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Browsing by Author "Burdullis, Todd"

Browsing by Author "Burdullis, Todd"

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  • An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb 
    Zang, Weicheng; Han, Cheongho; Kondo, Iona; Yee, Jennifer C.; Lee, Chung-Uk; Gould, Andrew; Mao, Shude; de Almeida, Leandro; Shvartzvald, Yossi; Zhang, Xiangyu; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Jung, Youn Kil; Ryu, Yoon-Hyun; Shin, In-Gu; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; Drummond, John; Tan, Thiam-Guan; do Nascimento, José Dias, Jr.; Maoz, Dan; Penny, Matthew T.; Zhu, Wei; Bond, Ian A.; Abe, Fumio; Barry, Richard; Bennett, David P.; Bhattacharya, Aparna; Donachie, Martin; Fujii, Hirosane; Fukui, Akihiko; Hirao, Yuki; Itow, Yoshitaka; Kirikawa, Rintaro; Koshimoto, Naoki; Alex Li, Man Cheung; Matsubara, Yutaka; Muraki, Yasushi; Miyazaki, Shota; Olmschenk, Greg; Ranc, Clément; Rattenbury, Nicholas J.; Satoh, Yuki; Shoji, Hikaru; Silva, Stela Ishitani; Sumi, Takahiro; Suzuki, Daisuke; Tanaka, Yuzuru; Tristram, Paul J.; Yamawaki, Tsubasa; Yonehara, Atsunori; Petric, Andreea; Burdullis, Todd; Fouqué, Pascal (2021)
    We report the discovery of KMT-2020-BLG-0414Lb, with a planet-to-host mass ratio q<SUB>2</SUB> = 0.9-1.2 × 10<SUP>-5</SUP> = 3-4 ? at 1s, which is the lowest mass-ratio microlensing planet to date. Together with two other ...
  • KMT-2018-BLG-0029Lb: A Very Low Mass-Ratio Spitzer Microlens Planet 
    Gould, Andrew; Ryu, Yoon-Hyun; Calchi Novati, Sebastiano; Zang, Weicheng; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha; Jung, Youn Kil; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; Beichman, Charles; Bryden, Geoff; Carey, Sean; Gaudi, B. Scott; Henderson, Calen B.; Zhu, Wei; Fouque, Pascal; Penny, Matthew T.; Petric, Andreea; Burdullis, Todd; Mao, Shude (2020)
    At q = (1.81+/-0.20)*10^-5, KMT-2018-BLG-0029Lb has the lowest planet-host mass ratio q of any microlensing planet to date by more than a factor of two. Hence, it is the first planet that probes below the apparent ...

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