Preparation of Kepler light curves for asteroseismic analyses

• Tipo: Artigo em Revista Científica Internacional
• Data: 2011

Autores

Garcia, RA (Autor) Outra; Hekker, S (Autor) Outra; Stello, D (Autor) Outra; Gutierrez Soto, J (Autor) Outra; Handberg, R (Autor) Outra; Huber, D (Autor) Outra; Karoff, C (Autor) Outra; Uytterhoeven, K (Autor) Outra; Appourchaux, T (Autor) Outra; Chaplin, WJ (Autor) Outra; Elsworth, Y (Autor) Outra; Mathur, S (Autor) Outra; Ballot, J (Autor) Outra; Christensen Dalsgaard, J (Autor) Outra; Gilliland, RL (Autor) Outra; Houdek, G (Autor) Outra; Jenkins, JM (Autor) Outra; Kjeldsen, H (Autor) Outra; McCauliff, S (Autor) Outra; Metcalfe, T (Autor) Outra; Middour, CK (Autor) Outra; Molenda Zakowicz, J (Autor) Outra; Monteiro, MJPFG (Autor) FCUP; Smith, JC (Autor) Outra; Thompson, MJ (Autor) Outra

Revista

Título: Monthly Notices of the Royal Astronomical Society

Vol. 414

Páginas: L6-L10

ISSN: 0035-8711

Editora: Oxford University Press

Indexação

ISI Web of Knowledge - 203 Citações

Scopus - 196 Citações

Classificação Científica

FOS: Ciências exactas e naturais > Física

CORDIS: Ciências Físicas > Astronomia

Outras Informações

ID Authenticus: P-002-R5H

DOI: 10.1111/j.1745-3933.2011.01042.x

Resumo (PT): The Kepler mission is providing photometric data of exquisite quality for the asteroseismic study of different classes of pulsating stars. These analyses place particular demands on the pre-processing of the data, over a range of time-scales from minutes to months. Here, we describe processing procedures developed by the Kepler Asteroseismic Science Consortium to prepare light curves that are optimized for the asteroseismic study of solar-like oscillating stars in which outliers, jumps and drifts are corrected.

Abstract (EN): The Kepler mission is providing photometric data of exquisite quality for the asteroseismic study of different classes of pulsating stars. These analyses place particular demands on the pre-processing of the data, over a range of time-scales from minutes to months. Here, we describe processing procedures developed by the Kepler Asteroseismic Science Consortium to prepare light curves that are optimized for the asteroseismic study of solar-like oscillating stars in which outliers, jumps and drifts are corrected.

Idioma: Inglês

Tipo (Avaliação Docente): Científica

Notas: Letter