Authors

Andrew Gould, Max Planck Institute for Astronomy
Cheongho Han, Chungbuk National University
Weicheng Zang, Tsinghua University
Hongjing Yang, Tsinghua University
Kyu Ha Hwang, Korea Astronomy and Space Science Institute
Andrzej Udalski, University of Warsaw
Ian A. Bond, Massey University Auckland
Michael D. Albrow, University of Canterbury
Sun Ju Chung, Korea Astronomy and Space Science Institute
Youn Kil Jung, Korea Astronomy and Space Science Institute
Yoon Hyun Ryu, Korea Astronomy and Space Science Institute
In Gu Shin, Chungbuk National University
Yossi Shvartzvald, Weizmann Institute of Science Israel
Jennifer C. Yee, Harvard-Smithsonian Center for Astrophysics
Sang Mok Cha, Korea Astronomy and Space Science Institute
Dong Jin Kim, Korea Astronomy and Space Science Institute
Hyoun Woo Kim, Korea Astronomy and Space Science Institute
Seung Lee Kim, Korea Astronomy and Space Science Institute
Chung Uk Lee, Korea Astronomy and Space Science Institute
Dong Joo Lee, Korea Astronomy and Space Science Institute
Yongseok Lee, Korea Astronomy and Space Science Institute
Byeong Gon Park, Korea Astronomy and Space Science Institute
Richard W. Pogge, The Ohio State University
Przemek Mróz, University of Warsaw
Michal K. Szymanski, University of Warsaw
Jan Skowron, University of Warsaw
Radek Poleski, University of Warsaw
Igor Soszynski, University of Warsaw
Pawel Pietrukowicz, University of Warsaw
Szymon Kozlowski, University of Warsaw
Krzysztof Ulaczyk, Faculty of Science, Engineering and Medicine
Krzysztof A. Rybicki, University of Warsaw
Patryk Iwanek, University of Warsaw

Document Type

Article

Publication Date

8-1-2022

Abstract

We complete the analysis of all 2018 prime-field microlensing planets identified by the Korea Microlensing Telescope Network (KMTNet) Anomaly Finder. Among the ten previously unpublished events with clear planetary solutions, eight are either unambiguously planetary or are very likely to be planetary in nature: OGLE-2018-BLG-1126, KMT-2018-BLG-2004, OGLE-2018-BLG-1647, OGLE-2018-BLG-1367, OGLE-2018-BLG-1544, OGLE-2018-BLG-0932, OGLE-2018-BLG-1212, and KMT-2018-BLG-2718. Combined with the four previously published new Anomaly Finder events and 12 previously published (or in preparation) planets that were discovered by eye, this makes a total of 24 2018 prime-field planets discovered or recovered by Anomaly Finder. Together with a paper in preparation on 2018 subprime planets, this work lays the basis for the first statistical analysis of the planet mass-ratio function based on planets identified in KMTNet data. By systematically applying the heuristic analysis to each event, we identified the small modification in their formalism that is needed to unify the so-called close-wide and inner-outer degeneracies.

Publication Source (Journal or Book title)

Astronomy and Astrophysics

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