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The Palermo four-color far infrared programA four-channel far-IR photometer designed for use with a balloon-borne 102-cm telescope is described. The data analysis system for this photometer is discussed, and a typical observational program is outlined. Possible objects that may be observed with the four-color far-IR photometer include molecular clouds, the galactic-center region, H II regions, quasars, Seyfert galaxies, and BL Lacertae objects.
Document ID
19790041418
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Peres, G. (Palermo Univ. Italy)
Serio, S. (Palermo Univ. Italy)
Vaiana, G. S. (Osservatorio Astronomico, Palermo, Italy; Harvard College Observatory and Smithsonian Astrophysical Observatory, Center for Astrophysics, Cambridge Mass., United States)
Cali, C. (Palermo Univ. Italy)
Daneu, V. (Palermo, Universita Palermo, Italy)
Maxson, C. (Palermo Univ. Italy)
Steier, M. (Harvard College Observatory and Smithsonian Astrophysical Observatory, Center for Astrophysics, Cambridge Mass., United States)
Date Acquired
August 9, 2013
Publication Date
March 1, 1978
Subject Category
Instrumentation And Photography
Accession Number
79A25431
Funding Number(s)
CONTRACT_GRANT: NSG-7176
Distribution Limits
Public
Copyright
Other

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