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researcher

Junpei Ito

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3

identity via Semantic Scholar / OpenAlex

activity
20222024
most cited2021 superoutburst of WZ Sge-type dwarf nova V627 Pegasi lacks an early superhump phase

6 citations · 9 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2024

Optical and soft X-ray light-curve analysis during the 2022 eruption of U Scorpii: structural changes in the accretion disk

Katsuki Muraoka, Naoto Kojiguchi, Junpei Ito +52

We present our optical photometric observations of the 2022 eruption of the recurrent nova U Scorpii (U Sco) using 49,152 data points over 70 d following the optical peak. We have…

astro-ph.SR2023★ 6 cited

2021 superoutburst of WZ Sge-type dwarf nova V627 Pegasi lacks an early superhump phase

Yusuke Tampo, Taichi Kato, Naoto Kojiguchi +27

Superoutbursts in WZ Sge-type dwarf novae (DNe) are characterized by both early superhumps and ordinary superhumps originating from the 2:1 and 3:1 resonances, respectively. Howeve…

astro-ph.SR2022★ 3 cited

PNV J00444033+4113068: early superhumps with 0.7 mag amplitude and non-red color

Yusuke Tampo, Keisuke Isogai, Naoto Kojiguchi +13

In the first days of WZ Sge-type dwarf nova (DN) outbursts, the 2:1 resonance induces a spiral arm structure in the accretion disk, which is observed as early superhumps in optical…

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