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AkademScholar

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National Institute for Nuclear Physics, Lecce Section

Nom variantlari: Istituto Nazionale di Fisica Nucleare, Sezione di Lecce · INFN Lecce · INFN Lecce Section · INFN Sezione di Lecce · INFN-LE

Davlat:
IT
ROR:
https://ror.org/00qrf6g60
7
h-indeks
249
Iqtiboslar
81
Asarlar
138
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
035810025507510020172018201920202021202220232024202520262017: Nashrlar 7, Iqtiboslar 02018: Nashrlar 2, Iqtiboslar 12019: Nashrlar 3, Iqtiboslar 112020: Nashrlar 6, Iqtiboslar 42021: Nashrlar 6, Iqtiboslar 32022: Nashrlar 2, Iqtiboslar 332023: Nashrlar 5, Iqtiboslar 172024: Nashrlar 3, Iqtiboslar 422025: Nashrlar 6, Iqtiboslar 832026: Nashrlar 2, Iqtiboslar 19

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 02018: Iqtiboslar 12019: Iqtiboslar 112020: Iqtiboslar 42021: Iqtiboslar 32022: Iqtiboslar 332023: Iqtiboslar 172024: Iqtiboslar 422025: Iqtiboslar 832026: Iqtiboslar 19

Nashr tarixi

03581020172018201920202021202220232024202520262017: Nashrlar 72018: Nashrlar 22019: Nashrlar 32020: Nashrlar 62021: Nashrlar 62022: Nashrlar 22023: Nashrlar 52024: Nashrlar 32025: Nashrlar 62026: Nashrlar 2

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 32018: h-indeks 32019: h-indeks 32020: h-indeks 32021: h-indeks 32022: h-indeks 42023: h-indeks 52024: h-indeks 52025: h-indeks 72026: h-indeks 7

Eng koʻp iqtibos qilingan asarlar

  1. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 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. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 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. Measurements of the cross sections for open charm and beauty production in γγ collisions at –202 GeV20012 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. <i>Euclid</i> preparation20251 iqtibos
  9. Measurement of the W-pair production cross section and W-decay branching fractions in e+e− interactions at GeV20001 iqtibos
  10. Search for anomalous ZZγ and Zγγ couplings in the process e+e−→Zγ at LEP20001 iqtibos