activity
20072026
most citedFive Intermediate-Period Planets from the N2K Sample

128 citations · 1.8k across the 80 of their papers we have counts for

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15 papers · 1 filter

astro-ph.SR2026

Unraveling Year-Long Radial Velocity Variations in Red Clump Region -- I: Comprehensive analysis of a K0 Giant star, 2 Draconis

Udomlerd Srisuchinwong, Jianzhao Zhou, Huan-Yu Teng +18

Slow-rotating evolved stars frequently exhibit radial velocity (RV) variations on annual timescales, complicated by instrumental systematics and aliasing in the one-year regime. He…

astro-ph.SR2026★ 1 cited

Discovery of a compact hierarchical triple main-sequence star system while searching for binary stars with compact objects

Ataru Tanikawa, Akito Tajitsu, Satoshi Honda +5

We have discovered a compact hierarchical triple main-sequence star system, which is cataloged as Gaia DR3 1010268155897156864 or TIC 21502513. Hereafter, we call it ``G1010''. G10…

astro-ph.SR2025★ 4 cited

Doppler imaging combined with high-cadence photometry. I. Revisiting the surface of a pre-main-sequence flare star

Sanghee Lee, Engin Bahar, Hakan Volkan Şenavcı +11

Latitude distribution of stellar magnetic activity is not well constrained by observations, despite its importance for a better understanding of stellar dynamos. We aim to obtain a…

astro-ph.SR2025

Direct Imaging Explorations for Companions from the Subaru/IRD Strategic Program II; Discovery of a Brown-dwarf Companion around a Nearby mid-M~dwarf LSPM~J1446+4633

Taichi Uyama, Masayuki Kuzuhara, Charles Beichman +35

We report the discovery of a new directly-imaged brown dwarf companion with Keck/NIRC2+pyWFS around a nearby mid-type M~dwarf LSPM~J1446+4633 (hereafter J1446). The -band contr…

astro-ph.SR2025★ 1 cited

Two unseen massive white dwarf candidates in close binaries

Yuta Shiraishi, Kenta Hotokezaka, Kento Masuda +10

We report the discovery of two binary systems, each consisting of a slightly bloated G-type main-sequence star and an unseen companion, identified through photometric data from TES…

astro-ph.SR2025

Elemental abundances of 44 very metal-poor stars determined from Subaru/IRD near-infrared spectra

Wako Aoki, Timothy C. Beers, Satoshi Honda +12

Abundances of five elements, Na, Mg, Al, Si, and Sr, are investigated for 44 very metal-poor stars (-4.0 < [Fe/H] < -1.5) in the Galactic halo system based on an Local Thermodinami…