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Gopal Bhatta

Soʻnggi maʼlum muassasa:
Institute of Nuclear Physics, Polish Academy of Sciences
ORCID:
0000-0002-0705-6619
3
h-indeks
1
i10-indeksi
41
Iqtiboslar
19
Asarlar
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Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0358100613192520122013201620182019202020222023202420252012: Nashrlar 0, Iqtiboslar 12013: 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 21

Iqtibos tarixi

0613192520122013201620182019202020222023202420252012: Iqtiboslar 12013: Iqtiboslar 12016: Iqtiboslar 12018: Iqtiboslar 12019: Iqtiboslar 12020: Iqtiboslar 32022: Iqtiboslar 02023: Iqtiboslar 12024: Iqtiboslar 112025: Iqtiboslar 21

Nashr tarixi

03581020122013201620182019202020222023202420252012: Nashrlar 02013: Nashrlar 02016: Nashrlar 02018: Nashrlar 02019: Nashrlar 02020: Nashrlar 02022: Nashrlar 22023: Nashrlar 92024: Nashrlar 42025: Nashrlar 3

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520122013201620182019202020222023202420252012: h-indeks 12013: 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 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 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
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