Absolute magnitudes for late-type dwarf stars for Sloan photometry

Details Absolute magnitudes for late-type dwarf stars for Sloan photometry Absolute magnitudes for late-type dwarf stars for Sloan photometry

2005-03-18

arxiv.org/abs/astro-ph/0503415v1

Astronomy and Astrophysics

Astrophysics

11 pages, 9 figures and 5 tables, accepted for publication in AN

Scientific paper

10.1002/asna.200510358

We present a new formula for absolute magnitude determination for late-type
dwarf stars as a function of (g-r) and (r-i) for Sloan photometry. The absolute
magnitudes estimated by this approach are brighter than those estimated by
colour-magnitude diagrams, and they reduce the luminosity function rather close
to the luminosity function of Hipparcos.

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