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AkademScholar

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Identifikatsiya

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University of Wisconsin–Madison

Nom variantlari: UW · UW–Madison · Universidad de Wisconsin-Madison · Université du Wisconsin à Madison

Davlat:
US
ROR:
https://ror.org/01y2jtd41
16
h-indeks
2,336
Iqtiboslar
592
Asarlar
908
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
013253850012525037550020172018201920202021202220232024202520262017: Nashrlar 28, Iqtiboslar 332018: Nashrlar 21, Iqtiboslar 372019: Nashrlar 18, Iqtiboslar 452020: Nashrlar 20, Iqtiboslar 882021: Nashrlar 29, Iqtiboslar 1422022: Nashrlar 19, Iqtiboslar 2132023: Nashrlar 29, Iqtiboslar 2002024: Nashrlar 16, Iqtiboslar 3522025: Nashrlar 11, Iqtiboslar 4542026: Nashrlar 11, Iqtiboslar 390

Iqtibos tarixi

012525037550020172018201920202021202220232024202520262017: Iqtiboslar 332018: Iqtiboslar 372019: Iqtiboslar 452020: Iqtiboslar 882021: Iqtiboslar 1422022: Iqtiboslar 2132023: Iqtiboslar 2002024: Iqtiboslar 3522025: Iqtiboslar 4542026: Iqtiboslar 390

Nashr tarixi

01325385020172018201920202021202220232024202520262017: Nashrlar 282018: Nashrlar 212019: Nashrlar 182020: Nashrlar 202021: Nashrlar 292022: Nashrlar 192023: Nashrlar 292024: Nashrlar 162025: Nashrlar 112026: Nashrlar 11

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0510152020172018201920202021202220232024202520262017: h-indeks 72018: h-indeks 72019: h-indeks 72020: h-indeks 82021: h-indeks 92022: h-indeks 102023: h-indeks 112024: h-indeks 112025: h-indeks 142026: h-indeks 16

Eng koʻp iqtibos qilingan asarlar

  1. Diluted magnetic semiconductor behavior in Co- and Gd-co-doped ZnO nanotubes for spintronic applications20234 iqtibos
  2. SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos20243 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. Dark Energy Survey: Galaxy sample for the baryonic acoustic oscillation measurement from the final dataset20243 iqtibos
  5. Determination of ππ scattering lengths from measurement of π+π− atom lifetime20112 iqtibos
  6. Study of correlations between secondary protons produced in proton-neon interactions at 300 GeV/<i>c</i>19841 iqtibos
  7. Neutral-strange-particle production in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mi/><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">Ne</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>20</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>pN</mml:mi></mml:math>interactions at 300 GeV19911 iqtibos
  8. Cumulative particle production in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">Ne</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>20</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow></mml:math>interactions at 300 GeV19921 iqtibos
  9. A BARYONIC SOLUTION TO THE MISSING SATELLITES PROBLEM20131 iqtibos
  10. SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets20241 iqtibos