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