Ke Fang

Assistant Professor

University of Wisconsin-Madison

United States

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About

Ke Fang is an Assistant Professor at the University of Wisconsin–Madison, USA. His research primarily focuses on high-energy astrophysics, including topics such as multimessenger emissions from black hole X-ray binaries and neutrino emissions from active galactic nuclei. Recent articles authored by him explore the role of gamma-ray emissions and ultrahigh-energy cosmic rays in astrophysical phenomena.

Articles (24)

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2020

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2020

Collaborators (11)

Rafael Alves Batista

Chaire de professeur junior

Sorbonne Université

FRANCE

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Sara Coutiño de León

Institut de Física Corpuscular

SPAIN

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University of Leicester

UNITED KINGDOM

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Sabrina Casanova

Associate Professor

Polska Akademia Nauk Instytut Fizyki

POLAND

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John Gallagher

Eemeritus Professor

UNITED STATES

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Ke Fang

Research Interests

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About

Articles (24)

High-energy Neutrino Source Cross-correlations with Nearest-neighbor Distributions

Multimessenger Emission by Magnetically Arrested Disks and Relativistic Jets of Black Hole X-Ray Binaries

Extended TeV Halos May Commonly Exist around Middle-Aged Pulsars

An NGC 1068-informed Understanding of Neutrino Emission of the Active Galactic Nucleus TXS 0506+056

Prospects for Observing Astrophysical Transients with Gigaelectronvolt Neutrinos

Cascaded Gamma-Ray Emission Associated with the KM3NeT Ultrahigh-energy Event KM3-230213A

Ultra-high-energy Cosmic-Ray Sources Can Be Gamma-Ray Dim

High-energy Neutrinos from Gamma-Ray-faint Accretion-powered Hypernebulae

Astroparticles from X-Ray Binary Coronae

Spectral Study of Very-high-energy Gamma Rays from SS 433 with HAWC

Ultra-high-energy gamma-ray bubble around microquasar V4641 Sgr

Limits on Leptonic TeV Emission from the Cygnus Cocoon with Swift-XRT

HAWC Detection of a TeV Halo Candidate Surrounding a Radio-quiet Pulsar

The Milky Way revealed to be a neutrino desert by the IceCube Galactic plane observation

Decomposing the Origin of TeV–PeV Emission from the Galactic Plane: Implications of Multimessenger Observations

High-energy Neutrinos from the Inner Circumnuclear Region of NGC 1068

Neutrinos from the Brightest Gamma-Ray Burst?

Evidence for PeV Proton Acceleration from Fermi-LAT Observations of SNR G106.3+2.7

The TeV Diffuse Cosmic Neutrino Spectrum and the Nature of Astrophysical Neutrino Sources

Hard X-Ray Emission from the Eastern Jet of SS 433 Powering the W50 “Manatee” Nebula: Evidence for Particle Reacceleration

Multimessenger Implications of Sub-PeV Diffuse Galactic Gamma-Ray Emission

High-energy Neutrinos and Gamma Rays from Nonrelativistic Shock-powered Transients

A Cross-correlation Study of High-energy Neutrinos and Tracers of Large-scale Structure

GeV–TeV Counterparts of SS 433/W50 from Fermi-LAT and HAWC Observations

Collaborators (11)

Rafael Alves Batista

Sara Coutiño de León

Eric Gotthelf

Brian Metzger

Shuo Zhang

Jessi Cisewski Kehe

Shigeo Kimura

Kohta Murase

Kim Page

Sabrina Casanova

John Gallagher

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