HIGHLIGHTS
SUMMARY
The authors thus considered as candidate new members all the stars in the northern CoRoT field that fall in this region of Fig 2 and that were not previously known as members (filled red circles). On the basis of the control field, however, 3.2% of the field stars are estimated to fall in the member-selection region of Fig 2. If the authors make the simplifying assumption that a negligible fraction of new members is present among the 2089 stars in the north field that are not known members, the authors estimate ~67 . . .
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