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2019MNRAS.484.5608D - Mon. Not. R. Astron. Soc., 484, 5608-5632 (2019/April-3)
OGLE-2014-BLG-1186: gravitational microlensing providing evidence for a planet orbiting the foreground star or for a close binary source?
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., HAUGBOLLE T., HINSE T.C., HORNE K., JORGENSEN 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., SZYMANSKI M.K., MROZ P., SKOWRON J., SOSZYNSKI I., ULACZYK K., POLESKI R., WYRZYKOWSKI L. and KOZLOWSKI S.
Abstract (from CDS):
Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): gravitational lensing: micro - methods: data analysis - methods: statistical - planets and satellites: detection - (stars:) binaries: eclipsing - Galaxy: kinematics and dynamics
Simbad objects: 2
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