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Table 2

Log and results of Keck II/NIRC2 observations.

MJD Date Filter Nexp tint Co-adds PI
combination [s]

56 458.61442 2013-06-15 PK50_1.5+Brγ 15 1.0 5 Marcy
56 845.42700 2014-07-07 PK50_1.5+Kcont 6 12.5 25 Knutson
56 845.43081 PK50_1.5+Jcont 6 12.5 50
56 845.43408 PK50_1.5+Hcont 6 12.5 50
57 643.28633a 2016-09-11 PK50_1.5+Kcont 5 12.5 25 Baranec
57 677.24852 2016-10-15 PK50_1.5+Kcont 8b 30/60 30/60 Baranec
57 677.25537 K+clear 3c 1.81/18.1 10/100

MJD ρAB θAB ρAC θAC ΔmagAB ΔmagAC
[mas] [°] [mas] [°] [mag] [mag]

56 458.61442 1151.51(39) 203.279(16) 3279.7(3.8) 287.794(71) 1.087(5) 5.00(13)
56 845.42700 1146.17(11) 203.503(12) 3266.48(33) 288.002(13) 1.104(5) 5.139(47)
56845.43081 1146.24(9) 203.509(13) 3267.28(67) 287.987(15) 1.368(7) 5.266(55)
56 845.43408 1146.42(8) 203.515(11) 3267.47(69) 287.990(15) 1.133(7) 5.168(22)
57 643.28633a 1131.76(20) 203.053(36) 3226(12) 287.862(47) 1.099(7) 5.3(2)
57 677.24852 1134.30(22) 203.490(22) 3242.38(52) 288.284(20) 1.125(5) 5.180(30)
57 677.25537 1134.67(39) 203.468(22) 3243.17(87) 288.290(26) 1.052(2) 5.053(34)

Notes. We show the date, filters (combination of two wheels), total number of exposures (Nexp), integration time per exposure (tint), and number of co-adds per exposure. In the lower part of the table we show angular separations (ρ) and position angles (θ) of stars B and C relatively to A, and their magnitude differences.

(a)

Observations with bad AO correction. Results were not used in the further analysis.

(b)

The first two frames are composed of 30 co-adds (1 s each), while the following six are composed of 60 co-adds (also 1 s).

(c)

The first frame is composed of ten co-adds (0.181 s each), while the following two are composed of 100 co-adds (also 0.181 s).

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