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

  • The KMTNet Collaboration
  • , The MAP, μFUN Follow-up Teams
  • , The Moa Collaboration.
  • Department of Astronomy
  • Tsinghua University
  • Max Planck Institute for Astronomy
  • Department of Astronomy
  • Ohio State University
  • Harvard-Smithsonian Center for Astrophysics
  • Korea Astronomy and Space Science Institute
  • Auckland Observatory
  • Department of Earth and Space Science
  • The University of Osaka
  • CAS - National Astronomical Observatories
  • Dept. of Physics and Astronomy
  • University of Canterbury
  • University of Science and Technology UST
  • Department of Physics
  • Chungbuk National University
  • Department of Particle Physics and Astrophysics
  • Weizmann Institute of Science
  • School of Space Research
  • Kyung Hee University
  • Possum Observatory
  • Centre for Backyard Astrophysics
  • Auckland University of Technology
  • Department of Physics & Astronomy
  • Louisiana State University
  • Massey University
  • Institute for Space-Earth Environmental Research
  • Nagoya University
  • NASA Goddard Space Flight Center
  • University of Maryland, College Park
  • Department of Physics
  • The University of Auckland
  • Department of Earth and Planetary Science
  • The University of Tokyo
  • Instituto de Astrofísica de Canarias
  • Department of Astronomy
  • National Institutes of Natural Sciences - National Astronomical Observatory of Japan

Research output: Contribution to journal › Article › peer-review

20 Scopus citations

Abstract

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.

Original languageEnglish
Pages (from-to)1894-1909
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Volume516
Issue number2
DOIs
StatePublished - 1 Oct 2022

Funding

FundersFunder number
SAAO
CTIO
National Research Foun
Korea Astronomy and Space Science Institute
National Research Foundation of KoreaCMS-CSST-2021-A11
Tsinghua University2019Z07L02017
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National Natural Science Foundation of China12133005, JP17H02871, JSPS24253004, JP19KK0082, JSPS15H00781, JSPS23340064, JSPS26247023, JP16H06287
National Science FoundationAST-2108414
Scleroderma Society of OntarioJSPS24253004, JSPS23340064, JSPS26247023

    Keywords

    • gravitational lensing: micro
    • planets
    • satellites: detection

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