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T. Varga

80 papers hereh-index 436.8k citations191 works total

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

author position
  • first author1
  • middle author49
  • last author4

Across the 54 of 80 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO50
  • astro-ph.GA20
  • astro-ph.IM4
  • astro-ph.HE3
  • astro-ph.SR2
  • hep-ph1
same name
  • T. Varga — 3 papers, h 11
  • T. Varga — 1 paper, h 20
  • T. Varga — 1 paper, h 4
  • T. Varga — 1 paper, h 1

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
20182026
most citedDES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys

160 citations · 835 across the 34 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

4 papers · 1 filter

astro-ph.IM2023★ 5 cited

The Dark Energy Survey Six-Year Calibration Star Catalog

E. S. Rykoff, D. L. Tucker, D. L. Burke +64

This Technical Note presents a catalog of calibrated reference stars that was generated by the Forward Calibration Method (FGCM) pipeline (arXiv:1706.01542) as part of the FGCM pho…

astro-ph.IM2021

The Dark Energy Survey Data Release 2

DES Collaboration, T. M. C. Abbott, M. Adamow +132

We present the second public data release of the Dark Energy Survey, DES DR2, based on optical/near-infrared imaging by the Dark Energy Camera mounted on the 4-m Blanco telescope a…

astro-ph.IM2020

Reducing ground-based astrometric errors with Gaia and Gaussian processes

W. F. Fortino, G. M. Bernstein, P. H. Bernardinelli +64

Stochastic field distortions caused by atmospheric turbulence are a fundamental limitation to the astrometric accuracy of ground-based imaging. This distortion field is measurable…

astro-ph.IM2020★ 12 cited

Noise from Undetected Sources in Dark Energy Survey Images

K. Eckert, G. M. Bernstein, A. Amara +66

For ground-based optical imaging with current CCD technology, the Poisson fluctuations in source and sky background photon arrivals dominate the noise budget and are readily estima…

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