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Pengfei Zhang

4 papers hereh-index 15 citations5 works total

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

author position
  • sole author1
  • middle author1
  • last author2

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

fields
  • astro-ph.HE4
same name
  • Pengfei Zhang — 19 papers, h 12
  • Pengfei Zhang — 13 papers, h 2
  • Pengfei Zhang — 11 papers, h 3
  • Pengfei Zhang — 10 papers, h 3
  • Pengfei Zhang — 8 papers, h 4
  • Pengfei Zhang — 8 papers, h 2

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
20242026
collaborators

4 papers

astro-ph.HE2026

Discovery of I^3-Ray Pulsations from the Extreme-Spin-Down Millisecond Pulsar PSR J0435+3233

Mengqing Zhang, Shengbin Pei, Pengfei Zhang

Motivated by the recent discovery of PSR~J0435+3233, a millisecond pulsar with an exceptionally large period derivative of P˙=4.9×10−17 ss−1 and a high s…

astro-ph.HE2025

Revisiting I^3-Ray Orbital Modulation in the Redback Millisecond Pulsar PSR J2039-5617

Mengqing Zhang, Shengbin Pei, Shan Chang +1

PSR J2039-5617 is a redback millisecond pulsar binary system consisting of a compact star with a mass of 1.1-1.6 M⊙​ and a low-mass companion of 0.15-0.22 M⊙​. For this…

astro-ph.HE2024

Investigating the Potential of LS 5039 as a Triple System Using Fermi-LAT Data

Lujun Zeng, Mengqing Zhang, Chongyang Ren +2

LS 5039 is one of a handful of I^3-ray binary systems in the Milky Way, comprising a pulsar and a massive O-type companion star with an orbital period of 3.9 day. Recently, we con…

astro-ph.HE2024

A New Puzzling Periodic Signal in GeV Energies of the I^3-Ray Binary LS I +61∘303

Pengfei Zhang

LS I + 61∘303 is a high-mass X-ray binary system comprising a massive Be star and a rapidly rotating neutron star. Its spectral energy distribution across multi-wavelengths…

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