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Table 2

Optical observations of Bol 126 with small telescopes.

Observatorya Date MJD Δtb Mag. GCc Mag. novad
[UT] [d] [d] [mag] [mag]
Ondřejov 2010-10-06T22:22:05 55 475.93 –4.58 16.72 ± 0.02 –
Super-LOTIS 2010-10-07T03:02:50 55 476.13 –4.38 16.67 ± 0.48 –
Ondřejov 2010-10-08T19:37:55  55 477.82 –2.69 16.69 ± 0.02 –
Super-LOTIS 2010-10-09T03:00:43 55 478.13 –2.38 16.53 ± 0.16 –
Miyaki-Argenteus 2010-10-09T14:19:17 55 478.60 –1.91 16.62 ± 0.16 –
Miyaki-Argenteus 2010-10-10T15:01:01 55 479.63 –0.88 16.69 ± 0.17 –
Ondřejov 2010-10-10T19:20:38 55 479.81 –0.70 16.70 ± 0.02 –
Super-LOTIS 2010-10-11T02:12:57 55 480.09 –0.42 16.65 ± 0.13 –
Xingming 2010-10-11T13:21:30 55 480.56 0.05 16.31 ± 0.22 17.60 ± 0.96
Super-LOTIS 2010-10-12T11:15:42 55 481.47 0.96 15.62 ± 0.14 16.12 ± 0.28
Xingming 2010-10-12T15:02:56 55 481.63 1.12 15.67 ± 0.26 16.21 ± 0.48
Ondřejov 2010-10-12T19:30:43 55 481.81 1.30 15.90 ± 0.02 16.61 ± 0.13
Xingming 2010-10-13T13:24:07 55 482.56 2.05 16.18 ± 0.23 17.23 ± 0.77
Ondřejov 2010-10-13T20:39:50 55 482.86 2.35 16.19 ± 0.02 17.26 ± 0.22
Xingming 2010-10-14T14:01:17 55 483.58 3.07 16.19 ± 0.29 17.25 ± 0.94
Miyaki-Argenteus 2010-10-15T13:35:27 55 484.57 4.06 16.30 ± 0.19 17.57 ± 0.83
Itagaki 2010-10-16T09:22:11 55 485.39 4.88 16.42 ± 0.29 18.04 ± 1.62
Xingming 2010-10-16T13:35:54 55 485.57 5.06 16.42 ± 0.21 18.03 ± 1.26
Miyaki-Argenteus 2010-10-16T14:59:20 55 485.62 5.11 16.48 ± 0.15 18.32 ± 1.25
Miyaki-Argenteus 2010-10-17T12:57:21 55 486.54 6.03 16.57 ± 0.14 18.94 ± 2.04
Xingming 2010-10-17T15:32:06 55 486.65 6.14 16.45 ± 0.25 18.19 ± 1.65
Itagaki 2010-10-17T15:43:06 55 486.65 6.14 16.49 ± 0.21 18.37 ± 1.66
Miyaki-Argenteus 2010-10-18T12:05:45 55 487.50 6.99 16.70 ± 0.18 –
Ondřejov 2010-10-19T00:14:24 55 488.01 7.50 16.54 ± 0.02 18.70 ± 0.78
Itagaki 2010-10-22T08:47:15 55 491.37 10.86 16.58 ± 0.29 –
Super-LOTIS 2010-10-25T05:14:32 55 494.22 13.71 16.47 ± 0.14 –
Miyaki-Argenteus 2010-10-26T13:11:55  55 495.55  15.04 16.48 ± 0.15 –
Super-LOTIS 2010-10-27T03:45:12 55 496.16 15.65 16.67 ± 0.14 –
Miyaki-Argenteus 2010-10-27T15:24:36 55 496.64 16.13 16.61 ± 0.17 –
Super-LOTIS 2010-10-28T02:39:48 55 497.11 16.60 16.70 ± 0.14 –
Ondřejov 2010-10-28T16:52:19 55 497.70 17.19 16.68 ± 0.02 –
Super-LOTIS 2010-10-29T01:55 :36 55 498.08 17.57 16.64 ± 0.13 –
Miyaki-Argenteus 2010-10-29T11:28:38 55 498.48 17.97 16.93 ± 0.19 –
Ondřejov 2010-10-29T17:03:50 55 498.71 18.20 16.70 ± 0.02 –
Super-LOTIS 2010-10-30T02:04:25 55 499.09 18.58 16.67 ± 0.12 –
Super-LOTIS 2010-11-01T05:35:20 55 501.23 20.72 16.65 ± 0.14 –
Miyaki-Argenteus 2010-11-01T12:35:39 55 501.52 21.01 16.79 ± 0.16 –
Super-LOTIS 2010-11-02T02:35:30 55 502.11 21.60 16.62 ± 0.13 –
Miyaki-Argenteus 2010-11-02T13:43:47 55 502.57 22.06 16.53 ± 0.14 –
Super-LOTIS 2010-11-03T02:34:53 55 503.11 22.60 16.55    ± 0.13 –
Miyaki-Argenteus 2010-11-03T12:01:05 55 503.50 22.99 16.50 ± 0.15 –
Super-LOTIS 2010-11-04T01:51:30 55 504.08 23.57 16.57 ± 0.12 –
Miyaki-Argenteus 2010-11-04T12:59:54 55 504.54 24.03 16.68 ± 0.13 –
Super-LOTIS 2010-11-05T01:50:35 55 505.08 24.57 16.63 ± 0.13 –
Miyaki-Argenteus 2010-11-05T11:26:58 55 505.48 24.97 16.68 ± 0.14 –
Super-LOTIS 2010-11-09T02:31:25 55 509.11 28.60 16.64 ± 0.13 –

Notes. 

(a)

See Sect. 2.2 for a description of the telescopes used.

(b)

Time in days after the optical nova outburst on MJD = 55 480.32.

(c)

R band magnitude of Bol 126, see also Fig. 2.

(d)

R band magnitude of M31N 2010-10f assuming a quiescence magnitude for Bol 126 of R = 16.7 mag, see also Fig. 5.

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