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M. Yamanaka

3 papers here

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

author position
  • middle author1
  • last author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.SR1
ORCID 0000-0001-9456-3709
same name
  • M. Yamanaka — 72 papers, h 27
  • M. Yamanaka — 48 papers, h 17
  • M. Yamanaka — 24 papers, h 9
  • M. Yamanaka — 10 papers, h 3
  • M. Yamanaka — 2 papers, h 2
  • M. Yamanaka — 2 papers, 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 citedGamma-Ray Emission Concurrent with the Nova in the Symbiotic Binary V407 Cygni

231 citations · 265 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2010★ 231 cited

Gamma-Ray Emission Concurrent with the Nova in the Symbiotic Binary V407 Cygni

LAT Collaboration

Novae are thermonuclear explosions on a white dwarf surface fueled by mass accreted from a companion star. Current physical models posit that shocked expanding gas from the nova sh…

astro-ph.HE2009

Anti-Correlation of the Near-Infrared and X-Ray Variations of the Microquasar GRS 1915+105 in Soft State

Akira Arai, Makoto Uemura, Mahito Sasada +21

We report detailed, long term near-infrared (NIR) light curves of GRS 1915+105 in 2007-2008, covering its long "soft state" for the first time. From our NIR monitoring and the X-ra…

astro-ph.SR2009★ 34 cited

The Extremely Luminous Supernova 2006gy at Late Phase: Detection of Optical Emission from Supernova

Koji S. Kawabata, Masaomi Tanaka, Keiichi Maeda +4

We performed optical spectroscopy and photometry of SN 2006gy at late time, ~400 days after the explosion, with the Subaru/FOCAS in a good seeing condition. We found that the SN fa…

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