Open Access

Table 1

Number of targets associated with the KEYSTONE study.

Cam. # targets # detections Success rate (%) Proposal(a) PI(b) Notes
1 24 4 17 1038 Chaplin High noise
2 33 5 15 2023 Chaplin High noise
3 33 24 73 3023 Chaplin South Galactic cap
4 31 2(c) 6 4074 Basu Hyades/Pleiades
5 51 6(d) 12 5074 Basu M44/M67
6 35 22 63 6039 Davies North Galactic cap
7 17 8 47 7039 Davies Near galactic centre
8 10 5 50 8002 Campante
9 0 0 Galactic centre
10 35 13 37 10 002 Campante North Galactic cap
11 28 18 64 11 012 Lund Galactic centre
12 37 24 65 12 012 Lund South Galactic cap
13 38 12 32 13 012 Lund Hyades
14 46 27 59 14010 Lund North Galactic cap
15 45 24 53 15 010 Lund
16 31 7 23 16010 Lund M44/M67
17 15 11 73 17036 Lund
18 21 10 48 18 036 Lund M44/M67
19 16 10 62 19036 Lund

546 (492) 232 (210(e)) 42 (43)

Notes. Overview of the number of targets associated with the KEYSTONE study that were observed in SC (not counting if only LC observations were obtained) in the different campaigns, together with the number of detections made. The bottom row provides sums of the columns, with values for the number of unique targets in parenthesis. (a)Proposal ID within the K2 guest observer (GO) program. (b)Principal investigator. (c)Hyades analysis by Lund et al. (2016a). (d)M67 analysis by Stello et al. (2016). (e)Three of these detections were only possible from combining several campaigns.

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