Asosiy kontentga oʻtish
AkademScholar
Muassasalar

Instituto Nacional de Investigaciones Nucleares

Nom variantlari: ININ

Davlat:
MX
ROR:
https://ror.org/00k7h5c65
7
h-indeks
196
Iqtiboslar
35
Asarlar
41
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
035810025507510020172018201920202021202220232024202520262017: Nashrlar 2, Iqtiboslar 22018: Nashrlar 0, Iqtiboslar 12019: Nashrlar 2, Iqtiboslar 22020: Nashrlar 0, Iqtiboslar 52021: Nashrlar 1, Iqtiboslar 02022: Nashrlar 1, Iqtiboslar 32023: Nashrlar 0, Iqtiboslar 62024: Nashrlar 4, Iqtiboslar 112025: Nashrlar 7, Iqtiboslar 1002026: Nashrlar 0, Iqtiboslar 18

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 22018: Iqtiboslar 12019: Iqtiboslar 22020: Iqtiboslar 52021: Iqtiboslar 02022: Iqtiboslar 32023: Iqtiboslar 62024: Iqtiboslar 112025: Iqtiboslar 1002026: Iqtiboslar 18

Nashr tarixi

03581020172018201920202021202220232024202520262017: Nashrlar 22018: Nashrlar 02019: Nashrlar 22020: Nashrlar 02021: Nashrlar 12022: Nashrlar 12023: Nashrlar 02024: Nashrlar 42025: Nashrlar 72026: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020172018201920202021202220232024202520262017: h-indeks 42018: h-indeks 42019: h-indeks 42020: h-indeks 42021: h-indeks 42022: h-indeks 42023: h-indeks 42024: h-indeks 42025: h-indeks 72026: h-indeks 7

Eng koʻp iqtibos qilingan asarlar

  1. The WEBT BL Lacertae Campaign 2000200228 iqtibos
  2. The WEBT BL Lacertae Campaign 2001 and its extension Optical light curves and colour analysis 1994-2002200416 iqtibos
  3. DESI 2024 II: sample definitions, characteristics, and two-point clustering statistics20259 iqtibos
  4. DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data20255 iqtibos
  5. A trio of gamma-ray burst supernovae:20142 iqtibos
  6. Estimation of 99Mo production rates from natural molybdenum in research reactors20162 iqtibos
  7. Application of the semimicroscopic algebraic cluster model to core<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mi>α</mml:mi></mml:mrow></mml:math>nuclei in the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>s</mml:mi><mml:mi>d</mml:mi></mml:mrow></mml:math>shells20121 iqtibos
  8. Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations measurements20251 iqtibos
  9. Screenings in modified gravity: a perturbative approach20191 iqtibos
  10. Microscopically derived potential energy surfaces from mostly structural considerations20161 iqtibos