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New periodic variables from the Hipparcos epoch photometry
Two selection statistics are used to extract new candidate periodicvariables from the epoch photometry of the Hipparcos catalogue. Theprimary selection criterion is a signal-to-noise ratio. The dependenceof this statistic on the number of observations is calibrated usingabout 30000 randomly permuted Hipparcos data sets. A significance levelof 0.1 per cent is used to extract a first batch of candidate variables.The second criterion requires that the optimal frequency be unaffectedif the data are de-trended by low-order polynomials. We find 2675 newcandidate periodic variables, of which the majority (2082) are from theHipparcos`unsolved' variables. Potential problems with theinterpretation of the data (e.g. aliasing) are discussed.
| The classification of intrinsic variable stars. II. The red variables of S and related types
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1972ApJ...177..489E&db_key=AST
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Observation and Astrometry data
| Constellation: | Puppis |
| Right ascension: | 07h40m13.77s |
| Declination: | -12°04'49.4" |
| Apparent magnitude: | 7.909 |
| Distance: | 350.877 parsecs |
| Proper motion RA: | -10.6 |
| Proper motion Dec: | -8.5 |
| B-T magnitude: | 7.795 |
| V-T magnitude: | 7.9 |
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