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AzTEC COSMOS Survey

Yun, Min Su, Ade, Peter A. R. ORCID: https://orcid.org/0000-0002-5127-0401, Aretxaga, I., Austermann, J., Bock, J. J., Hughes, D., Kang, Y., Lowenthal, J., Mauskopf, Philip Daniel ORCID: https://orcid.org/0000-0001-6397-5516, Scott, K. and Wilson, G. 2007. AzTEC COSMOS Survey. Presented at: 2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #95.03, Seattle, WA, USA, 5-10 January 2007.

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Abstract

The Cosmic Evolution Survey (COSMOS) is a 2 square degree HST/ACS survey specifically designed to probe galaxy evolution as a function of time and environment (PI: N. Scoville). In addition to the extensive HST data, the COSMOS team has acquired deep multi-wavelength data from radio to X-ray (VLA, Spitzer, NOAO, CFHT, Subaru, Galex, Chandra, XMM). Spectroscopic surveys are currently under way using Magellan, Kecks, and VLT, and an extensive photometric redshift database is also being assembled. Future surveys using major new instruments such as Herschel are also being planned. To take advantage of these rich complementary databases, we have undertaken a 1100 micron imaging survey of a 30' x 30' field centered just north of the earlier mm/submm surveys by the Bolocam on CSO and MAMBO on the 30-m telescope, with a small overlap. We will present some of the preliminary results from the survey.

Item Type: Conference or Workshop Item (Paper)
Date Type: Completion
Status: Unpublished
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Additional Information: Session: Galactic and Extragalactic Surveys Using AzTEC Presentation Number: 125.03 Abstract printed in the Bulletin of the American Astronomical Society, Vol. 38
Last Modified: 21 Oct 2022 10:44
URI: https://orca.cardiff.ac.uk/id/eprint/41178

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