Nature of the 1100 Micron AzTEC-COSMOS sources

Yun, Min Su, Aguirre, J., Aretxaga, I., Austermann, J., Bock, J., Fazio, G., Huang, J., Hughes, D., Kang, Y., Kim, S., Lowenthal, J., Ma, C., Mauskopf, Philip Daniel ORCID: https://orcid.org/0000-0001-6397-5516, Perera, T., Sanders, D., Scott, K., Scoville, N., Wilson, G. and Yoon, I. 2007. Nature of the 1100 Micron AzTEC-COSMOS sources. Presented at: 2007 AAS/AAPT Joint Meeting, Seattle, WA, Seattle, WA, USA, 5-10 January 2007. Bulletin of the American Astronomical Society. (38) American Astronomical Society,

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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). To take advantage of the extensive complementary databases already available through the COSMOS collaboration, 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 IRAM 30-m telescope. In this poster paper, we will compare the results of the AzTEC and Bolocam surveys and discuss the nature of the AzTEC sources based on the existing multi-wavelength data in hand.

Item Type:	Conference or Workshop Item (Poster)
Date Type:	Publication
Status:	Published
Schools:	Schools > Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	American Astronomical Society
Related URLs:	Organisation
Last Modified:	27 Oct 2022 10:10
URI:	https://orca.cardiff.ac.uk/id/eprint/69124

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