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researcher

Y. Tachibana

4 papers here

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

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.GA1
  • astro-ph.SR1
ORCID 0000-0001-6584-6945
same name
  • Y. Tachibana — 24 papers, h 17
  • Y. Tachibana — 21 papers, h 19
  • Y. Tachibana — 11 papers
  • Y. Tachibana — 5 papers, h 3
  • Y. Tachibana — 3 papers, h 10
  • Y. Tachibana — 1 paper, h 1

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

most citedKiso Supernova Survey (KISS): Survey Strategy

42 citations · 106 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2016★ 22 cited

High-Energy Non-Thermal and Thermal Emission from GRB141207A detected by Fermi

Makoto Arimoto, Katsuaki Asano, Masanori Ohno +5

The bright long gamma-ray burst GRB 141207A was observed by the {\it Fermi Gamma-ray Space Telescope} and detected by both instruments onboard. The observations show that the spect…

astro-ph.GA2014★ 17 cited

Discovery of Dramatic Optical Variability in SDSS J1100+4421: A Peculiar Radio-Loud Narrow-Line Seyfert 1 Galaxy?

Masaomi Tanaka, Tomoki Morokuma, Ryosuke Itoh +55

We present our discovery of dramatic variability in SDSS J1100+4421 by the high-cadence transient survey Kiso Supernova Survey (KISS). The source brightened in the optical by at le…

astro-ph.SR2014★ 42 cited

Kiso Supernova Survey (KISS): Survey Strategy

Tomoki Morokuma, Nozomu Tominaga, Masaomi Tanaka +58

The Kiso Supernova Survey (KISS) is a high-cadence optical wide-field supernova (SN) survey. The primary goal of the survey is to catch the very early light of a SN, during the sho…

astro-ph.HE2014★ 25 cited

MAXI observations of GRBs

Motoko Serino, Takanori Sakamoto, Nobuyuki Kawai +40

Monitor of all-sky image (MAXI) Gas Slit Camera (GSC) detects gamma-ray bursts (GRBs) including the bursts with soft spectra, such as X-ray flashes (XRFs). MAXI/GSC is sensitive to…

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