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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 2021Show all

3 papers · 1 filter

astro-ph.SR2021★ 144 cited

Probable detection of an eruptive filament from a superflare on a solar-type star

Kosuke Namekata, Hiroyuki Maehara, Satoshi Honda +20

Solar flares are often accompanied by filament/prominence eruptions (∼104 K and ∼1010−11 cm−3), sometimes leading to coronal mass ejections (CMEs) that direct…

astro-ph.HE2021★ 19 cited

Intermediate Luminosity Type Iax SN 2019muj With Narrow Absorption Lines: Long-Lasting Radiation Associated With a Possible Bound Remnant Predicted by the Weak Deflagration Model

Miho Kawabata, Keiichi Maeda, Masayuki Yamanaka +23

We present comprehensive spectroscopic and photometric analyses of the intermediate luminosity Type Iax supernova (SN Iax) 2019muj based on multi-band datasets observed through the…

astro-ph.SR2021★ 11 cited

ASASSN-18aan: An Eclipsing SU UMa-type Cataclysmic Variable with a 3.6-hour Orbital Period and a Late G-type Secondary Star

Yasuyuki Wakamatsu, John R. Thorstensen, Naoto Kojiguchi +41

We report photometric and spectroscopic observations of the eclipsing SU UMa-type dwarf nova ASASSN-18aan. We observed the 2018 superoutburst with 2.3 mag brightening and found the…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.