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M. E. Bertaina

Ism variantlari: М. Бертаина · m bertaina

Soʻnggi maʼlum muassasa:
University of Turin
ORCID:
0000-0003-1069-1397
3
h-indeks
0
i10-indeksi
49
Iqtiboslar
30
Asarlar
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Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0510152001325385020162017201920202021202220232024202520262016: Nashrlar 1, Iqtiboslar 02017: Nashrlar 0, Iqtiboslar 12019: Nashrlar 1, Iqtiboslar 02020: Nashrlar 2, Iqtiboslar 02021: Nashrlar 2, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 42023: Nashrlar 4, Iqtiboslar 02024: Nashrlar 4, Iqtiboslar 92025: Nashrlar 11, Iqtiboslar 262026: Nashrlar 3, Iqtiboslar 9

Iqtibos tarixi

01325385020162017201920202021202220232024202520262016: Iqtiboslar 02017: Iqtiboslar 12019: Iqtiboslar 02020: Iqtiboslar 02021: Iqtiboslar 02022: Iqtiboslar 42023: Iqtiboslar 02024: Iqtiboslar 92025: Iqtiboslar 262026: Iqtiboslar 9

Nashr tarixi

0510152020162017201920202021202220232024202520262016: Nashrlar 12017: Nashrlar 02019: Nashrlar 12020: Nashrlar 22021: Nashrlar 22022: Nashrlar 22023: Nashrlar 42024: Nashrlar 42025: Nashrlar 112026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520162017201920202021202220232024202520262016: h-indeks 02017: h-indeks 12019: h-indeks 12020: h-indeks 12021: h-indeks 12022: h-indeks 12023: h-indeks 12024: h-indeks 22025: h-indeks 32026: h-indeks 3

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. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  8. A comparison of the cosmic-ray energy scales of Tunka-133 and KASCADE-Grande via their radio extensions Tunka-Rex and LOPES20161 iqtibos
  9. A composition-informed search for large-scale anisotropy with the Pierre Auger Observatory20251 iqtibos
  10. AugerPrime: Status and first results20251 iqtibos

Hammualliflar

Yana 22 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 8 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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