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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 Distribution of the BD M-Type Stars Along the Galactic Equator.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1958ApJ...128..510N&db_key=AST
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| Takýmyýldýz: | Kugu |
| Sað Açýklýk: | 20h21m24.24s |
| Yükselim: | +30°51'51.3" |
| Görünürdeki Parlaklýk: | 7.65 |
| Uzaklýk: | 806.452 parsek |
| özdevim Sað Açýklýk: | -6.4 |
| özdevim Yükselim: | -10 |
| B-T magnitude: | 9.787 |
| V-T magnitude: | 7.827 |
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