Cloudy & Associates

Commit 7df8be33 authored by Chatzikos, Marios's avatar Chatzikos, Marios
Browse files

Merge branch 'update_hazy' into 'master'

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

See merge request !51
parents 69c3fa58 243f2f38
The Cloudy project subversion repository and its history
2020 Dec 2
This Git repository is a tip migration of a subversion repository which has our history going back about fifteen years. The subversion repository is maintained as a read-only reference at
https://viewvc.nublado.org or
https://trac.nublado.org/browser
The migration was done on 2020 Dec2 at r14364. Only the trunk and a few actively maintained branches were migrated.
For more information:
The project wiki: nublado.org
The Cloudy user group: https://cloudyastrophysics.groups.io/g/Main/topics
# Cloudy
Cloudy is an _ab initio_ spectral synthesis code designed to model a wide range
of interstellar "clouds", from H II regions and planetary nebulae, to Active
Galactic Nuclei, and the hot intracluster medium that permeates galaxy clusters.
Cloudy has been in continuous development since 1978, led by Gary Ferland, and
in close collaboration with a number of scientists -- see the
[list of contributors](others.txt).
# Version
The current version of Cloudy is C22, released in Fall 2022.
A summary of what is new is available
[here](https://gitlab.nublado.org/cloudy/cloudy/-/wikis/NewC22).
## Brief History
Cloudy recently migrated to a pure git version control system from a
subversion (SVN) system (with limited support for git).
Cloudy had been on a SVN repository for about 15 years, which is still
maintained as a read-only reference at
[https://viewvc.nublado.org](https://viewvc.nublado.org) or
[https://trac.nublado.org/browser](https://trac.nublado.org/browser).
The migration was done on 2020 Dec 2 at r14364.
Only the trunk and a few actively maintained branches were migrated.
Previous releases of Cloudy are still available on the SVN site,
as well as tarballs on our
[release folder](https://data.nublado.org/cloudy_releases).
# API
Cloudy's API is described with [Doxygen](https://doxygen.nl), and is available
[online](https://data.nublado.org/doxygen/c22.00).
# Contact us
See the project's [website](https://nublado.org) for new versions, bug fixes,
etc.
If you have any questions, please post them on the
[Cloudy user group](https://cloudyastrophysics.groups.io/g/Main/topics).
......@@ -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 +44,11 @@
\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}{Markus Spiske} on
\href{https://unsplash.com/license}{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}
}
......@@ -62,10 +62,12 @@ Hazy\\
\vspace{5mm}
\noindent
{\small
{\em Cover image:
{\em Cover image:}
The dawn of a new day, representing Cloudy's migration between
development platforms and new development plans. Photo by Federico Respini on Unsplash.
}
development platforms and new development plans.
Photo by
\href{https://unsplash.com/@federicorespini}{Federico Respini} on
\href{https://unsplash.com/license}{Unsplash}.
}
\clearpage
......
......@@ -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
$\rm{N_H} = 10^{23} \, \rm{cm}^{2}$.
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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