The Octave (Birmingham-Sheffield Hallam) automated pipeline for extracting oscillation parameters of solar-like main-sequence stars

Monthly Notices of the Royal Astronomical Society

Volumn 402, Issue 3, 2010, Pages 2049-2059

  Hekker, S ^a   Broomhall, A M ^a   Chaplin, W J ^a   Elsworth, Y P ^a   Fletcher, S T ^b   New, R ^b   Arentoft, T ^c   Quirion, P O ^c   Kjeldsen, H ^c  

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^b SHEFFIELD HALLAM UNIVERSITY   (United Kingdom)

^c AARHUS UNIVERSITY   (Denmark)

Author keywords

Methods: data analysis; Stars: late type; Stars: oscillations

Indexed keywords

AUTOMATION; NASA; STARS;

BIRMINGHAM; HIGH-PRECISION; MAIN SEQUENCE STARS; METHODS. DATA ANALYSIS; OSCILLATION PARAMETERS; PHOTOMETRICS; SHEFFIELD; SOLAR LIKE OSCILLATIONS; STAR OSCILLATIONS; STARS:LATE TYPE;

PIPELINES;

EID: 77949334598     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.16030.x     Document Type: Article

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