The Palermo four-color far infrared program

Details The Palermo four-color far infrared program The Palermo four-color far infrared program

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mmsai..49...95p&link_type=abstract

(Società Astronomica Italiana, Conference on Infrared Astronomy, 1st, Lecce, Italy, Sept. 22-24, 1977.) Società Astronomica Ital

Astronomy and Astrophysics

Astronomy

Balloon-Borne Instruments, Color Photography, Data Reduction, Far Infrared Radiation, Infrared Telescopes, Galactic Nuclei, H Ii Regions, Infrared Spectrophotometers, Multichannel Communication, Quasars, Seyfert Galaxies, Spectral Resolution

Scientific paper

A 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.

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