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Mualliflar

B. R. Dawson

Soʻnggi maʼlum muassasa:
The University of Adelaide
ORCID:
0000-0002-4271-3055
6
h-indeks
2
i10-indeksi
190
Iqtiboslar
67
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
05101520025507510020172018201920202021202220232024202520262017: Nashrlar 4, Iqtiboslar 12018: Nashrlar 1, Iqtiboslar 02019: Nashrlar 2, Iqtiboslar 92020: Nashrlar 5, Iqtiboslar 32021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 282023: Nashrlar 9, Iqtiboslar 22024: Nashrlar 4, Iqtiboslar 342025: Nashrlar 20, Iqtiboslar 862026: Nashrlar 3, Iqtiboslar 26

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 12018: Iqtiboslar 02019: Iqtiboslar 92020: Iqtiboslar 32021: Iqtiboslar 02022: Iqtiboslar 282023: Iqtiboslar 22024: Iqtiboslar 342025: Iqtiboslar 862026: Iqtiboslar 26

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 42018: Nashrlar 12019: Nashrlar 22020: Nashrlar 52021: Nashrlar 72022: Nashrlar 22023: Nashrlar 92024: Nashrlar 42025: Nashrlar 202026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 12018: h-indeks 12019: h-indeks 22020: h-indeks 22021: h-indeks 22022: h-indeks 32023: h-indeks 32024: h-indeks 42025: h-indeks 62026: h-indeks 6

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. Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 iqtibos
  10. A composition-informed search for large-scale anisotropy with the Pierre Auger Observatory20251 iqtibos

Hammualliflar

Yana 30 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 36 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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