The LEGUE Input Catalogue for Dark Night Observing in the LAMOST Pilot Survey
arXiv:1206.3576 · doi:10.1088/1674-4527/12/7/006
Abstract
We outline the design of the dark nights portion of the LAMOST Pilot Survey, which began observations in October 2011. In particular, we focus on Milky Way stellar candidates that are targeted for the LEGUE (LAMOST Experiment for Galactic Understanding and Exploration) survey. We discuss the regions of sky in which spectroscopic candidates were selected, and the motivations for selecting each of these sky areas. Some limitations due to the unique design of the telescope are discussed, including the requirement that a bright (V < 8) star be placed at the center of each plate for wavefront sensing and active optics corrections. The target selection categories and scientific goals motivating them are briefly discussed, followed by a detailed overview of how these selection functions were realized. We illustrate the difference between the overall input catalog - Sloan Digital Sky Survey (SDSS) photometry - and the final targets selected for LAMOST observation.
11 pages, 7 figures, accepted for publication in RAA
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Cited by in corpus (11)
- The First Data Release (DR1) of the LAMOST general survey
- LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) The survey science plan
- LAMOST Spectroscopic Survey of the Galactic Anti-centre (LSS-GAC): target selection and the first release of value-added catalogues
- Hot Subdwarf Stars Observed in LAMOST DR1 - Atmospheric parameters from single-lined spectra
- Hot subdwarf stars observed in Gaia DR2 and LAMOST DR5
- An Algorithm for Preferential Selection of Spectroscopic Targets in LEGUE
- The selection of LEGUE disk targets for LAMOST's pilot survey
- The site conditions of the Guo Shou Jing Telescope
- The LEGUE High Latitude Bright Survey Design for the LAMOST Pilot Survey
- Hydrogen lines in LAMOST low resolution spectra of RR Lyrae stars
- Fixing the Reference Frame for PPMXL Proper Motions Using Extragalactic Sources