J/AJ/164/45   grV light curve for 30 RR-Lyrae in the Kepler field  (Ngeow, 2022)
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Evaluating the V-band Photometric Metallicity with Fundamental Mode RR Lyrae in
the Kepler Field.
    Ngeow C.-C.
   <Astron. J., 164, 45 (2022)>
   =2022AJ....164...45N
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ADC_Keywords: Stars, variable; Photometry, G band; Photometry, VRI
Keywords: RR Lyrae variable stars ; Metallicity ; Light curves

Abstract:
    The aim of this work is to evaluate the performance of photometric
    metallicity [Fe/H], determined based on V-band light curves
    photometrically transformed from the gr-band light curves. We tested
    this by using a set of homogeneous samples of fundamental mode
    RR-Lyrae located in the Kepler field. It was found that the color term
    is necessary in such photometric transformation. We demonstrated that
    when including the color term the determined photometric [Fe/H] are in
    good agreement with the spectroscopic [Fe/H], either based on the
    calibrated or the transformed V-band light curves. We also tested the
    impact of Blazhko RR-Lyrae in determining the photometric [Fe/H], and
    found that Blazhko RR-Lyrae can give consistent photometric [Fe/H].
    Finally, we derived independent gVr-band [Fe/H]-ph31-P relations
    (where ph31 and P are the Fourier parameter and pulsation period,
    respectively) using our light curves. The V-band relation is in good
    agreement with the most recent determination given in the literature.

Description:
    Time-series observations of the 30 targeted RR-Lyrae in the Kepler
    field were carried out using the 0.41m SLT telescope located at Lulin
    Observatory. This telescope is an f/8.4 Ritchey-Chretien telescope and
    is equipped with an Andor iKon-L936 CCD camera, providing a pixel
    scale of 0.79"/pixel. Queue observations were executed, via commercial
    software MaxIm DL and ACP Observatory Control Software, from 2019 June
    18 to 2021 November 24 (weather permitting) in gVr filters. Depending
    on the brightness of the targeted RR Lyrae, exposure time varied
    between 2 to 300s in all filters.

File Summary:
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 FileName    Lrecl  Records  Explanations
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ReadMe          80        .  This file
targets.dat     19       30  Targets for this work
table1.dat     104     4012  grV-band calibrated light-curves for 30 ab-type
                              RR Lyrae in the Kepler Field
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See also:
 V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)
 J/A+AS/105/145 : RR Lyr stars of ome Cen (Petersen 1994)
 J/A+A/312/111  : [Fe/H] from RR Lyrae light curves (Jurcsik+, 1996)
 J/MNRAS/398/1757 : RR Lyraes in SDSS stripe 82 (Watkins+, 2009)
 J/ApJ/708/717  : Light curve templates of RR Lyrae stars (Sesar+, 2010)
 J/ApJ/750/99   : The Pan-STARRS1 photometric system (Tonry+, 2012)
 J/ApJ/908/20   : Use of field RRLyrae as galactic probes. II. (Crestani+, 2021)

Byte-by-byte Description of file: targets.dat
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  Bytes Format Units   Label   Explanations
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  1-  8  I8    ---     KIC     KIC identifier
 10- 19  F10.8 d       Per     [0.43/0.69] Period
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Byte-by-byte Description of file: table1.dat
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 Bytes   Format Units  Label Explanations
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   1-  8 I8     ---    KIC   KIC identifier
  10- 27 F18.10 d      HJDg  [2458653/2459544] Heliocentric Julian Date of
                              g-band observation
  29- 34 F6.3   mag    gmag  [7.16/17.8] Apparent g-band magnitude
  36- 40 F5.3   mag  e_gmag  [0.005/0.3] Uncertainty in gmag
  42- 59 F18.10 d      HJDr  [2458653/2459544] Heliocentric Julian Date of
                              r-band observation
  61- 66 F6.3   mag    rmag  [7.24/17.5] Apparent r-band magnitude
  68- 72 F5.3   mag  e_rmag  [0.005/0.4] Uncertainty in rmag
  74- 91 F18.10 d      HJDv  [2458653/2459544] Heliocentric Julian Date of
                              V-band observation
  93- 98 F6.3   mag    Vmag  [7.23/17.8] Apparent V-band magnitude
 100-104 F5.3   mag  e_Vmag  [0.009/0.3] Uncertainty in Vmag
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History:
    From electronic version of the journal

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(End)                          Prepared by [AAS], Coralie Fix [CDS], 24-Oct-2022
