Cloudy & Associates

Commit 283e2f4f authored by Chatzikos, Marios's avatar Chatzikos, Marios
Browse files

Update Hazy 2, 3, and QSG front-page images

parent 69c3fa58
......@@ -20,7 +20,7 @@
\emph{Quick Start Guide to \Cloudy\ C\VERSION}\\
\begin{figure}
\begin{center}
\includegraphics[clip=on,width=\columnwidth,height=0.7\textheight,keepaspectratio]{Greek_Foot-race_Panathenaic_Vase.jpg}
\includegraphics[clip=on,width=\columnwidth,height=0.7\textheight,keepaspectratio]{cycling_race.jpg}
\end{center}
\label{fig:header}
\end{figure}
......@@ -44,8 +44,13 @@
\vspace{5mm}
\noindent
{\small
{\em Cover image:} A black-figured ancient Greek vase of the Panathenaic class, given at Athens as a prize to the winner of a foot-race at the Panathenaea, with the foot-race (stadion) represented on it. Encyclop{\ae}dia Britannica (11th ed.), v. 12, 1911, p. 478, Fig. 15, so
public domain.}
{\em Cover image:} Bavarian Road Cycling Championship 2017,
in Baiersdorf (Middle Franconia).
Photo by
\href{https://unsplash.com/@markusspiske?utm_source=unsplash&utm_medium=referral&utm_content=creditCopyText}
{Markus Spiske} on
\href{https://unsplash.com/license?utm_source=unsplash&utm_medium=referral&utm_content=creditCopyText}
{Unsplash}.
\clearpage
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
......
......@@ -17674,3 +17674,47 @@ archivePrefix = "arXiv",
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
 
@ARTICLE{Chakraborty2020b,
crossref = "2020ApJ...901...69C"
}
@ARTICLE{2020ApJ...901...69C,
author = {{Chakraborty}, P. and {Ferland}, G.~J. and {Chatzikos}, M. and {Guzm{\'a}n}, F. and {Su}, Y.},
title = "{X-Ray Spectroscopy in the Microcalorimeter Era. II. A New Diagnostic on Column Density from the Case A to B Transition in H- and He-like Iron}",
journal = {\apj},
keywords = {Galaxy clusters, Perseus Cluster, X-ray astronomy, High resolution spectroscopy, Radiative transfer, Intracluster medium, 584, 1214, 1810, 2096, 1335, 857, Astrophysics - High Energy Astrophysical Phenomena},
year = 2020,
month = sep,
volume = {901},
number = {1},
eid = {69},
pages = {69},
doi = {10.3847/1538-4357/abaaac},
archivePrefix = {arXiv},
eprint = {2007.16106},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...901...69C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Chakraborty2022,
crossref = "2022ApJ...935...70C"
}
@ARTICLE{2022ApJ...935...70C,
author = {{Chakraborty}, Priyanka and {Ferland}, Gary J. and {Chatzikos}, Marios and {Fabian}, Andrew C. and {Bianchi}, Stefano and {Guzm{\'a}n}, Francisco and {Su}, Yuanyuan},
title = "{X-Ray Spectroscopy in the Microcalorimeter Era 4: Optical Depth Effects on the Soft X-Rays Studied with CLOUDY}",
journal = {\apj},
keywords = {X-ray binary stars, Atomic spectroscopy, 1811, 2099, Astrophysics - High Energy Astrophysical Phenomena},
year = 2022,
month = aug,
volume = {935},
number = {2},
eid = {70},
pages = {70},
doi = {10.3847/1538-4357/ac7eb9},
archivePrefix = {arXiv},
eprint = {2207.02267},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2022ApJ...935...70C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
......@@ -40,7 +40,7 @@ and test suite
\begin{figure}
\begin{center}
\includegraphics[clip=on,width=0.8\columnwidth,keepaspectratio]{Akras15}
\includegraphics[clip=on,width=0.8\columnwidth,keepaspectratio]{soft_xray_abs.jpg}
\end{center}
\end{figure}
......@@ -61,9 +61,10 @@ and test suite
\vspace{5mm}
\noindent
{\small
{\em Cover image:} The observed and modelled SED of Vy 1-2 in the wavelength range from 0.43 to 140 ${\mu}$m.
The data are from GSC2.2, GSC2.3, USNOB1, USNOB2, 2MASS, AKARI and WISE surveys.
Figure 17 from \citet{2015MNRAS.452.2911A}.
{\em Cover image:}
Continuum opacities plotted as a function of wavelength for a cloud with
$N_H = 10^{23} \, \rm{cm}^{2}$.
Figure 1 from \citet{Chakraborty2022}.
}
\clearpage
......
......@@ -31,7 +31,7 @@ Hazy\\
\begin{figure}
\begin{center}
\includegraphics[clip=on,keepaspectratio]{WarmAbsorberReynoldsFabian}
\includegraphics[clip=on,keepaspectratio,scale=3.5]{he_like_atom.jpg}
\end{center}
\end{figure}
......@@ -51,10 +51,9 @@ Hazy\\
\input{../frontis_common}
\vspace{5mm}
\noindent
{\small {\em Cover image:} The predicted X-ray spectrum of a warm absorber in
an Active Galactic Nucleus. Prominent emission and absorption lines are
present along with broad UTA absorption features. The parameters are from
\citet{Reynolds1995}.
{\small {\em Cover image:}
He-like atomic structure for the $n=2, 3$ configurations.
Figure 1 from \citet{Chakraborty2020b}.
}
\clearpage
......
......@@ -7,7 +7,7 @@
% latex does not like this, so CamelCase is used instead
% current version of Cloudy
\def\VERSION{17}
\def\VERSION{22}
% in cddefines.h
\def\LIMELM{30} % number of elements
......
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