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Table 1.

Observation log.

ID (a) Name Date_obs UT_mid texp S/N(b)
yyyy-mm-dd hh:mm (s)
39 BD+54 2812 2018-08-19 02:19 3600 106
56 HD 235888 2018-08-19 05:15 1183 125
56 HD 235888 2018-08-21 04:15 1410 147
214 TYC 3983-2832-1 2018-08-20 02:36 5700 90
266 BD+52 3260 2018-08-19 03:28 3600 111
378 TYC 3984-1809-1 2018-08-24 00:21 2820 153
435 TYC 3988-1537-1 2018-08-23 05:04 5700 81
466 HD 215178 2018-08-20 01:15 3600 419
490 TYC 3984-1751-1 2018-08-23 00:03 3600 70
492 TYC 3988-154-1 2018-08-23 23:19 3600 109
502 TYC 3988-282-1 2018-08-20 22:22 3600 75
517 TYC 3984-1588-1 2018-08-20 04:44 5700 80
554 TYC 3984-1107-1 2018-08-23 01:08 3600 132
565 TYC 3984-1717-1 2018-08-22 01:47 3600 121
708 TYC 3984-277-1 2018-08-19 04:31 3600 153
731 TYC 3988-1310-1 2018-08-22 02:41 1410 105
731 TYC 3988-1310-1 2018-08-23 01:52 1380 110
F1 J22452826+5347061 2019-08-11 00:50 4800 36
F2 J22311798+5502407 2019-08-11 02:23 4800 34

Notes.

(a)

Sequential number from Kharchenko et al. (2005) based on right ascension. F1 and F2 are two additional candidates not included in Kharchenko et al. (2005).

(b)

Signal-to-noise ratio per pixel at 6500 Å.

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