deletions | additions       diff --git a/section_Summary_of_existing_and__.tex b/section_Summary_of_existing_and__.tex  index 135a0c6..2408f35 100644  --- a/section_Summary_of_existing_and__.tex  +++ b/section_Summary_of_existing_and__.tex 
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\item 0.8 cm / 36 GHz \citep{Yusef-Zadeh2013a}  \item 42-50 GHz MOPRA CMZ \url{http://newt.phys.unsw.edu.au/mopracmz/survey.html#CMZ_7mm_Table} \citep{Jones2013}  \item 90-115 GHz MOPRA CMZ \url{http://newt.phys.unsw.edu.au/mopracmz/} \citep{Jones2012a}  \item PMO has been running a large scale CO/\cob/\coc\ (1--0) mapping survey, the  Milky Way Imaging Scroll Painting (MWISP, \citealt{Jiang2013-MWISP})  which will eventually map the northern Galactic plane within $b<|5|^\circ$. The project started in 2010 and so far a large fraction of plane has been observed. Progress can be found at \url{http://www.radioast.nsdc.cn/viewallobsed.php}.  \item THRUMMS, 3 mm b = $\pm$ 1 (but stops at l=358)  \item CARMA-CMZ 3 mm survey  \item SEDIGISM, 1 mm b = $\pm$ 1