Possible detection of phase changes from the non-transiting planet HD 46375b by CoRoT

Astronomy and Astrophysics

Volumn 518, Issue 22, 2010, Pages

  Gaulme, P ^a   Vannier, M ^b   Guillot, T ^b   Mosser, B ^c   Mary, D ^b   Weiss, W W ^d   Schmider, F X ^b   Bourguignon, S ^b   Deeg, H J ^e   Regulo C ^e   Aigrain, S ^f   Schneider, J ^c   Bruntt, H ^c   Deheuvels, S ^c   Donati, J F ^g   Appourchaux, T ^a   Auvergne, M ^c   Baglin, A ^c   Baudin, F ^a   Catala, C ^c   Michel, E ^c   Samadi, R ^c   more..

^a UNIVERSITÉ PARIS SUD   (France)

^b UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

^c OBSERVATOIRE DE PARIS   (France)

^d UNIVERSITY OF VIENNA   (Austria)

^e INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^f UNIVERSITY OF OXFORD   (United Kingdom)

^g CNRS   (France)

Author keywords

Methods: data analysis; Planetary systems; Stars: individual: HD 46375; Techniques: photometric

Indexed keywords

DATA REDUCTION; PHOTOMETRY; STARS; TIME SERIES; TIME SERIES ANALYSIS;

ASTEROSEISMOLOGY; BRIGHTNESS TEMPERATURES; DATA ANALYSIS; EXOPLANET; FOURIER SPECTRA; GROUND BASED; HIGH POTENTIAL; LIGHTCURVES; METHODS:DATA ANALYSIS; OPTICAL WAVELENGTH; ORBITAL PHASE; PHASE CHANGE; PLANETARY SYSTEM; REFLECTED LIGHT; RELATIVE AMPLITUDE; SEISMIC ANALYSIS; SINUSOIDAL SIGNALS; STAR MODEL; STARS: INDIVIDUAL; TECHNIQUES: PHOTOMETRIC; VELOCITY SIGNALS;

SIGNAL DETECTION;

EID: 77957839307     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014303     Document Type: Article

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