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Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Mualliflar

R. M. de Almeida

Soʻnggi maʼlum muassasa:
Federal University of Rio de Janeiro
ORCID:
0000-0003-3104-2724
3
h-indeks
0
i10-indeksi
27
Iqtiboslar
17
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
03581005101520201420192020202220232024202520262014: Nashrlar 1, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 12020: Nashrlar 1, Iqtiboslar 02022: Nashrlar 0, Iqtiboslar 32023: Nashrlar 0, Iqtiboslar 12024: Nashrlar 4, Iqtiboslar 22025: Nashrlar 7, Iqtiboslar 122026: Nashrlar 3, Iqtiboslar 8

Iqtibos tarixi

05101520201420192020202220232024202520262014: Iqtiboslar 02019: Iqtiboslar 12020: Iqtiboslar 02022: Iqtiboslar 32023: Iqtiboslar 12024: Iqtiboslar 22025: Iqtiboslar 122026: Iqtiboslar 8

Nashr tarixi

035810201420192020202220232024202520262014: Nashrlar 12019: Nashrlar 12020: Nashrlar 12022: Nashrlar 02023: Nashrlar 02024: Nashrlar 42025: Nashrlar 72026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

01345201420192020202220232024202520262014: h-indeks 02019: h-indeks 12020: h-indeks 12022: h-indeks 12023: h-indeks 12024: h-indeks 22025: h-indeks 22026: h-indeks 3

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. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  8. 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
  9. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 iqtibos
  10. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos

Hammualliflar

Yana 16 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 1 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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