SIMBAD references

2022MNRAS.515..928Z - Mon. Not. R. Astron. Soc., 515, 928-939 (2022/September-1)

Systematic KMTNet planetary anomaly search. IV. Complete sample of 2019 prime-field.

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

Abstract (from CDS):

We report the complete statistical planetary sample from the prime fields (Γ >= 2 h–1) of the 2019 Korea Microlensing Telescope Network (KMTNet) microlensing survey. We develop the optimized KMTNet AnomalyFinder algorithm and apply it to the 2019 KMTNet prime fields. We find a total of 13 homogeneously selected planets and report the analysis of three planetary events, KMT-2019-BLG-(1042,1552,2974). The planet-host mass ratios, q, for the three planetary events are 6.34 x 10–4, 4.89 x 10–3, and 6.18 x 10–4, respectively. A Bayesian analysis indicates the three planets are all cold giant planets beyond the snow line of their host stars. The 13 planets are basically uniform in log q over the range -5.0 < log q < -1.5. This result suggests that the planets below qbreak = 1.7 x 10–4 proposed by the MOA-II survey may be more common than previously believed. This work is an early component of a large project to determine the KMTNet mass-ratio function, and the whole sample of 2016-2019 KMTNet events should contain about 120 planets.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

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

Simbad objects: 24

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