Mapping the Local Dust Distribution with SDSS

Details Mapping the Local Dust Distribution with SDSS Mapping the Local Dust Distribution with SDSS

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..317..199m&link_type=abstract

Milky Way Surveys: The Structure and Evolution of our Galaxy, Proceedings of ASP Conference #317. The 5th Boston University Ast

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The narrow range of M dwarf g-r colors in SDSS photometry permits study of the three-dimensional dust distribution within 1 kpc. Distances to early M dwarfs are assigned using reddening-invariant photometric parallaxes and clouds are identified by persistent shifts in mean g-r colors along the line of sight. The observed reddening is compared against that predicted by Schlegel, Finkbeiner & Davis (1998).

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