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Mualliflar

Fabio Convenga

Ism variantlari: F. Convenga

Soʻnggi maʼlum muassasa:
Gran Sasso Science Institute
ORCID:
0000-0002-2841-1034
5
h-indeks
1
i10-indeksi
98
Iqtiboslar
50
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
05101520013253850201920202021202220232024202520262019: Nashrlar 1, Iqtiboslar 02020: Nashrlar 4, Iqtiboslar 02021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 112023: Nashrlar 9, Iqtiboslar 02024: Nashrlar 4, Iqtiboslar 222025: Nashrlar 20, Iqtiboslar 502026: Nashrlar 3, Iqtiboslar 15

Iqtibos tarixi

013253850201920202021202220232024202520262019: Iqtiboslar 02020: Iqtiboslar 02021: Iqtiboslar 02022: Iqtiboslar 112023: Iqtiboslar 02024: Iqtiboslar 222025: Iqtiboslar 502026: Iqtiboslar 15

Nashr tarixi

05101520201920202021202220232024202520262019: Nashrlar 12020: Nashrlar 42021: Nashrlar 72022: Nashrlar 22023: Nashrlar 92024: Nashrlar 42025: Nashrlar 202026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

01345201920202021202220232024202520262019: h-indeks 02020: h-indeks 02021: h-indeks 02022: h-indeks 22023: h-indeks 22024: h-indeks 32025: h-indeks 42026: h-indeks 5

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. 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
  6. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  7. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  8. Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 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 29 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 21 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan