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Table 1

Overview of the LK–MRS plates observed in the period September 2017–June 2018 that have objects in common with the Kepler field.

Plan ID RA (2000) hh:mm:ss.ss Dec (2000) dd:mm:ss.ss Date yyyy-mm-dd Seeing (arcsec) Exposure (s) Number of targets
Total hot cool unclass
HIP9645901 19:36:37.98 +44:41:41.77 2017-09-28 2.9 600 × 4 1337 97 1023 217
HIP9286201 18:55:20.10 +43:56:45.93 2017-10-03 3.4 600 × 3 1320 19 745 556
HIP9737201 19:47:26.83 +47:54:27.24 2017-10-03 3.3 600 × 3 1329 78 782 469
HIP9380801 19:06:17.04 +41:24:49.61 2017-10-04 2.5 600 × 3 1287 55 965 267
HIP9587901 19:29:58.91 +46:56:47.36 2017-10-04 2.9 600 × 3 1288 73 944 271
HIP9448701 19:13:53.55 +48:20:57.43 2017-10-05 3.3 600 × 3 1219 36 793 390
HIP9511901 19:21:02.82 +42:41:13.07 2018-05-24 2.8 900 × 5 2968 126 1806 1036
HIP95119KP01 19:21:02.82 +42:41:13.07 2018-05-28 3.0 900 × 7 2961 122 1814 1025
HIP95119KP01 19:21:02.82 +42:41:13.07 2018-05-29 2.3 600 × 9 2980 119 1821 1040
HIP95119KP01 19:21:02.82 +42:41:13.07 2018-05-30 2.4 900 × 5 2971 124 1784 1063
HIP95119KP01 19:21:02.82 +42:41:13.07 2018-05-31 2.3 1200 × 4 2969 127 1787 1055
TOTAL 22629 976 14264 7389

Notes. For each plate, we give the identifier, the right ascension and declination of the central star, the seeing during the observations, the exposure times, and the number of targets. The identifiers of the plates observed during the regular LAMOST survey are written in italic.

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