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Millimeter Observations of Optically Selected Quasars

Published online by Cambridge University Press:  07 August 2017

J. Keene ,
G. Neugebauer ,
D. Carico ,
D. Sanders  and
T. Soifer
J. Keene
Affiliation:
Division of Physics, Mathematics and Astronomy, California Institute of Technology, Downs Laboratory of Physics, 320-47, Pasadena CA, 91125, USA
G. Neugebauer
Affiliation:
Division of Physics, Mathematics and Astronomy, California Institute of Technology, Downs Laboratory of Physics, 320-47, Pasadena CA, 91125, USA
D. Carico
Affiliation:
Division of Physics, Mathematics and Astronomy, California Institute of Technology, Downs Laboratory of Physics, 320-47, Pasadena CA, 91125, USA
D. Sanders
Affiliation:
Division of Physics, Mathematics and Astronomy, California Institute of Technology, Downs Laboratory of Physics, 320-47, Pasadena CA, 91125, USA
T. Soifer
Affiliation:
Division of Physics, Mathematics and Astronomy, California Institute of Technology, Downs Laboratory of Physics, 320-47, Pasadena CA, 91125, USA

Extract

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We have observed a group of optically selected quasars at a wavelength of 1.25mm with the Caltech Submillimeter Observatory in 1988 May. Except for Mrk 231, they were chosen from the PG sample of quasars (Schmidt and Green 1983) and are thus UV bright objects. All of them, except for PG 2209+184, were also detected at 60μm by IRAS.

Type
Part 7: Dust, Molecules, Infrared and MM Radiation
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 396 - 397
Copyright
Copyright © Kluwer 1989 

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