2022MNRAS.516.1894Y


Query : 2022MNRAS.516.1894Y

2022MNRAS.516.1894Y - Mon. Not. R. Astron. Soc., 516, 1894-1909 (2022/October-3)

KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: two microlensing planets in the KMTNet high-cadence fields with followup observations.

YANG H., ZANG W., GOULD A., YEE J.C., HWANG K.-H., CHRISTIE G., SUMI T., ZHANG J., MAO S. (The Leading Authors), ALBROW M.D., CHUNG S.-J., HAN C., JUNG Y.K., RYU Y.-H., SHIN I.-G., SHVARTZVALD Y., CHA S.-M., KIM D.-J., KIM H.-W., KIM S.-L., LEE C.-U., LEE D.-J., LEE Y., PARK B.-G., POGGE R.W. (The KMTNet Collaboration), DRUMMOND J., MAOZ D., McCORMICK J., NATUSCH T., PENNY M.T., ZHU W. (The MAP and {mu}FUN Follow-up Teams), BOND I.A., ABE F., BARRY R., BENNETT D.P., BHATTACHARYA A., DONACHIE M., FUJII H., FUKUI A., HIRAO Y., ITOW Y., KIRIKAWA R., KONDO I., KOSHIMOTO N., LI M.C.A., MATSUBARA Y., MURAKI Y., MIYAZAKI S., OLMSCHENK G., RANC C., RATTENBURY N.J., SATOH Y., SHOJI H., ISHITANI SILVA S., SUZUKI D., TANAKA Y., TRISTRAM P.J., YAMAWAKI T., YONEHARA A. (The MOA Collaboration)

Abstract (from CDS):

Follow-up observations of high-magnification gravitational microlensing events can fully exploit their intrinsic sensitivity to detect extrasolar planets, especially those with small mass ratios. To make followup observations more uniform and efficient, we develop a system, HighMagFinder, to automatically alert possible ongoing high-magnification events based on the real-time data from the Korea Microlensing Telescope Network (KMTNet). We started a new phase of follow-up observations with the help of HighMagFinder in 2021. Here we report the discovery of two planets in high-magnification microlensing events, KMT-2021-BLG-0171 and KMT-2021-BLG-1689, which were identified by the HighMagFinder. We find that both events suffer the 'central-resonant' caustic degeneracy. The planet-host mass-ratio is q ∼ 4.7 × 10–5 or q ∼ 2.2 × 10–5 for KMT-2021-BLG-0171, and q ∼ 2.5 × 10–4 or q ∼ 1.8 × 10–4 for KMT-2021-BLG-1689. Together with two other events, four cases that suffer such degeneracy have been discovered in the 2021 season alone, indicating that the degenerate solutions may have been missed in some previous studies. We also propose a quantitative factor to weight the probability of each solution from the phase space. The resonant interpretations for the two events are disfavoured under this consideration. This factor can be included in future statistical studies to weight degenerate solutions.

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: 17

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Number of rows : 17
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 KMT-2021-BLG-0247b Pl? 17 37 55.890 -27 23 56.29           ~ 1 0
2 OGLE-2011-BLG-0251 * 17 38 14.1795898344 -27 08 10.054235616           ~ 8 1
3 KMT-2021-BLG-0240 * 17 50 18.550 -30 00 17.89           ~ 12 0
4 KMT-2021-BLG-1253 Lev 17 50 28.130 -29 16 45.41           ~ 7 0
5 KMT-2021-BLG-0185c Pl? 17 53 43.860 -32 24 45.22           ~ 1 0
6 KMT-2021-BLG-0185b Pl? 17 53 43.860 -32 24 45.22           ~ 1 0
7 KMT-2021-BLG-0171b Pl? 17 56 58.180 -30 05 34.58           ~ 3 0
8 KMT-2021-BLG-0171 Lev 17 56 58.180 -30 05 34.58           ~ 9 0
9 KMT-2021-BLG-1689 Lev 17 58 18.620 -30 08 43.12           ~ 6 0
10 KMT-2021-BLG-1689b Pl? 17 58 18.620 -30 08 43.12           ~ 2 0
11 MOA 2011-BLG-262 * 18 00 23.480 -31 14 42.93           ~ 28 0
12 OGLE-2019-BLG-1053 * 18 00 39.93 -27 20 29.7           ~ 12 0
13 KMT-2021-BLG-1391 Lev 18 02 44.060 -28 03 37.80           ~ 11 0
14 NAME Baade Window reg 18 03.5 -30 01           ~ 643 3
15 MOA 2007-BLG-192 * 18 08 03.798 -27 09 00.27           ~ 56 1
16 KMT-2021-BLG-1547b Pl? 18 09 35.900 -29 05 02.18           ~ 2 0
17 NAME Galactic Bulge reg ~ ~           ~ 4794 0

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