The continuous period search method and its application to the young solar analogue HD 116956

2010/07/31 by J. Lehtinen, L. Jetsu, T. Hackman +2 · 29 citations
Physics and Astronomy · #Period (music) #Photometry (optics) #Scientific Research and Discoveries #Series (stratigraphy) #Solar and Space Plasma Dynamics #Solar minimum #Solar physics #Spectrum analysis #Stellar, planetary, and galactic studies #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201015454

published in Astronomy and Astrophysics 527, A136 (EDP Sciences) · 14 pages, 11 figures, 3 tables

openalex publication_date 2010/12/16 · arxiv created 2011/03/03 · arxiv updated 2015/05/19 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We formulate an improved time series analysis method for the analysis of photometry of active stars. This new continuous period search (CPS) method is applied to 12 years of V band photometry of the young solar analogue HD 116956 (NQ UMa).

Citations

• Least-squares frequency analysis of unequally spaced data
• Studies in astronomical time series analysis. II - Statistical aspects of spectral analysis of unevenly spaced data
• Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I.
• Late-type members of young stellar kinematic groups - I. Single stars