Processing of CCD images of star fields using the MIDAS/ROMAFOT software package

Details Processing of CCD images of star fields using the MIDAS/ROMAFOT software package Processing of CCD images of star fields using the MIDAS/ROMAFOT software package

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003kfnts...4...71a&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 4, p. 71-74

Astronomy and Astrophysics

Astronomy

Scientific paper

We suggest a new procedure to take into account the flat-field effect based on compensating for the gradient and local irregularities of the image background. It was tested by reducing numerous CCD images taken with the S1C-017 camera and the Zeiss-600 astrograph of Andrushivka Astronomical Observatory (observatory code A50). No auxiliary flat-field image is used. The MIDAS software package is described for preliminary reduction of stellar images. The rms method error of determination of single position is several arc sec.

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