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0000-0002-0891-1007
8
h-indeks
4
i10-indeksi
117
Iqtiboslar
17
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

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010613192520162017201820192020202220232024202520262016: Nashrlar 0, Iqtiboslar 102017: Nashrlar 0, Iqtiboslar 22018: Nashrlar 0, Iqtiboslar 32019: Nashrlar 0, Iqtiboslar 62020: Nashrlar 0, Iqtiboslar 222022: Nashrlar 0, Iqtiboslar 12023: Nashrlar 0, Iqtiboslar 122024: Nashrlar 0, Iqtiboslar 72025: Nashrlar 0, Iqtiboslar 22026: Nashrlar 0, Iqtiboslar 4

Iqtibos tarixi

0613192520162017201820192020202220232024202520262016: Iqtiboslar 102017: Iqtiboslar 22018: Iqtiboslar 32019: Iqtiboslar 62020: Iqtiboslar 222022: Iqtiboslar 12023: Iqtiboslar 122024: Iqtiboslar 72025: Iqtiboslar 22026: Iqtiboslar 4

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Yillar boʻyicha jamlangan h-indeks

03581020162017201820192020202220232024202520262016: h-indeks 42017: h-indeks 42018: h-indeks 42019: h-indeks 52020: h-indeks 72022: h-indeks 72023: h-indeks 72024: h-indeks 82025: h-indeks 82026: h-indeks 8

Eng koʻp iqtibos qilingan asarlar

  1. The WEBT BL Lacertae Campaign 2001 and its extension Optical light curves and colour analysis 1994-2002200416 iqtibos
  2. The awakening of BL Lacertae: observations by Fermi, Swift and the GASP-WEBT★201312 iqtibos
  3. The correlated optical and radio variability of BL Lacertae20099 iqtibos
  4. Variability of the blazar 4C 38.41 (B3 1633+382) from GHz frequencies to GeV energies20129 iqtibos
  5. Results of WEBT, VLBA and RXTE monitoring of 3C 279 during 2006–200720088 iqtibos
  6. WEBT and XMM-Newton observations of 3C 454.3 during the post-outburst phase. Detection of the little and big blue bumps20074 iqtibos
  7. Multi-frequency monitoring of γ-ray loud blazars20063 iqtibos
  8. beta-DELAYED gamma-RAY SPECTROSCOPY OF HEAVY NEUTRON RICH NUCLEI "SOUTH" OF LEAD20090 iqtibos
  9. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi>z</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>−</mml:mo><mml:mn>1</mml:mn><mml:mo>→</mml:mo><mml:mn>0</mml:mn></mml:mrow></mml:math><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>β</mml:mi></mml:math>decays of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">Ni</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>54</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">Fe</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>50</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">Cr</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>46</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>, and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">Ti</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>42</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>and comparison with mirror<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mo>(</mml:mo><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:math>measurements20150 iqtibos
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