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L. Anchordoqui

Ism variantlari: Luis A. Anchordoqui

Soʻnggi maʼlum muassasa:
City University of New York
ORCID:
0000-0003-1463-7136
3
h-indeks
0
i10-indeksi
41
Iqtiboslar
21
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0358100613192519982000201720202021202220232024202520261998: Nashrlar 1, Iqtiboslar 02000: Nashrlar 1, Iqtiboslar 02017: Nashrlar 1, Iqtiboslar 02020: Nashrlar 0, Iqtiboslar 12021: Nashrlar 5, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 12023: Nashrlar 0, Iqtiboslar 52024: Nashrlar 3, Iqtiboslar 122025: Nashrlar 7, Iqtiboslar 212026: Nashrlar 1, Iqtiboslar 1

Iqtibos tarixi

0613192519982000201720202021202220232024202520261998: Iqtiboslar 02000: Iqtiboslar 02017: Iqtiboslar 02020: Iqtiboslar 12021: Iqtiboslar 02022: Iqtiboslar 12023: Iqtiboslar 52024: Iqtiboslar 122025: Iqtiboslar 212026: Iqtiboslar 1

Nashr tarixi

03581019982000201720202021202220232024202520261998: Nashrlar 12000: Nashrlar 12017: Nashrlar 12020: Nashrlar 02021: Nashrlar 52022: Nashrlar 22023: Nashrlar 02024: Nashrlar 32025: Nashrlar 72026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134519982000201720202021202220232024202520261998: h-indeks 02000: h-indeks 02017: h-indeks 02020: h-indeks 12021: h-indeks 12022: h-indeks 12023: h-indeks 12024: h-indeks 32025: h-indeks 32026: h-indeks 3

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. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  5. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with 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. 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
  9. Measuring the muon content of inclined air showers using AERA and the water-Cherenkov detectors of the Pierre Auger Observatory20250 iqtibos
  10. Search for Ultra-high-energy Neutrons from Galactic Sources with the Pierre Auger Observatory20260 iqtibos
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