Mapping the Galactic Halo. I. The “Spaghetti” Survey
We describe a major survey of the Milky Way halo designed to test for kinematic substructure caused by destruction of accreted satellites. We use the Washington photometric syst...
We describe a major survey of the Milky Way halo designed to test for kinematic substructure caused by destruction of accreted satellites. We use the Washington photometric syst...
We describe the development and implementation of the Sloan Extension for Galactic Exploration and Understanding (SEGUE) Stellar Parameter Pipeline (SSPP). The SSPP is derived, ...
We validate the accuracy and precision of the current SEGUE (Sloan Extension for Galactic Understanding and Exploration) Stellar Parameter Pipeline (SSPP), which determines stel...
We present techniques for the estimation of stellar atmospheric parameters (Teff, log g, [Fe/H]) for stars from the SDSS/SEGUE survey. The atmospheric parameters are derived fro...
h-index: Number of publications with at least h citations each.