Improved formulae for the transformation of CGCG magnitudes to the BT super S system

Details Improved formulae for the transformation of CGCG magnitudes to the BT super S system Improved formulae for the transformation of CGCG magnitudes to the BT super S system

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pasp...98.1213a&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 98, Nov. 1986, p. 1213-1219. NSERC-supported research.

Mathematics

Logic

5

Astronomical Catalogs, Astronomical Photometry, Galaxies, Magnitude, Regression Analysis

Scientific paper

New formulae are presented to transform CGCG magnitudes to the de Vaucouleurs BTS system. The transformations use the galaxy surface brightness and morphological type as estimated from data in either the Second Reference Catalogue or the Uppsala General Catalogue. Formulae are provided for both cases. The characteristic dispersions of the corrected CGCG magnitudes for the sample of galaxies in this study are 0m.19 and 0m.21, respectively.

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