diff --git a/adv_lab.bib b/adv_lab.bib
index f047cad..c409675 100644
--- a/adv_lab.bib
+++ b/adv_lab.bib
@@ -1,3 +1,23 @@
+
+@ARTICLE{2005Natur.435..629S,
+   author = {{Springel}, V. and {White}, S.~D.~M. and {Jenkins}, A. and {Frenk}, C.~S. and 
+  {Yoshida}, N. and {Gao}, L. and {Navarro}, J. and {Thacker}, R. and 
+  {Croton}, D. and {Helly}, J. and {Peacock}, J.~A. and {Cole}, S. and 
+  {Thomas}, P. and {Couchman}, H. and {Evrard}, A. and {Colberg}, J. and 
+  {Pearce}, F.},
+    title = "{Simulations of the formation, evolution and clustering of galaxies and quasars}",
+  journal = {\nat},
+   eprint = {astro-ph/0504097},
+     year = 2005,
+    month = jun,
+   volume = 435,
+    pages = {629-636},
+      doi = {10.1038/nature03597},
+   adsurl = {http://adsabs.harvard.edu/abs/2005Natur.435..629S},
+  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+
 @Article{C3CS60279F,
 author ="Price, Sarah L.",
 title  ="Predicting crystal structures of organic compounds",
diff --git a/feedback/0504097.pdf b/feedback/0504097.pdf
new file mode 100644
index 0000000..52e7565
Binary files /dev/null and b/feedback/0504097.pdf differ
diff --git a/feedback/report/report.tex b/feedback/report/report.tex
new file mode 100644
index 0000000..01cfac1
--- /dev/null
+++ b/feedback/report/report.tex
@@ -0,0 +1,60 @@
+
+
+
+\documentclass[11pt,letterpaper]{article}
+
+%\usepackage{aas_macros}
+\usepackage{biblatex}
+\usepackage{graphicx}
+\usepackage[margin=1.in,centering]{geometry}
+\usepackage{hyperref}
+\usepackage{caption}
+\usepackage[export]{adjustbox}
+\usepackage{float}
+\usepackage{gensymb}
+
+\bibliography{/home/caes/wmu/phy-4660/adv_lab.bib}
+
+\begin{document}
+
+
+%\newcommand{}$^7\textrm{Li(p,}\alpha)^4\textrm{He}$ reaction.\\
+
+\newcommand{\LCDM}{$\Lambda$CDM}
+
+
+
+
+
+\title{Active Galactic Nuclei in Cosmology}
+\author{Otho Ulrich}
+\maketitle
+
+\begin{abstract}
+    Active Galactic Nuclei (AGN) play a role in cosmology as both component and probe.
+    They are used to contrain cosmological parameters, to characterize the intergalactic medium, and as a .
+    AGN interact with their host galaxies, influencing its evolution through a process called AGN feedback.
+    Modeling AGN feedback presents significant challenges, but has improved upon the \LCDM model as tested by the Millenium Simulation. \cite{2005Natur.435..629S}
+\end{abstract}
+
+
+%─────────────
+\section{Introduction}
+    \label{sec:intro}
+
+%─────────────
+\section{Cosmology}
+    \label{sec:cosmology}
+
+    \subsection{Millenium Simulation}
+    The Millenium Simulation tests the \LCDM cosmology 
+
+
+%─────────────
+\section{Conclusion}
+    \label{sec:conclusion}
+
+
+\printbibliography
+
+\end{document}