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Denise Boncioli

Ism variantlari: D. Boncioli

Soʻnggi maʼlum muassasa:
Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso
ORCID:
0000-0003-1186-9353
5
h-indeks
0
i10-indeksi
123
Iqtiboslar
49
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

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035810025507510020162017201920202021202220232024202520262016: Nashrlar 1, Iqtiboslar 02017: Nashrlar 4, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 12020: Nashrlar 5, Iqtiboslar 22021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 3, Iqtiboslar 12023: Nashrlar 9, Iqtiboslar 32024: Nashrlar 4, Iqtiboslar 352025: Nashrlar 6, Iqtiboslar 812026: Nashrlar 1, Iqtiboslar 0

Iqtibos tarixi

025507510020162017201920202021202220232024202520262016: Iqtiboslar 02017: Iqtiboslar 02019: Iqtiboslar 12020: Iqtiboslar 22021: Iqtiboslar 02022: Iqtiboslar 12023: Iqtiboslar 32024: Iqtiboslar 352025: Iqtiboslar 812026: Iqtiboslar 0

Nashr tarixi

03581020162017201920202021202220232024202520262016: Nashrlar 12017: Nashrlar 42019: Nashrlar 12020: Nashrlar 52021: Nashrlar 72022: Nashrlar 32023: Nashrlar 92024: Nashrlar 42025: Nashrlar 62026: Nashrlar 1

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0134520162017201920202021202220232024202520262016: h-indeks 02017: h-indeks 02019: h-indeks 12020: h-indeks 12021: h-indeks 12022: h-indeks 22023: h-indeks 22024: h-indeks 32025: h-indeks 52026: 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. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  6. 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
  7. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 iqtibos
  8. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos
  9. The Pierre Auger Observatory open data20250 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 Observatory20250 iqtibos
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