Reduction of CCD observations obtained with the Fabry-Perot scanning interferometer. II. Additional Procedures

Details Reduction of CCD observations obtained with the Fabry-Perot scanning interferometer. II. Additional Procedures Reduction of CCD observations obtained with the Fabry-Perot scanning interferometer. II. Additional Procedures

2008-05-15

arxiv.org/abs/0805.2367v1

Astrophys.Bull.63:181,2008

Astronomy and Astrophysics

Astrophysics

Corrected version, 11 pages, 9 EPS figures

Scientific paper

10.1134/S1990341308020089

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.

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