{ "id": "astro-ph/0303515", "version": "v2", "published": "2003-03-24T20:14:12.000Z", "updated": "2004-04-23T02:58:10.000Z", "title": "ACBAR: The Arcminute Cosmology Bolometer Array Receiver", "authors": [ "M. C. Runyan", "P. A. R. Ade", "R. S. Bhatia", "J. J. Bock", "M. D. Daub", "J. H. Goldstein", "C. V. Haynes", "W. L. Holzapfel", "C. L. Kuo", "A. E. Lange", "J. Leong", "M. Lueker", "M. Newcomb", "J. B. Peterson", "J. Ruhl", "G. Sirbi", "E. Torbet", "C. Tucker", "A. D. Turner", "D. Woolsey" ], "comment": "59 pages, 16 figures -- updated to reflect version published in ApJS", "journal": "Astrophys.J.Suppl. 149 (2003) 265", "doi": "10.1086/379099", "categories": [ "astro-ph" ], "abstract": "We describe the Arcminute Cosmology Bolometer Array Receiver (ACBAR); a multifrequency millimeter-wave receiver designed for observations of the Cosmic Microwave Background (CMB) and the Sunyaev-Zel'dovich effect in clusters of galaxies. The ACBAR focal plane consists of a 16-pixel, background-limited, 240 mK bolometer array that can be configured to observe simultaneously at 150, 220, 280, and 350 GHz. With 4-5' FWHM Gaussian beam sizes and a 3 degree azimuth chop, ACBAR is sensitive to a wide range of angular scales. ACBAR was installed on the 2 m Viper telescope at the South Pole in January 2001. We describe the design of the instrument and its performance during the 2001 and 2002 observing seasons.", "revisions": [ { "version": "v2", "updated": "2004-04-23T02:58:10.000Z" } ], "analyses": { "keywords": [ "arcminute cosmology bolometer array receiver", "fwhm gaussian beam sizes", "acbar focal plane consists", "multifrequency millimeter-wave receiver", "mk bolometer array" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 59, "language": "en", "license": "arXiv", "status": "editable", "inspire": 615602 } } }