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LIP - Laboratory of Instrumentation and Experimental Particle Physics

Nom variantlari: LIP · LIP - Laboratório de Instrumentação e Física Experimental de Partículas · Laboratory of Instrumentation and Experimental Particles Physics · Laboratório de Instrumentação e Física Experimental de Partículas

Davlat:
PT
ROR:
https://ror.org/01hys1667
7
h-indeks
280
Iqtiboslar
110
Asarlar
143
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
05101520025507510020172018201920202021202220232024202520262017: Nashrlar 8, Iqtiboslar 22018: Nashrlar 4, Iqtiboslar 32019: Nashrlar 6, Iqtiboslar 112020: Nashrlar 13, Iqtiboslar 92021: Nashrlar 7, Iqtiboslar 82022: Nashrlar 5, Iqtiboslar 332023: Nashrlar 6, Iqtiboslar 332024: Nashrlar 4, Iqtiboslar 412025: Nashrlar 19, Iqtiboslar 902026: Nashrlar 4, Iqtiboslar 34

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 22018: Iqtiboslar 32019: Iqtiboslar 112020: Iqtiboslar 92021: Iqtiboslar 82022: Iqtiboslar 332023: Iqtiboslar 332024: Iqtiboslar 412025: Iqtiboslar 902026: Iqtiboslar 34

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 82018: Nashrlar 42019: Nashrlar 62020: Nashrlar 132021: Nashrlar 72022: Nashrlar 52023: Nashrlar 62024: Nashrlar 42025: Nashrlar 192026: Nashrlar 4

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 22018: h-indeks 32019: h-indeks 32020: h-indeks 32021: h-indeks 32022: h-indeks 42023: h-indeks 42024: h-indeks 42025: h-indeks 62026: h-indeks 7

Eng koʻp iqtibos qilingan asarlar

  1. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  2. Actinide signatures in low electron fraction kilonova ejecta20243 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 mass and width of the Z0-particle from multihadronic final states produced in e+e− annihilations19892 iqtibos
  5. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  6. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  7. Study of the leptonic decays of the Z0 boson19902 iqtibos
  8. A study of intermittency in hadronic Z0 decays19901 iqtibos
  9. Production of hydrogen isotopes and charged pions in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>p</mml:mi></mml:math> (3.5 GeV) <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mo>+</mml:mo><mml:mo> </mml:mo><mml:mmultiscripts><mml:mi>Nb</mml:mi><mml:mprescripts/><mml:none/><mml:mn>93</mml:mn></mml:mmultiscripts></mml:math> reactions20231 iqtibos
  10. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos