activity
20002023
most citedKilonova from post-merger ejecta as an optical and near-infrared counterpart of GW170817

340 citations · 3.2k across the 80 of their papers we have counts for

collaborators

81 papers

astro-ph.EP2023

Two long-period giant planets around two giant stars: HD 112570 and HD 154391

Guang-Yao Xiao, Huan-Yu Teng, Jianzhao Zhou +24

We present the discoveries of two giant planets orbiting the red giant branch (RGB) star HD 112570 and the red clump (RC) star HD 154391, based on the radial velocity (RV) measurem…

astro-ph.EP2023

Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars

Huan-Yu Teng, Bun'ei Sato, Masayuki Kuzuhara +15

In this study, we revisit 32 planetary systems around evolved stars observed within the framework of the Okayama Planet Search Program and its collaborative framework of the EAPS-N…

astro-ph.HE2022★ 19 cited

Narrow Fe-K Reverberation Mapping Unveils the Deactivated Broad-Line Region in a Changing-Look Active Galactic Nucleus

Hirofumi Noda, Taisei Mineta, Takeo Minezaki +11

"Changing-look active galactic nuclei" (CLAGNs) are known to change their apparent types between types 1 and 2, usually accompanied by a drastic change in their luminosity on times…

astro-ph.EP2022★ 3 cited

A Close-in Planet Orbiting Giant Star HD 167768

Huan-Yu Teng, Bun'ei Sato, Masanobu Kunitomo +12

We report the detection of a giant planet orbiting a G-type giant star HD 167768 from radial velocity measurements using HIgh Dispersion Echelle Spectrograph (HIDES) at Okayama Ast…

astro-ph.EP2022★ 3 cited

A Trio of Giant Planets Orbiting Evolved Star HD 184010

Huan-Yu Teng, Bun'ei Sato, Takuya Takarada +11

We report the discovery of a triple-giant-planet system around an evolved star HD 184010 (HR 7421, HIP 96016). This discovery is based on observations from Okayama Planet Search Pr…

astro-ph.SR2022★ 14 cited

Starspots, chromospheric emission lines, and flares of zero-age main-sequence stars

Mai Yamashita, Yoichi Itoh, Yumiko Oasa

Zero-age main-sequence (ZAMS) stars are considered to have enormous starspots and show strong chromospheric emission lines because of their strong surface magnetic field. We discus…