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researcher

K. Fang

90 papers hereh-index 446.5k citations172 works total

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

author position
  • sole author1
  • first author25
  • middle author30
  • last author3

Across the 59 of 90 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE77
  • astro-ph.IM9
  • hep-ex3
  • hep-ph1
same name
  • K. Fang — 81 papers, h 7
  • K. Fang — 60 papers, h 15
  • K. Fang — 44 papers, h 24
  • K. Fang — 32 papers, h 9
  • K. Fang — 25 papers, h 16
  • K. Fang — 20 papers, h 7

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
20122023
most citedDepth of Maximum of Air-Shower Profiles at the Pierre Auger Observatory: Composition Implications

309 citations · 4.3k across the 87 of their papers we have counts for

collaborators
Showing 2021Show all

4 papers · 1 filter

astro-ph.HE2021

HAWC Study of the Ultra-High-Energy Spectrum of MGRO J1908+06

HAWC Collaboration, A. Albert, R. Alfaro +97

We report TeV gamma-ray observations of the ultra-high-energy source MGRO J1908+06 using data from the High Altitude Water Cherenkov (HAWC) Observatory. This source is one of the h…

astro-ph.HE2021

Studying High-Mass Microquasars with HAWC

Chang Dong Rho, Ke Fang, Se Yeon Hwang +1

High-mass microquasars (HMMQs) are powerful particle accelerators, but their mechanism of the high-energy emission is poorly understood. To date, only a handful of these particle e…

astro-ph.HE2021★ 2 cited

Multi-messenger Implications of Sub-PeV Diffuse Galactic Gamma-Ray Emission

Ke Fang, Kohta Murase

The diffuse Galactic gamma-ray flux between 0.1 and 1 PeV has recently been measured by the Tibet ASγ Collaboration. The flux and spectrum are consistent with the decay of neutra…

astro-ph.HE2021★ 2 cited

HAWC Search for High-Mass Microquasars

HAWC Collaboration, A. Albert, R. Alfaro +87

Microquasars with high-mass companion stars are promising very-high-energy (VHE; 0.1-100 TeV) gamma-ray emitters, but their behaviors above 10 TeV are poorly known. Using the High…

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