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that case the discrepancy was not improved.
\section{Summary}
The formation energy, $\Delta E$, magnetic, $S_{magn}$, and configuration, $S_{conf}$, entropy contributions
were calculated and analyzed in the full range of the FeV-$\sigma$-phase
existence using the electronic band structure calculations by means of th... | the occupancies of the sites B, C
and D showed a higher sensitivity to $T$ and $x$. The KKR calculations combined
with the analysis of the entropy contributions clearly showed that
Fe atoms preferably occupy A and D sites in the FeV-$\sigma$ phase. This agrees well
with the neutron diffraction measurements, and it con... |
\section{Introduction}
\label{sec:introduction}
Turbulence in galaxy clusters can arise from many sources, ranging from mergers and cosmological structure formation \citep{lau09,vazza09,vazza11,zuhone10}, to galactic wakes \citep{kim07,ruszkowski11}, and AGN feedback (\citet{mcnamara07}, and references therein). It is... | and Fisher matrix techniques are also further
enlarged.
The presence of the continuum and line blending limit the
domain of the WD regime, which is no longer strictly independent of
$s/(\sigma_{1}+\sigma_{2})$. For instance, if we assume $v_{\rm rel} =
50 \, {\rm km \, s^{-1}}$ (corresponding to
$s/(\sigma_{1}+\sigm... |
\section{Case Study of Narrative Transitions}
In this section, we take clips from one data video as a case to illustrate the effect of transitions in connecting narratives and visualizations.
We highlight characteristic clips of these videos and mark transitions in \textbf{bold} texts.
This video is about global wea... | .~\cite{Hullman2013} investigated the arrangements of narrative sequences based on transitions.
Furthermore, Kim et al.~\cite{Kim2017} developed GraphScape, a synthetic model to evaluate the transition cost of visualization sequences.
Researchers also use transitions to make stories cohesive in timelines~\cite{Brehmer2... |
"\\section{Introduction}\n\nThe limiting behaviour of empirical measures is of paramount importance (...TRUNCATED) | "_1}{\\epsilon} = \\lim_{n \\rightarrow \\infty} \\frac{EX_n^{\\epsilon, p_k, \\nu}}n - \\frac{||q-p(...TRUNCATED) |
" rotating convection systems are used to make predictions about their convective behaviors in Secti(...TRUNCATED) | "R}=100(2E)^{-12/7}$ \\citep[][]{GastineEA16}, then the $E=3.0 \\times 10^{-4}$ model would best cha(...TRUNCATED) |
"\\section{Introduction}\n\nThe $n$-dimensional hypercube $Q_{n}$ has vertex-set the power set\n${\\(...TRUNCATED) | " initial segment of the colexicographic\norder of size $\\left|{\\cal A}\\right|$, and set $C=X^{(\(...TRUNCATED) |
"\\section{Appendix} \\label{sec:appendix}\n\nWe calculate all of the actions of $\\mathbb{A}^{0|1}\(...TRUNCATED) | "To prove this it suffices to check it on representables for which it is clear.\n\n\n\\begin{cor} \\(...TRUNCATED) |
"# \\mathcal{M}_2 ) \\cdot ( \\# \\mathcal{M}_3)\n\\]\nof the numbers of elements of $\\mathcal{M}_m(...TRUNCATED) | "eqnarray*}\n16c^{-1}_{4}k(g-1)(h-1) \\leq ||M|| \\leq 16c_{4}k(g-1)(h-1). \n\\end{eqnarray*}\nOn t(...TRUNCATED) |
"\n\\part{\\xspace}}\n\\def\\ensuremath{D^{*+}}\\xspace {\\ensuremath{D^{*+}}\\xspace}\n\\def\\ensu(...TRUNCATED) | "1.38$, and $\\chi^2/92=1.07$, respectively.} \n \\end{centering}\n\\end{figure*}\n\\end{comment}\n(...TRUNCATED) |
"\\section{Introduction}\n\nThe discipline of star formation, in all of its aspects, has always been(...TRUNCATED) | " on, $\\rho$ Ophiuchi) since we intend to explore in detail its relation with the bulk of USCO. We (...TRUNCATED) |
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