The Concept of Few-Parameter Modeling of Eclipsing Binary and Exoplanet Transit Light Curves
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F15%3A00086958" target="_blank" >RIV/00216224:14310/15:00086958 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
The Concept of Few-Parameter Modeling of Eclipsing Binary and Exoplanet Transit Light Curves
Original language description
We present a new, few-parameter phenomenological model of light curves of eclipsing binaries and stars with transiting planets. The model is able to fit the observed light curves with an accuracy better than 1% of their amplitudes. It can be used for appropriate descriptions of light curve shapes, classification, mid-eclipse time determination, and detailed period analyses.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
S - Specificky vyzkum na vysokych skolach
Others
Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
LIVING TOGETHER: PLANETS, HOST STARS, AND BINARIES
ISBN
9781583818770
ISSN
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e-ISSN
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Number of pages
5
Pages from-to
176-180
Publisher name
ASTRONOMICAL SOC PACIFIC
Place of publication
SAN FRANCISCO
Event location
Litomysl, CZECH REPUBLIC
Event date
Sep 8, 2014
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000369467900027