/ftp/cats/aliases/G/./GGSS_2_



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J/AJ/140/1911       Astrometric Grid Giant Star Survey. II.  (Bizyaev+, 2010)
The following files can be converted to FITS (extension .fit or fit.gz)
	table3.dat table1.dat table2.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/AJ/140/1911
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drwxr-xr-x 52 cats archive 4096 Mar 4 2016 [Up] drwxr-xr-x 4 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 487 Dec 19 2022 .message -r--r--r-- 1 cats archive 5584 Jun 5 2015 ReadMe -rw-r--r-- 1 cats archive 859 Apr 28 2016 +footg5.gif -rw-r--r-- 1 cats archive 6835 Apr 28 2016 +footg8.gif -r--r--r-- 1 cats archive 7520 Jul 13 2012 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2411 Jul 13 2012 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 65598 Dec 7 2012 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/AJ/140/1911 Astrometric Grid Giant Star Survey. III. (Bizyaev+, 2010) ================================================================================ The Space Interferometry Mission Astrometric Grid Giant Star Survey. III. Basic stellar parameters for an extended sample. Bizyaev D., Smith V.V., Cunha K. <Astron. J., 140, 1911-1918 (2010)> =2010AJ....140.1911B ================================================================================ ADC_Keywords: Stars, late-type ; Spectroscopy ; Radial velocities; Abundances, [Fe/H] Keywords: stars: abundances - stars: atmospheres - stars: fundamental parameters - stars: late-type - stars: rotation Abstract: We present results of high-resolution ( 55000) spectral observations of 830 photometrically pre-selected candidate red giants in the magnitude range of V=9-12. We develop a pipeline for automated determination of the stellar atmospheric parameters from these spectra and estimate Teff, logg, [Fe/H], microturbulence velocity, and projected rotational velocities, vsin i, for the stars. The analysis confirms that the candidate selection procedure yielded red giants with very high success rate. We show that most of these stars are G and K giants with slightly subsolar metallicity ([Fe/H] -0.3dex). An analysis of Mg abundances in the sample results in consistency of the [Mg/Fe] vs [Fe/H] trend with published results. Description: Observations were conducted using the 2.1m telescope at the McDonald Observatory and the Sandiford Cassegrain echelle spectrograph, which provides a nominal resolution R=55000.