Reduction of CCD observations of visual binaries using the ``Tepui'' function as PSF

Details Reduction of CCD observations of visual binaries using the ``Tepui'' function as PSF Reduction of CCD observations of visual binaries using the ``Tepui'' function as PSF

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...416..811a&link_type=abstract

Astronomy and Astrophysics, v.416, p.811-814 (2004)

Astronomy and Astrophysics

Astrophysics

3

Stars: General, Astrometry, Techniques: Photometric

Scientific paper

429 CCD measurements of relative positions and magnitude differences in V and R photometric bands for 165 visual double and multiple stars are given. CCD frames were taken at the 1.52 m Spanish telescope of the Spanish-German Center of Astronomy at Calar Alto (Almería, Spain). During the reduction process a ``Tepui" function was used as the PSF function.
Tables 1 and 2 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/416/811

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