Eric Ford
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Modeling Kepler Transit Light Curves as False Positives: Rejection of Blend Scenarios for Kepler-9, and Validation of Kepler-9 d, A Super-earth-size Planet in a Multiple System
G. Torres
,
F. Fressin
,
N. M. Batalha
,
W. J. Borucki
,
T. M. Brown
,
S. T. Bryson
,
L. A. Buchhave
,
D. Charbonneau
,
D. R. Ciardi
,
E. W. Dunham
,
D. C. Fabrycky
,
Eric B. Ford
,
III, T. N. Gautier
,
R. L. Gilliland
,
M. J. Holman
,
S. B. Howell
,
H. Isaacson
,
J. M. Jenkins
,
D. G. Koch
,
D. W. Latham
,
J. J. Lissauer
,
G. W. Marcy
,
D. G. Monet
,
A. Prsa
,
S. N. Quinn
,
Darin Ragozzine
,
J. F. Rowe
,
D. D. Sasselov
,
J. H. Steffen
,
W. F. Welsh
January 1, 2011
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Project
Project
DOI
Type
Journal article
Publication
ApJ
binaries: eclipsing
planetary systems
stars: individual: Kepler-9 KIC 3323887 KOI-377
stars: statistics
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