J/ApJS/244/8              M-type stars in LAMOST DR5              (Zhong+, 2019)

Value-added catalogs of M-type stars in LAMOST DR5. Zhong J., Li J., Carlin J.L., Chen L., Mendez R.A., Hou J. <Astrophys. J. Suppl. Ser., 244, 8-8 (2019)> =2019ApJS..244....8Z 2019ApJS..244....8Z (SIMBAD/NED BibCode)
ADC_Keywords: Stars, M-type; Spectra, optical; Photometry, infrared; Stars, giant; Stars, dwarfs Keywords: catalogs; stars: carbon; stars: late-type; surveys Abstract: We present new catalogs of M giant and M dwarf stars from the Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) data release 5 (DR5). In total, 39796 M giants and 501152 M dwarfs are identified from the classification pipeline. The template-fitting results contain M giants with 7 temperature subtypes from M0 to M6, M dwarfs with 18 temperature subtypes from K7.0 to M8.5, and 12 metallicity subclasses from dMr to usdMp. We cross-matched our M-type catalog with the Two Micron All-Sky Survey (2MASS) and Wide-field Infrared Survey Explorer (WISE) catalog to obtain infrared magnitude and colors. Adopting the distances derived from the parallaxes in Gaia DR2, the MG versus (Gbp-Grp)0 diagram shows that there are also early-type stars and white dwarf-M dwarf binaries included in our M-type stars sample, with a contamination rate of about 4.6% for M giants and 0.48% for M dwarfs. We found that CaH spectral indices are an efficient selection criteria for carbon stars. A total of 289 carbon stars were identified from the M giants sample, and further confirmed by LAMOST spectra. Description: As the most efficient spectroscopic survey telescope, the LAMOST, also known as the Guo Shou Jing Telescope, has finished the first stage of its regular survey (LAMOST-I; 2011-2017; including the pilot survey), and provided 9,017,844 low-resolution (R∼1800) optical spectra in its fifth data release, of which 8,171,443 are stellar spectra. In this work we have adopted the template-fitting pipeline of Li+ 2016, J/ApJ/823/59 combined with a classification algorithm (Zhong+ 2015, J/AJ/150/42) and revised M-type spectral templates (Zhong+ 2015, J/other/RAA/15.1154) to identify and classify M-type stars from LAMOST DR5. After excluding outlier spectra and combining duplicated spectra, a total of 540,948 spectra were identified as M-type stars, including 39,796 M giant spectra and 501,152 M dwarf spectra. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 197 540948 The M giant and M dwarf catalog -------------------------------------------------------------------------------- See also: III/198 : Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+, 2003) II/328 : AllWISE Data Release (Cutri+, 2013) I/345 : Gaia DR2 (Gaia, 2018) I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018) V/153 : LAMOST DR4 catalogs (Luo+, 2018) V/164 : LAMOST DR5 catalogs (Luo+, 2019) J/AJ/128/1177 : Galactic stellar abundances (Venn+, 2004) J/ApJ/670/346 : M giant stars in the Sagittarius dwarf galaxy. V. (Chou+, 2007) J/ApJ/783/130 : Parallaxes of high mass star forming regions (Reid+, 2014) J/AJ/147/76 : Photometry of M giant cand. in the Milky Way (Bochanski+, 2014) J/AJ/150/42 : Catalog of 2612 M dwarfs from LAMOST (Zhong+, 2015) J/other/RAA/15.1154 : M-giant star candidates in LAMOST DR 1 (Zhong+, 2015) J/other/RAA/15.1182 : M Dwarf catalog of LAMOST DR1 (Guo+, 2015) J/other/RAA/15.1671 : New carbon stars from LAMOST survey (Si+, 2015) J/ApJ/823/59 : WISE and 2MASS photometry of M giant stars (Li+, 2016) J/ApJS/226/1 : Carbon stars from LAMOST DR2 data (Ji+, 2016) J/ApJS/234/31 : Carbon stars from LAMOST using machine learning (Li+, 2018) J/A+A/616/A10 : 46 open clusters GaiaDR2 HR diagrams (Gaia Collaboration, 2018) J/ApJS/240/31 : M-subdwarf research. I. LAMOST DR4 spectra obs. (Zhang+, 2019) J/ApJS/243/28 : M-type star magnetic activities from LAMOST+Kepler (Lu+, 2019) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- OT M type: G=Giant (39796 stars) or D=Dwarf (501152 stars) 3- 21 A19 --- Name LAMOST DR5 identifier (JHHMMSS.ss+DDMMSS.s) 23- 32 F10.6 deg RAdeg Right Ascension in decimal degrees (J2000) 34- 42 F9.6 deg DEdeg Declination in decimal degrees (J2000) 44- 48 F5.3 --- CaH2 [0.02/1.6] LAMOST CaH2 spectral index 50- 54 F5.3 --- CaH3 [0.3/1.754] LAMOST CaH3 spectral index 56- 60 F5.3 --- TiO5 [0.002/1.2] LAMOST TiO5 spectral index 62- 66 F5.1 --- SNR [0/999] SNR of i filter in LAMOST spectrum 68- 75 A8 --- SpT Spectral subtype classified by the template-fitting algorithm 77- 82 F6.3 mag Gmag [5/21.3]? Gaia DR2 dereddened G band magnitude 84- 89 F6.3 mag GBPmag [5/21]? Gaia DR2 dereddened Blue Passband magnitude 91- 96 F6.3 mag GRPmag [3.9/20]? Gaia DR2 dereddened Red Passband magnitude 98-103 F6.3 mag Jmag [1.6/17.4]? 2MASS dereddened J band magnitude 105-110 F6.3 mag Hmag [0.7/17]? 2MASS dereddened H band magnitude 112-117 F6.3 mag Ksmag [0.4/17.4]? 2MASS dereddened Ks band magnitude 119-124 F6.3 mag W1mag [-2.1/17.5]? WISE dereddened 3.4um band magnitude 126-131 F6.3 mag W2mag [-1.1/17.5]? WISE dereddened 4.6um band magnitude 133-136 F4.2 mag E(B-V) [0/3.1]? 3D dust mapped reddening 138-142 I5 pc Dist [10/18024]? Gaia DR2 parallax distance 144-149 I6 km/s RVel [-30417/30537]? LAMOST radial velocity 151-156 F6.1 [Sun] [M/H] [-590/0.2]? M giant estimated photometric metallicity 158-162 I5 pc X [-1950/441]? Galactocentric X coordinate (to the direction opposite to that of the Sun) 164-168 I5 pc Y [-7150/17205]? Galactocentric Y coordinate (to the direction of Galactic rotation) 170-174 I5 pc Z [-6521/12835]? Galactocentric Z coordinate (toward the North Galactic Pole) 176-181 I6 km/s U [-27840/29401]? Galactic space velocity along X 183-188 I6 km/s V [-32272/30745]? Galactic space velocity along V 190-195 I6 km/s W [-30652/31108]? Galactic space velocity along W 197 A1 --- Cl Subsample label (1) -------------------------------------------------------------------------------- Note (1): Subsample label as follows: m = confirmed M type star (505519 occurrences); n = non-M type star (3921 occurrences); c = carbon star (289 occurrences); w = white dwarf binary (72 occurrences); u = unconfirmed M type star due to lack of Gaia data (31147 occurrences). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 11-Feb-2020
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