deletions | additions       diff --git a/Observations.tex b/Observations.tex  index 6cef0f5..b01ff5c 100644  --- a/Observations.tex  +++ b/Observations.tex 
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detection of the transient source itself (as we will see below, it had  already faded back to its quiescent state by that time). However, it  did provide an unambiguous redshift for the host galaxy of  $z=1.0054\pm0.0002$ from \Ha\ and \ion{O}{2}. \ion{O}{[ii]}.  These line identifications are consistent with two measures of the photometric  redshift of the host: $z=1.00+-0.02$ from the BPZ algorithm  \citep{Benitez:2000}, and $z=0.92\pm0.05$, derived using the EAZY 
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