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T. Otani

3 papers hereh-index 329 citations5 works total

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

author position
  • first author2
  • middle author1

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

fields
  • astro-ph.SR3
same name
  • T. Otani — 1 paper, h 2
  • T. Otani — 1 paper, h 5

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
20172025
most citedThe EXOTIME project: Signals in the O−C diagrams of the rapidly pulsating subdwarfs DW Lyn, V1636 Ori, QQ Vir, and V541 Hya

5 citations · 5 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2025

Binary Systems Search with TESS

Tomomi Otani, A. S. Baran, Lindsay C. Spence +3

Hot subdwarf B (sdB) stars are post-main-sequence stars of high temperature and gravity. Approximately 30% of sdBs exhibit stable pressure and/or gravity-mode pulsations, which…

astro-ph.SR2020★ 5 cited

The EXOTIME project: Signals in the O−C diagrams of the rapidly pulsating subdwarfs DW Lyn, V1636 Ori, QQ Vir, and V541 Hya

F. Mackebrandt, S. Schuh, R. Silvotti +17

We aim to investigate variations in the arrival time of coherent stellar pulsations due to the light-travel time effect to test for the presence of sub-stellar companions. Those co…

astro-ph.SR2017

Orbital Characteristics of the Subdwarf-B and F V Star Binary EC~20117-4014(=V4640 Sgr)

T. Otani, T. Oswalt, A. E. Lynas-Gray +4

Among the competing evolution theories for subdwarf-B (sdB) stars is the binary evolution scenario. EC~20117-4014 (=V4640~Sgr) is a spectroscopic binary system consisting of a puls…

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