deletions | additions       diff --git a/UNid.tex b/UNid.tex  index 9187412..77584d0 100644  --- a/UNid.tex  +++ b/UNid.tex 
...
Optical and spectrosopic identification of LAT sources from   Acero et al astro-ph 1310.6735.  \subsection{Unid0143-5844}  Do we have NTT or GMOS data?  Acero et al:\\  three x-ray sources in LAT error ellipse, A2 and A3 are faint soft sources  and A1 is the brightest, some variability (?), however the hardness rasio   does not change, an possibly an AGN.   All three sources were UV detected, A1 did not show variability in UV.\\  A1, A2, A3 were detected in radio, however A1 is the strongest radio source  (Roopesh, are the A2 A3 radio detections real?). Petrov et al (2013) detected this  (these?) in radio as well.\\  A1 is a blazar candidate as it has flat radio sepctrum SED like a blazar SED  and based on Massaro et al (2013) WISE data this is a BL Lac candidate.  \subsection{Unid0523-2530}  Acreo et al found only a dim X-ray source on the 2FGL field and non-detection in UV.  In radsio the X-ray counter part was detected only in the lowest radio frequency.  $\gamma$, X-ray, radio data might suggest a pulsar origin.  EF $i > $21.8mag (9-11-2013)\\  Next:\\ 
...
14-01-2014 i 6x60sec ALxa140100 clouds\\  \subsection{UNid0746-0222}\\  2013-01-21T01:55 R 60 ALwa200129\\  2014-01-14 R,i attempt, ALxa140170 thick clouds\\  \subsection{UNid0803-0339}  Next: \\ 
...
\textbf{Spectroscopy:}\\  2013-11-08T05:18 gr4 1000 ALwk070169\\  \subsection{UNid0746-0222}\\  2013-01-21T01:55 R 60 ALwa200129\\  2014-01-14 R,i attempt, ALxa140170 thick clouds\\  \subsection{UNid0838-2828}\\  2013-01-21T02:00 R 60 ALwa200130\\