Authors

Youn Kil Jung, Korea Astronomy and Space Science Institute
Weicheng Zang, Tsinghua University
Hanyue Wang, Harvard-Smithsonian Center for Astrophysics
Cheongho Han, Chungbuk National University
Andrew Gould, Max Planck Institute for Astronomy
Andrzej Udalski, University of Warsaw
Wei Zhu, Tsinghua University
Michael D. Albrow, University of Canterbury
Sun Ju Chung, Korea Astronomy and Space Science Institute
Kyu Ha Hwang, Korea Astronomy and Space Science Institute
Yoon Hyun Ryu, Korea Astronomy and Space Science Institute
In Gu Shin, Harvard-Smithsonian Center for Astrophysics
Yossi Shvartzvald, Weizmann Institute of Science Israel
Hongjing Yang, Tsinghua University
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
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
Dan Maoz, Tel Aviv University
Michał K. Szymański, University of Warsaw
Jan Skowron, University of Warsaw
Radek Poleski, University of Warsaw
Igor Soszyński, University of Warsaw
Paweł Pietrukowicz, University of Warsaw
Szymon Kozłowski, 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

6-1-2023

Abstract

We complete the publication of all microlensing planets (and “possible planets”) identified by the uniform approach of the KMT AnomalyFinder system in the 21 KMT subprime fields during the 2019 observing season, namely, KMT-2019-BLG-0298, KMT-2019-BLG-1216, KMT-2019-BLG-2783, OGLE-2019-BLG-0249, and OGLE-2019-BLG-0679 (planets), as well as OGLE-2019-BLG-0344 and KMT-2019-BLG-0304 (possible planets). The five planets have mean log mass ratio measurements of (−2.6, −3.6, −2.5, −2.2, −2.3), median mass estimates of (1.81, 0.094, 1.16, 7.12, 3.34) M Jup, and median distance estimates of (6.7, 2.7, 5.9, 6.4, 5.6) kpc, respectively. The main scientific interest of these planets is that they complete the AnomalyFinder sample for 2019, which has a total of 25 planets that are likely to enter the statistical sample. We find statistical consistency with the previously published 33 planets from the 2018 AnomalyFinder analysis according to an ensemble of five tests. Of the 58 planets from 2018-2019, 23 were newly discovered by AnomalyFinder. Within statistical precision, half of the planets have caustic crossings, while half do not; an equal number of detected planets result from major- and minor-image light-curve perturbations; and an equal number come from KMT prime fields versus subprime fields.

Publication Source (Journal or Book title)

Astronomical Journal

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