2023A&A...675A..36H


Query : 2023A&A...675A..36H

2023A&A...675A..36H - Astronomy and Astrophysics, volume 675A36 (2023/7-1)

KMT-2021-BLG-1150Lb: Microlensing planet detected through a densely covered planetary-caustic signal.

HAN C., JUNG Y.K., BOND I.A., GOULD A., CHUNG S.-J., ALBROW M.D., HWANG K.-H., RYU Y.-H., SHIN I.-G., SHVARTZVALD Y., YANG H., YEE J.C., ZANG W., CHA S.-M., KIM D., KIM D.-J., KIM S.-L., LEE C.-U., LEE D.-J., LEE Y., PARK B.-G., POGGE R.W., ABE F., BARRY R., BENNETT D.P., BHATTACHARYA A., FUJII H., FUKUI A., HAMADA R., HIRAO Y., ISHITANI SILVA S., ITOW Y., KIRIKAWA R., KONDO I., KOSHIMOTO N., MATSUBARA Y., MATSUMOTO S., MIYAZAKI S., MURAKI Y., OKAMURA A., OLMSCHENK G., RANC C., RATTENBURY N.J., SATOH Y., SUMI T., SUZUKI D., TODA T., TOMOYOSHI M., TRISTRAM P.J., VANDOROU A., YAMA H. and YAMASHITA K.

Abstract (from CDS):

Aims. Recently, there have been reports of various types of degeneracies in the interpretation of planetary signals induced by planetary caustics. In this work we check whether such degeneracies persist in the case of well-covered signals by analyzing the lensing event KMT-2021-BLG-1150, the light curve of which exhibits a densely and continuously covered short-term anomaly.
Methods. In order to identify degenerate solutions, we thoroughly investigated the parameter space by conducting dense grid searches for the lensing parameters. We then checked the severity of the degeneracy among the identified solutions.
Results. We identify a pair of planetary solutions resulting from the well-known inner-outer degeneracy, and find that interpreting the anomaly is not subject to any degeneracy other than the inner-outer degeneracy. The measured parameters of the planet separation (normalized to the Einstein radius) and mass ratio between the lens components are (s, q)in ∼ (1.297, 1.10 × 10–3) for the inner solution and (s, q)out ∼ (1.242, 1.15 × 10–3) for the outer solution. According to a Bayesian estimation, the lens is a planetary system consisting of a planet with a mass Mp = 0.88–0.36+0.38Mj and its host with a mass Mh = 0.73–0.30+0.32M⊙ lying toward the Galactic center at a distance DL = 3.8–1.2+1.3 kpc. By conducting analyses using mock data sets prepared to mimic those obtained with data gaps and under various observational cadences, we find that gaps in data can result in various degenerate solutions, while the observational cadence does not pose a serious degeneracy problem as long as the anomaly feature can be delineated.

Abstract Copyright: © The Authors 2023

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

Simbad objects: 20

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Number of rows : 20
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-0909 Lev 17 42 28.850 -27 38 20.90           ~ 2 0
2 KMT-2018-BLG-1497 Lev 17 44 20.190 -25 58 25.00           ~ 3 0
3 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
4 KMT-2016-BLG-1105 Lev 17 45 47.340 -26 15 58.93           ~ 6 0
5 OGLE-2017-BLG-1806 Lev 17 46 29.580 -24 16 20.17           ~ 7 0
6 NAME EWS 2005-BLG-071b Pl 17 50 09.77 -34 40 23.5           ~ 52 1
7 KMT-2018-BLG-0173 Lev 17 50 11.750 -21 35 40.56           ~ 2 0
8 KMT-2021-BLG-1554 * 17 51 12.820 -31 51 51.70           ~ 5 0
9 OGLE-2016-BLG-1266 BD? 17 51 24.86 -29 44 32.1           ~ 7 0
10 OGLE-2017-BLG-0173 * 17 51 52.95 -29 16 16.9           ~ 21 0
11 KMT-2021-BLG-1150 Lev 17 55 09.630 -31 18 47.99           ~ 2 0
12 KMT-2021-BLG-0712 Lev 17 57 08.560 -31 11 04.09           ~ 2 0
13 OGLE-2017-BLG-0373 * 17 57 19.06 -31 57 06.2           ~ 12 0
14 MOA 2003-BLG-53 * 18 05 16.35 -28 53 42.0           GIV 59 1
15 MOA 2003-BLG-53b Pl 18 05 16.35 -28 53 42.0           ~ 26 1
16 NAME EWS 2005-BLG-169b Pl 18 06 05.32 -30 43 57.5           ~ 42 1
17 MOA 2007-BLG-192b Pl 18 08 03.798 -27 09 00.27           ~ 33 1
18 KMT-2021-BLG-0748 Lev 18 09 41.120 -25 44 47.69           ~ 3 0
19 KMT-2017-BLG-1194 Lev 18 17 17.310 -25 19 26.18           ~ 5 0
20 NAME Galactic Bulge reg ~ ~           ~ 4794 0

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