1. Detectability of HD and non-equilibrium species in the upper atmospheres of the giant planets from their submillimeter spectrum;Bezard;Astronomy and Astrophysics,1986
2. J. Beeman, E.E. Haller, Lawrence Berkley National Laboratory, USA, private communication, 1996.
3. Morphology of the interstellar cooling lines detected by COBE;Bennet;Astrophysical Journal,1994
4. F. Cartier, F.K. Kneubühl, D. Huguenin, E.A. Müller, Submillimetre-wave brightness temperature of solar active zones and sunspot measured from a balloon-borne platform, Proc. Workshop on Scientific Importance of Submillimeter Observations, Noordwijkerhout, May 10–12, 1982, pp. 175–179.
5. The ISO long-wavelength spectrometer;Clegg;Astronomy and Astrophysics,1996