Overview of the identified Ru147 cluster members in K2. The histogram in panel a shows the fraction of stars in each membership catalog that was observed during K2 as compared with the total number of identified stars. Panel b: Gaia vector point diagram for our compiled member list. We note that certain observed stars (encircled: EPIC 219665632, 219515762, 219560884, 219437560, and 219855372) are apparent outliers. However, with the exception of EPIC 219515762 (encircled twice), none are in our final sample, and 219515762 itself is discarded from the interpretation of the results since it is clearly past the cluster turnoff. Panel c: map of the sky centered on Ru147, with all member stars from our merged sample, assimilated from Cu13, CG18, GC18, and Ol19 (gray). Red symbols indicate those stars which have counterparts in EPIC while the green ones are those that were actually observed. The shaded regions indicate the approximate layout of the CCDs in the Kepler/K2 field of view. Panel d: distance-corrected (but not reddening-corrected) CMD of Ru147 cluster members with the color coding as in panel b.