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A. di Matteo

Ism variantlari: Armando di Matteo

Soʻnggi maʼlum muassasa:
Istituto Nazionale di Fisica Nucleare, Sezione di Torino
ORCID:
0000-0002-8260-1867
4
h-indeks
0
i10-indeksi
83
Iqtiboslar
36
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

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

Iqtibos tarixi

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

Nashr tarixi

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

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520162017201920202021202220232024202520262016: h-indeks 02017: h-indeks 02019: h-indeks 12020: h-indeks 12021: h-indeks 12022: h-indeks 22023: h-indeks 22024: h-indeks 22025: h-indeks 42026: h-indeks 4

Eng koʻp iqtibos qilingan asarlar

  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 iqtibos
  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 iqtibos
  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 iqtibos
  4. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  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 iqtibos
  6. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 iqtibos
  7. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos
  8. The Pierre Auger Observatory open data20250 iqtibos
  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 iqtibos
  10. Measuring the muon content of inclined air showers using AERA and the water-Cherenkov detectors of the Pierre Auger Observatory20250 iqtibos
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