J/A+A/614/A76       CARMENES input catalogue of M dwarfs. III.  (Jeffers+, 2018)
CARMENES input catalogue of M dwarfs.
III. Rotation and activity from high-resolution spectroscopic observations.
    Jeffers S.V., Schofer P., Lamert A., Reiners A., Montes D., Caballero J.A.,
    Cortes-Contreras M., Marvin C.J., Passegger V.M., Zechmeister M.,
    Quirrenbach A., Alonso-floriano F.J., Amado P.J., Bauer F.F., Casal E.,
    Diez Alonso E., Herrero E., Morales J.C., Mundt R., Ribas I.,
    Sarmiento L.F.
   <Astron. Astrophys., 614, A76-76 (2018)>
   =2018A&A...614A..76J 2018A&A...614A..76J    (SIMBAD/NED BibCode)
ADC_Keywords: Stars, standard ; Stars, dwarfs ; Stars, M-type ;
              Stars, late-type ; Stars, double and multiple ;
              Radial velocities ; Rotational velocities ; Equivalent widths
Keywords: stars: activity - stars: rotation - techniques: spectroscopic -
          catalogs
Abstract:
    CARMENES is a spectrograph for radial velocity surveys of M dwarfs
    with the aim of detecting Earth-mass planets orbiting in the habitable
    zones of their host stars. To ensure an optimal use of the CARMENES
    guaranteed time observations, in this paper we investigate the
    correlation of activity and rotation for approximately 2200 M dwarfs,
    ranging in spectral type from M0.0 V to M9.0 V. We present new
    high-resolution spectroscopic observations with FEROS, CAFE, and HRS
    of approximately 500 M dwarfs. For each new observation, we determined
    its radial velocity and measured its Hα activity index and its
    rotation velocity. Additionally, we have multiple observations of many
    stars to investigate if there are any radial velocity variations due
    to multiplicity. The results of our survey confirm that early-M dwarfs
    are Hα inactive with low rotational velocities and that late-M
    dwarfs are Hα active with very high rotational velocities. The
    results of this high-resolution analysis comprise the most extensive
    catalogue of rotation and activity in M dwarfs currently available.
Description:
    Based on observations made at the Calar Alto Observatory, Spain, the
    European Southern Observatory, La Silla, Chile and McDonald
    Observatory, USA.
File Summary:
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 FileName      Lrecl  Records   Explanations
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ReadMe            80        .   This file
tablea1.dat       85     1377   Journal of new high-resolution spectroscopic
                                 observations of Carmencita stars
tablea2.dat       58      408   Observations with CAFE and FEROS
tablea3.dat       79     2133   The full Carmencita catalogue
refs.dat          79       53   References
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See also:
 J/A+A/577/A128 : CARMENES input catalog of M dwarfs I (Alonso-Floriano+, 2015)
 J/A+A/597/A47  : CARMENES input catalog of M dwarfs II (Cortes-Contreras+ 2017)
Byte-by-byte Description of file: tablea1.dat
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   Bytes Format Units         Label     Explanations
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   1- 11  A11   ---           Karmn     Carmencita identifier (G1)
  14- 15  I2    h             RAh       Right ascension (J2000)
  17- 18  I2    min           RAm       Right ascension (J2000)
  20- 24  F5.2  s             RAs       Right ascension (J2000)
      26  A1    ---           DE-       Declination sign (J2000)
  27- 28  I2    deg           DEd       Declination (J2000)
  30- 31  I2    arcmin        DEm       Declination (J2000)
  33- 36  F4.1  arcsec        DEs       Declination (J2000)
  38- 42  A5    ---           Inst      Used instrument
  44- 53  A10   "YYYY-MM-DD"  Obs.date  Observing night (from noon to noon)
  55- 62  A8    "h:m:s"       Obs.time  UT of mid-point of observation
  64- 67  I4    s             ExTime    Exposure time
  69- 75  F7.2  km/s          RV        Radial velocity
  77- 81  F5.2  km/s        e_RV        Radial velocity error
  83- 85  I3    ---           S/N       Signal-to-noise ratio of the
                                         corresponding spectrum
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Byte-by-byte Description of file: tablea2.dat
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   Bytes Format Units   Label     Explanations
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   1- 11  A11   ---     Karmn     Carmencita identifier (G1)
  13- 32  A20   ---     Name      Alternative name
  34- 36  F3.1  ---     SpType    Spectral Type (M V)
  38- 42  A5    0.1nm   pEWHa     Halpha pseudo-equivalent width
  44- 46  F3.1  0.1nm e_pEWHa     Error of Halpha pseudo-equivalent width
  48- 52  A5    km/s    vsini     Rotational velocity
  54- 58  A5    ---     Inst      Used instrument
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Byte-by-byte Description of file: tablea3.dat
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   Bytes Format Units   Label     Explanations
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   1- 11  A11   ---     Karmn     Carmencita identifier (G1)
  13- 35  A23   ---     Name      Alternative name
  37- 39  F3.1  ---     SpType    Spectral Type (M V)
  41- 47  F7.3  0.1nm   pEWHa     ? Halpha pseudo-equivalent width
  49- 53  F5.3  0.1nm e_pEWHa     ? Error of Halpha pseudo-equivalent width
  55- 56  A2    ---   r_pEWHa     Reference for pseudo-equivalent width,
                                     in refs.dat file
      59  A1    ---   l_vsini     Limit flag on vsini
  60- 65  F6.2  km/s    vsini     ? Rotational velocity
  66- 70  F5.2  km/s  e_vsini     ? Error of rotational velocity
  72- 73  A2    ---   r_vsini     Reference for rotational velocity,
                                     in refs.dat file
  75- 79  F5.2  [-]     logRHK    ? log R'HK activity index
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Byte-by-byte Description of file: refs.dat
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   Bytes Format Units   Label     Explanations
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   1-  2  A2    ---     Ref       Reference code
   4- 22  A19   ---     BibCode   BibCode
  24- 41  A18   ---     Aut       Author's name
  45- 79  A35   ---     Com       Comments
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Global notes:
Note (G1): Carmencita identifier (Quirrenbach et al. 2015, 18th Cambridge
     Workshop on Cool Stars, Stellar Systems, and the Sun, 18, 897;
     Alonso-Floriano et al., Cat. J/A+A/577/A128).
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Acknowledgements:
    Sandra Jeffers, jeffers(at)astro.physik.uni-goettingen.de
(End)                                      Patricia Vannier [CDS]    05-Mar-2019