Four microlensing planets with faint-source stars identified in the 2016 and 2017 season data

Aims. Microlensing planets occurring on faint-source stars can escape detection due to their weak signals. Occasionally, detections of such planets are not reported due to the difficulty of extracting high-profile scientific issues on the detected planets. Methods. For the solid demographic census o...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2020-10, Vol.642, p.A110
Hauptverfasser:	Han, Cheongho, Udalski, Andrzej, Kim, Doeon, Jung, Youn Kil, Ryu, Yoon-Hyun, Albrow, Michael D., Chung, Sun-Ju, Gould, Andrew, Hwang, Kyu-Ha, Lee, Chung-Uk, Shin, In-Gu, Shvartzvald, Yossi, Yee, Jennifer C., Zang, Weicheng, Cha, Sang-Mok, Kim, Dong-Jin, Kim, Hyoun-Woo, Kim, Seung-Lee, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Kim, Chun-Hwey, Kim, Woong-Tae, Mróz, Przemek, Szymański, Michał K., Skowron, Jan, Poleski, Radek, Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Ulaczyk, Krzysztof, Rybicki, Krzysztof A., Iwanek, Patryk, Wrona, Marcin
Format:	Artikel
Sprache:	eng
Schlagworte:	Galactic disk Lenses Light curve Microlenses Parameters Planetary systems Planets Stars
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