SIMBAD references

2022A&A...658A..93H - Astronomy and Astrophysics, volume 658A93-93 (2022/2-1)

OGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star.

HAN C., UDALSKI A., LEE C.-U., KIM D., ZHU W., ALBROW M.D., CHUNG S.-J., GOULD A., HWANG K.-H., JUNG Y.K., KIM H.-W., RYU Y.-H., SHIN I.-G., SHVARTZVALD Y., YEE J.C., ZANG W., CHA S.-M., KIM D.-J., KIM S.-L., LEE D.-J., LEE Y., PARK B.-G., POGGE R.W., KIM C.-H., KIM W.-T., MROZ P., SZYMANSKI M.K., SKOWRON J., POLESKI R., SOSZYNSKI I., PIETRUKOWICZ P., KOZLOWSKI S., RYBICKI K.A., IWANEK P., ULACZYK K., WRONA M., GROMADZKI M., BUCKLEY D., DONG S. and LUO A.

Abstract (from CDS):


Aims. With the aim of interpreting anomalous lensing events with no suggested models, we conducted a project of reinvestigating microlensing data collected in and before the 2019 season. In this work, we report a multi-planet system, OGLE-2019-BLG-0468L, that was found as a result of this project.
Methods. The light curve of the lensing event OGLE-2019-BLG-0468, which consists of three distinctive anomaly features, could not be explained by the usual binary-lens or binary-source interpretations. We find a solution that explains all anomaly features with a triple-lens interpretation, in which the lens is composed of two planets and their host, making the lens the fourth multi-planet system securely found by microlensing.
Results. The two planets have masses of ∼3.4 MJ and ∼10.2 MJ, and they are orbiting around a G-type star with a mass of ∼0.9 M☉ and a distance of ∼4.4 kpc. The host of the planets is most likely responsible for the light of the baseline object, although the possibility of the host being a companion to the baseline object cannot be ruled out.

Abstract Copyright: © ESO 2022

Journal keyword(s): gravitational lensing: micro - planets and satellites: detection

Simbad objects: 31

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