Abstract
We introduce an improvement to a periodicity metric we have introduced in a previous paper. We improve on the Hoeffding-test periodicity metric, using the Blum-Kiefer-Rosenblatt (BKR) test. Besides a consistent improvement over the Hoeffding-test approach, the BKR approach turns out to perform superbly when applied to very short time series of sawtooth-like shapes. The expected astronomical implications are much more detections of RR-Lyrae stars and Cepheids in sparse photometric data bases, and of eccentric Keplerian radial-velocity (RV) curves, such as those of exoplanets in RV surveys.
| Original language | English |
|---|---|
| Pages (from-to) | L118-L121 |
| Journal | Monthly Notices of the Royal Astronomical Society: Letters |
| Volume | 457 |
| Issue number | 1 |
| DOIs | |
| State | Published - 7 Jan 2016 |
Keywords
- Binaries: spectroscopic
- Methods: data analysis
- Methods: statistical
- Stars: individual: HIP 101453
- Stars: variables: RR lyrae
- Stars: variables: cepheids
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
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