J/AJ/165/224    Distance determinations for LAMOST DR8 K-giants   (Zhang+, 2023)

A Catalog of Distance Determinations for the LAMOST DR8 K-Giants in the Galactic Halo. Zhang L., Xue X.-X., Yang C., Wang F., Rix H.-W., Zhao G., Liu C. <Astron. J., 165, 224 (2023)> =2023AJ....165..224Z 2023AJ....165..224Z
ADC_Keywords: Milky Way; Stars, K-type; Stars, giant; Spectra, optical; Radial velocities; Effective temperatures Keywords: Distance measure ; Stellar distance ; K giant stars ; Milky Way stellar halo Abstract: We present a catalog of distances for 19544 K-giants drawn from Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) DR8. Most of them are located in the halo of the Milky Way up to ∼120kpc. There are 15% K-giants without Sloan Digital Sky Survey (SDSS) photometry, for which we supplements with Pan-STARRS1 (PS1) photometry calibrated to SDSS photometric system. The possible contamination of the red clumps/horizontal branch are removed according to metallicities and colors before the distance determination. Combining the LAMOST spectroscopic metallicities with the SDSS/PS1 photometry, we estimate the absolute magnitudes in the SDSS r-band, the distance moduli, and the corresponding uncertainties through an Bayesian approach devised by Xue et al. for the Sloan Extension for Galactic understanding and exploration halo K-giants. The typical distance precision is about 11%. The stars in the catalog lie in a region of 4-126kpc from the Galactic center, of which with 6320 stars beyond 20kpc and 273 stars beyond 50kpc, forming the largest spectroscopic sample of distant tracers in the Milky Way halo so far. Description: Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) is a quasimeridian reflecting Schmidt telescope with an effective aperture of 4m and 4000 optical fibers, from which numerous low-resolution (R∼1800) spectra covering a wavelength range of 3700<λ<9000Å of stars with r<19 can be obtained simultaneously at one exposure. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 219 19544 Catalog of 19544 K-giants selected from LAMOST DR8 -------------------------------------------------------------------------------- See also: I/337 : Gaia DR1 (Gaia Collaboration, 2016) VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006) V/146 : LAMOST DR1 catalogs (Luo+, 2015) V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020) J/ApJ/518/262 : CCD VIc Photometry of M30 Stars (Sandquist+, 1999) J/ApJ/684/1143 : BHB candidates in the Milky Way (Xue+, 2008) J/AJ/137/4377 : List of SEGUE plate pairs (Yanny+, 2009) J/other/RAA/11.924 : Atmospheric parameters for 771 stars (Wu+, 2011) J/ApJ/738/79 : SDSS-DR8 BHB stars in the Milky Way's halo (Xue+, 2011) J/ApJ/783/130 : Parallaxes of high mass star forming regions (Reid+, 2014) J/ApJ/784/170 : SEGUE K giant survey. II. Dist of 6036 stars (Xue+, 2014) J/ApJ/886/154 : Sgr stream K- & M-giants and BHB stars (Yang+, 2019) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 22 F22.18 deg RAdeg [0/360] Right Ascension (J2000) 24- 45 F22.19 deg DEdeg [-9/87] Declination (J2000) 47- 53 F7.4 mag rmag [12.8/18.1] Intrinsic, r-band magnitude 55- 60 F6.4 mag e_rmag [0.03/0.07] Uncertainty in rmag 62- 67 F6.4 mag (g-r) [0.52/1.41] Intrinsic (g-r) color 69- 74 F6.4 mag e_(g-r) [0.01/0.07] Uncertainty in (G-R) 76- 82 F7.2 km/s RVel [-495/452] Radial velocity 84- 88 F5.2 km/s e_RVel [1.65/88.9]? Uncertainty in RVel 90- 93 I4 K Teff [3812/5597] Effective temperature 95- 97 I3 K e_Teff [11/867]? Uncertainty in Teff 99-104 F6.3 [cm/s2] logg [-0.04/4] log surface gravity 106-110 F5.3 [cm/s2] e_logg [0.01/2]? Uncertainty in logg 112-117 F6.3 [Sun] [Fe/H] [-2.5/0.31] Metallicity 119-123 F5.3 [Sun] e_[Fe/H] [0.01/0.9]? Uncertainty in [Fe/H] 125-131 F7.4 mag DM5 [10/21] Distance modulus at the 5% confidence level 133-139 F7.4 mag DM16 [11/21] Distance modulus at the 16% confidence level 141-147 F7.4 mag DM50 [12/21] Distance modulus at the 50% confidence level 149-155 F7.4 mag DM84 [12/21] Distance modulus at the 84% confidence level 157-163 F7.4 mag DM95 [13/21] Distance modulus at the 95% confidence level 165-170 F6.4 mag e_DM50 [0.05/0.7] Uncertainty in DM50 172-178 F7.4 mag rMAG [-3.14/1.29] Absolute r band magnitude 180-185 F6.4 mag e_rMAG [0.06/0.7] Uncertainty in rMag 187-194 F8.4 kpc Dist [2.95/122] Distance 196-202 F7.4 kpc e_Dist [0.3/16] Uncertainty in Dist 204-211 F8.4 kpc rGC [3.79/126] Galactocentric distance 213-219 F7.4 kpc e_rGC [0.001/16] Uncertainty in rGC -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 03-Oct-2023
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line