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researcher

S. Ando

95 papers hereh-index 353.8k citations143 works total

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

author position
  • sole author8
  • first author35
  • middle author27
  • last author23

Across the 93 of 95 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO26
  • astro-ph25
  • astro-ph.HE24
  • hep-ph16
  • astro-ph.GA3
  • astro-ph.IM1
same name
  • S. Ando — 58 papers, h 17
  • S. Ando — 6 papers, h 2
  • S. Ando — 5 papers, h 4
  • S. Ando — 5 papers, h 7
  • S. Ando — 4 papers, h 13
  • S. Ando — 4 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

activity
20012023
most citedKlein-Nishina Effects on Optically Thin Synchrotron and Synchrotron Self-Compton Spectrum

223 citations · 4.5k across the 94 of their papers we have counts for

collaborators
Showing 2004Show all

3 papers · 1 filter

astro-ph2004★ 12 cited

Does regenerated emission change the high-energy signal from gamma-ray burst afterglows?

Shin'ichiro Ando

We study regenerated high-energy emission from the gamma-ray burst (GRB) afterglows, and compare its flux with the direct component from the same afterglow. When the intrinsic emis…

hep-ph2004★ 39 cited

Appearance of neutronization peak and decaying supernova neutrinos

Shin'ichiro Ando

Nonradiative neutrino decay, which is not satisfactorily constrained, possibly and significantly changes the detected neutrino signal from galactic supernova explosions. We focus o…

astro-ph2004★ 43 cited

Cosmic Star Formation History and the Future Observation of Supernova Relic Neutrinos

Shin'ichiro Ando

We investigate the flux and event rate of supernova relic neutrinos (SRNs) and discuss their implications for the cosmic star formation rate. As reference models, we adopt the supe…

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