We present a fresh analysis of the light curves of Kepler-6, Kepler-8 and Kepler-40 star-planet systems using ∼3 years of observations by the Kepler space telescope. Transit light curves were solved using WinFitter code. The proximity effects (ellipticity and reflection effects) and Doppler beaming effect were also examined using the Fourier series method. Mid-transit times of the light curves of the three exoplanets observed during the Kepler mission were recomputed, and transit timing variations for each exoplanet were analyzed.
REFERENCES
1.
2.
B.M.S.
Hansen
& T.
Barman
, Astrophys. J.
, 671
, 861
–871
(2007
).3.
B.-O.
Demory
& S.
Seager
, in IAU Symp. 276, The Astrophysics of Planetary Systems–Formation, Structure, and Dynamical Evolution, eds. A.
Sozzetti
, M. G.
Lattanzi
, & A. P.
Boss
(Cambridge
: Cambridge Univ. Press
), 475
–476
(2011
).4.
D.
Angerhausen
, E.
DeLarme
, J. A.
Morse
, Publ. Astron. Soc. Pac.
, 127
, 1113
–1130
(2015
).5.
6.
E. W.
Dunham
, W. J.
Borucki
, D. G.
Koch
, et al., Astrophys. J.
, 713
, 136
–139
(2010
).7.
J. M.
Jenkins
, W. J.
Borucki
, D. G.
Koch
, et al., Astrophys. J.
, 724
, 1108
–1119
(2010
).8.
J.-M.
Désert
, D.
Charbonneau
, J. J.
Fortney
, et al., Astrophys. J. Suppl.
, 197
, 11
, 1
–11
(2011
).9.
10.
L. J.
Esteves
, E. J. W.
De Mooij
, R.
Jayawardhana
, Astrophys. J.
, 772
, 51
, 1
–14
(2013
).11.
S.
Faigler
& T.
Mazeh
, Mon. Not. R. Astron. Soc.
, 415
, 3921
–3928
(2011
).12.
V. S.
Safronov
, Evolution of the Protoplanetary Cloud and Formation of the Earth and Planets (Jerusalem: Israel Program for Scientific Translation)
, Keter Publishing House
(1972
).13.
This content is only available via PDF.
© 2018 Author(s).
2018
Author(s)
You do not currently have access to this content.