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Rikkyo University

Nom variantlari: Rikkyō daigaku · Saint Paul's Universit

Davlat:
JP
ROR:
https://ror.org/00x194q47
7
h-indeks
162
Iqtiboslar
41
Asarlar
60
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
013450510152020172018201920202021202220232024202520262017: Nashrlar 0, Iqtiboslar 12018: Nashrlar 3, Iqtiboslar 22019: Nashrlar 1, Iqtiboslar 42020: Nashrlar 2, Iqtiboslar 72021: Nashrlar 0, Iqtiboslar 152022: Nashrlar 0, Iqtiboslar 52023: Nashrlar 0, Iqtiboslar 202024: Nashrlar 1, Iqtiboslar 202025: Nashrlar 2, Iqtiboslar 122026: Nashrlar 5, Iqtiboslar 16

Iqtibos tarixi

0510152020172018201920202021202220232024202520262017: Iqtiboslar 12018: Iqtiboslar 22019: Iqtiboslar 42020: Iqtiboslar 72021: Iqtiboslar 152022: Iqtiboslar 52023: Iqtiboslar 202024: Iqtiboslar 202025: Iqtiboslar 122026: Iqtiboslar 16

Nashr tarixi

0134520172018201920202021202220232024202520262017: Nashrlar 02018: Nashrlar 32019: Nashrlar 12020: Nashrlar 22021: Nashrlar 02022: Nashrlar 02023: Nashrlar 02024: Nashrlar 12025: Nashrlar 22026: Nashrlar 5

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 42018: h-indeks 42019: h-indeks 42020: h-indeks 52021: h-indeks 52022: h-indeks 52023: h-indeks 52024: h-indeks 62025: h-indeks 72026: h-indeks 7

Eng koʻp iqtibos qilingan asarlar

  1. Introduction20100 iqtibos
  2. Introduction20100 iqtibos
  3. Doubly resonant coherent excitation in the x-ray regime: <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mn>1</mml:mn><mml:mi>s</mml:mi><mml:mtext>−</mml:mtext><mml:mn>3</mml:mn><mml:mi>d</mml:mi></mml:mrow></mml:math> transition in H-like <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msup><mml:mrow><mml:mi>Ar</mml:mi></mml:mrow><mml:mrow><mml:mn>17</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:math>20240 iqtibos
  4. XRISM Constraints on Unidentified X-Ray Emission Lines, Including the 3.5 keV Line, in the Stacked Spectrum of 10 Galaxy Clusters20250 iqtibos
  5. Vigorous turbulence driven by quasar-mode feedback in a cluster core20260 iqtibos
  6. Chemical enrichment of the Perseus cluster core seen by <i>XRISM</i> /Resolve20260 iqtibos
  7. Probable Detection of a Cooler Gas Component in the Perseus Cluster with XRISM20260 iqtibos
  8. Sloshing Motions in Abell 3571 Revealed by XRISM/Resolve Velocity Mapping20260 iqtibos
  9. Sloshing Motions in Abell 3571 Revealed by XRISM/Resolve Velocity Mapping20260 iqtibos