J/AJ/144/114         Radial velocities of 6 field RR Lyrae        (Sesar+, 2012)
Template RR Lyrae Hα, Hβ, and Hγ velocity curves.
    Sesar B.
   <Astron. J., 144, 114 (2012)>
   =2012AJ....144..114S 2012AJ....144..114S
ADC_Keywords: Stars, variable ; Radial velocities
Keywords: stars: horizontal-branch - stars: Population II
          stars: variables: RR Lyrae - techniques: radial velocities
Abstract:
    We present template radial velocity curves of ab-type RR Lyrae stars
    constructed from high-precision measurements of Hα, Hβ, and
    Hγ lines. Amplitude correlations between the Balmer line
    velocity curves, Johnson V band, and Sloan Digital Sky Survey (SDSS)
    g- and r-band light curves are also derived. Compared to previous
    methods, these templates and derived correlations reduce the
    uncertainty in measured systemic (center-of-mass) velocities of RR
    Lyrae stars by up to 15km/s, and will be of particular interest to
    wide-area spectroscopic surveys such as the SDSS and LAMOST Experiment
    for Galactic Understanding and Exploration.
Description:
    The six field RR Lyrae type ab stars (Z Mic, CD Vel, WY Ant, DT Hya,
    XZ Aps, and RV Oct) were observed between 2006 and 2009 by George W.
    Preston with the echelle spectrograph of the du Pont 2.5m telescope at
    the Las Campanas Observatory. The stars have V-band light-curve
    amplitudes (AV) ranging from 0.64mag (Z Mic) to 1.13mag (RV Oct), as
    measured by the All Sky Automated Survey (ASAS). The observations are
    described in detail in For et al. (2011, cat. J/ApJS/194/38).
File Summary:
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 FileName    Lrecl   Records    Explanations
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ReadMe          80         .    This file
table1.dat      71         6    ASAS RR Lyrae stars
velocity.dat    21      1925    Hα, Hβ, Hγ, and metallic
                                radial velocities template
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See also:
 J/ApJS/194/38    : Radial velocities of 11 field RR Lyrae (For+, 2011)
 J/ApJ/708/717    : Light curve templates of RR Lyrae stars (Sesar+, 2010)
 J/MNRAS/377/1263 : Multiperiodic RR Lyrae in ASAS catalog (Szczygiel+, 2007)
 J/A+AS/125/321   : RR Lyrae radial velocities and [Fe/H] II. (Solano+ 1997)
 J/A+AS/113/483   : Photometric and RV of RRLyr stars (Carrillo+, 1997)
 J/AJ/108/1016    : Kinematics of local RR lyrae stars. I. (Layden, 1994)
Byte-by-byte Description of file: table1.dat
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   Bytes Format Units   Label    Explanations
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   1-  6  A6    ---     Name     Name of the ab-type RR Lyrae star
   8-  9  I2    h       RAh      Hour of Right Ascension (J2000)
  11- 12  I2    min     RAm      Minute of Right Ascension (J2000)
  14- 18  F5.2  s       RAs      Second of Right Ascension (J2000)
      20  A1    ---     DE-      Sign of the Declination (J2000)
  21- 22  I2    deg     DEd      Degree of Declination (J2000)
  24- 25  I2    arcmin  DEm      Arcminute of Declination (J2000)
  27- 30  F4.1  arcsec  DEs      Arcsecond of Declination (J2000)
  32- 35  F4.2  mag     Vamp     V-band light-curve amplitude (from ASAS)
  37- 41  F5.2  mag     Vmax     Maximum light in the V band from ASAS
  43- 45  A3    ---     Bl       [Yes No] Blazhko effect in the light curve? (1)
  47- 49  I3    ---     N        [96/241] Number of observations
  51- 54  F4.1  km/s    DRV1     Best-fit metallic radial velocity amplitude
  56- 60  F5.1  km/s    DRV2     Best-fit Hα radial velocity amplitude
  62- 66  F5.1  km/s    DRV3     Best-fit Hβ radial velocity amplitude
  68- 71  F4.1  km/s    DRV4     Best-fit Hγ radial velocity amplitude
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Note (1): Blazkhko RR Lyrae stars according to Szczygiel & Fabrycky (2007,
          cat. J/MNRAS/377/1263).
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Byte-by-byte Description of file: velocity.dat
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   Bytes Format Units   Label     Explanations
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   1-  8  A8    ---     Line      Line identification (Hα, Hβ,
                                   Hγ, or metallic)
  10- 14  F5.3  ---     Phase     [0/1] Phase (1)
  16- 21  F6.3  km/s    RV        [-0.748/0.408] Normalized radial velocity
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Note (1): Calculated using periods and epochs of maximum light listed in
     table 5 of For et al. (2011, cat. J/ApJS/194/38), with the time of
     maximum light corresponding to phase of zero.
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History:
    From electronic version of the journal
(End)                                    Sylvain Guehenneux [CDS]    21-Jan-2014