Reduction of CCD observations obtained with the Fabry-Perot scanning interferometer. II. Additional Procedures
arXiv:0805.2367 · doi:10.1134/S1990341308020089
Abstract
We describe a software package used at the Special Astrophysical Observatory of the Russian Academy of Sciences to reduce and analyze the data obtained with the Fabry-Perot scanning interferometer. We already described most of the algorithms employed in our earlier Paper I (Moiseev, 2002). In this paper we focus on extra procedures required in the case of the use of a high-resolution Fabry-Perot interferometer: removal of ghosts and measurement of the velocity dispersion of ionized gas in galactic and extragalactic objects.
Corrected version, 11 pages, 9 EPS figures
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