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Geophysical Survey

Russia

17 papers here125 citations across 17
fields
  • cs.CV3
  • astro-ph.CO2
  • astro-ph.SR2
  • physics.geo-ph2
  • astro-ph.GA1
  • astro-ph.HE1
  • cs.LG1
  • hep-th1
ROR 05sbpak56OpenAlex

affiliations via OpenAlex

output
20072026
most citedDetectors and flux instrumentation for future neutrino facilities

36 citations

researchers with a paper here
  • G. Ryabinin3 · h 5
  • A. Coerver2 · h 10
  • A. Gambrel2 · h 20
  • A. Hryciuk2 · h 7
  • A. Lowitz2 · h 27
  • A. Ouellette2 · h 4
  • A. Rahlin2 · h 32
  • A. R. Khalife2 · h 8
  • A. Simpson2 · h 4
  • A. Vitrier2 · h 7
  • A. Weber2 · h 2
  • B. Thorne2 · h 27
collaborating institutions
  • Xi'an Jiaotong UniversityCN4 papers
  • Argonne National LaboratoryUS3 papers
  • Fermi National Accelerator LaboratoryUS3 papers
  • High Energy Accelerator Research OrganizationJP3 papers
  • Michigan State UniversityUS3 papers
  • Stony Brook UniversityUS3 papers
  • University of GenevaCH3 papers
  • University of Illinois Urbana-ChampaignUS3 papers
  • Ashland (United States)US2 papers
  • Astronomy and SpaceAU2 papers
  • California Institute of TechnologyUS2 papers
  • Canadian Institute for Advanced ResearchCA2 papers
Showing astro-ph.HEShow all

1 paper · 1 filter

astro-ph.HE2025★ 3 cited

What determines the γ-ray luminosities of classical novae?

Peter Craig, Elias Aydi, Laura Chomiuk +25

Classical novae in the Milky Way have now been well-established as high-energy GeV γ-ray sources. In novae with main-sequence companions, this emission is believed to result from…

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