A FIR Photometer for Ground-Based Astronomical Observations

Details A FIR Photometer for Ground-Based Astronomical Observations A FIR Photometer for Ground-Based Astronomical Observations

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984infph..24..493c&link_type=abstract

Infrared Physics, vol. 24, p. 493-497

Physics

2

Cryostats, Infrared Photometry, Millimeter Waves, Bolometers

Scientific paper

A description is given of a photometer which is suitable for
astronomical observations through millimetric atmospheric windows. It
consists of a Ge-Ga bolometer operating at 1.0 K, with a throughput AW =
0.3 cm2 sr and a NET = 1 mK Hz-1/2. Two metallic mesh filters set the
windows at about 10 and 5 cm-1.

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