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20162026
most citedRepetitive Patterns in Rapid Optical Variations in the Nearby Black-hole Binary V404 Cygni

86 citations · 402 across the 39 of their papers we have counts for

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astro-ph.SR2026

A probable inside-out dwarf nova outburst from the period bouncer candidate ASASSN-25dc

Yusuke Tampo, Naoto Kojiguchi, Mariko Kimura +13

We report optical time-resolved photometric observations of a newly-discovered outbursting system, ASASSN-25dc. Its 8-mag amplitude, 40-day duration, 1-mag dip in the outburst plat…

astro-ph.SR2025

TESS and ground-based observations of WZ Sge-type dwarf novae in outburst

Y. Tampo, N. Kojiguchi, K. Isogai +30

Dwarf nova (DN) superoutbursts are accompanied by superhumps, which change their periods and profiles over a superoutburst. We present the TESS and ground-based observations of nin…

astro-ph.SR2025

ASASSN-24hd; a dwarf nova bridging WZ Sge-type and SU UMa-type superoutbursts

Yusuke Tampo, Naoto Kojiguchi, Taichi Kato +9

WZ Sge-type dwarf novae (DNe) form a subclass in cataclysmic variables, characterized by short-period variations called superhumps during an outburst. Here we present optical groun…

astro-ph.SR2025

Spectral evolution of the narrow emission line components in optical during the 2022 nova eruption of U Scorpii

Katsuki Muraoka, Naoto Kojiguchi, Junpei Ito +20

There remains debate over whether the accretion disk survives or is entirely disrupted after the nova eruption. In our previous paper, Muraoka et al. (2024, PASJ, 76, 293) have pho…

astro-ph.SR2024

Smart Kanata: A Framework for Autonomous Decision Making in Rapid Follow-up Observations of Cataclysmic Variables

Makoto Uemura, Yuzuki Koga, Ryosuke Sazaki +11

Studying the early stages of transient events provides crucial information about the fundamental physical processes in cataclysmic variables (CVs). However, determining an appropri…

astro-ph.SR2024

MASTER OT J030227.28+191754.5: an unprecedentedly energetic dwarf nova outburst

Yusuke Tampo, Taichi Kato, Keisuke Isogai +60

We present a detailed study of the MASTER OT J030227.28+191754.5 outburst in 2021-2022, reaching an amplitude of 10.2 mag and a duration of 60 d. The detections of (1) the double-p…