- Record: found
- Abstract: not found
- Article: not found
The lowest mass ratio planetary microlens: OGLE 2016–BLG–1195Lb
I. A. Bond ,
D. P. Bennett ,
T. Sumi ,
A. Udalski ,
D. Suzuki ,
N. J. Rattenbury ,
V. Bozza ,
N. Koshimoto ,
F. Abe ,
Y. Asakura ,
R. K. Barry ,
A. Bhattacharya ,
M. Donachie ,
P. Evans ,
A. Fukui ,
Y. Hirao ,
Y. Itow ,
M. C. A. Li ,
C. H. Ling ,
K. Masuda ,
Y. Matsubara ,
Y. Muraki ,
M. Nagakane ,
K. Ohnishi ,
C. Ranc ,
To. Saito ,
A. Sharan ,
D. J. Sullivan ,
P. J. Tristram ,
T. Yamada ,
T. Yamada ,
A. Yonehara ,
J. Skowron ,
M. K. Szymański ,
R. Poleski ,
P. Mróz ,
I. Soszyński ,
P. Pietrukowicz ,
S. Kozłowski ,
K. Ulaczyk ,
M. Pawlak
May 01 2017
May 01 2017
Read this article at
There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.
Related collections
Most cited references42
- Record: found
- Abstract: not found
- Article: not found
Toward a Deterministic Model of Planetary Formation. II. The Formation and Retention of Gas Giant Planets around Stars with a Range of Metallicities
Shigeru Ida, D. Lin (2004)
- Record: found
- Abstract: not found
- Article: not found
Gravitational microlensing by double stars and planetary systems
Shunde Mao, Bohdan Paczynski (1991)