Detection of Neptune-size planetary candidates with CoRoT data: Comparison with the planet occurrence rate derived from Kepler

Astronomy and Astrophysics

Volumn 547, Issue , 2012, Pages

  Bonomo, A S ^a,b   Chabaud, P Y ^a   Deleuil, M ^a   Moutou, C ^a   Bouchy, F ^c,d   Cabrera, J ^e   Lanza, A F ^f   Mazeh, T ^g   Aigrain, S ^h   Alonso, R ⁱ   Guterman, P ^a   Santerne, A ^a,d   Schneider, J ^j  

^a AIX MARSEILLE UNIVERSITÉ   (France)

^b OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

^c INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^d AIX MARSEILLE UNIVERSITY   (France)

^e GERMAN AEROSPACE CENTER DLR   (Germany)

^f INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^g TEL AVIV UNIVERSITY   (Israel)

^h UNIVERSITY OF OXFORD   (United Kingdom)

ⁱ UNIVERSITY OF GENEVA   (Switzerland)

^j UNIVERSITÉ PARIS DIDEROT   (France)

more..

Author keywords

Planetary systems; Stars: solar type; Stars: statistics; Techniques: photometric

Indexed keywords

DETECTION RATES; GENERAL TRENDS; LIGHT CURVES; MULTIPLE SYSTEMS; NEPTUNE; ORBITAL PERIODS; PLANETARY SYSTEM; SIGNAL TO NOISE (S/N) RATIOS; SPACE MISSIONS; STARS: STATISTICS; STELLAR POPULATIONS; TECHNIQUES: PHOTOMETRIC;

INTERPLANETARY FLIGHT; STARS;

PLANETS;

EID: 84868618168     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219780     Document Type: Article

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