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researcher

K. Fang

44 papers hereh-index 242.3k citations103 works total

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

author position
  • sole author1
  • first author12
  • middle author18
  • last author1

Across the 32 of 44 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE41
  • astro-ph.IM1
  • physics.acc-ph1
  • physics.ins-det1
same name
  • K. Fang — 90 papers, h 44
  • K. Fang — 81 papers, h 7
  • K. Fang — 60 papers, h 15
  • 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
20152023
most citedFirst Detection of sub-PeV Diffuse Gamma Rays from the Galactic Disk: Evidence for Ubiquitous Galactic Cosmic Rays beyond PeV Energies

234 citations · 2.5k across the 44 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.HE2018★ 41 cited

GeV observations of the extended pulsar wind nebulae constrain the pulsar interpretations of the cosmic-ray positron excess

Shao-Qiang Xi, Ruo-Yu Liu, Zhi-Qiu Huang +2

It has long been suggested that nearby pulsars within ∼1kpc are the leading candidate of the 10-500 GeV cosmic-ray positron excess measured by PAMELA and other exper…

astro-ph.HE2018★ 11 cited

Inefficient cosmic ray diffusion around Vela X : constraints from H.E.S.S. observations of very high-energy electrons

Zhi-Qiu Huang, Kun Fang, Ruo-Yu Liu +1

Vela X is a nearby pulsar wind nebula (PWN) powered by a ∼104 year old pulsar. Modeling of the spectral energy distribution of the Vela X PWN has shown that accelerated elec…

astro-ph.HE2018★ 98 cited

Two-zone diffusion of electrons and positrons from Geminga explains the positron anomaly

Kun Fang, Xiao-Jun Bi, Peng-Fei Yin +1

The recent HAWC observations of very-high-energy γ-ray halo around Geminga and Monogem indicate a very slow diffusion of cosmic rays, which results in tiny contribution of positr…

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