OGLE-2008-BLG-510: first automated real-time detection of a weak microlensing 
anomaly - brown dwarf or stellar binary?

Bozza, V.; Dominik, M.; Rattenbury, N. J.; Jørgensen, U. G.; Tsapras, Y.; Bramich, D. M.; Udalski, A.; Bond, I. A.; Liebig, C.; Cassan, A.; Fouqué, P.; Fukui, A.; Hundertmark, M.; Shin, I.-G.; Lee, S. H.; Choi, J.-Y.; Park, S.-Y.; Gould, A.; Allan, A.; Mao, S.; Wyrzykowski, Ł.; Street, R. A.; Buckley, D.; Nagayama, T.; Mathiasen, M.; Hinse, T. C.; Novati, S. C.; Harpsœ, K.; Mancini, L.; Scarpetta, G.; Anguita, T.; Burgdorf, M. J.; Horne, K.; Hornstrup, A.; Kains, N.; Kerins, E.; Kjærgaard, P.; Masi, G.; Rahvar, S.; Ricci, D.; Snodgrass, C.; Southworth, J.; Steele, I. A.; Surdej, J.; Thöne, C. C.; Wambsganss, J.; Zub, M.; Albrow, M. D.; Batista, V.; Beaulieu, J.-P.; Bennett, D. P.; Caldwell, J. A. R.; Cole, A. A.; Cook, K. H.; Coutures, C.; Dieters, S.; Prester, D. D.; Donatowicz, J.; Greenhill, J.; Kane, S. R.; Kubas, D.; Marquette, J.-B.; Martin, R.; Menzies, J.; Pollard, K. R.; Sahu, K. C.; Williams, A.; Szymański, M. K.; Kubiak, M.; Pietrzyński, G.; Soszyński, I.; Poleski, R.; Ulaczyk, K.; DePoy, D. L.; Dong, S.; Han, C.; Janczak, J.; Lee, C.-U.; Pogge, R. W.; Abe, F.; Furusawa, K.; Hearnshaw, J. B.; Itow, Y.; Kilmartin, P. M.; Korpela, A. V.; Lin, W.; Ling, C. H.; Masuda, K.; Matsubara, Y.; Miyake, N.; Muraki, Y.; Ohnishi, K.; Perrott, Y. C.; Saito, T.; Skuljan, L.; Sullivan, D. J.; Sumi, T.; Suzuki, D.; Sweatman, W. L.; Tristram, P. J.; Wada, K.; Yock, P. C. M.; Gulbis, A.; Hashimoto, Y.; Kniazev, A.; Vaisanen, P.

doi:10.1111/j.1365-2966.2012.21233.x

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OGLE-2008-BLG-510: first automated real-time detection of a weak microlensing anomaly - brown dwarf or stellar binary?

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Snodgrass, C.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Bozza, V., Dominik, M., Rattenbury, N. J., Jørgensen, U. G., Tsapras, Y., Bramich, D. M., et al. (2012). OGLE-2008-BLG-510: first automated real-time detection of a weak microlensing anomaly - brown dwarf or stellar binary? Mon. Not. Roy. Astron. Soc., 424, 902-918. doi:10.1111/j.1365-2966.2012.21233.x.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-09FB-F

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