The Sloan Extension for Galactic Understanding and Exploration (SEGUE) Survey obtained ≈240,000 moderate-resolution (R ∼ 1800) spectra from 3900 Å to 9000 Å of fainter Milky Way stars (14.0 < g < 20.3) of a wide variety of spectral types, bot
We present a chemical abundance analysis of 300S-1, the brightest likely member star of the 300 km s...
We report high-resolution spectroscopy of 125 field stars previously observed as part of the Sloan D...
We report on efforts to identify large samples of very and extremely metal-poor stars based on mediu...
The Sloan Extension for Galactic Understanding and Exploration (SEGUE) Survey obtained ââ°Ë240,00...
The Sloan Extension for Galactic Understanding and Exploration (SEGUE) Survey obtained approximate t...
The Sloan Extension for Galactic Understanding and Exploration (SEGUE) Survey obtained ≈240,000 mode...
The authors report high-resolution spectroscopy of 125 field stars previously observed as part of th...
We propose an imaging and spectroscopic survey to unravel the structure, formation history, kinemati...
We describe the development and implementation of the Sloan Extension for Galactic Exploration and U...
We announce the discovery of a new Milky Way satellite Segue 2 found in the data of the Sloan Extens...
SDSS and its extensions use a dedicated 2.5m telescope to obtain ugriz imaging and resolution (defin...
We report on the development, calibration, and refinement of the SDSS-I Value Added Catalog (VAC) of...
Massive spectroscopic surveys of stars in the thick disk and halo populations of the Galaxy hold the...
We present an online catalog of distance determinations for 6036 K giants, most of which are members...
We investigate the kinematic and photometric properties of the Segue 3 Milky Way companion using Kec...
We present a chemical abundance analysis of 300S-1, the brightest likely member star of the 300 km s...
We report high-resolution spectroscopy of 125 field stars previously observed as part of the Sloan D...
We report on efforts to identify large samples of very and extremely metal-poor stars based on mediu...
The Sloan Extension for Galactic Understanding and Exploration (SEGUE) Survey obtained ââ°Ë240,00...
The Sloan Extension for Galactic Understanding and Exploration (SEGUE) Survey obtained approximate t...
The Sloan Extension for Galactic Understanding and Exploration (SEGUE) Survey obtained ≈240,000 mode...
The authors report high-resolution spectroscopy of 125 field stars previously observed as part of th...
We propose an imaging and spectroscopic survey to unravel the structure, formation history, kinemati...
We describe the development and implementation of the Sloan Extension for Galactic Exploration and U...
We announce the discovery of a new Milky Way satellite Segue 2 found in the data of the Sloan Extens...
SDSS and its extensions use a dedicated 2.5m telescope to obtain ugriz imaging and resolution (defin...
We report on the development, calibration, and refinement of the SDSS-I Value Added Catalog (VAC) of...
Massive spectroscopic surveys of stars in the thick disk and halo populations of the Galaxy hold the...
We present an online catalog of distance determinations for 6036 K giants, most of which are members...
We investigate the kinematic and photometric properties of the Segue 3 Milky Way companion using Kec...
We present a chemical abundance analysis of 300S-1, the brightest likely member star of the 300 km s...
We report high-resolution spectroscopy of 125 field stars previously observed as part of the Sloan D...
We report on efforts to identify large samples of very and extremely metal-poor stars based on mediu...