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AkademScholar

Mahsulotlar

Ishlab chiquvchilar uchun

AkademBasetez oradaDasturchilar API
Mualliflar

Mario Buscemi

Soʻnggi maʼlum muassasa:
Istituto Nazionale di Fisica Nucleare, Sezione di Catania
ORCID:
0000-0003-2123-5434
5
h-indeks
0
i10-indeksi
113
Iqtiboslar
39
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
035810025507510020162017201820192020202120222023202420252016: Nashrlar 1, Iqtiboslar 02017: Nashrlar 4, Iqtiboslar 02018: Nashrlar 1, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 22020: Nashrlar 5, Iqtiboslar 32021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 22023: Nashrlar 9, Iqtiboslar 22024: Nashrlar 2, Iqtiboslar 322025: Nashrlar 3, Iqtiboslar 72

Iqtibos tarixi

025507510020162017201820192020202120222023202420252016: Iqtiboslar 02017: Iqtiboslar 02018: Iqtiboslar 02019: Iqtiboslar 22020: Iqtiboslar 32021: Iqtiboslar 02022: Iqtiboslar 22023: Iqtiboslar 22024: Iqtiboslar 322025: Iqtiboslar 72

Nashr tarixi

03581020162017201820192020202120222023202420252016: Nashrlar 12017: Nashrlar 42018: Nashrlar 12019: Nashrlar 12020: Nashrlar 52021: Nashrlar 72022: Nashrlar 22023: Nashrlar 92024: Nashrlar 22025: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520162017201820192020202120222023202420252016: h-indeks 02017: h-indeks 02018: h-indeks 02019: h-indeks 12020: h-indeks 22021: h-indeks 22022: h-indeks 22023: h-indeks 22024: h-indeks 32025: h-indeks 5

Eng koʻp iqtibos qilingan asarlar

  1. Testing hadronic-model predictions of depth of maximum of air-shower profiles and ground-particle signals using hybrid data of the Pierre Auger Observatory20242 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 Learning20252 iqtibos
  3. 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 learning20252 iqtibos
  4. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20201 iqtibos
  5. Search for photons above <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>18</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math> by simultaneously measuring the atmospheric depth and the muon content of air showers at the Pierre Auger Observatory20240 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 Observatory20250 iqtibos
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