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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 2016Show all

3 papers · 1 filter

astro-ph.SR2016★ 34 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. VIII: The Eighth Year (2015-2016)

Taichi Kato, Franz-Josef Hambsch, Berto Monard +75

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 128 SU UMa-type dwarf novae observed mainly during the 2015-2016…

astro-ph.SR2016★ 13 cited

Superoutburst of CR Bootis: Estimation of Mass Ratio of a typical AM CVn star by Stage A Superhumps

Keisuke Isogai, Taichi Kato, Tomohito Ohshima +31

We report on two superoutbursts of the AM CVn-type object CR Boo in 2014 April--March and 2015 May--June. A precursor outburst acompanied both of these superoutbursts. During the r…

astro-ph.HE2016★ 20 cited

No Evidence of Intrinsic Optical/Near-Infrared Linear Polarization for V404 Cygni During its Bright Outburst in 2015: Broadband Modeling and Constraint on Jet Parameters

Y. T. Tanaka, R. Itoh, M. Uemura +39

We present simultaneous optical and near-infrared (NIR) polarimetric results for the black hole binary V404 Cygni spanning the duration of its 7-day long optically-brightest phase…

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