July
2016
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2016ApJ...825...60Z
Authors
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Zhu, Wei
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Calchi Novati, S.
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Gould, A.
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Udalski, A.
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Han, C.
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Shvartzvald, Y.
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Ranc, C.
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Jørgensen, U. G.
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Poleski, R.
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Bozza, V.
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Beichman, C.
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Bryden, G.
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Carey, S.
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Gaudi, B. S.
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Henderson, C. B.
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Pogge, R. W.
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Porritt, I.
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Wibking, B.
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Yee, J. C.
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SPITZER Team
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Pawlak, M.
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Szymański, M. K.
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Skowron, J.
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Mróz, P.
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Kozłowski, S.
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Wyrzykowski, Ł.
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Pietrukowicz, P.
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Pietrzyński, G.
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Soszyński, I.
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Ulaczyk, K.
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OGLE Group
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Choi, J. -Y.
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Park, H.
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Jung, Y. K.
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Shin, I. -G.
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Albrow, M. D.
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Park, B. -G.
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Kim, S. -L.
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Lee, C. -U.
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Cha, S. -M.
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Kim, D. -J.
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Lee, Y.
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KMTNET Group
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Friedmann, M.
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Kaspi, S.
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Maoz, D.
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WISE Group
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Hundertmark, M.
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Street, R. A.
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Tsapras, Y.
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Bramich, D. M.
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Cassan, A.
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Dominik, M.
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Bachelet, E.
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Dong, Subo
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Figuera Jaimes, R.
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Horne, K.
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Mao, S.
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Menzies, J.
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Schmidt, R.
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Snodgrass, C.
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Steele, I. A.
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Wambsganss, J.
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RoboNeT Team
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Skottfelt, J.
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Andersen, M. I.
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Burgdorf, M. J.
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Ciceri, S.
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D'Ago, G.
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Evans, D. F.
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Gu, S. -H.
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Hinse, T. C.
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Kerins, E.
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Korhonen, H.
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Kuffmeier, M.
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Mancini, L.
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Peixinho, N.
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Popovas, A.
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Rabus, M.
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Rahvar, S.
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Tronsgaard, R.
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Scarpetta, G.
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Southworth, J.
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Surdej, J.
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von Essen, C.
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Wang, Y. -B.
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Wertz, O.
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MiNDSTEP Group
Abstract
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We report on the mass and distance measurements of two single-lens events from the 2015 Spitzer microlensing campaign. With both finite-source effect and microlens parallax measurements, we find that the lens of OGLE-2015-BLG-1268 is very likely a brown dwarf (BD). Assuming that the source star lies behind the same amount of dust as the Bulge red clump, we find the lens is a 45 ± 7 {M}{{J}} BD at 5.9 ± 1.0 kpc. The lens of of the second event, OGLE-2015-BLG-0763, is a 0.50 ± 0.04 {M}⊙ star at 6.9 ± 1.0 kpc. We show that the probability to definitively measure the mass of isolated microlenses is dramatically increased once simultaneous ground- and space-based observations are conducted.
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