Lonsdale, Carol J. and Hurt, Robert and Smith, Harding E. and Levine, Deborah and Beichman, Chas and Helou, George and Cesarsky, Catherine J. and Lemke, Dietrich and Klaas, Ulrich and Elbaz, David (2000) ISO-IRAS Faint Galaxy Survey: ISOCAM Imaging and Optical Spectroscopy. In: ISO Surveys of a Dusty Universe. Lecture Notes in Physics. No.548. Springer , Berlin, pp. 267-274. ISBN 978-3-540-67479-5. https://resolver.caltech.edu/CaltechAUTHORS:20200225-110915168
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Abstract
The goal of the ISO-IRAS Faint Galaxy Survey was to obtain a sample of the most distant, highest luminosity infrared galaxies from the 0.75 million sources in the IRAS Faint Source Survey. The strategy involved providing a large sample of sources, selected to be faint, high-luminosity (hence highredshift) infrared galaxies, that ISO could select from to fill short (∼ 12 mins) schedule gaps. The initial observing program involved CAM LW10 imaging at 12μm plus PHT 90μm photometry (PHT22) in order to obtain SED information and to provide good positions and reliable identifications for optical spectroscopy and other follow-up observations.
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| Additional Information: | © 2000 Springer-Verlag Berlin Heidelberg. This research has been supported in part by grants from NASA to IPAC and UCSD and by the US NSF to UCSD. | ||||||||||
| Group: | Infrared Processing and Analysis Center (IPAC) | ||||||||||
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| Subject Keywords: | Background Source; Color Selection; Infrared Galaxy; Narrow Slice; Emission Line Galaxy | ||||||||||
| Series Name: | Lecture Notes in Physics | ||||||||||
| Issue or Number: | 548 | ||||||||||
| Record Number: | CaltechAUTHORS:20200225-110915168 | ||||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20200225-110915168 | ||||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||
| ID Code: | 101534 | ||||||||||
| Collection: | CaltechAUTHORS | ||||||||||
| Deposited By: | Tony Diaz | ||||||||||
| Deposited On: | 25 Feb 2020 20:29 | ||||||||||
| Last Modified: | 25 Feb 2020 20:29 |
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