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@ARTICLE{2017ApJ...837..149G,
author = {{Gaspari}, M. and {S{\c a}dowski}, A.},
title = "{Unifying the Micro and Macro Properties of AGN Feeding and Feedback}",
journal = {\apj},
archivePrefix = "arXiv",
eprint = {1701.07030},
primaryClass = "astro-ph.HE",
keywords = {black hole physics, galaxies: active, galaxies: clusters: intracluster medium, galaxies: groups: general, hydrodynamics, methods: numerical},
year = 2017,
month = mar,
volume = 837,
eid = {149},
pages = {149},
doi = {10.3847/1538-4357/aa61a3},
adsurl = {http://adsabs.harvard.edu/abs/2017ApJ...837..149G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2010A&A...523A..32K,
author = {{Kroupa}, P. and {Famaey}, B. and {de Boer}, K.~S. and {Dabringhausen}, J. and
{Pawlowski}, M.~S. and {Boily}, C.~M. and {Jerjen}, H. and {Forbes}, D. and
{Hensler}, G. and {Metz}, M.},
title = "{Local-Group tests of dark-matter concordance cosmology . Towards a new paradigm for structure formation}",
journal = {\aap},
archivePrefix = "arXiv",
eprint = {1006.1647},
keywords = {galaxies: dwarf, galaxies: evolution, gravitation, Local Group, dark matter, cosmology: theory},
year = 2010,
month = nov,
volume = 523,
eid = {A32},
pages = {A32},
doi = {10.1051/0004-6361/201014892},
adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...523A..32K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{2006astro.ph..8019L, @ARTICLE{2006astro.ph..8019L,
author = {{Lemson}, G. and {Virgo Consortium}, t.}, author = {{Lemson}, G. and {Virgo Consortium}, t.},
title = "{Halo and Galaxy Formation Histories from the Millennium Simulation: Public release of a VO-oriented and SQL-queryable database for studying the evolution of galaxies in the LambdaCDM cosmogony}", title = "{Halo and Galaxy Formation Histories from the Millennium Simulation: Public release of a VO-oriented and SQL-queryable database for studying the evolution of galaxies in the LambdaCDM cosmogony}",

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\label{sec:cosmology} \label{sec:cosmology}
\subsection{Millenium Simulation} \subsection{Millenium Simulation}
The Millenium Simulation tests the \LCDM cosmology The Millenium Run and its following iterations are N-body simulations that predict the evolution of the matter in the universe. It is considered a (successful) test of the \LCDM cosmology.
%───────────── %─────────────
\section{Quasar Feedback Simulations} \section{Quasar Feedback Simulations}
\label{sec:feedbacksims} \label{sec:feedbacksims}
It is strongly believed by cosmologists that
%───────────── %─────────────
\section{Conclusion} \section{Conclusion}