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| Paper: |
Mapping the Local Dust Distribution with SDSS |
| Volume: |
317, Milky Way Surveys: The Structure and Evolution of Our Galaxy |
| Page: |
199 |
| Authors: |
McGehee, P.M. |
| Abstract: |
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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