J/A+A/660/A38       Ultracool dwarfs with spectra in LAMOST DR7    (Wang+, 2022)
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Ultracool dwarfs identified with spectra in LAMOST DR7.
    Wang Y.-F., Luo A-L., Chen W.-P., Jones H.R.A., Du B., Li Y.-B., Zhang S.,
    Bai Z.-R., Kong X., Guo Y.-X.
    <Astron. Astrophys. 660, A38 (2022)>
    =2022A&A...660A..38W        (SIMBAD/NED BibCode)
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ADC_Keywords: Surveys ; Stars, dwarfs ; Stars, late-type ; Spectroscopy ;
              Optical
Keywords: surveys - stars: low-mass - brown dwarfs - binaries: visual -
          stars: late-type

Abstract:
    We identify 734 ultracool dwarfs having spectral type M6 or later
    including one L0, of which, 625 are having spectral observation for
    the first time with LAMOST. All these ultracool dwarfs are within 360
    pc, with the Gaia G magnitude brighter than ~19.2mag. Studying the
    spectra and checking their stellar parameters (Teff, logg and
    [M/H]) derived with the LAMOST pipeline, we found their cool red
    nature and their metallicity consistent with being Galaxy thin disk
    objects. Furthermore, 77 of them show lithium absorption line at
    6708{AA} indicating their young ages and substellar nature. Kinematics
    obtained through LAMOST radial velocities combining with the proper
    motion and parallax from Gaia EDR3, also suggest the majority of our
    targets are thin disk objects. Kinematic ages are estimated through
    the relationship between the velocity dispersion and the average age
    for a certain population. Moreover, 35 binaries are identified, among
    which 6 are reported as binaries for the first time.

Description:
    734 late-type M dwarfs identified visually from LAMOST DR7 are
    presented in Table 1. The atmospheric parameters(Teff, Logg, and M/H),
    radial velocity and signal to noise in SDSS i and z band, and radial
    velocity from LAMOST DR7 are presented in Table 2. We also listed the
    flag of the lithium strength in Table 2. In Table 3, we list the
    kinematic parameters calculated for 571 objects of our ultracool dwarf
    sample with radial velocity from LAMOST DR7, and photometry and
    astrometric from Gaia EDR3.

File Summary:
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 FileName     Lrecl  Records   Explanations
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ReadMe           80        .   This file
table1.dat      173      734   The ultracool dwarfs
table2.dat      102      734   Radial velocity and atmosphere parameters in LDR7
table3.dat      155      571   Kinematic parameters
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See also:
    I/350 : Gaia EDR3 (Gaia Collaboration, 2020)

    http://dr7.lamost.org : LAMOST DR7 Home Page

Byte-by-byte Description of file: table1.dat
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   Bytes Format Units     Label     Explanations
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   1-  5  I5    ---       Seq       [1/734] Running number
   6- 15  A10   ---       obsid     LAMOST obsid
  16- 27  F12.5 deg       RAdeg     Right ascension (J2000.0)
  28- 39  F12.5 deg       DEdeg     Declination (J2000.0)
  40- 44  A5    ---       SpType1   Spectral type from LAMOST DR7
  45- 64  A20   ---       GaiaEDR3  Gaia EDR3 source_id
  65- 74  F10.2 mas       plx       ?=-9999.99 parallax from Gaia EDR3
  75- 84  F10.2 mas     e_plx       ?=-9999.99 uncertainty of parallax
                                     from Gaia EDR3
  85- 94  F10.2 mas/yr    pmRA      ?=-9999.99 Proper motion in RA direction,
                                     pmRA*cosDE, from Gaia EDR3
  95-104  F10.2 mas/yr  e_pmRA      ?=-9999.99 Uncertainty of proper motion in
                                     RA direction
                                     from Gaia EDR3
 105-114  F10.2 mas/yr    pmDE      ?=-9999.99 Proper motion in Dec direction
                                     from Gaia EDR3
 115-124  F10.2 mas/yr  e_pmDE      ?=-9999.99 Uncertainty of proper motion
                                     in Dec direction from Gaia EDR3
 125-134  F10.3 ---       RUWE      ?=-9999.99 RUWE from Gaia EDR3
 139-144  F6.3  mag       Gmag      G band magnitude from Gaia EDR3
 145-154  F10.3 mag       BPmag     ?=-9999.99 BP band magnitude from Gaia EDR3
 155-164  F10.3 mag       RPmag     ?=-9999.99 RP band magnitude from Gaia EDR3
 165-173  A9    ---       SpType2   Spectral type from the literature (SIMBAD)
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Byte-by-byte Description of file: table2.dat
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   Bytes Format Units     Label    Explanations
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   1-  3  I3    ---       Seq      [1/734] Running number
   6- 14  F9.5  deg       RAdeg    Right ascension (J2000.0)
  18- 26  F9.5  deg       DEdeg    Declination (J2000.0)
  27- 34  F8.2  km/s      RV       ?=-9999 Radial velocity from LAMOST DR7
  36- 40  I5    K         Teff     ?=-9999 Effective temperature from LAMOST DR7
  42- 46  I5    K       e_Teff     ?=-9999 Uncertainty of effective temperature
                                    from LAMOST DR7
  49- 56  F8.2  [cm/s2]   logg     ?=-9999.99 Surface gravity from LAMOST DR7
  59- 66  F8.2  [cm/s2] e_logg     ?=-9999.99 Uncertainty of surface gravity
                                    from LMAOST DR7
  69- 76  F8.2  [-]       MH       ?=-9999.99 Metallicity  from LAMOST DR7
  79- 86  F8.2  [-]     e_MH       ?=-9999.99 Uncertainty of metallicity
                                    from LAMOST DR7
      90  A1    ---       Li       [HMLN] Flag of the lithium strength (1)
  94- 96  I3    ---       SNRi     Signal to noise ratio in SDSS i band
                                    from LAMOST DR7
  98-102  I5    ---       SNRz     Signal to noise ratio in SDSS z band
                                    from LAMOST DR7
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Note (1): Flag of the lithium strength as follows:
           H = strong
           M = medium
           L = weak
           N = no
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Byte-by-byte Description of file: table3.dat
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   Bytes Format Units   Label     Explanations
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   1-  3  I3    ---     Seq       [1/733] Running number
   5- 13  F9.5  deg     RAdeg     Right ascension (J2000.0)
  17- 25  F9.5  deg     DEdeg     Declination (J2000.0)
  27- 33  F7.2  km/s    U         Galactic U velocity
  36- 39  F4.2  km/s  E_U         Upper uncertainty of Galactic U velocity
  43- 46  F4.2  km/s  e_U         Lower uncertainty of Galactic U velocity
  48- 54  F7.2  km/s    V         Galactic V velocity
  57- 60  F4.2  km/s  E_V         Upper uncertainty of Galactic V velocity
  64- 67  F4.2  km/s  e_V         Lower uncertainty of Galactic V velocity
  69- 75  F7.2  km/s    W         Galactic W velocity
  77- 81  F5.2  km/s  E_W         Upper uncertainty of Galactic W velocity
  84- 88  F5.2  km/s  e_W         Lower uncertainty of Galactic W velocity
  90- 96  F7.2  pc      zgal      Galactic height
  98-102  F5.2  pc    E_zgal      Upper uncertainty of Galactic height
 105-109  F5.2  pc    e_zgal      Lower uncertainty of Galactic height
 115-121  F7.2  pc      rgal      Distance to the Galactic center on the
                                   Galactic plane
 124-128  F5.2  pc    E_rgal      Upper uncertainty of distance to the
                                   Galactic center on the Galactic plane
 131-135  F5.2  pc    e_rgal      Lower uncertainty of distance to the
                                   Galactic center on the Galactic plane
 138-145  F8.2  ---     TDD       ?=-9999.99 probability ratio of thick disk
                                   over disk
 151-155  I5    ---     TDH       ?=-9999 probability ratio of thick disk
                                   over halo
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Acknowledgements:
    Ali Luo, lal(at)bao.ac.cn

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(End)   Ali Luo [NAOC, China], Patricia Vannier [CDS]                28-Mar-2022
