Numerical methods for processing of the surface photometry of galaxies consisting of smoothing, filtering and computation of two-dimensional correlation functions are given. Methods are adapted for the application to the photometry of Markaryan galaxies. A new processing of published data for the galaxies Mrk 7, 8, 10, 11, 12, 13, 185, 186, and 190 has begun and some illustrative results are given. Results of the surface photometry of Mrk 10 for a diaphragm of 3.5 x 3.5 are presented.

Smoothing

10.1007/bf01005392

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Citations (5)

Four-color photometry of compact groups of compact galaxies

Astrophysics (1975)

F. B�rngen A. T. Kalloglyan

10.1007/bf01005173

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Method of detecting compact galaxies

Astrophysics (1977)

A. T. Kalloglyan F. B�rngen

10.1007/bf01000939

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Morphology of compact galaxies. II

Astrophysics (1982)

F. B�rngen A. T. Kalloglyan

Morphology

10.1007/bf01004460

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Four-color photometry of spiral galaxies. Comparison with Markaryan galaxies

Astrophysics (1984)

A. T. Kalloglyan F. B�rngen

The results are given of UBVR surface photometry of seven normal spiral galaxies. The photometric parameters determined for these galaxies and galaxies with an ultraviolet excess in their radiation are compared. In particular, it is shown that after subtraction of the brightness of the nuclei from the integrated brightness the galaxies of these two types exhibit an almost identical distribution in the (U-B, B-V) diagram.

Surface brightness fluctuation

10.1007/bf01007333

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