Borys, Colin (2006) 350μm Observations of Local IRAS Galaxies Using SHARC-II. In: Multiwavelength Mapping of Galaxy Formation and Evolution. Springer , Berlin, pp. 359-360. ISBN 978-3-540-25665-6. https://resolver.caltech.edu/CaltechAUTHORS:20191127-135934134
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Abstract
The cosmologically significant population of dusty galaxies detected at sub-mm and mm wavelengths by SCUBA and MAMBO have played a central part in many of the discussions at this workshop. Obtaining their redshifts is critical in understanding their role in galaxy formation and evolution, but this is a challenging task. Nevertheless, Chapman et al. [1] have made significant process by obtaining spectroscopic redshifts of the subset of sub-mm galaxies detected in deep radio images that have optical counterparts. This exploits the well-known Far-Infrared/Radio correlation, and allows the high resolution radio maps to be used as a surrogate for finding the correct optical counterpart for which spectroscopy can then be attempted.
| Item Type: | Book Section | |||||||||
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| Additional Information: | © 2005 Springer-Verlag Berlin Heidelberg. First Online: 05 January 2006. | |||||||||
| Subject Keywords: | Spectral Energy Distribution; Galaxy Formation; Nearby Galaxy; Galaxy Evolution; Bright Galaxy | |||||||||
| DOI: | 10.1007/10995020_60 | |||||||||
| Record Number: | CaltechAUTHORS:20191127-135934134 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20191127-135934134 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 100115 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 28 Nov 2019 01:56 | |||||||||
| Last Modified: | 16 Nov 2021 17:51 |
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