The Lowest Mass Ratio Planetary Microlens: OGLE 2016–BLG–1195Lb von Bond, I. A., Bennett, D. P., Sumi, T., Udalski, A., Suzuki, D., Rattenbury, N. J., Bozza, V., Koshimoto, N., Abe, F., Asakura, Y., Barry, R. K., Bhattacharya, A., Donachie, M., Evans, P., Fukui, A., Hirao, Y., Itow, Y., Li, M. C. A., Ling, C. H., Masuda, K., Matsubara, Y., Muraki, Y., Nagakane, M., Ohnishi, K., Ranc, C., Saito, To, Sharan, A., Sullivan, D. J., Tristram, P. J., Yamada, T., Yamada, T., Yonehara, A., Skowron, J., Szyma´nski, M. K., Poleski, R., Mr´oz, P., Soszy´nski, I., Pietrukowicz, P., Kozłowski, S., Ulaczyk, K., Pawlak, M.

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Microlensing optical depth toward the Galactic Bulge using bright sources from OGLE-II von Sumi, T, Wozniak, P. R, Udalski, A, Szymanski, M, Kubiak, M, Pietrzynski, G, nski, I. Soszy, Zebrun, K, Szewczyk, O, Wyrzykowski, L, Paczynski, B

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Microlensing optical depth toward the Galactic Bulge using bright sources from OGLE-II von Sumi, T, Wozniak, P R, Udalski, A, Szymanski, M, Kubiak, M, Pietrzynski, G, nski, I Soszy, Zebrun, K, Szewczyk, O, Wyrzykowski, L, Paczynski, B

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