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Identifikatsiya

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Mualliflar

Gopal Bhatta

Soʻnggi maʼlum muassasa:
Institute of Nuclear Physics
ORCID:
0000-0002-0705-6619
3
h-indeks
1
i10-indeksi
46
Iqtiboslar
19
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0358100613192520132016201820192020202220232024202520262013: Nashrlar 0, Iqtiboslar 12016: Nashrlar 0, Iqtiboslar 12018: Nashrlar 0, Iqtiboslar 12019: Nashrlar 0, Iqtiboslar 12020: Nashrlar 0, Iqtiboslar 32022: Nashrlar 2, Iqtiboslar 02023: Nashrlar 9, Iqtiboslar 12024: Nashrlar 4, Iqtiboslar 112025: Nashrlar 3, Iqtiboslar 212026: Nashrlar 0, Iqtiboslar 5

Iqtibos tarixi

0613192520132016201820192020202220232024202520262013: Iqtiboslar 12016: Iqtiboslar 12018: Iqtiboslar 12019: Iqtiboslar 12020: Iqtiboslar 32022: Iqtiboslar 02023: Iqtiboslar 12024: Iqtiboslar 112025: Iqtiboslar 212026: Iqtiboslar 5

Nashr tarixi

03581020132016201820192020202220232024202520262013: Nashrlar 02016: Nashrlar 02018: Nashrlar 02019: Nashrlar 02020: Nashrlar 02022: Nashrlar 22023: Nashrlar 92024: Nashrlar 42025: Nashrlar 32026: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520132016201820192020202220232024202520262013: h-indeks 12016: h-indeks 12018: h-indeks 12019: h-indeks 12020: h-indeks 12022: h-indeks 12023: h-indeks 12024: h-indeks 22025: 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 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. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  5. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  6. 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
  7. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 iqtibos
  8. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos

Hammualliflar

Yana 8 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 11 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

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