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AkademScholar

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Identifikatsiya

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Gran Sasso Science Institute

Nom variantlari: GSSI · INFN Gran Sasso Science Institute · INFN-GSSI

Davlat:
IT
ROR:
https://ror.org/043qcb444
11
h-indeks
865
Iqtiboslar
124
Asarlar
93
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0510152006312518825020172018201920202021202220232024202520262017: Nashrlar 18, Iqtiboslar 42018: Nashrlar 9, Iqtiboslar 102019: Nashrlar 15, Iqtiboslar 342020: Nashrlar 19, Iqtiboslar 382021: Nashrlar 9, Iqtiboslar 522022: Nashrlar 8, Iqtiboslar 762023: Nashrlar 6, Iqtiboslar 912024: Nashrlar 7, Iqtiboslar 1412025: Nashrlar 11, Iqtiboslar 2202026: Nashrlar 5, Iqtiboslar 192

Iqtibos tarixi

06312518825020172018201920202021202220232024202520262017: Iqtiboslar 42018: Iqtiboslar 102019: Iqtiboslar 342020: Iqtiboslar 382021: Iqtiboslar 522022: Iqtiboslar 762023: Iqtiboslar 912024: Iqtiboslar 1412025: Iqtiboslar 2202026: Iqtiboslar 192

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 182018: Nashrlar 92019: Nashrlar 152020: Nashrlar 192021: Nashrlar 92022: Nashrlar 82023: Nashrlar 62024: Nashrlar 72025: Nashrlar 112026: Nashrlar 5

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0510152020172018201920202021202220232024202520262017: h-indeks 22018: h-indeks 32019: h-indeks 42020: h-indeks 42021: h-indeks 52022: h-indeks 62023: h-indeks 72024: h-indeks 82025: h-indeks 92026: h-indeks 11

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. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  8. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  9. AGILE, <i>Fermi</i>, <i>Swift</i>, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C +71.07 in outburst20181 iqtibos
  10. Towards Interferometric Triggering on Air Showers Induced by Tau Neutrino Interactions20191 iqtibos