2021AJ....162...17K

Query : 2021AJ....162...17K

2021AJ....162...17K - Astron. J., 162, 17-17 (2021/July-0)

KMT-2019-BLG-0371 and the limits of Bayesian analysis.

KIM Y.H., CHUNG S.-J., YEE J.C., UDALSKI A., BOND I.A., JUNG Y.K., GOULD A., ALBROW M.D., HAN C., HWANG K.-H., RYU Y.-H., SHIN I.-G., SHVARTZVALD Y., ZANG W., 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), POLESKI R., MROZ P., SKOWRON J., SZYMANSKI M.K., SOSZYNSKI I., PIETRUKOWICZ P., KOZLOWSKI S., ULACZYK K., RYBICKI K.A., IWANEK P., WRONA M., GROMADZKI M. (The OGLE Collaboration), ABE F., BARRY R., BENNETT D.P., BHATTACHARYA A., DONACHIE M., FUJII H., FUKUI A., ITOW Y., HIRAO Y., KIRIKAWA R., KONDO I., KOSHIMOTO N., MATSUBARA Y., MURAKI Y., MIYAZAKI S., RANC C., RATTENBURY N.J., SATOH Y., SHOJI H., SUMI T., SUZUKI D., TRISTRAM P.J., TANAKA Y., YAMAWAKI T., YONEHARA A. (The MOA Collaboration)

Abstract (from CDS):

We show that the perturbation at the peak of the light curve of microlensing event KMT-2019-BLG-0371 is explained by a model with a mass ratio between the host star and planet of q ∼ 0.08. Due to the short event duration (tE ∼ 6.5 days), the secondary object in this system could potentially be a massive giant planet. A Bayesian analysis shows that the system most likely consists of a host star with a mass Mh=0.09–0.05+0.14M☉ and a massive giant planet with a mass Mp=7.70–3.90+11.34MJup. However, the interpretation of the secondary as a planet (i.e., as having Mp < 13MJup) rests entirely on the Bayesian analysis. Motivated by this event, we conduct an investigation to determine which constraints meaningfully affect Bayesian analyses for microlensing events. We find that the masses inferred from such a Bayesian analysis are determined almost entirely by the measured value of θE and are relatively insensitive to other factors such as the direction of the event (l, b), the lens-source relative proper motion µrel, or the specific Galactic model prior.

Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.

Journal keyword(s): Binary lens microlensing

VizieR on-line data: <Available at CDS (J/AJ/162/17): fig1.dat>

Simbad objects: 54

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Number of rows : 54
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 OGLE-2011-BLG-0417 * 17 34 33.11 -27 06 39.3           ~ 17 0
2 KMT-2016-BLG-1089 * 17 42 23.31 -33 45 35.2           ~ 11 0
3 KMT-2016-BLG-2364 * 17 42 51.760 -27 26 08.02           ~ 6 0
4 OGLE-2019-BLG-1019 * 17 42 58.42 -25 34 26.1           ~ 8 0
5 KMT-2016-BLG-2397 * 17 44 51.010 -23 12 04.97           ~ 7 0
6 KMT-2016-BLG-1107 * 17 45 40.260 -26 01 54.48           ~ 13 0
7 MOA-bin-1 * 17 51 10.20 -29 47 38.3         23 ~ 26 1
8 KMT-2018-BLG-0748 * 17 51 29.880 -30 38 47.00           ~ 11 0
9 OGLE-2017-BLG-0604 * 17 51 34.00 -30 56 47.6           ~ 6 0
10 OGLE BLG-LPV-79048 LP* 17 51 51.32856 -30 27 31.3416     19.472   14.966 ~ 10 0
11 OGLE-2017-BLG-0173 * 17 51 52.95 -29 16 16.9           ~ 21 0
12 KMT-2016-BLG-2142 * 17 52 26.880 -29 23 04.42           ~ 8 0
13 MOA 2013-BLG-618 * 17 52 30.370 -30 17 33.70           ~ 6 0
14 MOA 2015-BLG-379 * 17 52 38.11 -28 33 06.9           ~ 8 0
15 OGLE-2008-BLG-513 * 17 52 43.51 -30 51 33.2           ~ 7 0
16 OGLE-2019-BLG-0505 * 17 53 32.140 -31 33 18.08           ~ 9 0
17 OGLE-2019-BLG-0763 * 17 53 50.030 -29 52 38.78           ~ 9 0
18 MOA 2009-BLG-411 * 17 53 58.400 -29 44 56.01           ~ 7 0
19 MOA 2008-BLG-310 * 17 54 14.53 -34 46 41.0           GV 51 1
20 OGLE-2005-BLG-390 * 17 54 19.2 -30 22 38           KIII 54 1
21 OGLE-2018-BLG-0677 * 17 55 00.270 -32 00 59.51           ~ 15 0
22 KMT-2016-BLG-1820 * 17 55 03.540 -29 31 00.91           ~ 9 0
23 OGLE-2015-BLG-1771 * 17 55 11.76 -28 51 45.9           ~ 8 0
24 MOA 2011-BLG-291 * 17 55 28.290 -29 10 14.38           ~ 6 0
25 MOA 2012-BLG-323 * 17 55 52.39 -29 49 06.7           ~ 7 0
26 MOA 2018-BLG-182 * 17 56 03.36 -29 04 58.4           ~ 26 0
27 MOA 2007-BLG-308 * 17 56 25.96 -32 14 14.7           GV 25 1
28 OGLE-2017-BLG-1375 * 17 56 37.17 -30 18 41.1           ~ 8 0
29 OGLE-2016-BLG-0613 ** 17 57 02.50 -28 06 58.2           ~ 29 0
30 OGLE-2006-BLG-238 * 17 57 11.66 -30 48 06.0           ~ 3 0
31 OGLE-2017-BLG-0373 * 17 57 19.06 -31 57 06.2           ~ 12 0
32 NAME MOA-bin-29 * 17 57 30.3406342848 -29 44 12.292325304           ~ 4 0
33 MOA 2014-BLG-547 * 17 57 38.160 -28 57 47.37           ~ 6 0
34 KMT-2017-BLG-0165 * 17 58 35.920 -28 08 01.21           ~ 4 0
35 KMT-2015-BLG-0048 * 17 58 39.01 -28 01 54.1           ~ 7 0
36 OGLE-2018-BLG-1269 * 17 58 46.42 -27 37 04.6           ~ 6 0
37 MOA 2008-BLG-379 * 17 58 49.435 -30 11 48.95           ~ 14 0
38 MOA 2013-BLG-148 ** 17 59 03.45552 -28 25 14.1348           ~ 6 0
39 MOA 2008-BLG-288 * 17 59 08.81 -30 45 34.1           ~ 14 0
40 OGLE-2008-BLG-210 * 17 59 22.97 -27 42 30.2           ~ 4 0
41 OGLE-2018-BLG-1700 * 17 59 49.45 -28 31 43.1           ~ 26 0
42 OGLE-2012-BLG-1323 * 18 00 18.51 -28 35 01.7           ~ 13 0
43 MOA 2011-BLG-262 * 18 00 23.480 -31 14 42.93           ~ 28 0
44 OGLE-2015-BLG-0954 * 18 00 44.24 -28 39 39.2           ~ 8 0
45 OGLE-2016-BLG-1540 * 18 00 47.00 -28 21 35.2           ~ 17 0
46 OGLE-2017-BLG-1522 * 18 01 16.65 -28 27 43.1           ~ 10 0
47 MOA 2015-BLG-404 * 18 04 49.210 -32 37 58.90           ~ 3 0
48 MOA 2011-BLG-322 * 18 04 53.630 -27 13 15.05           ~ 16 0
49 MOA 2010-BLG-353 * 18 05 12.940 -27 17 35.64           ~ 12 0
50 MOA 2003-BLG-53 * 18 05 16.35 -28 53 42.0           GIV 59 1
51 MOA 2009-BLG-319 * 18 06 58.0 -26 49 11           K 16 1
52 MOA 2015-BLG-337 * 18 07 47.71 -28 10 12.6           ~ 13 0
53 OGLE-2012-BLG-0838 * 18 12 00.7378 -25 42 41.790           ~ 7 0
54 NAME Galactic Bulge reg ~ ~           ~ 4794 0

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