deletions | additions       diff --git a/section_Summary_incomplete_SMBH_grow__.tex b/section_Summary_incomplete_SMBH_grow__.tex  index 9150042..8cd66d2 100644  --- a/section_Summary_incomplete_SMBH_grow__.tex  +++ b/section_Summary_incomplete_SMBH_grow__.tex 
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We have observed that mergers increase AGN activity which translates to enhanced (increased) jet or radio activity, and we can now conclude that perhaps the most active AGN today may be the result of the merging of smaller galaxies.  one of the main challenges in the study is the physical limitations of the SDSS. It is harder to get data Observations  at smaller projected separations are hampered  as these small separations  are difficult to resolve using current SDSS technology. This in turn limits the ability to make solid inferences on the available data.