Review of coherent and incoherent detection techniques: Outlook and limitation

Details Review of coherent and incoherent detection techniques: Outlook and limitation Review of coherent and incoherent detection techniques: Outlook and limitation

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.260...15d&link_type=abstract

In ESA Proceedings of an ESA Workshop on a Spaceborne Submillimeter Astronomy Mission. A Cornerstone of the ESA Long Term Scienc

Astronomy and Astrophysics

Astronomy

Esa Satellites, Far Infrared Radiation, Infrared Astronomy, Radio Astronomy, Satellite-Borne Instruments, Spaceborne Astronomy, Submillimeter Waves, Infrared Spectrometers, Infrared Spectrophotometers, Superheterodyne Receivers

Scientific paper

The ESA Far Infrared and Submillimeter Space Telescope (FIRST) model payload is described. The frequency/wavelength coverage versus spectral resolution capabilities of FIRST submillimeter heterodyne receivers, a short wavelength spectrometer, and multiband array photometer are shown. At 1hr intervals, photometric and infrared spectroscopic sensitivities are 1mJy and 100 mJy respectively. For heterodyne spectroscopy, Tsyst = (Frequency in Ghz) x K.

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