Asosiy kontentga oʻtish
AkademScholar
Mualliflar

J. Agramunt

Soʻnggi maʼlum muassasa:
University of Valencia
ORCID:
0000-0002-0891-1007
8
h-indeks
4
i10-indeksi
117
Iqtiboslar
17
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
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

h-indeks evolyutsiyasi

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

Hammualliflar

  1. B. Rubio2 ta umumiy asar2009–2015
  2. N. Kurz2 ta umumiy asar2009–2015
  3. W. Prokopowicz2 ta umumiy asar2009–2015
  4. S. J. Steer2 ta umumiy asar2009–2015
  5. S. Piétri2 ta umumiy asar2009–2015
  6. R. Hoischen2 ta umumiy asar2009–2015
  7. J. Gerl2 ta umumiy asar2009–2015
  8. H. J. Wollersheim2 ta umumiy asar2009–2015
  9. P. Doornenbal2 ta umumiy asar2009–2015
  10. J. Grȩbosz2 ta umumiy asar2009–2015

Yana 6 ta asar katta kollaboratsiyada (50 dan ortiq muallif) — hammualliflar roʻyxatiga kiritilmagan

Skelet yozuvlar: 7 — katta kollaboratsiyada (50 dan ortiq muallif), hammualliflar roʻyxatiga kiritilmagan

Barcha hammualliflar →