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T. Fujii

39 papers hereh-index 323.9k citations102 works total

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

author position
  • middle author14
  • last author2

Across the 16 of 39 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE22
  • astro-ph7
  • astro-ph.IM6
  • astro-ph.CO3
  • physics.ao-ph1
same name
  • T. Fujii — 84 papers, h 32
  • T. Fujii — 30 papers, h 21
  • T. Fujii — 28 papers, h 15
  • T. Fujii — 17 papers, h 11
  • T. Fujii — 14 papers, h 20
  • T. Fujii — 13 papers, h 9

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
19972024
most citedThe surface detector array of the Telescope Array experiment

399 citations · 2.6k across the 38 of their papers we have counts for

collaborators
Showing 2010Show all

3 papers · 1 filter

astro-ph.CO2010★ 23 cited

Ly alpha emissters at z=6.5 in the SSA22 field: An area more neutral or void at the end of the reionization epoch

E. Nakamura, A. K. Inoue, T. Hayashino +4

We present results of a survey of Lyman α emitters (LAEs) at z=6.5 which is thought to be the final epoch of the cosmic reionization. In a ≈530 arcmin2 deep image of…

astro-ph.CO2010★ 108 cited

The Subaru Ly-alpha blob survey: A sample of 100 kpc Ly-alpha blobs at z=3

Y. Matsuda, T. Yamada, T. Hayashino +11

We present results of a survey for giant Ly-alpha nebulae (LABs) at z=3 with Subaru/Suprime-Cam. We obtained Ly-alpha imaging at z=3.09+-0.03 around the SSA22 protocluster and in s…

astro-ph.CO2010★ 9 cited

A search for galaxies in and around an HI overdense region at z=5

Y. Matsuda, J. Richard, Ian Smail +7

We present the discovery of a large-scale structure of emission-line galaxies at redshift z=4.86 behind a massive cluster of galaxies, A1689. Previous spectroscopic observations of…

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