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researcher

György Mező

4 papers here

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

author position
  • last author4

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

fields
  • astro-ph.HE2
  • astro-ph.GA1
  • astro-ph.SR1
ORCID 0000-0002-0686-7479
same name
  • György Mező — 1 paper, h 0
  • György Mező — 1 paper, 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
20202025
most citedCosmic neutrinos from temporarily gamma-suppressed blazars

36 citations · 45 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2025

High-resolution radio imaging of TGSSJ1530+1049, a radio galaxy in a dense environment at z=4

K. É. Gabányi, S. Frey, L. I. Gurvits +10

High-redshift radio galaxies can provide insights into the structure formation and galaxy evolution at earlier cosmological epochs. TGSSJ1530+1049 was selected as a candidate high-…

astro-ph.HE2023★ 8 cited

Searching for temporary gamma-ray dark blazars associated with IceCube neutrinos

Emma Kun, Imre Bartos, Julia Becker Tjus +4

Tensions between the diffuse gamma-ray sky observed by the Fermi Large Area Telescope (LAT) and the diffuse high-energy neutrino sky detected by the IceCube South Pole Neutrino Obs…

astro-ph.SR2022★ 1 cited

GD 99: Re-investigation of an old ZZ Ceti companion

Zs. Bognár, Á. Sódor, Gy. Mező

Context. Thanks to photometric space missions, we have access to more and more information on the properties of white dwarf stars, especially pulsating ones. In the case of pulsato…

astro-ph.HE2020★ 36 cited

Cosmic neutrinos from temporarily gamma-suppressed blazars

Emma Kun, Imre Bartos, Julia Becker Tjus +3

Despite the uncovered association of a high-energy neutrino with the apparent flaring state of blazar TXS 0506+056 in 2017, the mechanisms leading to astrophysical particle acceler…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.