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AkademScholar

Kashfiyot

Xizmatlar

Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

Institute of Physics Rosario

Nom variantlari: IFIR · Instituto de Física Rosario

Davlat:
AR
ROR:
https://ror.org/03v7tny92
4
h-indeks
68
Iqtiboslar
29
Asarlar
24
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
03581001325385020162017201920202021202220232024202520262016: Nashrlar 1, Iqtiboslar 02017: Nashrlar 2, Iqtiboslar 02019: Nashrlar 0, Iqtiboslar 12020: Nashrlar 0, Iqtiboslar 12021: Nashrlar 4, Iqtiboslar 22022: Nashrlar 2, Iqtiboslar 52023: Nashrlar 10, Iqtiboslar 42024: Nashrlar 2, Iqtiboslar 192025: Nashrlar 5, Iqtiboslar 302026: Nashrlar 1, Iqtiboslar 6

Iqtibos tarixi

01325385020162017201920202021202220232024202520262016: Iqtiboslar 02017: Iqtiboslar 02019: Iqtiboslar 12020: Iqtiboslar 12021: Iqtiboslar 22022: Iqtiboslar 52023: Iqtiboslar 42024: Iqtiboslar 192025: Iqtiboslar 302026: Iqtiboslar 6

Nashr tarixi

03581020162017201920202021202220232024202520262016: Nashrlar 12017: Nashrlar 22019: Nashrlar 02020: Nashrlar 02021: Nashrlar 42022: Nashrlar 22023: Nashrlar 102024: Nashrlar 22025: Nashrlar 52026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520162017201920202021202220232024202520262016: h-indeks 02017: h-indeks 02019: h-indeks 12020: h-indeks 12021: h-indeks 12022: h-indeks 22023: h-indeks 22024: h-indeks 32025: h-indeks 42026: h-indeks 4

Eng koʻp iqtibos qilingan asarlar

  1. 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
  2. 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
  3. A Search for Photons with Energies Above 2 × 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory20222 iqtibos
  4. 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
  5. Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory20240 iqtibos
  6. Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory20250 iqtibos
  7. The Pierre Auger Observatory open data20250 iqtibos
  8. Measuring the muon content of inclined air showers using AERA and the water-Cherenkov detectors of the Pierre Auger Observatory20250 iqtibos
  9. Long-term monitoring of the optical performance of the primary mirrors at the Coihueco and Loma Amarilla sites of the Pierre Auger Observatory20260 iqtibos