1 code implementation • 15 Jul 2015 • Teresa Antoja, Cecilia Mateu, Luis Aguilar, Francesca Figueras, Erika Antiche, Fabiola Hernandez-Perez, Anthony Brown, Octavio Valenzuela, Antonio Aparicio, Sebastian Hidalgo, Hector Velazquez
We characterize the detection limits as function of the number of observable stars by Gaia in the UFDGs with respect to that of the background and their apparent sizes in the sky and proper motion planes.
Astrophysics of Galaxies
