In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no. 3
Ľ. Hambálek - T. Krejčová
Detaily:
Rok, strany: 2014, 438 - 439
Kľúčové slová:
stars, variables, exoplanets, photometry
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2014/Vol_43/No_3/pp438-439_abstract.html
O článku:
The KEPLER spacecraft provides accurate (up to 40 ppm of flux for stars near 7 mag) light-curves (LCs), enough to theoretically distinguish the occultation of the exoplanet by its parent star (e.g. the secondary minimum). We have selected KEPLER Objects of Interest KOI-2.01 and KOI-13.01 with the deepest secondary minima; co-added many single phase LCs and modeled them with a simplex algorithm to measure the depths of primary and secondary minima; and calculate the radii of the star and the exoplanet.
Ako citovať:
ISO 690:
Hambálek, Ľ., Krejčová, T. 2014. Planetary occultations from KEPLER data. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no.3, pp. 438-439. 1335-1842.
APA:
Hambálek, Ľ., Krejčová, T. (2014). Planetary occultations from KEPLER data. Contributions of the Astronomical Observatory Skalnaté Pleso, 43(3), 438-439. 1335-1842.