this is for holding javascript data
Refiloe edited subsection_Comparison_with_X_ray__.tex
over 8 years ago
Commit id: b6facaf2fe1250e0a269fa7eada66d8351565504
deletions | additions
diff --git a/subsection_Comparison_with_X_ray__.tex b/subsection_Comparison_with_X_ray__.tex
index 7bcc658..c4d5b61 100644
--- a/subsection_Comparison_with_X_ray__.tex
+++ b/subsection_Comparison_with_X_ray__.tex
...
\subsection{Comparison with X-ray-selected AGN pairs}
Both
our study (Liu et at 2011) \cite{Liu_2011} and
Koss et el \cite{Koss_2012} use imaging spectroscopy to select data points for dual (pair) AGN samples. A small pair separation is also present in both studies with most of the Lui AGN detections at separation less than 100
kick, kpc, and those of
Koss at \cite{Koss_2012} found at separations less than 30 kpc. Both papers note that the luminosities of AGN pairs increase with a decrease in separation between galaxies (in a pair), suggesting that mergers promote AGN
activity. (Liu et al 2011, Koss et al). activity (\cite{Liu_2011} , \cite{Koss_2012}). Both papers also acknowledge the limitations experienced in selecting the appropriate sample data due to SDSS’ fixed
fibre fiber size. On this point, Koss notes that due to SDSS
fibre fiber being 3”, it is sensitive to smaller physical scales.
##May include Ellison et al. (2015) later, but not a priority. Koss