deletions | additions       diff --git a/subsection_Source_detection_All_images__.tex b/subsection_Source_detection_All_images__.tex  index 24da6a4..de09acb 100644  --- a/subsection_Source_detection_All_images__.tex  +++ b/subsection_Source_detection_All_images__.tex 
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\end{tabular}  \end{table}  Because of the vast variety of cameras (WFC3, ACS, and  WFPC2), low NUV brightness, and mildWCS dierences which were  not correct-able with tweakreg due to low source counts, images were  not able to be combined into a white light source. Instead, separate  source catalogs were found for both the ACS f330w and WFPC2  f555w lters and cross-compared.  Introduce that HST data are what is used. Different filters for each galaxy, reference table.  Info on how point (or close to point) sources were found using the two different methods. Reference the table for which method used for each galaxy as well as the relevant thresholds used. 
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  TABLE: galaxy name, filters, method, thresholds, distand modulus, mass detection threshold.