VizieR Online Data Catalog: Stellar groups in Taurus field from Gaia DR2 & LAMOST (Liu+, 2021)
Abstract
In order to fully explore the Taurus region, we use a large searching area: 55°<=RA<=90° and 10°<=DEC<=35°.
The spectroscopic data used in this work are taken from the Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) DR5. LAMOST is a 4m Schmidt telescope of the National Astronomical Observatories of China, located at Xinglong Observing Station, China. In this work, we use the LAMOST DR5 data set. In order to construct the spectral energy distribution of each source and estimate its extinction, we used optical photometry in the g, r, i, z, and y bands from Pan-STARRS (Cat. II/349) and G, GBP, and GRP bands from Gaia DR2 (Cat. I/345), near-infrared photometry in the J, H, and KS bands from the Two-Micron All Sky Survey (2MASS; see Cat. II/246), and near- and mid-infrared photometry in the W1 (3.4um), W2 (4.6um), W3 (12um), and W4 (22um) bands from the WISE (see Cat. II/311) all-sky survey. (2 data files).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- August 2021
- DOI:
- 10.26093/cds/vizier.22540020
- Bibcode:
- 2021yCat..22540020L
- Keywords:
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- Associations: stellar;
- Stars: distances;
- Spectral types;
- YSOs;
- Star Forming Region