New Insights into Time Series Analysis IV: Panchromatic and Flux Independent Period Finding Methods
arXiv:2101.00918 · doi:10.1093/mnras/staa3967
Abstract
New time-series analysis tools are needed in disciplines as diverse as astronomy, economics and meteorology. In particular, the increasing rate of data collection at multiple wavelengths requires new approaches able to handle these data. The panchromatic correlated indices and are adapted to quantify the smoothness of a phased light-curve resulting in new period-finding methods applicable to single- and multi-band data. Simulations and observational data are used to test our approach. The results were used to establish an analytical equation for the amplitude of the noise in the periodogram for different false alarm probability values, to determine the dependency on the signal-to-noise ratio, and to calculate the yield-rate for the different methods. The proposed method has similar efficiency to that found for the String Length period method. The effectiveness of the panchromatic and flux independent period finding methods in single waveband as well as multiple-wavebands that share a fundamental frequency is also demonstrated in real and simulated data.
arXiv comment14 pages, 7 figures
References in corpus (33)
- The Gaia mission
- The Transiting Exoplanet Survey Satellite
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- The generalised Lomb-Scargle periodogram. A new formalism for the floating-mean and Keplerian periodograms
- The PLATO 2.0 Mission
- Understanding the Lomb-Scargle Periodogram
- ATLAS: A High-Cadence All-Sky Survey System
- VISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way
- The WFCAM Science Archive
- The Catalina Surveys Periodic Variable Star Catalog
- The UKIRT Wide Field Camera ZYJHK Photometric System: Calibration from 2MASS
- Periodograms for Multiband Astronomical Time Series
- Automated supervised classification of variable stars I. Methodology
- Discovery of 9,000 new RR Lyrae in the Southern Catalina Surveys
- Stellar Cycles from Photometric Data: CoRoT Stars
- Overview of semi-sinusoidal stellar variability with the CoRoT satellite
- The rotational behavior of Kepler Stars with Planets
- Planetary transit candidates in the CoRoT LRa01 field
- Search for high-amplitude Delta Scuti and RR Lyrae stars in Sloan Digital Sky Survey Stripe 82 using principal component analysis
- The VVV Templates Project. Towards an Automated Classification of VVV Light-Curves. I. Building a database of stellar variability in the near-infrared
- Archiving multi-epoch data and the discovery of variables in the near infrared
- An Updated Catalog of 4680 Northern Eclipsing Binaries with Algol-Type light curve morphology in the Catalina Sky Surveys
- A study of periodograms standardized using training data sets and application to exoplanet detection
- CoRoT space photometry of seven Cepheids
- A Hybrid Algorithm for Period Analysis from Multi-band Data with Sparse and Irregular Sampling for Arbitrary Light Curve Shapes
- New Insights into Time Series Analysis II -- No Correlated Observations
- New Insights into Time Series Analysis - I - Correlated observations
- The VVV Infrared Variability Catalog (VIVA-I)
- The variability behavior of CoRoT M-giant Stars
- A Multiband Generalization of the Analysis of Variance Period Estimation Algorithm and the Effect of Inter-band Observing Cadence on Period Recovery Rate
- Discovery of fast, large-amplitude optical variability of V648 Car (=SS73-17)
- New Insights into Time Series Analysis III - Setting constraints on period analysis