmology Experiments

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cpa..conf..302r&link_type=abstract

PROCEEDINGS OF THE 2002 INTERNATIONAL SYMPOSIUM ON COSMOLOGY AND PARTICLE ASTROPHYSICS (CosPA 02). Held 31 May ?2 June 2002 in T

Astronomy and Astrophysics

Astrophysics

Scientific paper

Spectacular progress has been made in obtaining information about the early universe from the cosmic microwave background (CMB). Much more can be learned from observations with high sensitivity and precision. One important requirement for progress is improvements in receiver sensitivity. The types of detectors used for CMB research are approaching fundamental sensitivity limits. Future progress will come from the use of large format detector arrays. The detector types most suitable for large arrays are discussed. Several new experiments being developed by the Berkeley group are described which will make use of arrays of 300 to 1000 bolometric detectors.

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