Estimated contamination levels for distinct stellar populations measured from the control fields.
|[N arcmin−2]||[N arcmin−2]||[N arcmin−2]|
|ACS/WFC||0.19 ± 0.06||0.06 ± 0.10||1.24 ± 0.41|
|WFC3/UVIS||0.48 ± 0.34||0.24 ± 0.15||0.83 ± 0.27|
|WFPC2||0.88 ± 0.61||0.16 ± 0.19||3.01 ± 2.23|
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