Solar-like oscillations in red giants observed with Kepler: Comparison of global oscillation parameters from different methods

Astronomy and Astrophysics

Volumn 525, Issue 8, 2010, Pages

  Hekker, S ^a   Elsworth, Y ^a   De Ridder, J ^b   Mosser, B ^c   Garcia R A ^d   Kallinger, T ^e,f   Mathur, S ^g   Huber, D ^h   Buzasi, D L ⁱ   Preston, H L ^i,j   Hale, S J ^a   Ballot, J ^k   Chaplin, W J ^a   Regulo C ^l,m   Bedding, T R ^h   Stello, D ^h   Borucki, W J ⁿ   Koch, D G ⁿ   Jenkins, J ⁿ   Allen, C ⁿ   Gilliland, R L ^o   Kjeldsen, H ^p   Christensen Dalsgaard, J ^p   more..

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^b KU LEUVEN   (Belgium)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^f UNIVERSITY OF VIENNA   (Austria)

^g NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^h UNIVERSITY OF SYDNEY   (Australia)

ⁱ EUREKA SCIENTIFIC   (United States)

^j UNIVERSITY OF SOUTH AFRICA   (South Africa)

^k UNIVERSITÉ DE TOULOUSE   (France)

^l UNIVERSIDAD DE LA LAGUNA   (Spain)

^m INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

ⁿ NASA AMES RESEARCH CENTER   (United States)

^o AURA for the European Space Agency   (United States)

^p AARHUS UNIVERSITY   (Denmark)

more..

Author keywords

asteroseismology; methods: observational; stars: late type; techniques: photometric

Indexed keywords

PHOTOMETRY; STOCHASTIC SYSTEMS; UNCERTAINTY ANALYSIS;

ASTEROSEISMOLOGY; METHODS:OBSERVATIONAL; OSCILLATION PARAMETERS; OSCILLATION POWER; SOLAR LIKE OSCILLATIONS; STARS:LATE TYPE; STOCHASTIC SIGNALS; TECHNIQUES: PHOTOMETRIC;

GIANT STARS;

EID: 78649939613     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: None     Document Type: Article

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