1 code implementation • 30 Mar 2012 • J. J. Dalcanton, B. F. Williams, D. Lang, T. R. Lauer, J. S. Kalirai, A. C. Seth, A. Dolphin, P. Rosenfield, D. R. Weisz, E. F. Bell, L. C. Bianchi, M. L. Boyer, N. Caldwell, H. Dong, C. E. Dorman, K. M. Gilbert, L. Girardi, S. M. Gogarten, K. D. Gordon, P. Guhathakurta, P. W. Hodge, J. A. Holtzman, L. Johnson, S. S. Larsen, A. Lewis, J. L. Melbourne, K. A. G. Olsen, H. -W. Rix, K. Rosema, A. Saha, A. Sarajedini, E. D. Skillman, K. Z. Stanek
We report on initial fits to the structure of M31's disk, derived from the density of RGB stars, in a way that is independent of the assumed M/L and is robust to variations in dust extinction.
Cosmology and Nongalactic Astrophysics Solar and Stellar Astrophysics
1 code implementation • 19 Jun 2007 • S. Koposov, V. Belokurov, N. W. Evans, P. C. Hewett, M. J. Irwin, G. Gilmore, D. B. Zucker, H. -W. Rix, M. Fellhauer, E. F. Bell, E. V. Glushkova
We quantify the detectability of stellar Milky Way satellites in the Sloan Digital Sky Survey (SDSS) Data Release 5.
