Laurent, G. T., Aguirre, J. E., Bock, J., Edgington, S., Enoch, M., Glenn, J., Goldin, A., Golwala, S., Haig, D. J., Maloney, P., Mauskopf, Philip Daniel ![]() |
Abstract
Submillimeter galaxies are dusty, high-redshift galaxies with extreme luminosities (>1012 L\sun) and implied star formation rates (100-1000 M\sun per year). Characterizing submillimeter galaxies is crucial to understanding galaxy formation and evolution. Cumulatively, surveys to date have detected hundreds of these galaxies. Bolocam is a millimeter-wavelength bolometer-array camera designed for mapping large fields. This survey uses Bolocam to detect submillimeter galaxies at the bright end of the luminosity function. Due to the strong negative K-correction at 1.1 mm, Bolocam's detection sensitivity is approximately uniform for galaxies of a given intrinsic luminosity for redshifts 1 < z < 10. We present preliminary results from our 1.1 mm galaxy survey made with the Caltech Submillimeter Observatory during January and May 2003. We achieved a sensitivity of 24 mJy s1/2 and integrated down to an rms noise level of approximately 1 mJy over 400 arcmin2 in the Lockman Hole. The data have been processed using our IDL-based analysis pipeline, which removes atmospheric noise and provides diagnostic quantities. Monte Carlo simulations have been implemented to quantify uncertainties, systematic effects, completeness, and source confusion.
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 |
ISSN: | 0002-7537 |
Related URLs: | |
Last Modified: | 27 Oct 2022 10:12 |
URI: | https://orca.cardiff.ac.uk/id/eprint/69266 |
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