\begin{table} %ta.1 \caption{\label{tab:app}RBC clusters serendipitously imaged in our survey.} %\centering \small \begin{tabular} {@{}lcccc@{}} \hline \hline\noalign{\smallskip} Name & $f^1$ & Field & Chip & Comment \\ \hline B014D & 2 & B015D & PC & cluster \\ [1ex] B061D & 2 & NB16 & WF & cluster \\ B256D & 2 & B257D & WF & cluster\tablefootmark{2} \\ B256D & 2 & B475 & WF & cluster\tablefootmark{2} \\ SK067B & 2 & B015D & WF & not a star \\ SK071C & 2 & B475 & WF & not a star \\ SK185B & 2 & B475 & WF & not a star \\ B068D & 2 & NB16 & WF & not a star \\ B068D & 2 & NB67 & WF & not a star \\ B019D & 2 & V031 & WF & not a star \\ NB64 & 2 & NB16 & WF & star? \\ NB64 & 2 & NB67 & WF & star? \\ SK091B & 2 & B066 & WF & star \\ B048D & 2 & B081 & PC & star \\ SK091C & 2 & B374 & WF & star \\ SK188B & 2 & B475 & WF & star \\ NB47 & 2 & NB16 & WF & star \\ SK083B & 2 & B043 & WF & 2 stars + nebula? \\ [1ex] B057D & 2 & NB16 & WF & 2 stars \\ NB43 & 2 & NB67 & WF & 2 stars \\ B192D & 2 & B327 & WF & galaxy \\ SK194C & 2 & B376 & WF & galaxy \\ % VDB0 & 1 & B327 & WF & cluster \\ B376 & 1 & B374 & WF & cluster \\ B257D & 1 & B475 & WF & cluster \\ B319 & 1 & B318 & WF & cluster \\ % NB16 & 1 & NB67 & WF & cluster?/galaxy? \\ DAO84 & 1 & B374 & WF & not a star\tablefootmark{3} \\ DAO84 & 1 & B376 & WF & not a star\tablefootmark{3} \\ SK047A & 1 & B081 & WF & two stars \\ NB68 & 6 & NB16 & WF & star? \\ NB68 & 6 & NB67 & WF & star? \\ B113 & 6 & NB16 & WF & star? \\ [1ex] SK069D & 6 & B083 & WF & star \\ B185D & 6 & B318 & PC & star \\ SK046D & 6 & B327 & WF & star \\ % NB67 & 6 & NB16 & WF & star \\ B065D & 6 & NB67 & WF & star \\ SK041D & 6 & B321 & WF & two stars \\[1ex] B121 & 3 & NB16 & WF & star? \\[1ex] B121 & 3 & NB67 & WF & star \\ [1ex] \hline \end{tabular} \tablefoot{\tablefoottext{1}{$f$ is the original RBC classification flag (1 globular cluster, 2~candidate globular cluster, 3 controversial object, 6 star/s).} \tablefoottext{2}{While the visual inspection of the images does not permit a clear cut classification, the objective analysis performed in Pap-II recognizes B256D as a star cluster.} \tablefoottext{3}{DAO84 has a radial velocity estimate that clearly identifies it as a member of M~31 (see the RBC).}} \end{table}