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AkademScholar

Kashfiyot

Xizmatlar

Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

University of Salento

Nom variantlari: Università degli Studi di Lecce · Università del Salento · Universität Salento · Université du salento

Davlat:
IT
ROR:
https://ror.org/03fc1k060
7
h-indeks
279
Iqtiboslar
108
Asarlar
160
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
06131925025507510020172018201920202021202220232024202520262017: Nashrlar 9, Iqtiboslar 52018: Nashrlar 4, Iqtiboslar 12019: Nashrlar 5, Iqtiboslar 122020: Nashrlar 12, Iqtiboslar 52021: Nashrlar 6, Iqtiboslar 12022: Nashrlar 8, Iqtiboslar 312023: Nashrlar 7, Iqtiboslar 182024: Nashrlar 7, Iqtiboslar 552025: Nashrlar 21, Iqtiboslar 982026: Nashrlar 5, Iqtiboslar 38

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 52018: Iqtiboslar 12019: Iqtiboslar 122020: Iqtiboslar 52021: Iqtiboslar 12022: Iqtiboslar 312023: Iqtiboslar 182024: Iqtiboslar 552025: Iqtiboslar 982026: Iqtiboslar 38

Nashr tarixi

0613192520172018201920202021202220232024202520262017: Nashrlar 92018: Nashrlar 42019: Nashrlar 52020: Nashrlar 122021: Nashrlar 62022: Nashrlar 82023: Nashrlar 72024: Nashrlar 72025: Nashrlar 212026: Nashrlar 5

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 32023: h-indeks 32024: h-indeks 52025: h-indeks 62026: 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. 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. Harnessing chickpea bacterial endophytes for improved plant health and fitness20243 iqtibos
  4. 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
  5. 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
  6. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  7. 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
  8. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  9. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  10. <i>Euclid</i> preparation20251 iqtibos