Asosiy kontentga oʻtish
AkademScholar

Kashfiyot

Xizmatlar

Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Mualliflar

Teresa Bister

Ism variantlari: T. Bister

Soʻnggi maʼlum muassasa:
National Institute for Subatomic Physics
ORCID:
0000-0003-4005-0857
4
h-indeks
1
i10-indeksi
93
Iqtiboslar
49
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0510152001325385020202021202220232024202520262020: Nashrlar 4, Iqtiboslar 02021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 102023: Nashrlar 9, Iqtiboslar 02024: Nashrlar 4, Iqtiboslar 212025: Nashrlar 20, Iqtiboslar 482026: Nashrlar 3, Iqtiboslar 14

Iqtibos tarixi

01325385020202021202220232024202520262020: Iqtiboslar 02021: Iqtiboslar 02022: Iqtiboslar 102023: Iqtiboslar 02024: Iqtiboslar 212025: Iqtiboslar 482026: Iqtiboslar 14

Nashr tarixi

0510152020202021202220232024202520262020: Nashrlar 42021: Nashrlar 72022: Nashrlar 22023: Nashrlar 92024: Nashrlar 42025: Nashrlar 202026: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520202021202220232024202520262020: h-indeks 02021: h-indeks 02022: h-indeks 22023: h-indeks 22024: h-indeks 32025: 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 Observatory20243 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 Learning20253 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 learning20253 iqtibos
  4. 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
  5. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  6. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  7. Measurement of the Inelastic Proton-Proton Cross-Section at $\sqrt{s} \geq 40$ TeV Using the Hybrid Data of the Pierre Auger Observatory20251 iqtibos
  8. A composition-informed search for large-scale anisotropy with the Pierre Auger Observatory20251 iqtibos
  9. Calibration and Performance of the Surface Scintillator Detector of the Pierre Auger Observatory20251 iqtibos
  10. AugerPrime: Status and first results20251 iqtibos

Hammualliflar

Yana 28 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 21 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

AkademIndex'da koʻrish →