Now showing items 1-2 of 2

    • Modelling the rotation period distribution of M dwarfs in the Kepler field 

      Koen, Chris (Springer Verlag, 2018)
      McQuillan et al. (Mon. Not. R. Astron. Soc.432:1203, 2013) presented 1570 periods P of M dwarf stars in the field of view of the Kepler telescope. It is expected that most of these reflect rotation periods, due to starspots. ...
    • Starspot modelling of the TESS light curve of CVSO 30 

      Koen, C (EDP Sciences, 2021)
      Aims. I aim to investigate whether the photometric variability in the candidate host star CVSO 30 can be explained by starspots. Methods. The Transiting Exoplanet Survey Satellite (TESS) light curve of CVSO 30 is separated ...