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T. Ohshima

38 papers hereh-index 154.1k citations39 works total

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

author position
  • sole author1
  • first author1
  • middle author24

Across the 26 of 38 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR26
  • astro-ph.HE6
  • astro-ph.GA4
  • astro-ph1
  • astro-ph.EP1
same name
  • T. Ohshima — 194 papers, h 73
  • T. Ohshima — 146 papers
  • T. Ohshima — 54 papers, h 54
  • T. Ohshima — 49 papers, h 8
  • T. Ohshima — 23 papers, h 22
  • T. Ohshima — 14 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20012026
most citedKilonova from post-merger ejecta as an optical and near-infrared counterpart of GW170817

340 citations · 1.9k across the 38 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.SR2012★ 79 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. IV: The Fourth Year (2011-2012)

Taichi Kato, Franz-Josef Hambsch, Hiroyuki Maehara +85

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we studied 86 SU UMa-type dwarf novae. We confirmed the general trends such as the relation between period…

astro-ph.SR2012★ 29 cited

Discovery of Negative Superhumps during a Superoutburst of January 2011 in ER Ursae Majoris

Tomohito Ohshima, Taichi Kato, Elena P. Pavlenko +19

We report on a discovery of "negative" superhumps during the 2011 January superoutburst of ER UMa. During the superoutburst which started on 2011 January 16, we detected negative s…

astro-ph.GA2012★ 22 cited

Reconstruction of the Structure of Accretion Disks in Dwarf Novae from the Multi-Band Light Curves of Early Superhumps

M. Uemura, T. Kato, T. Ohshima +1

We propose a new method to reconstruct the structure of accretion disks in dwarf novae using multi-band light curves of early superhumps. Our model assumes that early superhumps ar…

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