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T. Sakai

70 papers hereh-index 343.2k citations147 works total

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

author position
  • first author6
  • middle author52
  • last author5

Across the 63 of 70 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA42
  • astro-ph.SR18
  • astro-ph6
  • astro-ph.IM3
  • astro-ph.CO1
same name
  • T. Sakai — 90 papers, h 26
  • T. Sakai — 31 papers, h 14
  • T. Sakai — 15 papers, h 8
  • T. Sakai — 14 papers, h 14
  • T. Sakai — 9 papers, h 47
  • T. Sakai — 8 papers, h 2

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 citedThe ALMA Survey of 70 μm dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

207 citations · 2.7k across the 70 of their papers we have counts for

collaborators
Showing 2008Show all

3 papers · 1 filter

astro-ph2008★ 49 cited

A New 100-GHz Band Front-End System with a Waveguide-Type Dual-Polarization Sideband-Separating SIS Receiver for the NRO 45-m Radio Telescope

Taku Nakajima, Masayuki Kawamura, Kimihiro Kimura +8

We developed a waveguide-type dual-polarization sideband-separating SIS receiver system of the 100-GHz band for the 45-m radio telescope at the Nobeyama Radio Observatory, Japan. T…

astro-ph2008★ 81 cited

A Molecular Line Observation toward Massive Clumps Associated with Infrared Dark Clouds

Takeshi Sakai, Nami Sakai, Kazuhisa Kamegai +4

We have surveyed the N2H+ J=1-0, HC3N J=5-4, CCS J_N=4_3-3_2, NH3 (J, K) = (1, 1), (2, 2), (3, 3), and CH3OH J=7-6 lines toward the 55 massive clumps associated with infrared dark…

astro-ph2008★ 41 cited

Detection of HCO2+ toward the Low-Mass Protostar IRAS 04368+2557 in L1527

Nami Sakai, Takeshi Sakai, Yuri Aikawa +1

The millimeter-wave rotational emission lines (4(04)-3(03) and 5(05)-4(04)) of protonated carbon dioxide, HCO2+(HOCO+), has been detected toward the low-mass class 0 protostar IRAS…

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