Table 2
Details on individual light curves reported in this paper.
| Date UT (epoch) | Telescope | Filter | Γ | pnr | X | Sky conditions |
|
|
||||||
| 2011 Aug. 01 (181) | Volk.Kirch. 0.6 m | none | 0.87 | 3.68 | 1.05 → 1.03 → 1.05 | Clear |
| 2012 Dec. 13 (533) | Torun 0.6 m | none | 1.06 | 2.43 | 1.12 → 1.55 | Clear |
| 2013 Sep. 03 (719) | Torun 0.6 m | none | 1.51 | 2.51 | 1.02 → 1.14 | Clear |
| 2013 Sep. 30 (738) | Torun 0.6 m | none | 1.24 | 2.09 | 1.03 → 1.22 | Photometric |
| 2013 Nov. 26 (778) | Trebur 1.2 m | none | 1.39 | 1.18 | 1.07 → 1.14 | Photometric |
| 2013 Dec. 20 (795) | Jena 0.9 m | R B | 1.12 | 2.67 | 1.23 → 1.81 | Clear |
| 2014 Mar. 25 (862) | Trebur 1.2 m | none | 0.40 | 4.36 | 2.10 → 1.43 | Passing clouds |
| 2014 Apr. 02 (867) | Rozhen 2.0 m | R C | 1.22 | 1.47 | 1.60 → 1.22 | Photometric |
| Torun 0.6 m | none | 1.82 | 2.36 | 1.41 → 1.14 | Clear | |
| 2014 May 16 (898) | OSN 1.5 m | R C | 1.09 | 2.21 | 1.48 → 1.14 | Mostly clear, some high clouds |
| 2014 May 26 (905) | OSN 1.5 m | R C | 1.33 | 1.39 | 1.62 → 1.16 | Mostly photometric |
| 2014 Jun. 22 (924) | OSN 1.5 m | R C | 1.09 | 1.61 | 1.37 → 1.13 | Mostly photometric, occasionally |
| passing high clouds before ingress | ||||||
| 2014 Jul. 01 (931) | Trebur 1.2 m | R B | 0.88 | 2.64 | 1.17 → 1.03 | Photometric, first half of series |
| partly obscured by the dome slit | ||||||
| 2014 Sep. 10 (981) | OSN 1.5 m | R C | 1.33 | 1.29 | 1.14 → 1.13 → 1.37 | Photometric |
| 2014 Sep. 18 (986) | Jena 0.9 m | R B | 1.16 | 2.25 | 1.19 → 1.66 | Photometric |
| 2014 Sep. 27 (993) | Jena 0.9 m | R B | 1.14 | 2.02 | 1.12 → 1.54 | Photometric |
| Torun 0.6 m | R C | 0.95 | 3.74 | 1.14 → 1.53 | Clear, high humidity | |
| 2014 Oct. 27 (1014) | Torun 0.6 m | R C | 0.86 | 3.45 | 1.05 → 1.21 | High humidity, occasionally passing |
| high clouds | ||||||
Notes. Date UT is given for mid-transit time. Epoch is the transit number from the initial ephemeris given in Alsubai et al. (2011). RC and RB denote Cousins and Bessell R-band filters, respectively. Γ is the median number of exposures per minute. pnr is the photometric scatter in millimag per minute as defined by Fulton et al. (2011). X shows the airmass change during transit observations.
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