Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ncimc..13..313a&link_type=abstract
Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 13 C, Jan.-Feb. 1990, p. 313-320.
Astronomy and Astrophysics
Astronomy
Infrared Sources (Astronomy), Infrared Telescopes, Millimeter Waves, Photometers, Continuous Radiation, Infrared Photometry, Interstellar Matter
Scientific paper
The techniques and instrumentation used to observe cold galactic and extragalactic sources at the Italian IR observatory TIRGO are briefly characterized. The photometer employs uncooled optics to match the detector and telescope f-numbers, an optical alignment device, a focal-plane modulator, a reference source for atmospheric-transmission measurements, and a Chanin-type He-3-cooled bolometer detector with optical NEP 8.0 fW/sq rt Hz, corresponding to noise-equivalent flux 13 Jy/sq rt Hz under good atmospheric conditions (precipitable water 1 mm). Typical results from transmittance measurements and observations performed in 1988 are presented in tables; it is found that atmospheric transmission alone does not determine the quality of the observing conditions, which are affected by patchiness and time variation in the water-vapor content. It is suggested that the use of a three-beam modulation technique could improve the results significantly.
Aiello Santi
Barbis Alessandra
Bonetti Alberto
Natale Vincenzo
Ventura Giulio
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