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

Author:

Yang HongjingORCID,Zang WeichengORCID,Gould Andrew12,Yee Jennifer C3ORCID,Hwang Kyu-Ha4,Christie Grant5,Sumi Takahiro6,Zhang JiyuanORCID,Mao ShudeORCID,Albrow Michael D7ORCID,Chung Sun-Ju48,Han Cheongho9,Jung Youn Kil4,Ryu Yoon-Hyun4,Shin In-Gu39,Shvartzvald Yossi10,Cha Sang-Mok411,Kim Dong-Jin4,Kim Hyoun-Woo4,Kim Seung-Lee48,Lee Chung-Uk4,Lee Dong-Joo4,Lee Yongseok411,Park Byeong-Gon48,Pogge Richard W24,Drummond John12,Maoz Dan13,McCormick Jennie14,Natusch Tim515,Penny Matthew T16ORCID,Zhu Wei,Bond Ian A17,Abe Fumio18,Barry Richard19,Bennett David P1920,Bhattacharya Aparna1920,Donachie Martin21,Fujii Hirosane6,Fukui Akihiko2223,Hirao Yuki6,Itow Yoshitaka618,Kirikawa Rintaro6,Kondo Iona6,Koshimoto Naoki2425,Li Man Cheung Alex21,Matsubara Yutaka18,Muraki Yasushi18,Miyazaki Shota6,Olmschenk Greg19,Ranc Clément19,Rattenbury Nicholas J21,Satoh Yuki6,Shoji Hikaru6,Silva Stela Ishitani2619,Suzuki Daisuke27,Tanaka Yuzuru6,Tristram Paul J28,Yamawaki Tsubasa6,Yonehara Atsunori29, , , ,

Affiliation:

1. Max-Planck-Institute for Astronomy , Königstuhl 17, D-69117 Heidelberg, Germany

2. Department of Astronomy, Ohio State University , 140 W. 18th Ave., Columbus, OH 43210, USA

3. Center for Astrophysics | Harvard & Smithsonian 60 Garden St. , Cambridge, MA 02138, USA

4. Korea Astronomy and Space Science Institute , Daejon 34055, Republic of Korea

5. Auckland Observatory , Auckland 1023, New Zealand

6. Department of Earth and Space Science, Graduate School of Science , Osaka University, Toyonaka, Osaka 560-0043, Japan

7. University of Canterbury, Department of Physics and Astronomy , Private Bag 4800, Christchurch 8020, New Zealand

8. University of Science and Technology , Korea, (UST), 217 Gajeong-ro Yuseong-gu, Daejeon 34113, Republic of Korea

9. Department of Physics, Chungbuk National University , Cheongju 28644, Republic of Korea

10. Department of Particle Physics and Astrophysics, Weizmann Institute of Science , Rehovot 76100, Israel

11. School of Space Research, Kyung Hee University , Yongin, Kyeonggi 17104, Republic of Korea

12. Possum Observatory , Patutahi, Gisbourne, New Zealand

13. School of Physics and Astronomy, Tel-Aviv University , Tel-Aviv 6997801, Israel

14. Farm Cove Observatory, Centre for Backyard Astrophysics , Pakuranga, Auckland 2010, New Zealand

15. Institute for Radio Astronomy and Space Research (IRASR) , AUT University, Auckland 1142, New Zealand

16. Department of Physics and Astronomy, Louisiana State University , Baton Rouge, LA 70803 USA

17. Institute of Natural and Mathematical Sciences, Massey University , Auckland 0745, New Zealand

18. Institute for Space-Earth Environmental Research, Nagoya University , Nagoya 464-8601, Japan

19. Code 667 , NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA

20. Department of Astronomy, University of Maryland , College Park, MD 20742, USA

21. Department of Physics, University of Auckland , Private Bag 92019, Auckland, New Zealand

22. Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo , 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

23. Instituto de Astrofísica de Canarias , Vía Láctea s/n, E-38205 La Laguna, Tenerife, Spain

24. Department of Astronomy, Graduate School of Science, The University of Tokyo , 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

25. National Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

26. Department of Physics, The Catholic University of America , Washington, DC 20064, USA

27. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency , 3-1-1 Yoshinodai, Chuo, Sagamihara, Kanagawa, 252-5210, Japan

28. University of Canterbury Mt. John Observatory , PO Box 56, Lake Tekapo 8770, New Zealand

29. Department of Physics, Faculty of Science, Kyoto Sangyo University , 603-8555 Kyoto, Japan

Abstract

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.

Funder

National Natural Science Foundation of China

Korea Astronomy and Space Science Institute

JSPS

NSF

National Research Foundation of Korea

Tsinghua University

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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