Classification of variable stars in the WFCAM Transit Survey

The WFCAM Transit Survey is a photometric survey in the near-infrared and aims at finding Earth-like planets transiting M-dwarf stars. As a by-product of the survey, a variety of variable stars has been detected. We report the discovery and classification of 192 periodic variable stars in the WFCAM...

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Main Authors: Moya Andrés, Barrado David, Sarro Luis M., Stoev Hristo
Format: Article
Language:English
Published: EDP Sciences 2013-04-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20134701007
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author Moya Andrés
Barrado David
Sarro Luis M.
Stoev Hristo
author_facet Moya Andrés
Barrado David
Sarro Luis M.
Stoev Hristo
author_sort Moya Andrés
collection DOAJ
description The WFCAM Transit Survey is a photometric survey in the near-infrared and aims at finding Earth-like planets transiting M-dwarf stars. As a by-product of the survey, a variety of variable stars has been detected. We report the discovery and classification of 192 periodic variable stars in the WFCAM Transit Survey. 185 of those objects are previously unknown variable sources. The derived parameters of their light curves will be helpful for the creation of a robust sample of light curves (and their parameters thereof) of classified variable stars in the near-infrared for the automatic classification of light curves of stellar objects in the J-band.
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spelling doaj.art-ff4c3845077643879009a7fb5a9dfb5e2022-12-21T16:43:07ZengEDP SciencesEPJ Web of Conferences2100-014X2013-04-01470100710.1051/epjconf/20134701007Classification of variable stars in the WFCAM Transit SurveyMoya AndrésBarrado DavidSarro Luis M.Stoev HristoThe WFCAM Transit Survey is a photometric survey in the near-infrared and aims at finding Earth-like planets transiting M-dwarf stars. As a by-product of the survey, a variety of variable stars has been detected. We report the discovery and classification of 192 periodic variable stars in the WFCAM Transit Survey. 185 of those objects are previously unknown variable sources. The derived parameters of their light curves will be helpful for the creation of a robust sample of light curves (and their parameters thereof) of classified variable stars in the near-infrared for the automatic classification of light curves of stellar objects in the J-band.http://dx.doi.org/10.1051/epjconf/20134701007
spellingShingle Moya Andrés
Barrado David
Sarro Luis M.
Stoev Hristo
Classification of variable stars in the WFCAM Transit Survey
EPJ Web of Conferences
title Classification of variable stars in the WFCAM Transit Survey
title_full Classification of variable stars in the WFCAM Transit Survey
title_fullStr Classification of variable stars in the WFCAM Transit Survey
title_full_unstemmed Classification of variable stars in the WFCAM Transit Survey
title_short Classification of variable stars in the WFCAM Transit Survey
title_sort classification of variable stars in the wfcam transit survey
url http://dx.doi.org/10.1051/epjconf/20134701007
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AT barradodavid classificationofvariablestarsinthewfcamtransitsurvey
AT sarroluism classificationofvariablestarsinthewfcamtransitsurvey
AT stoevhristo classificationofvariablestarsinthewfcamtransitsurvey