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AkademScholar

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Rio de Janeiro Federal Institute of Education, Science and Technology

Nom variantlari: Instituto Federal do Rio de Janeiro · Centro Federal de Educação Tecnológica de Química de Nilópolis · Federal Institute of Rio de Janeiro · IFRJ · Instituto Federal de Educação, Ciência e Tecnologia do Rio de Janeiro

Davlat:
BR
ROR:
https://ror.org/007qd1t98
3
h-indeks
43
Iqtiboslar
19
Asarlar
23
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0358100510152020132016201720202021202220232024202520262013: Nashrlar 2, Iqtiboslar 02016: Nashrlar 1, Iqtiboslar 02017: Nashrlar 1, Iqtiboslar 02020: Nashrlar 1, Iqtiboslar 02021: Nashrlar 1, Iqtiboslar 22022: Nashrlar 2, Iqtiboslar 22023: Nashrlar 4, Iqtiboslar 12024: Nashrlar 1, Iqtiboslar 132025: Nashrlar 6, Iqtiboslar 182026: Nashrlar 0, Iqtiboslar 7

Iqtibos tarixi

0510152020132016201720202021202220232024202520262013: Iqtiboslar 02016: Iqtiboslar 02017: Iqtiboslar 02020: Iqtiboslar 02021: Iqtiboslar 22022: Iqtiboslar 22023: Iqtiboslar 12024: Iqtiboslar 132025: Iqtiboslar 182026: Iqtiboslar 7

Nashr tarixi

03581020132016201720202021202220232024202520262013: Nashrlar 22016: Nashrlar 12017: Nashrlar 12020: Nashrlar 12021: Nashrlar 12022: Nashrlar 22023: Nashrlar 42024: Nashrlar 12025: Nashrlar 62026: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520132016201720202021202220232024202520262013: h-indeks 02016: h-indeks 02017: h-indeks 02020: h-indeks 02021: h-indeks 12022: h-indeks 22023: h-indeks 22024: h-indeks 22025: h-indeks 32026: h-indeks 3

Eng koʻp iqtibos qilingan asarlar

  1. 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
  2. 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
  3. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  4. Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 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. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos
  7. The Pierre Auger Observatory open data20250 iqtibos
  8. Expanding the Pierre Auger Observatory Open Data program20250 iqtibos