Planetary occultations from KEPLER data

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F14%3A00107115" target="_blank" >RIV/00216224:14310/14:00107115 - isvavai.cz</a>

Result on the web

<a href="http://articles.adsabs.harvard.edu/pdf/2014CoSka..43..438H" target="_blank" >http://articles.adsabs.harvard.edu/pdf/2014CoSka..43..438H</a>

DOI - Digital Object Identifier

—

Result language

angličtina

Original language name

Planetary occultations from KEPLER data

Original language description

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.

Czech name

—

Czech description

—

Type

J_imp - Article in a specialist periodical, which is included in the Web of Science database

CEP classification

—

OECD FORD branch

10308 - Astronomy (including astrophysics,space science)

Project

—

Continuities

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2014

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Contributions of the Astronomical Observatory Skalnaté Pleso

ISSN

1335-1842

e-ISSN

—

Volume of the periodical

43

Issue of the periodical within the volume

3

Country of publishing house

SK - SLOVAKIA

Number of pages

2

Pages from-to

438-439

UT code for WoS article

000338483100054

EID of the result in the Scopus database

2-s2.0-84901634782