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AkademScholar

Kashfiyot

Xizmatlar

Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

Institute of Plant Sciences of Paris Saclay

Nom variantlari: Institut des Sciences des Plantes de Paris Saclay · IPS2 · Paris Saclay Institute of Plant Sciences · UMR 9213 · UMR9213

Davlat:
FR
ROR:
https://ror.org/00ajjta07
4
h-indeks
66
Iqtiboslar
28
Asarlar
80
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0134503581020172018201920202021202220232024202520262017: Nashrlar 1, Iqtiboslar 12018: Nashrlar 4, Iqtiboslar 22019: Nashrlar 1, Iqtiboslar 32020: Nashrlar 0, Iqtiboslar 22021: Nashrlar 1, Iqtiboslar 12022: Nashrlar 0, Iqtiboslar 42023: Nashrlar 1, Iqtiboslar 22024: Nashrlar 0, Iqtiboslar 62025: Nashrlar 1, Iqtiboslar 92026: Nashrlar 0, Iqtiboslar 8

Iqtibos tarixi

03581020172018201920202021202220232024202520262017: Iqtiboslar 12018: Iqtiboslar 22019: Iqtiboslar 32020: Iqtiboslar 22021: Iqtiboslar 12022: Iqtiboslar 42023: Iqtiboslar 22024: Iqtiboslar 62025: Iqtiboslar 92026: Iqtiboslar 8

Nashr tarixi

0134520172018201920202021202220232024202520262017: Nashrlar 12018: Nashrlar 42019: Nashrlar 12020: Nashrlar 02021: Nashrlar 12022: Nashrlar 02023: Nashrlar 12024: Nashrlar 02025: Nashrlar 12026: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520172018201920202021202220232024202520262017: h-indeks 32018: h-indeks 32019: h-indeks 32020: h-indeks 32021: h-indeks 32022: h-indeks 32023: h-indeks 32024: h-indeks 42025: h-indeks 42026: h-indeks 4

Eng koʻp iqtibos qilingan asarlar

  1. Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory20195 iqtibos
  2. Interplay between Single-Particle and Collective Effects in the Odd-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>A</mml:mi></mml:math>Cu Isotopes beyond<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn>40</mml:mn></mml:math>20082 iqtibos
  3. Neutron-rich nuclei produced at zero degrees in damped collisions induced by a beam of 18O on a 238U target20181 iqtibos
  4. The response of BGO scintillation detectors to light charged nuclei19920 iqtibos
  5. The yrast superdeformed band in 194Pb. Differences with 192Hg19950 iqtibos
  6. K-Isomers in Very Neutron-Rich Nuclei Around Mass 18020000 iqtibos
  7. Discrete decay of the yrast superdeformed band in the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Tb</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>151</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>nucleus20080 iqtibos
  8. EXILL - Pu241 spectroscopy20130 iqtibos
  9. Measurement of <sup>19</sup>Ne spectroscopic properties via a new method of inelastic scattering to study novae20180 iqtibos
  10. Accessing tens-to-hundreds femtoseconds nuclear state lifetimes with low-energy binary heavy-ion reactions20210 iqtibos