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researcher

K. Murata

43 papers hereh-index 221.5k citations82 works total

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

author position
  • first author2
  • middle author36
  • last author1

Across the 39 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE16
  • astro-ph.GA10
  • astro-ph.SR7
  • astro-ph.EP5
  • astro-ph.CO3
  • astro-ph.IM2
same name
  • K. Murata — 14 papers, h 7
  • K. Murata — 11 papers, h 33
  • K. Murata — 8 papers, h 16
  • K. Murata — 4 papers, h 5
  • K. Murata — 2 papers, h 11
  • K. Murata — 2 papers, h 3

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
20092024
most citedA nearby long gamma-ray burst from a merger of compact objects

284 citations · 1.8k across the 43 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.EP2014★ 18 cited

Dust from Comet 209P/LINEAR during its 2014 Return: Parent Body of a New Meteor Shower, the May Camelopardalids

Masateru Ishiguro, Daisuke Kuroda, Hidekazu Hanayama +29

We report a new observation of the Jupiter-family comet 209P/LINEAR during its 2014 return. The comet is recognized as a dust source of a new meteor shower, the May Camelopardalids…

astro-ph.GA2014★ 20 cited

Variable optical polarization during high state in gamma-ray loud narrow line Seyfert 1 galaxy 1H 0323+342

Ryosuke Itoh, Yasuyuki T. Tanaka, Hiroshi Akitaya +34

We present results of optical polarimetric and multi-band photometric observations for gamma-ray loud narrow-line Seyfert 1 galaxy 1H 0323+342. This object has been monitored by 1.…

astro-ph.GA2014★ 55 cited

Evolution of the Fraction of Clumpy Galaxies at 0.2<z<1.0 in the COSMOS field

K. L. Murata, M. Kajisawa, Y. Taniguchi +7

Using the Hubble Space Telescope/Advanced Camera for Surveys data in the COSMOS field, we systematically searched clumpy galaxies at 0.2<z<1.0 and investigated the fraction of clum…

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