LabCompass

G. H. Sembroski

Physics and Astronomy · Purdue University West Lafayette

OpenAlex ORCID
Established · publishing since 1986Rising activity
Gamma-ray bursts and supernovaeAstrophysics and Cosmic PhenomenaDark Matter and Cosmic PhenomenaAstrophysical Phenomena and ObservationsPulsars and Gravitational Waves Research

Publications

116

Citations

2,190

Est. group size

~1

Recurring co-author estimate

Active years

40

Publishing since 1986

Research summary
AI-generated

G. H. Sembroski works in high-energy astrophysics, studying sources of gamma-ray and X-ray emission such as supernova remnants, pulsars, blazars, and gamma-ray bursts using large observatories like VERITAS, HAWC, Fermi-LAT, and XMM-Newton. This research involves multiwavelength observations that combine data from different telescopes to identify and characterize energetic cosmic objects, and also touches on searches for exotic particles like axion-like particles.

Gamma-ray astronomySupernova remnants and pulsarsMultiwavelength observational astrophysicsBlazars and active galactic nucleiDark matter and particle astrophysics searches

Publication output has fluctuated year to year over the last decade but shows an overall increase, with notably higher counts in 2021, 2023, and 2025 compared to earlier years.

Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026

Publication cadence
Publications per year over the last 10 years — averaging 6.6/year recently
2017: 1 publication172018: 5 publications182019: 5 publications192020: 4 publications202021: 9 publications212022: 1 publication222023: 15 publications15232024: 7 publications242025: 10 publications2526
Recent publications
Publishes in
  • The Astrophysical Journal×19
  • arXiv (Cornell University)×14
  • Desy publication database (The Deutsches Elektronen-Synchrotron)×7
  • Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)×4
  • Monthly Notices of the Royal Astronomical Society×2
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By research-topic overlap

This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.

Last updated Jul 20, 2026.

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