Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994an....315..431a&link_type=abstract
Astronomische Nachrichten (ISSN 0004-6337), vol. 315, no. 6, p. 431-437
Astronomy and Astrophysics
Astronomy
7
Astronomical Models, Astronomical Photometry, Photographic Measurement, Photographic Plates, Sky Surveys (Astronomy), Statistical Analysis, Stellar Magnitude, Ubv Spectra, Coefficients, Least Squares Method, Mathematical Models, Optimization, Polynomials, Schmidt Telescopes, Spectral Bands
Scientific paper
Photometric properties of deep Tautenburg Schmidt plates in the UBV system over the whole field and over a wide range of stellar magnitudes are discussed. Different reduction models based on the calibration curve alone and with additional terms containing color and plate coordinates are considered. With the filter-emulsion combinations used the Johnson UBV system can be reproduced quite well by the Tautenburg telescope. The accuracy of photometric data can be improved if geometrical terms are taken into account. For deep plates with a significant effect of background nebulosity a supplementary term is to be included in the reduction model. The polynomial coefficients vary in dependence on spectral bands and individual properties of each plate.
Andruk V.
Kharchenko Nina
Schilbach Elena
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