Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984spie..445..279t&link_type=abstract
Instrumentation in astronomy V, p. 279 - 283
Astronomy and Astrophysics
Astronomy
Infrared Telescopes:Balloon-Borne
Scientific paper
A balloon-borne 75 cm aperture Cassegrain telescope has been developed for far-infrared astronomical observations. This telescope uses a three axis stabilised platform which is designed to orient the optic axis with an accuracy of ≈0.5 min of arc. A star sensor is used for the guidance. The secondary mirror is chopped at 20 Hz and the signals from the infrared detector are analysed by a phase sensitive detector (PSD). The gain of the PSD can be changed during the flight to provide an overall dynamic range of 1.5×105. The telescope was flown at an altitude of 32 km for photometric observations in 80 μm to 120 μm wavelength band. An aperture of 4 min of arc was used and a sensitivity of 100 Jy was expected.
Daniel R. R.
Ghosh Sanjay K.
Iyengar V. K. K.
Rengarajan T. N.
Tandon Shyam N.
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