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

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dc.creatorD'esert, F. -X.
dc.creatorBenoit, A.
dc.date1999-01-29
dc.date.accessioned2026-07-07T02:30:15Z
dc.date.available2026-07-07T02:30:15Z
dc.descriptionWe 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.
dc.description8 pages, 1 figure eps appeared in Scientific contribution to IRAM Newsletter Nr 38
dc.identifierhttps://arxiv.org/abs/astro-ph/9901414
dc.identifierhttp://arxiv.org/abs/astro-ph/9901414
dc.identifierIRAM Newsletter Nr 38, January 1999, http://iram.fr/ARN/jan99/jan99.html
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13755
dc.subjectAstrophysics
dc.titleThe case for a bolometric millimetre camera at the IRAM 30m telescope
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