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Table A.1:

RBC clusters serendipitously imaged in our survey.

Name
f1 Field Chip Comment
B014D 2 B015D PC cluster
B061D 2 NB16 WF cluster
B256D 2 B257D WF cluster2
B256D 2 B475 WF cluster2
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?
B057D 2 NB16 WF 2 stars
NB43 2 NB67 WF 2 stars
B192D 2 B327 WF galaxy
SK194C 2 B376 WF galaxy
B376 1 B374 WF cluster
B257D 1 B475 WF cluster
B319 1 B318 WF cluster
DAO84 1 B374 WF not a star3
DAO84 1 B376 WF not a star3
SK047A 1 B081 WF two stars
NB68 6 NB16 WF star?
NB68 6 NB67 WF star?
B113 6 NB16 WF star?
SK069D 6 B083 WF star
B185D 6 B318 PC star
SK046D 6 B327 WF star
B065D 6 NB67 WF star
SK041D 6 B321 WF two stars
B121 3 NB16 WF star?
B121 3 NB67 WF star

Notes. (1) f is the original RBC classification flag (1 globular cluster, 2 candidate globular cluster, 3 controversial object, 6 star/s). (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. (3) DAO84 has a radial velocity estimate that clearly identifies it as a member of M 31 (see the RBC).


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