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19 April 2024
 
  » arxiv » 1411.0235

 Article overview


Asteroseismic based estimation of the surface gravity for the LAMOST giant stars
Chao Liu ; Min Fang ; Yue Wu ; Li-Cai Deng ; Liang Wang ; Wei Wang ; Jian-Ning Fu ; Yong-Hui Hou ; Guang-Wei Li ; Yong Zhang ;
Date 2 Nov 2014
AbstractAsteroseismology is one of the most accurate approaches to estimate the surface gravity of a star. However, most of the data from the current spectroscopic surveys do not have asteroseismic measurements, which is very expensive and time consuming. In order to improve the spectroscopic surface gravity estimates for a large amount of survey data with the help of the small subset of the data with seismic measurements, we set up a support vector regression model for the estimation of the surface gravity supervised by more than 3000 LAMOST giant stars with Kepler measured seismic surface gravity. The new approach can reduce the uncertainty of the estimates down to about 0.1 dex, which is better than other non-seismic methods by at least a factor of 2, for the spectra with signal-to-noise ratio higher than 20. Compared with the logg estimated from the LAMOST pipeline, not only the systematic overestimation for the RGB stars has been corrected, but also the artificial effect around the red clump stars disappears. Moreover, even the red bump stars, which extend to only about 0.1dex in logg, can be discriminated from the new estimated surface gravity. The method is then applied to about 380,000 LAMOST metal-rich giant stars to provide improved surface gravity estimates. In general, it can be applied to any other spectroscopic survey data with proper cross-calibration to the LAMOST.
Source arXiv, 1411.0235
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