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Teresa Bister

Ism variantlari: T. Bister

Soʻnggi maʼlum muassasa:
National Institute for Subatomic Physics
ORCID:
0000-0003-4005-0857
4
h-indeks
0
i10-indeksi
69
Iqtiboslar
33
Asarlar
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Iqtibos sharhi

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03581001325385020202021202220232024202520262020: Nashrlar 4, Iqtiboslar 02021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 02023: Nashrlar 9, Iqtiboslar 02024: Nashrlar 4, Iqtiboslar 212025: Nashrlar 6, Iqtiboslar 482026: Nashrlar 1, Iqtiboslar 0

Iqtibos tarixi

01325385020202021202220232024202520262020: Iqtiboslar 02021: Iqtiboslar 02022: Iqtiboslar 02023: Iqtiboslar 02024: Iqtiboslar 212025: Iqtiboslar 482026: Iqtiboslar 0

Nashr tarixi

03581020202021202220232024202520262020: Nashrlar 42021: Nashrlar 72022: Nashrlar 22023: Nashrlar 92024: Nashrlar 42025: Nashrlar 62026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520202021202220232024202520262020: h-indeks 02021: h-indeks 02022: h-indeks 02023: h-indeks 02024: h-indeks 22025: h-indeks 42026: h-indeks 4

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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