OGLE-2019-BLG-0960 Lb: the Smallest Microlensing Planet-Reference-Cited by-同舟云学术

OGLE-2019-BLG-0960 Lb: the Smallest Microlensing Planet

Published:2021-10-06 Issue:5 Volume:162 Page:180
ISSN:0004-6256
Container-title:The Astronomical Journal
language:
Short-container-title:AJ

Author:

Yee Jennifer C.^ORCID,Zang Weicheng^ORCID,Udalski Andrzej^ORCID,Ryu Yoon-Hyun^ORCID,Green Jonathan,Hennerley Steve,Marmont Andrew,Sumi Takahiro^ORCID,Mao Shude^ORCID,Gromadzki Mariusz^ORCID,Mróz Przemek^ORCID,Skowron Jan^ORCID,Poleski Radoslaw^ORCID,Szymański Michał K.^ORCID,Soszyński Igor^ORCID,Pietrukowicz Paweł^ORCID,Kozłowski Szymon^ORCID,Ulaczyk Krzysztof^ORCID,Rybicki Krzysztof A.,Iwanek Patryk^ORCID,Wrona Marcin^ORCID,Albrow Michael D.^ORCID,Chung Sun-Ju^ORCID,Gould Andrew,Han Cheongho^ORCID,Hwang Kyu-Ha^ORCID,Jung Youn Kil,Kim Hyoun-Woo^ORCID,Shin In-Gu^ORCID,Shvartzvald Yossi^ORCID,Cha Sang-Mok,Kim Dong-Jin,Kim Seung-Lee^ORCID,Lee Chung-Uk^ORCID,Lee Dong-Joo,Lee Yongseok,Park Byeong-Gon^ORCID,Pogge Richard W.^ORCID,Bachelet Etienne^ORCID,Christie Grant,Hundertmark Markus P. G.,Maoz Dan^ORCID,McCormick Jennie,Natusch Tim,Penny Matthew T.^ORCID,Street Rachel A.^ORCID,Tsapras Yiannis^ORCID,Beichman Charles A.,Bryden Geoffery^ORCID,Novati Sebastiano Calchi,Carey Sean,Gaudi B. Scott^ORCID,Henderson Calen B.^ORCID,Johnson Samson,Zhu Wei,Bond Ian A.,Abe Fumio,Barry Richard^ORCID,Bennett David P.^ORCID,Bhattacharya Aparna,Donachie Martin,Fujii Hirosane,Fukui Akihiko^ORCID,Hirao Yuki^ORCID,Silva Stela Ishitani,Itow Yoshitaka^ORCID,Kirikawa Rintaro,Kondo Iona^ORCID,Koshimoto Naoki^ORCID,Alex Li Man Cheung,Matsubara Yutaka,Muraki Yasushi^ORCID,Miyazaki Shota^ORCID,Olmschenk Greg^ORCID,Ranc Clément^ORCID,Rattenbury Nicholas J.^ORCID,Satoh Yuki,Shoji Hikaru,Suzuki Daisuke^ORCID,Tanaka Yuzuru,Tristram Paul J.,Yamawaki Tsubasa,Yonehara Atsunori

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-3881/ac1582/pdf

Reference77 articles.

1. Extending the planetary mass function to Earth mass by microlensing at moderately high magnification

2. Predicting stellar angular diameters from V, IC, H and K photometry

3. Image subtraction using a space-varying kernel

4. A Method for Optimal Image Subtraction

5. Difference imaging photometry of blended gravitational microlensing events with a numerical kernel

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