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AkademScholar

Mahsulotlar

Ishlab chiquvchilar uchun

AkademBasetez oradaDasturchilar API
Mualliflar

C. Dobrigkeit

Ism variantlari: J. A. Chinellato

Soʻnggi maʼlum muassasa:
Universidade Estadual de Campinas (UNICAMP)
ORCID:
0000-0002-1236-0789
5
h-indeks
0
i10-indeksi
133
Iqtiboslar
52
Asarlar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
035810025507510020172018201920202021202220232024202520262017: Nashrlar 4, Iqtiboslar 02018: Nashrlar 1, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 22020: Nashrlar 5, Iqtiboslar 42021: Nashrlar 7, Iqtiboslar 02022: Nashrlar 2, Iqtiboslar 22023: Nashrlar 7, Iqtiboslar 22024: Nashrlar 4, Iqtiboslar 312025: Nashrlar 6, Iqtiboslar 882026: Nashrlar 1, Iqtiboslar 2

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 02018: Iqtiboslar 02019: Iqtiboslar 22020: Iqtiboslar 42021: Iqtiboslar 02022: Iqtiboslar 22023: Iqtiboslar 22024: Iqtiboslar 312025: Iqtiboslar 882026: Iqtiboslar 2

Nashr tarixi

03581020172018201920202021202220232024202520262017: Nashrlar 42018: Nashrlar 12019: Nashrlar 12020: Nashrlar 52021: Nashrlar 72022: Nashrlar 22023: Nashrlar 72024: Nashrlar 42025: Nashrlar 62026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520172018201920202021202220232024202520262017: h-indeks 12018: h-indeks 12019: h-indeks 12020: h-indeks 22021: h-indeks 22022: h-indeks 22023: h-indeks 22024: h-indeks 32025: h-indeks 52026: h-indeks 5

Eng koʻp iqtibos qilingan asarlar

  1. Observation of a high-energy cosmic-ray family caused by a Centauro-type nuclear interaction in the joint emulsion chamber experiment at the Pamirs19874 iqtibos
  2. Observation of very high energy cosmic-ray families in emulsion chambers at high mountain altitudes (I)19923 iqtibos
  3. 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
  4. 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
  5. 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
  6. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20201 iqtibos
  7. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  8. Nuclear interactions of super high energy cosmic-rays observed in mountain emulsion chambers19811 iqtibos
  9. 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
  10. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 iqtibos
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