OGLE-2014-BLG-1186: gravitational microlensing providing evidence for a planet orbiting the foreground star or for a close binary source?
Authors: Dominik, M., Bachelet, E., Bozza, V., Street, R. A., Han, C., Hundertmark, M., Udalski, A., Bramich, D. M., Alsubai, K. A., Calchi Novati, S., Ciceri, S., D'Ago, G., Figuera Jaimes, R., Haugbølle, T., Hinse, T. C., Horne, K., Jørgensen, U. G., Juncher, D., Kains, N., Korhonen, H., Mancini, L., Menzies, J., Popovas, A., Rabus, M., Rahvar, S., Scarpetta, G., Schmidt, R., Skottfelt, J., Snodgrass, C., Southworth, J., Starkey, D., Steele, I. A., Surdej, J., Tsapras, Y., Wambsganss, J., Wertz, O., Pietrukowicz, P., Szymański, M. K., Mróz, P., Skowron, J., Soszyński, I., Ulaczyk, K., Poleski, R., Wyrzykowski, Ł., Kozłowski, S.
Published in: Monthly Notices of the Royal Astronomical Society
Publication type: article
Subject areas: Earth and Planetary Sciences; Physics and Astronomy
SJR best quartile: Q1