The observational sequence is simple and is aimed at obtaining light curves of the target listed below. These observations are time-critical, so we provide the starting and ending times for each target. All the observations have to be carried-out in the R-filter (or V if R shows fringing). In the attached finding charts, it is shown a proposed window that would help reducing the overhead time per exposure. In the name of each finding chart we added the proposed window size (in pixels) for each target. It is noteworthy that the targets with (CV) after the V-magnitude in the table below can show strong outburst that could increase the brightness in several magnitudes. These burst are not predictable, so in the case any of these two targets appear much brigher than the mentiones V-magnitude, the exposure time shuld be decreased accordingly. Thank you very much! #----- Night of 2016-01-25 ----- # Target Start End #=============================== OYCar -> 00:35 - 01:45 UT 0:40.8 UT - zaciatok SDSSJ0303+0054 -> 01:55 - 03:00 UT RRCae -> 03:10 - 05:25 UT SDSSJ1329+1230 -> 05:35 - 06:25 UT WD1333+005 -> 06:35 - 07:05 UT QSVir -> 07:15 - 09:30 UT 9:10.2 UT - koniec Target information: Name RA(J2000) DEC(J2000) Mag CV? ToT RA(FoV) DEC (FoV) Size(FoV) ========================================================================================================== OY Car - 10:06:22.07 -70:14:04.6 V~15.5 (CV) Exp= 10s 10:06:03.00000 -70:14:09.0000 900x 500 pix 6.0 x 3.3 arcmin R SDSS J0303+0054 - 03:03:08.36 +00:54:43.8 V=17.7 Exp= 20s 03:03:10.80000 +00:55:00.0000 500x1000 pix 3.3 x 6.7 M RR Cae - 04:21:05.56 -48:39:07.0 V=14.5 Exp= 5s 04:20:50.03000 -48:39:05.0000 1000x1000 pix 6.7 x 6.7 M SDSSJ1329+1230 13:29:25.21 +12:30:25.4 V=17.2 Exp= 16s 13:29:28.50000 +12:31:40.7000 300x 900 pix 2.0 x 6.0 R (vychadza) WD1333+005 13:36:16.05 +00:17:31.9 V=17.2 Exp= 16s 13:36:16.07000 +00:17:31.5000 900x 900 pix 6.0 x 6.0 R QSVir 13:49:51.95 -13:13:37.5 V=15.4 Exp= 8s 13:49:54.00000 -13:14:10.0000 1000x1200 pix 6.7 x 8.0 R (aj M)