Submillimetric photometry of the integrated galactic emission

Details Submillimetric photometry of the integrated galactic emission Submillimetric photometry of the integrated galactic emission

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...154...55p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 154, no. 1-2, Jan. 1986, p. 55-60. Research supported by the Institut National

Astronomy and Astrophysics

Astronomy

11

Astronomical Photometry, Galactic Radiation, Galactic Structure, Milky Way Galaxy, Radio Astronomy, Submillimeter Waves, Atmospheric Attenuation, Calibrating, Signal Processing

Scientific paper

A program of photometric observations which have been carried in the submillimeter range using the Canada-France-Hawaii telescope is described. The field of view of the observations was 0.5 degrees and the range of submillimeter wavelengths was 0.7-2.0 mm. The internal calibration and signal processing components of the photometer system are outlined, and results on galactic emission are presented for a region in the galactic plane between 0 and 30 degrees longitude. The variation in brightness temperature of atmospheric emission in the photometer bands is given in a table as a function of the water vapor content.

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