Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.177..209t&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 177, no. 1-2, March 1991, p. 209-212.
Astronomy and Astrophysics
Astrophysics
3
Astrometry, Astronomical Photography, Astronomical Photometry, Celestial Reference Systems, Red Shift, Calcium, Quasars, Spatial Distribution, Spectrum Analysis
Scientific paper
The proper choice of the wavelength reference point is essential for the determination of redshifts free of systematic and large random errors. This paper describes the procedure of astrometric determination of the reference point for wavelength measurements from low-dispersion objective prism plates, which were part of the Muenster Redshift Project. Special attention is given to the quadratic model used for the transformation from the direct plate positions to positions on the objective prism plate, as well as to the measurements and reductions.
Horstmann H.
Schuecker Peter
Seitter W.
Tucholke Hans-Joachim
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