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researcher

S. Frey

4 papers here

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

author position
  • first author1
  • middle author2
  • last author1

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

fields
  • astro-ph3
  • astro-ph.GA1
ORCID 0000-0003-3079-1889
same name
  • S. Frey — 121 papers, h 25
  • S. Frey — 16 papers, h 4
  • S. Frey — 7 papers, h 2
  • S. Frey — 6 papers, h 15
  • S. Frey — 3 papers, h 6
  • S. Frey — 2 papers, h 4

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
19982011
most citedThe ``angular size - redshift'' relation for compact radio structures in quasars and radio galaxies

50 citations · 76 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2011★ 14 cited

VLBI search for the radio counterpart of HESS J1943+213

K. E. Gabanyi, G. Dubner, E. Giacani +3

HESS J1943+213, a TeV point source close to the Galactic plane recently discovered by the H.E.S.S. collaboration, was proposed to be an extreme BL Lacertae object, though a pulsar…

astro-ph2005★ 9 cited

VSOP monitoring of the compact BL Lac object AO 0235+164

S. Frey, L. I. Gurvits, D. C. Gabuzda +7

In 1999, the highly compact and variable BL Lac object AO 0235+164 was identified as the highest brightness temperature active galactic nucleus observed with the VLBI Space Observa…

astro-ph1999★ 3 cited

VLBI imaging of extremely high redshift quasars at 5 GHz

Z. Paragi, S. Frey, L. I. Gurvits +5

We present very long baseline interferometry (VLBI) images of ten very high redshift (z>3) quasars at 5 GHz. The sources 0004+139, 0830+101, 0906+041, 0938+119 and 1500+045 were ob…

astro-ph1998★ 50 cited

The ``angular size - redshift'' relation for compact radio structures in quasars and radio galaxies

L. I. Gurvits, K. I. Kellermann, S. Frey

We discuss the ``angular size - redshift'' relation for compact radio sources distributed over a wide range of redshifts 0.01 < z < 4.73. Our study is based on a sample of 330 5 GH…

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