Search for high-amplitude δ Scuti and RR Lyrae stars in Sloan Digital Sky Survey Stripe 82 using principal component analysis

Monthly Notices of the Royal Astronomical Society

Volumn 424, Issue 4, 2012, Pages 2528-2550

  Suveges M ^a,b   Sesar, B ^c   Varadi M ^b   Mowlavi, N ^a,b   Becker, A C ^d   Ivezic Z ^d   Beck, M ^a,b   Nienartowicz, K ^a,b   Rimoldini, L ^a,b   Dubath, P ^a,b   Bartholdi, P ^b   Eyer, L ^b  

^a UNIVERSITY OF GENEVA   (Switzerland)

^b UNIVERSITÉ DE GENÈVE   (Switzerland)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d UNIVERSITY OF WASHINGTON   (United States)

Author keywords

Methods: data analysis; Methods: statistical; Stars: variables: RR Lyrae; Stars: variables: Scuti; Surveys

Indexed keywords

PRINCIPAL COMPONENT ANALYSIS; SIGNAL TO NOISE RATIO; STARS; TIME SERIES;

HIGH AMPLITUDES; METHODS. DATA ANALYSIS; METHODS:STATISTICAL; PRINCIPAL-COMPONENT ANALYSIS; RR LYRAE STARS; SLOAN DIGITAL SKY SURVEY; STAR: VARIABLE: Δ SCUTI; STARS: VARIABLES; STARS: VARIABLES: RR LYRAE; Δ SCUTI;

SURVEYS;

EID: 84864925789     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2012.21229.x     Document Type: Article

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