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Lowell Observatory

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8
h-indeks
318
Iqtiboslar
76
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40
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Iqtibos sharhi

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035810025507510020172018201920202021202220232024202520262017: Nashrlar 1, Iqtiboslar 02018: Nashrlar 1, Iqtiboslar 52019: Nashrlar 5, Iqtiboslar 112020: Nashrlar 4, Iqtiboslar 202021: Nashrlar 10, Iqtiboslar 52022: Nashrlar 10, Iqtiboslar 52023: Nashrlar 6, Iqtiboslar 222024: Nashrlar 4, Iqtiboslar 522025: Nashrlar 1, Iqtiboslar 632026: Nashrlar 2, Iqtiboslar 82

Iqtibos tarixi

025507510020172018201920202021202220232024202520262017: Iqtiboslar 02018: Iqtiboslar 52019: Iqtiboslar 112020: Iqtiboslar 202021: Iqtiboslar 52022: Iqtiboslar 52023: Iqtiboslar 222024: Iqtiboslar 522025: Iqtiboslar 632026: Iqtiboslar 82

Nashr tarixi

03581020172018201920202021202220232024202520262017: Nashrlar 12018: Nashrlar 12019: Nashrlar 52020: Nashrlar 42021: Nashrlar 102022: Nashrlar 102023: Nashrlar 62024: Nashrlar 42025: Nashrlar 12026: Nashrlar 2

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 72024: h-indeks 72025: h-indeks 72026: h-indeks 8

Eng koʻp iqtibos qilingan asarlar

  1. The awakening of BL Lacertae: observations by Fermi, Swift and the GASP-WEBT★201312 iqtibos
  2. Blazar spectral variability as explained by a twisted inhomogeneous jet201712 iqtibos
  3. Variability of the blazar 4C 38.41 (B3 1633+382) from GHz frequencies to GeV energies20129 iqtibos
  4. Multiwavelength behaviour of the blazar OJ 248 from radio to γ-rays★20157 iqtibos
  5. Dark Energy Survey: Galaxy sample for the baryonic acoustic oscillation measurement from the final dataset20243 iqtibos
  6. Asteroid pairs: A complex picture20192 iqtibos
  7. Investigating the multiwavelength behaviour of the flat spectrum radio quasar CTA 102 during 2013–201720192 iqtibos
  8. SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets20241 iqtibos
  9. Photometry of the Didymos System across the DART Impact Apparition20241 iqtibos
  10. Superhumps in Cataclysmic Binaries. XXV. q crit , \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\mathstrut{{\mbox{\boldmath $\varepsilon$}}} $ \end{document} ( q ), and Mass‐Radius20050 iqtibos