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AkademScholar

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National Institute for Nuclear Physics, Milan Unit

Nom variantlari: Istituto Nazionale di Fisica Nucleare, Sezione di Milano · INFN Milan · INFN Milan Unit · INFN Milano · INFN Sezione di Milano · INFN-MI

Davlat:
IT
ROR:
https://ror.org/04w4m6z96
12
h-indeks
1,196
Iqtiboslar
318
Asarlar
326
Mualliflar
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Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
013253850012525037550020172018201920202021202220232024202520262017: Nashrlar 8, Iqtiboslar 22018: Nashrlar 11, Iqtiboslar 212019: Nashrlar 12, Iqtiboslar 182020: Nashrlar 24, Iqtiboslar 132021: Nashrlar 14, Iqtiboslar 712022: Nashrlar 14, Iqtiboslar 572023: Nashrlar 11, Iqtiboslar 1892024: Nashrlar 9, Iqtiboslar 1782025: Nashrlar 36, Iqtiboslar 3612026: Nashrlar 28, Iqtiboslar 182

Iqtibos tarixi

012525037550020172018201920202021202220232024202520262017: Iqtiboslar 22018: Iqtiboslar 212019: Iqtiboslar 182020: Iqtiboslar 132021: Iqtiboslar 712022: Iqtiboslar 572023: Iqtiboslar 1892024: Iqtiboslar 1782025: Iqtiboslar 3612026: Iqtiboslar 182

Nashr tarixi

01325385020172018201920202021202220232024202520262017: Nashrlar 82018: Nashrlar 112019: Nashrlar 122020: Nashrlar 242021: Nashrlar 142022: Nashrlar 142023: Nashrlar 112024: Nashrlar 92025: Nashrlar 362026: Nashrlar 28

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0510152020172018201920202021202220232024202520262017: h-indeks 32018: h-indeks 32019: h-indeks 42020: h-indeks 42021: h-indeks 42022: h-indeks 52023: h-indeks 82024: h-indeks 82025: h-indeks 112026: h-indeks 12

Eng koʻp iqtibos qilingan asarlar

  1. Euclid Quick Data Release (Q1)20256 iqtibos
  2. Cosmology and fundamental physics with the Euclid satellite20185 iqtibos
  3. <i>Euclid</i> preparation20255 iqtibos
  4. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  5. 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
  6. <i>Euclid</i> preparation20253 iqtibos
  7. Euclid Quick Data Release (Q1)20253 iqtibos
  8. Measurement of the mass and width of the Z0-particle from multihadronic final states produced in e+e− annihilations19892 iqtibos
  9. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  10. 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