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Authors

L. Chytka

Last known institution:
Palacký University Olomouc
ORCID:
0000-0001-5741-259X
4
h-index
0
i10-index
73
Citations
36
Works
Trends over time

Performance over time

Citation overview

Publications (bars) and citations (line) by year

  • Publications
  • Citations
0358100255075100201920202021202220232024202520262019: Publications 1, Citations 02020: Publications 5, Citations 02021: Publications 7, Citations 02022: Publications 2, Citations 02023: Publications 9, Citations 02024: Publications 4, Citations 222025: Publications 6, Citations 512026: Publications 2, Citations 0

Citation history

0255075100201920202021202220232024202520262019: Citations 02020: Citations 02021: Citations 02022: Citations 02023: Citations 02024: Citations 222025: Citations 512026: Citations 0

Publication history

035810201920202021202220232024202520262019: Publications 12020: Publications 52021: Publications 72022: Publications 22023: Publications 92024: Publications 42025: Publications 62026: Publications 2

h-index evolution

Cumulative h-index by year

01345201920202021202220232024202520262019: h-index 02020: h-index 02021: h-index 02022: h-index 02023: h-index 02024: h-index 22025: h-index 42026: h-index 4

Most-cited works

  1. Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory20242 citations
  2. Inference of the Mass Composition of Cosmic Rays with Energies from <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>18.5</mml:mn></mml:msup></mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:mrow></mml:math> Using the Pierre Auger Observatory and Deep Learning20252 citations
  3. Measurement of the depth of maximum of air-shower profiles with energies between <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>18.5</mml:mn></mml:msup></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>20</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> using the surface detector of the Pierre Auger Observatory and deep learning20252 citations
  4. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20201 citations
  5. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 citations
  6. Search for photons above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>18</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory20240 citations
  7. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 citations
  8. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 citations
  9. The Pierre Auger Observatory open data20250 citations
  10. Energy Spectrum of Ultrahigh-Energy Cosmic Rays across Declinations <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mo>−</mml:mo> <mml:mn>9</mml:mn> <mml:mn>0</mml:mn> <mml:mi>°</mml:mi> </mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mo>+</mml:mo> <mml:mn>44.8</mml:mn> <mml:mi>°</mml:mi> </mml:math> as Measured at the Pierre Auger Observatory20250 citations
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