|
|
|
|
|
Yiannis Tsapras
Gravitational microlensing finds planets through their gravitational influence on the light coming from a more distant background star. The presence of the planet is then inferred from the tell-tale brightness variations of the background star during the...
ver más
|
|
|
|
|
|
|
|
|
|
|
M. Lensing, J. D. van der Klis, I. Yoon, and D. T. Moore
Pág. 1590 - 1597
|
|
|
|
|
|
|
|
|
|
|
M. Lensing, J. D. van der Klis, T. Fabri, A. Cazemier, and A. J. Else
Pág. 2401 - 2409
|
|
|
|
|
|
|
|
|
|
|
Y. Fan, C. Zhao, J. Degallaix, L. Ju, D. G. Blair, B. J. J. Slagmolen, D. J. Hosken, A. F. Brooks, P. J. Veitch, and J. Munch
|
|
|
|
|
|
|
|
|
|
|
Proskurnin, M. A. Kononets, M. Y. Bendrysheva, S. N. Proskurnina, E. V. Nedosekin, D. A. Khrycheva, A. D.
Pág. 334 - 336
|
|
|
|
|
|
|
|
|
|
|
Orlova, N. V. Proskurnin, M. A. Samburova, V. A. Dryagleva, I. D. Brusnichkin, A. V.
Pág. 506 - 508
|
|
|
|
|
|
|
|
|
|
|
Proskurnin, M. A. Kononets, M. Y. Min kovskii, E. M. Proskurnina, E. V. Bendrysheva, S. N. Tarasov, A. R. Lisichkin, G. V.
Pág. 739 - 741
|
|
|
|
|
|
|
|
|
|
|
Cruz-Cabrera, A A; Yang, M; Behrman, E C; Steck, J E; Skinner, S R
Pág. 1450 - 1457
|
|
|
|
|
|