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AkademScholar

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Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

Laboratory of Subatomic Physics and Cosmology

Nom variantlari: Laboratoire de Physique Subatomique et de Cosmologie · LPSC · UMR 5821 · UMR5821

Davlat:
FR
ROR:
https://ror.org/03f0apy98
8
h-indeks
408
Iqtiboslar
96
Asarlar
95
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0510152005010015020020172018201920202021202220232024202520262017: Nashrlar 7, Iqtiboslar 42018: Nashrlar 2, Iqtiboslar 62019: Nashrlar 3, Iqtiboslar 92020: Nashrlar 2, Iqtiboslar 72021: Nashrlar 0, Iqtiboslar 112022: Nashrlar 1, Iqtiboslar 242023: Nashrlar 6, Iqtiboslar 272024: Nashrlar 17, Iqtiboslar 462025: Nashrlar 19, Iqtiboslar 1532026: Nashrlar 2, Iqtiboslar 95

Iqtibos tarixi

05010015020020172018201920202021202220232024202520262017: Iqtiboslar 42018: Iqtiboslar 62019: Iqtiboslar 92020: Iqtiboslar 72021: Iqtiboslar 112022: Iqtiboslar 242023: Iqtiboslar 272024: Iqtiboslar 462025: Iqtiboslar 1532026: Iqtiboslar 95

Nashr tarixi

0510152020172018201920202021202220232024202520262017: Nashrlar 72018: Nashrlar 22019: Nashrlar 32020: Nashrlar 22021: Nashrlar 02022: Nashrlar 12023: Nashrlar 62024: Nashrlar 172025: Nashrlar 192026: Nashrlar 2

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 22018: h-indeks 22019: h-indeks 22020: h-indeks 32021: h-indeks 32022: h-indeks 52023: h-indeks 52024: h-indeks 52025: h-indeks 82026: h-indeks 8

Eng koʻp iqtibos qilingan asarlar

  1. Mitigating imaging systematics for DESI 2024 emission Line Galaxies and beyond20255 iqtibos
  2. Validating the Galaxy and Quasar Catalog-Level Blinding Scheme for the DESI 2024 analysis20244 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. Optimal Reconstruction of Baryon Acoustic Oscillations for DESI 202420243 iqtibos
  5. Optimal reconstruction of baryon acoustic oscillations for DESI 202420253 iqtibos
  6. Dark Energy Survey: Galaxy sample for the baryonic acoustic oscillation measurement from the final dataset20243 iqtibos
  7. 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
  8. 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
  9. Fiducial-cosmology-dependent systematics for the DESI 2024 BAO analysis20252 iqtibos
  10. Large-scale Cosmic-ray Anisotropies with 19 yr of Data from the Pierre Auger Observatory20241 iqtibos