Browsing by Author "Han, C."
Now showing 1 - 9 of 9
Results Per Page
Sort Options
- ItemA super-jupiter orbiting a late-type star : a refined analysis of microlensing event OGLE-2012-BLG-0406(2014) Tsapras, Y.; Choi, J.-Y; Street, R.; Han, C.; Bozza, V.; Gould, A.; Dominik, M.; Beaulieu, J. P.; Udalski, A.; Rabus, Markus
- ItemMASS. MEASUREMENTS. OF. ISOLATED. OBJECTS. FROM. SPACE-BASED. MICROLENSING(2016) Zhu, W.; Novati, S.; Gould, A.; Udalski, A.; Han, C.; Shvartzvald, Y.; Ranc, C.; Jorgensen, U.; Poleski, R.; Rabus, Markus; Bozza, V.; Beichman, C.; Bryden, G.; Carey, S.; Gaudi, B.; Henderson, C.
- ItemOGLE-2014-BLG-1186 : gravitational microlensing providing evidence for a planet orbiting the foreground star or for a close binary source?(2019) Dominik, M.; Bachelet, E.; Bozza, V.; Street, R.A.; Han, C.; Hundertmark, M.; Udalski, A.; Bramich, D.M; Alsubai, K.A.; Rabus, Markus; Novati, S.C.; Ciceri, S.; D'Ago, G.; Jaimes, R.F.; Haugbolle, T.; Hinse, T.C.; Horne, K.; Jorgensen, U.G.; Juncher, D.; Kains, N.; Korhonen, H.
- ItemOGLE-2015-BLG-0479LA,B. : BINARY. GRAVITATIONAL. MICROLENS. CHARACTERIZED. by SIMULTANEOUS. GROUND-BASED. and SPACE-BASED. OBSERVATIONS(2016) Han, C.; Udalski, A.; Gould, A.; Zhu, WeI.; Street, R. A.; Yee, J. C.; Beichman, C.; Bryden, C.; Novati, S. CalchI.; Rabus, Markus; Carey, S.; Fausnaugh, M.; Gaudi, B.S.; Henderson, Calen B.; Shvartzvald, Y.; Wibking, B.; Szymański, M. K.; Soszyński, I.; Skowron, J.; Mróz, P.; Poleski, R.
- ItemOGLE-2017-BLG-0329L : a microlensing binary characterized with dramatically enhanced precision using data from space-based observations(2018) Han, C.; Calchi Novati, S.; Udalski, A.; Lee, C.U.; Gould, A.; Bozza, V.; Mróz, P.; Pietrukowicz, Pawel; Skowron, J.; Rabus, Markus
- ItemOGLE-2017-BLG-0406 : Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk(2020) Hirao, Y.; Bennett, D. P.; Ryu, Y. H.; Koshimoto, N.; Udalski, A.; Yee, J. C.; Sumi, T.; Bond, I. A.; Shvartzvald, Y.; Rabus, Markus; Abe, F.; Barry, R. K.; Bhattacharya, A.; Donachie, M.; Fukui, A.; Itow, Y.; Kondo, I.; Alex Li, M. C.; Matsubara, Y.; Matsuo, T.; Miyazaki, S.; Muraki, Y.; Nagakane, M.; Ranc, C.; Rattenbury, N. J.; Suematsu, H.; Shibai, H.; Suzuki, D.; Tristram, P. J.; Yonehara, A.; Skowron, J.; Poleski, R.; Mróz, P.; Szymański, M. K.; Soszyński, I.; Kozłowski, S.; Pietrukowicz, Pawel; Ulaczyk, K.; Rybicki, K.; Iwanek, P. D.; Albrow, M.; Chung, S. J.; Gould, A.; Han, C.; Hwang, K. H.; Jung, Y. K.; Shin, I. G.; Zang, W.; Cha, S. M.; Kim, D. J.
- ItemPrecision measurement of a brown dwarf mass in a binary system in the microlensing event OGLE-2019-BLG-0033/MOA-2019-BLG-035(2022) Herald, A.; Udalski, A.; Bozza, V.; Rota, P.; Bond, I. A.; Yee, J. C.; Sajadian, S.; Mroz, P.; Poleski, R.; Skowron, J.; Szymanski, M. K.; Soszynski, I.; Pietrukowicz, P.; Kozlowski, S.; Ulaczyk, K.; Rybicki, K. A.; Iwanek, P.; Wrona, M.; Gromadzki, M.; Abe, F.; Barry, R.; Bennett, D. P.; Bhattacharya, A.; Fukui, A.; Fujii, H.; Hirao, Y.; Itow, Y.; Kirikawa, R.; Kondo, I.; Koshimoto, N.; Matsubara, Y.; Matsumoto, S.; Miyazaki, S.; Muraki, Y.; Olmschenk, G.; Ranc, C.; Okamura, A.; Rattenbury, N. J.; Satoh, Y.; Sumi, T.; Suzuki, D.; Silva, S. Ishitani; Toda, T.; Tristram, P. J.; Vandorou, A.; Yama, H.; Beichman, C. A.; Bryden, G.; Novati, S. Calchi; Carey, S.; Gaudi, B. S.; Gould, A.; Henderson, C. B.; Johnson, S.; Shvartzvald, Y.; Zhu, W.; Dominik, M.; Hundertmark, M.; Jorgensen, U. G.; Longa-Pena, P.; Skottfelt, J.; Tregloan-Reed, J.; Bach-Moller, N.; Burgdorf, M.; D'Ago, G.; Haikala, L.; Hitchcock, J.; Khalouei, E.; Peixinho, N.; Rahvar, S.; Snodgrass, C.; Southworth, J.; Spyratos, P.; Zang, W.; Yang, H.; Mao, S.; Bachelet, E.; Maoz, D.; Street, R. A.; Tsapras, Y.; Christie, G. W.; Cooper, T.; de Almeida, L.; do Nascimento, J. -D., Jr.; Green, J.; Han, C.; Hennerley, S.; Marmont, A.; McCormick, J.; Monard, L. A. G.; Natusch, T.; Pogge, R.Context. Brown dwarfs are transition objects between stars and planets that are still poorly understood, for which several competing mechanisms have been proposed to describe their formation. Mass measurements are generally difficult to carry out for isolated objects as well as for brown dwarfs orbiting low-mass stars, which are often too faint for a spectroscopic follow-up.
- ItemRed noise versus planetary interpretations in the microlensing event OGLE-2013-BLG-446(2015) Bachelet, E.; Bramich, D. M.; Han, C.; Greenhill, J.; Street, R. A.; Gould, A.; D'Ago, G.; AlSubai, K.; Dominik, M.; Rabus, Markus
- ItemSPITZER. OBSERVATIONS. OF. OGLE-2015-BLG-1212 REVEAL. A. NEW. PATH. TOWARD. BREAKING. STRONG. MICROLENS. DEGENERACIES(2016) Bozza, V.; Shvartzvald, Y.; Udalski, A.; Novati, S. Calchi; Bond, I. A.; Han, C.; Hundertmark, M.; Poleski, R.; Pawlak, M.; Rabus, Markus