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Annika H. G. Peter

4 papers hereh-index 16 citations4 works total

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

author position
  • middle author1
  • last author3

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • hep-ph1
same name
  • Annika H. G. Peter — 10 papers, h 4
  • Annika H. G. Peter — 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

collaborators

4 papers

astro-ph.HE2026

First Observations of Solar Halo Gamma Rays Over a Full Solar Cycle

Tim Linden, Jung-Tsung Li, Bei Zhou +4

We analyze 15 years of Fermi-LAT data and produce a detailed model of the Sun's inverse-Compton scattering emission (solar halo), which is powered by interactions between ambient c…

astro-ph.HE2026

Convection-Driven Multi-Scale Magnetic Fields Determine the Observed Solar-Disk Gamma Rays

Jung-Tsung Li, Mahboubeh Asgari-Targhi, John F. Beacom +1

The solar disk is a continuous source of GeV--TeV gamma rays. The emission is thought to originate from hadronic Galactic cosmic rays (GCRs) interacting with the gas in the photosp…

astro-ph.HE2025

Are X-Ray Detected Active Galactic Nuclei in Dwarf Galaxies Gamma-Ray Bright?

Milena Crnogorčević, Tim Linden, Annika H. G. Peter

The I^3-ray emission from active galactic nuclei (AGN), including both beamed blazars and misaligned-AGN, dominates the extragalactic I^3-ray point-source population count and fl…

hep-ph2025

Angular Distribution of Gamma Rays Produced in Proton-Proton Collisions

Spencer Griffith, John F. Beacom, Jung-Tsung Li +1

Accurate modeling of how high-energy proton-proton collisions produce gamma rays through the decays of pions and other secondaries is needed to correctly interpret astrophysical ob…

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