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Mualliflar

A. di Matteo

Ism variantlari: Armando di Matteo

Soʻnggi maʼlum muassasa:
National Institute for Nuclear Physics, Turin Section
ORCID:
0000-0002-8260-1867
6
h-indeks
1
i10-indeksi
112
Iqtiboslar
48
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
05101520025507510020162017201920202021202220232024202520262016: Nashrlar 1, Iqtiboslar 02017: Nashrlar 3, Iqtiboslar 02019: Nashrlar 0, Iqtiboslar 32020: Nashrlar 4, Iqtiboslar 22021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 152023: Nashrlar 8, Iqtiboslar 02024: Nashrlar 4, Iqtiboslar 212025: Nashrlar 15, Iqtiboslar 582026: Nashrlar 3, Iqtiboslar 13

Iqtibos tarixi

025507510020162017201920202021202220232024202520262016: Iqtiboslar 02017: Iqtiboslar 02019: Iqtiboslar 32020: Iqtiboslar 22021: Iqtiboslar 02022: Iqtiboslar 152023: Iqtiboslar 02024: Iqtiboslar 212025: Iqtiboslar 582026: Iqtiboslar 13

Nashr tarixi

0510152020162017201920202021202220232024202520262016: Nashrlar 12017: Nashrlar 32019: Nashrlar 02020: Nashrlar 42021: Nashrlar 72022: Nashrlar 22023: Nashrlar 82024: Nashrlar 42025: Nashrlar 152026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020162017201920202021202220232024202520262016: h-indeks 02017: h-indeks 02019: h-indeks 12020: h-indeks 22021: h-indeks 22022: h-indeks 22023: h-indeks 22024: h-indeks 32025: h-indeks 52026: h-indeks 6

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 Observatory20243 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 Learning20253 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 learning20253 iqtibos
  4. 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 Observatory20252 iqtibos
  5. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  6. A composition-informed search for large-scale anisotropy with the Pierre Auger Observatory20251 iqtibos
  7. Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory20251 iqtibos
  8. Publisher's Note:20220 iqtibos
  9. 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
  10. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 iqtibos

Hammualliflar

Yana 23 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 25 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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