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The 2L1S/1L2S Degeneracy for Two Microlensing Planet Candidates Discovered by the KMTNet Survey in 2017We report two microlensing planet candidates discovered by the Korea Microlensing Telescope Network (KMTNet) survey in 2017. However, both events have the 2L1S/1L2S degeneracy, which is an obstacle to claiming the discovery of the planets with certainty unless the degeneracy can be resolved. For KMT-2017-BLG-0962, the degeneracy cannot be resolved. If the 2L1S solution is correct, KMT-2017-BLG-0962 might be produced by a super Jupiter-mass planet orbiting a mid-M-dwarf host star. For KMT-2017-BLG-1119, the light-curve modeling favors the 2L1S solution but higher-resolution observations of the baseline object tend to support the 1L2S interpretation rather than the planetary interpretation. This degeneracy might be resolved by a future measurement of the lens-source relative proper motion. This study shows that the problem of resolving 2L1S/1L2S degeneracy exists over a much wider range of conditions than those considered by the theoretical study of Gaudi (1998).
Document ID
20205002080
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
I.-G. Shin
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
J. C. Yee
(Harvard-Smithsonian Center for Astrophysics Cambridge, Massachusetts, United States)
A. Gould
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
M. T. Penny
(The Ohio State University Columbus, Ohio, United States)
I. A. Bond
(Massey University Palmerston North, New Zealand)
M. D. Albrow
(University of Canterbury Christchurch, New Zealand)
S.-J. Chung
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
C. Han
(Chungbuk National University Cheongju-si, South Korea)
K.-H. Hwang
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
Y. K. Jung
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
Y.-H. Ryu
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
Y. Shvartzvald
(California Institute of Technology Pasadena, California, United States)
S.-M. Cha
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
D.-J. Kim
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
H.-W. Kim
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
S.-L. Kim
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
C.-U. Lee
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
D.-J. Lee
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
Y. Lee
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
B.-G. Park
(Korea Astronomy and Space Science Institute Daejeon, South Korea)
R. W. Pogge
(The Ohio State University Columbus, Ohio, United States)
F. Abe
(Nagoya University Nagoya, Japan)
R Barry
(Goddard Space Flight Center Greenbelt, Maryland, United States)
D P Bennett
(University of Maryland, College Park College Park, Maryland, United States)
A Bhattacharya
(University of Maryland, College Park College Park, Maryland, United States)
M. Donachie
(University of Auckland Auckland, New Zealand)
H. Fujii
(Nagoya University Nagoya, Japan)
A. Fukui
(National Astronomical Observatory of Japan Mitaka-shi, Japan)
Y. Hirao
(Osaka University Osaka, Japan)
Y. Itow
(Nagoya University Nagoya, Japan)
Y. Kamei
(Nagoya University Nagoya, Japan)
Iona Kondo
(Osaka University Osaka, Japan)
N. Koshimoto
(Osaka University Osaka, Japan)
M. C. A. Li
(University of Auckland Auckland, New Zealand)
Y. Matsubara
(Nagoya University Nagoya, Japan)
S. Miyazaki
(Osaka University Osaka, Japan)
Y. Muraki
(Nagoya University Nagoya, Japan)
M. Nagakane
(Osaka University Osaka, Japan)
C Ranc
(Goddard Space Flight Center Greenbelt, Maryland, United States)
N. J. Rattenbury
(University of Auckland Auckland, New Zealand)
Harmon Suematsu
(Osaka University Osaka, Japan)
D. J. Sullivan
(Victoria University Kampala, Uganda)
T. Sumi
(Osaka University Osaka, Japan)
Daisuke Suzuki
(Institute of Space and Astronautical Science Tokyo, Japan)
P. J. Tristram
(University of Canterbury Christchurch, New Zealand)
T. Yamakawa
(Nagoya University Nagoya, Japan)
A. Yonehara
(Kyoto Sangyo University Kyoto, Kyôto, Japan)
P. Fouqué
(Canada–France–Hawaii Telescope Waimea, Hawaii, United States)
W. Zang
(Tsinghua University Beijing, Beijing, China)
Date Acquired
May 12, 2020
Publication Date
October 24, 2019
Publication Information
Publication: The Astronomical Journal
Publisher: The American Astronomical Society
Volume: 158
Issue: 5
Issue Publication Date: November 1, 2019
ISSN: 0004-6256
e-ISSN: 1538-3881
Subject Category
Astrophysics
Astronomy
Funding Number(s)
WBS: 134180.04.04.01
CONTRACT_GRANT: JPL 1500811
CONTRACT_GRANT: AST-1516842
CONTRACT_GRANT: FP 7 ERC 321035
CONTRACT_GRANT: 2017R1A4A1015178
CONTRACT_GRANT: NNX16AC62G
CONTRACT_GRANT: NNG16PJ32C
CONTRACT_GRANT: JSPS24253004
CONTRACT_GRANT: JSPS26247023
CONTRACT_GRANT: JSPS23340064
CONTRACT_GRANT: JSPS15H00781
CONTRACT_GRANT: JP16H06287
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
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