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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.
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Datos observacionales y astrométricos
| Constelación: | Paloma |
| Ascensión Recta: | 06h14m11.92s |
| Declinación: | -34°15'18.0" |
| Magnitud Aparente: | 9.056 |
| Distancia: | 338.983 parsecs |
| Movimiento Propio en Ascensión Recta: | 15.6 |
| Movimiento Propio en Declinación: | -4 |
| B-T magnitude: | 10.905 |
| V-T magnitude: | 9.209 |
Catálogos y designaciones:
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