The surface photometry of NGC 3379 |
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| Authors: | F X Hu M Hamabe S Okamura H J Su |
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| Institution: | (1) Kiso Observatory, Institute of Astronomy, The University of Tokyo, Japan;(2) Present address: Purple Mountain Observatory, Academia Sinica, Nanjing, China |
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| Abstract: | Surface photometry is carried out for the photometric standard galaxy NGC 3379 on the basis of two plates in the blue band taken with the Bejing Schmidt telescope. The results, including luminosity profiles, photometric parameters, integrated luminosity distribution, ellipticity and position angle variation, are presented in various forms of figures and tables. Especially our geometric profiles, i.e., ellipticity and position angle variations reach up to  5 , much fainter region than that any previous study did. The accuracy of the present data is checked by comparing them with the surface photometry in the literature. We find the zero-point 0.12 mag brighter than the calibration of de Vaucouleurs and Capaccioli (1979), which agrees with the values 0.10–0.15 mag difference claimed by recent observations. The systematic differences is found to be less than 0.1 mag. |
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