J/MNRAS/331/45      New periodic variables                   (Koen+, 2002)
New periodic variables from the Hipparcos epoch photometry.
    Koen C., Eyer L.
   <Mon. Not. R. Astron. Soc. 331, 45 (2002)>
   =2002MNRAS.331...45K 2002MNRAS.331...45K
ADC_Keywords: Stars, variable ; Magnitudes
Keywords: methods: data analysis - methods: statistical -
          stars: variables: other
Abstract:
    Two selection statistics are used to extract new candidate periodic
    variables from the epoch photometry of the Hipparcos catalogue. The
    primary selection criterion is a signal-to-noise ratio. The dependence
    of this statistic on the number of observations is calibrated using
    about 30000 randomly permuted Hipparcos data sets. A significance
    level of 0.1 per cent is used to extract a first batch of candidate
    variables. The second criterion requires that the optimal frequency be
    unaffected if the data are de-trended by low-order polynomials. We
    find 2675 new candidate periodic variables, of which the majority
    (2082) are from the Hipparcos unsolved variables. Potential problems
    with the interpretation of the data (e.g. aliasing) are discussed.
File Summary:
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 FileName    Lrecl  Records   Explanations
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ReadMe          80        .   This file
table5.dat      54     2675   The selected candidate variable stars
table5.tex      78     2702   LaTeX version of table5
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See also:
   I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)
Byte-by-byte Description of file: table5.dat
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   Bytes Format Units  Label     Explanations
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   1-  6  I6    ---    HIP       HIP number
   8- 12  F5.2  mag    Vmag      V magnitude
  14- 21  F8.5  d-1    Freq      Frequency (1)
  23- 28  F6.4  mag    Amp       Amplitude of the sinusoid (1)
  30- 32  I3    ---    Npoint    Number of datapoints accepted
  34- 39  F6.3  ---    R*        Signal-to-noise ratio statistic (2)
  41- 52  A12   ---    SpType    MK Spectral classification
      54  A1    ---    VarClass  [CMU] Hipparcos variability classification (3)
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Note (1): The frequency corresponding to the periodogram maximum was noted, 
    and a sinusoid with this frequency fitted to the data by linear least
    squares.
Note (2): Candidate variables selected on the basis of sufficiently large 
          R* (R*>3.543) have good probabilities of being true variables.
    See text for more explanations.
Note (3): Hipparcos variability:
      C: constant
      M: microvariable
      U: unsolved
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Acknowledgements: Chris Koen 
(End)                         James Marcout, Patricia Bauer [CDS]    06-May-2002