Skip to content
AkademScholar

Products

For developers

AkademBasesoonDeveloper API
Authors

Mario Buscemi

Last known institution:
Istituto Nazionale di Fisica Nucleare, Sezione di Catania
ORCID:
0000-0003-2123-5434
5
h-index
0
i10-index
113
Citations
39
Works
Trends over time

Performance over time

Citation overview

Publications (bars) and citations (line) by year

  • Publications
  • Citations
035810025507510020162017201820192020202120222023202420252016: Publications 1, Citations 02017: Publications 4, Citations 02018: Publications 1, Citations 02019: Publications 1, Citations 22020: Publications 5, Citations 32021: Publications 7, Citations 02022: Publications 2, Citations 22023: Publications 9, Citations 22024: Publications 2, Citations 322025: Publications 3, Citations 72

Citation history

025507510020162017201820192020202120222023202420252016: Citations 02017: Citations 02018: Citations 02019: Citations 22020: Citations 32021: Citations 02022: Citations 22023: Citations 22024: Citations 322025: Citations 72

Publication history

03581020162017201820192020202120222023202420252016: Publications 12017: Publications 42018: Publications 12019: Publications 12020: Publications 52021: Publications 72022: Publications 22023: Publications 92024: Publications 22025: Publications 3

h-index evolution

Cumulative h-index by year

0134520162017201820192020202120222023202420252016: h-index 02017: h-index 02018: h-index 02019: h-index 12020: h-index 22021: h-index 22022: h-index 22023: h-index 22024: h-index 32025: h-index 5

Most-cited works

  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 citations
  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 citations
  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 citations
  4. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20201 citations
  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 citations
  6. 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 citations
View in AkademIndex →