Asosiy kontentga oʻtish
AkademScholar

Kashfiyot

Xizmatlar

Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

Instituto de Tecnologías en Detección y Astropartículas

Nom variantlari: ITeDA

Davlat:
AR
ROR:
https://ror.org/048f36m54
7
h-indeks
204
Iqtiboslar
57
Asarlar
450
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
035810025507510020172018201920202021202220232024202520262017: Nashrlar 4, Iqtiboslar 02018: Nashrlar 1, Iqtiboslar 02019: Nashrlar 3, Iqtiboslar 102020: Nashrlar 6, Iqtiboslar 42021: Nashrlar 8, Iqtiboslar 02022: Nashrlar 3, Iqtiboslar 292023: Nashrlar 10, Iqtiboslar 22024: Nashrlar 4, Iqtiboslar 402025: Nashrlar 6, Iqtiboslar 942026: Nashrlar 4, Iqtiboslar 24

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 02018: Iqtiboslar 02019: Iqtiboslar 102020: Iqtiboslar 42021: Iqtiboslar 02022: Iqtiboslar 292023: Iqtiboslar 22024: Iqtiboslar 402025: Iqtiboslar 942026: Iqtiboslar 24

Nashr tarixi

03581020172018201920202021202220232024202520262017: Nashrlar 42018: Nashrlar 12019: Nashrlar 32020: Nashrlar 62021: Nashrlar 82022: Nashrlar 32023: Nashrlar 102024: Nashrlar 42025: Nashrlar 62026: Nashrlar 4

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 12018: h-indeks 12019: h-indeks 22020: h-indeks 32021: h-indeks 32022: h-indeks 32023: h-indeks 32024: h-indeks 42025: h-indeks 62026: h-indeks 7

Eng koʻp iqtibos qilingan asarlar

  1. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  2. 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
  3. 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
  4. 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
  5. A 3‐Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic‐Ray Observatory20202 iqtibos
  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 Observatory20252 iqtibos
  7. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  8. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos
  9. Searches for Anisotropies in the Arrival Directions of the Highest Energy Cosmic Rays Detected by the Pierre Auger Observatory20150 iqtibos
  10. Publisher's Note:20220 iqtibos