Wavelets: a powerful tool for studying rotation, activity, and pulsation in Kepler and CoRoT stellar light curves

dc.contributor.authorBravo, J. P.
dc.contributor.authorRoque, S.
dc.contributor.authorEstrela, R.
dc.contributor.authorLeão, I. C.
dc.contributor.authorMedeiros, José Renan de
dc.date.accessioned2020-05-19T22:21:00Z
dc.date.available2020-05-19T22:21:00Z
dc.date.issued2014
dc.description.resumoAims. The wavelet transform has been used as a powerful tool for treating several problems in astrophysics. In this work, we show that the time–frequency analysis of stellar light curves using the wavelet transform is a ractical tool for identifying rotation, magnetic activity, and pulsation signatures. We present the wavelet spectral composition and multiscale variations of the time series for four classes of stars: targets dominated by magnetic activity, stars with transiting planets, those with binary transits, and pulsating stars. Methods. We applied the Morlet wavelet (6th order), which offers high time and frequency resolution. By applying the wavelet transform to the signal, we obtain the wavelet local and global power spectra. The first is interpreted as energy distribution of the signal in time–frequency space, and the second is obtained by time integration of the local map. Results. Since the wavelet transform is a useful mathematical tool for nonstationary signals, this technique applied to Kepler and CoRoT light curves allows us to clearly identify particular signatures for different phenomena. In particular, patterns were identified for the temporal evolution of the rotation period and other periodicity due to active regions affecting these light curves. In addition, a beat-pattern signature in the local wavelet map of pulsating stars over the entire time span was also detected.pt_BR
dc.identifier.citationMEDEIROS, José Renan de et al. Wavelets: a powerful tool for studying rotation, activity, and pulsation in and CoRoT stellar light curves. Astronomy & Astrophysics (Berlin. Print), v. 568, p. A34-44, 2014. ISSN 1432-0746 versão online. DOI https://doi.org/10.1051/0004-6361/201323032. Disponível em: https://www.aanda.org/articles/aa/abs/2014/08/aa23032-13/aa23032-13.html. Acesso em: 19 maio 2020. Reproduzido com permissão da Astronomy & Astrophysics, © ESO.pt_BR
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201323032
dc.identifier.issn0004-6361 (print), 1432-0746 (online)
dc.identifier.urihttps://repositorio.ufrn.br/jspui/handle/123456789/29023
dc.languageenpt_BR
dc.publisherEDP Sciencespt_BR
dc.subjectMethods: data analysispt_BR
dc.subjectTechniques: photometricpt_BR
dc.subjectStars: rotationpt_BR
dc.subjectStars: activitypt_BR
dc.subjectStars: oscillationspt_BR
dc.subjectBinaries: eclipsingpt_BR
dc.titleWavelets: a powerful tool for studying rotation, activity, and pulsation in Kepler and CoRoT stellar light curvespt_BR
dc.typearticlept_BR

Arquivos

Pacote Original

Agora exibindo 1 - 1 de 1
Carregando...
Imagem de Miniatura
Nome:
WaveletsAPowerfulToolForStudyingRotationActivity_Medeiros_2014.pdf
Tamanho:
5.96 MB
Formato:
Adobe Portable Document Format
Carregando...
Imagem de Miniatura
Baixar

Licença do Pacote

Agora exibindo 1 - 1 de 1
Nenhuma Miniatura disponível
Nome:
license.txt
Tamanho:
1.45 KB
Formato:
Item-specific license agreed upon to submission
Nenhuma Miniatura disponível
Baixar