deletions | additions       diff --git a/Integration time [1].tex b/Integration time [1].tex  index fe83d38..8ac83a7 100644  --- a/Integration time [1].tex  +++ b/Integration time [1].tex 
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\section{Integration time}   An important observational parameter is the total integration time. Chaning this will change how much mass can be seen, and We analyzed  how accurately the velocity of the outflow can been seen.  The determine the effect of changes to  the total  integration time of affected  the usefullness of observations, observations. We used  observations R23-R26, all of which used the full ALMA array  with varying 10s pointings, but varied the total  integration times were taken. between 300s and 7200s.  \subsection{Mass}  We found that longer observations obtained accurate results for mass with |V| > 1km/s. Shorter observations remained useful until they became dominated by noise.