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Jaime Álvarez-Muñiz

Ism variantlari: J. Alvarez-Muñiz

Soʻnggi maʼlum muassasa:
Universidade de Santiago de Compostela
ORCID:
0000-0002-2367-0803
5
h-indeks
1
i10-indeksi
152
Iqtiboslar
52
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
035810025507510020172018201920202021202220232024202520262017: Nashrlar 4, Iqtiboslar 02018: Nashrlar 1, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 22020: Nashrlar 4, Iqtiboslar 42021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 3, Iqtiboslar 22023: Nashrlar 9, Iqtiboslar 32024: Nashrlar 5, Iqtiboslar 392025: Nashrlar 6, Iqtiboslar 972026: Nashrlar 1, Iqtiboslar 5

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 02018: Iqtiboslar 02019: Iqtiboslar 22020: Iqtiboslar 42021: Iqtiboslar 02022: Iqtiboslar 22023: Iqtiboslar 32024: Iqtiboslar 392025: Iqtiboslar 972026: Iqtiboslar 5

Nashr tarixi

03581020172018201920202021202220232024202520262017: Nashrlar 42018: Nashrlar 12019: Nashrlar 12020: Nashrlar 42021: Nashrlar 72022: Nashrlar 32023: Nashrlar 92024: Nashrlar 52025: Nashrlar 62026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520172018201920202021202220232024202520262017: h-indeks 02018: h-indeks 02019: h-indeks 12020: h-indeks 22021: h-indeks 22022: 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. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 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. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 iqtibos
  7. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos
  8. The Pierre Auger Observatory open data20250 iqtibos
  9. 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
  10. Measuring the muon content of inclined air showers using AERA and the water-Cherenkov detectors of the Pierre Auger Observatory20250 iqtibos
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