Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Mass Production of 2023 KMTNet Microlensing Planets. I. Low Mass Ratio

  • Authors: Yoon-Hyun Ryu, Andrzej Udalski, Hongjing Yang, Kyu-Ha Hwang, Weicheng Zang, Yang Huang, Andrew Gould, Michael D. Albrow, Ping Chen, Sun-Ju Chung, Subo Dong, Cheongho Han, Youn Kil Jung, In-Gu Shin, Yossi Shvartzvald, Jennifer C. Yee, Sang-Mok Cha, Dong-Jin Kim, Seung-Lee Kim, Chung-Uk Lee, Dong-Joo Lee, Yongseok Lee, Byeong-Gon Park, Richard W. Pogge, Przemek Mróz, Radosław Poleski, Jan Skowron, Michał K. Szymański, Igor Soszyński, Paweł Pietrukowicz, Szymon Kozłowski, Krzysztof Ulaczyk, Krzysztof A. Rybicki, Patryk Iwanek, Marcin Wrona, Mariusz Gromadzki, Mateusz J. Mróz

Yoon-Hyun Ryu et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 9.

The spectrum of KMT-2023-BLG-0164 with the best-matched template. The black line shows the observed spectrum of the target obtained with IMACS, while the red line represents one of the best-matched MILES template spectrum (HD186427; Teff = 5762 K, ﹩\mathrm{log}\,g=4.43﹩, and [Fe/H] = 0.07), convolved to a resolution of R = 1000. All spectra are continuum normalized. The three shaded regions indicate the masked wavelength ranges affected by interstellar absorption features, including the Na I D doublet and the DIBs at 5780 and 6283 Å.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse