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Millimeter Observations of Luminous IRAS Galaxies

Keene, J. and Carico, D. P. and Neugebauer, G. and Soifer, B. T. (1990) Millimeter Observations of Luminous IRAS Galaxies. In: Submillimetre Astronomy. Astrophysics and Space Science Library. No.158. Springer , Dordrecht, pp. 209-210. ISBN 978-94-015-6852-4. https://resolver.caltech.edu/CaltechAUTHORS:20170227-153007615

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Abstract

We have observed a group of luminous IRAS galaxies in the continuum at 1.25mm with the Caltech Submillimeter Observatory in 1988 May and September. Table I lists the galaxies and their measured flux densities in a 30 beam. The observing conditions for these observations were excellent and stable. Uranus was the fundamental flux density calibrator, it was assumed to have a brightness temperature of 100 K at 1.25 mm (Hildebrand et al. 1985; Ulich 1974). Integration times were typically a half hour per night, repeated for a total of two or three nights. The bolometer NEFD is 0.5 Jy Hz^(-1/2) giving statistical errors of 8 to 12 mJy. Systematic uncertainties have not been included in the error estimates, but we believe that they are small, at most 20%.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1007/978-94-015-6850-0_76DOIArticle
https://rdcu.be/b37toPublisherFree ReadCube access
Additional Information:© 1990 Springer Science+Business Media Dordrecht. The CSO is supported by NSF grant # AST 83-11849. D.P.C., G.N. and B.T.S. are supported in part by the NSF and by the IRAS Extended Mission Program.
Funders:
Funding AgencyGrant Number
NSFAST 83-11849
Infrared Astronomical Satellite (IRAS)UNSPECIFIED
Series Name:Astrophysics and Space Science Library
Issue or Number:158
DOI:10.1007/978-94-015-6850-0_76
Record Number:CaltechAUTHORS:20170227-153007615
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170227-153007615
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74560
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:28 Feb 2017 00:02
Last Modified:11 Nov 2021 05:28

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