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Authors

A. di Matteo

Name variants: Armando di Matteo

Last known institution:
Istituto Nazionale di Fisica Nucleare, Sezione di Torino
ORCID:
0000-0002-8260-1867
4
h-index
0
i10-index
83
Citations
36
Works
Trends over time

Performance over time

Citation overview

Publications (bars) and citations (line) by year

  • Publications
  • Citations
035810025507510020162017201920202021202220232024202520262016: Publications 1, Citations 02017: Publications 3, Citations 02019: Publications 0, Citations 12020: Publications 4, Citations 22021: Publications 7, Citations 02022: Publications 1, Citations 12023: Publications 8, Citations 02024: Publications 4, Citations 212025: Publications 6, Citations 582026: Publications 1, Citations 0

Citation history

025507510020162017201920202021202220232024202520262016: Citations 02017: Citations 02019: Citations 12020: Citations 22021: Citations 02022: Citations 12023: Citations 02024: Citations 212025: Citations 582026: Citations 0

Publication history

03581020162017201920202021202220232024202520262016: Publications 12017: Publications 32019: Publications 02020: Publications 42021: Publications 72022: Publications 12023: Publications 82024: Publications 42025: Publications 62026: Publications 1

h-index evolution

Cumulative h-index by year

0134520162017201920202021202220232024202520262016: h-index 02017: h-index 02019: h-index 12020: h-index 12021: h-index 12022: h-index 22023: h-index 22024: 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. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 citations
  5. 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
  6. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 citations
  7. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 citations
  8. The Pierre Auger Observatory open data20250 citations
  9. 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
  10. Measuring the muon content of inclined air showers using AERA and the water-Cherenkov detectors of the Pierre Auger Observatory20250 citations
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