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2017MNRAS.467.1890X - Mon. Not. R. Astron. Soc., 467, 1890-1914 (2017/May-2)

LAMOST Spectroscopic Survey of the Galactic Anticentre (LSS-GAC): the second release of value-added catalogues.

XIANG M.-S., LIU X.-W., YUAN H.-B., HUO Z.-Y., HUANG Y., WANG C., CHEN B.-Q., REN J.-J., ZHANG H.-W., TIAN Z.-J., YANG Y., SHI J.-R., ZHAO J.-K., LI J., ZHAO Y.-H., CUI X.-Q., LI G.-P., HOU Y.-H., ZHANG Y., ZHANG W., WANG J.-L., WU Y.-Z., CAO Z.-H., YAN H.-L., YAN T.-S., LUO A.-L., ZHANG H.-T., BAI Z.-R., YUAN H.-L., DONG Y.-Q., LEI Y.-J. and LI G.-W.

Abstract (from CDS):

We present the second release of value-added catalogues of the LAMOST Spectroscopic Survey of the Galactic Anticentre (LSS-GAC DR2). The catalogues present values of radial velocity Vr, atmospheric parameters - effective temperature Teff, surface gravity log g, metallicity [Fe/H], α-element to iron (metal) abundance ratio [α/Fe] ([α/M]), elemental abundances [C/H] and [N/H] and absolute magnitudes MV and MK s_ deduced from 1.8 million spectra of 1.4 million unique stars targeted by the LSS-GAC since 2011 September until 2014 June. The catalogues also give values of interstellar reddening, distance and orbital parameters determined with a variety of techniques, as well as proper motions and multiband photometry from the far-UV to the mid-IR collected from the literature and various surveys. Accuracies of radial velocities reach 5 km s–1 for the late-type stars, and those of distance estimates range between 10 and 30 per cent, depending on the spectral signal-to-noise ratios. Precisions of [Fe/H], [C/H] and [N/H] estimates reach 0.1 dex, and those of [α/Fe] and [α/M] reach 0.05 dex. The large number of stars, the contiguous sky coverage, the simple yet non-trivial target selection function and the robust estimates of stellar radial velocities and atmospheric parameters, distances and elemental abundances make the catalogues a valuable data set to study the structure and evolution of the Galaxy, especially the solar-neighbourhood and the outer disc.

Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): techniques: spectroscopic - Galaxy: abundance - Galaxy: disc - Galaxy: evolution - Galaxy: formation - Galaxy: formation

Simbad objects: 3

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