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The case for a bolometric millimetre camera at the IRAM 30m telescope

F. -X. D'esert·A. Benoit
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Abstract

We describe here the important astrophysical results that could be obtained by using large format (say 32 by 32) bolometric detectors at 1 and 2 mm with the IRAM 30m telescope: having a confusion-limited 1 mm extragalactic survey containing a large fraction of high redshift objects, mapping star formation regions in our galaxy at 1 mm, and mapping the Sunyaev-Zeldovich effect at 2 mm in tens of high-redshift clusters. We also show a first optical implementation and the key points of this project.

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F. -X. D'esert, A. Benoit. 1999-01-29. The case for a bolometric millimetre camera at the IRAM 30m telescope. https://arxiv.org/abs/astro-ph/9901414

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