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Identifikatsiya

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Mualliflar

G. Cataldi

Soʻnggi maʼlum muassasa:
National Institute for Nuclear Physics, Lecce Section
ORCID:
0000-0001-8066-7718
6
h-indeks
2
i10-indeksi
182
Iqtiboslar
61
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
05101520025507510020172018201920202021202220232024202520262017: Nashrlar 4, Iqtiboslar 12018: Nashrlar 1, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 92020: Nashrlar 5, Iqtiboslar 32021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 272023: Nashrlar 8, Iqtiboslar 22024: Nashrlar 4, Iqtiboslar 312025: Nashrlar 16, Iqtiboslar 842026: Nashrlar 3, Iqtiboslar 24

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 12018: Iqtiboslar 02019: Iqtiboslar 92020: Iqtiboslar 32021: Iqtiboslar 02022: Iqtiboslar 272023: Iqtiboslar 22024: Iqtiboslar 312025: Iqtiboslar 842026: Iqtiboslar 24

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 42018: Nashrlar 12019: Nashrlar 12020: Nashrlar 52021: Nashrlar 72022: Nashrlar 22023: Nashrlar 82024: Nashrlar 42025: Nashrlar 162026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 12018: h-indeks 12019: h-indeks 22020: h-indeks 22021: h-indeks 22022: h-indeks 32023: h-indeks 32024: h-indeks 42025: h-indeks 62026: h-indeks 6

Eng koʻp iqtibos qilingan asarlar

  1. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  2. 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
  3. 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
  4. 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
  5. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  6. 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
  7. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  8. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  9. A composition-informed search for large-scale anisotropy with the Pierre Auger Observatory20251 iqtibos
  10. Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory20251 iqtibos

Hammualliflar

Yana 26 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 35 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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