From 37226baf50b7452c1f31c1766eb27b62271297b8 Mon Sep 17 00:00:00 2001
From: caes <caes>
Date: Mon, 24 Apr 2017 03:48:58 -0400
Subject: [PATCH] update

---
 adv_lab.bib                | 42 ++++++++++++++++++++++++++++++++++++++
 feedback/report/report.tex |  4 ++--
 2 files changed, 44 insertions(+), 2 deletions(-)

diff --git a/adv_lab.bib b/adv_lab.bib
index 3f826dd..7bb499b 100644
--- a/adv_lab.bib
+++ b/adv_lab.bib
@@ -1,3 +1,45 @@
+
+@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,
    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}",
diff --git a/feedback/report/report.tex b/feedback/report/report.tex
index 42bdb41..37e8459 100644
--- a/feedback/report/report.tex
+++ b/feedback/report/report.tex
@@ -47,14 +47,14 @@
     \label{sec:cosmology}
 
     \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}
 \label{sec:feedbacksims}
 
-    
+    It is strongly believed by cosmologists that 
 
 %─────────────
 \section{Conclusion}