OGLE-2014-BLG-1186: gravitational microlensing providing evidence for a planet orbiting the foreground star or for a close binary source?

Research output: Contribution to journalJournal articleResearchpeer-review

M. Dominik, E. Bachelet, V. Bozza, R. A. Street, C. Han, M. Hundertmark, A. Udalski, D. M. Bramich, K. A. Alsubai, S. Calchi Novati, S. Ciceri, G. D'Ago, R. Figuera Jaimes, T. Haugbolle, T. C. Hinse, K. Horne, U. G. Jorgensen, D. Juncher, N. Kains, H. Korhonen & 25 others L. Mancini, J. Menzies, A. Popovas, M. Rabus, S. Rahvar, G. Scarpetta, R. Schmidt, J. Skottfelt, C. Snodgrass, J. Southworth, D. Starkey, I. A. Steele, J. Surdej, Y. Tsapras, J. Wambsganss, O. Wertz, P. Pietrukowicz, M. K. Szymanski, P. Mroz, J. Skowron, I. Soszynski, K. Ulaczyk, R. Poleski, L. Wyrzykowski, S. Kozlowski

Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume484
Issue number4
Pages (from-to)5608-5632
ISSN0035-8711
DOIs
Publication statusPublished - Apr 2019

    Research areas

  • gravitational lensing: micro, methods: data analysis, methods: statistical, planets and satellites: detection, (stars:) binaries: eclipsing, Galaxy: kinematics and dynamics

ID: 225759459