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Table 2
Times of mid-eclipse for V1094 Tau.
| HJD-2 400 000 | Type | Source | |
|
|
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| 49 653.632 | ±0.003 | S | Kaiser et al. (1995) |
| 49 656.762 | ±0.003 | P | Kaiser & Frey (1998) |
| 49 680.597 | ±0.003 | S | Kaiser et al. (1995) |
| 49 683.727 | ±0.003 | P | Kaiser & Frey (1998) |
| 49 701.7061 | ±0.0014 | P | Kaiser & Frey (1998) |
| 49 707.5649 | ±0.0019 | S | Kaiser et al. (1995) |
| 49 710.6950 | ±0.0021 | P | Kaiser & Frey (1998) |
| 49 755.6355 | ±0.0021 | P | Kaiser & Frey (1998) |
| 50 456.7393 | ±0.0021 | P | Kaiser & Frey (1998) |
| 50 474.7156 | ±0.0021 | P | Kaiser & Frey (1998) |
| 52 278.2875 | ±0.0011 | S | Wolf et al. (2010) |
| 52 362.3148 | ±0.0011 | P | Wolf et al. (2010) |
| 52 601.87780 | ±0.00140 | S | V, URSA |
| 52 628.84325 | ±0.00062 | S | V, URSA |
| 52 637.83158 | ±0.00065 | S | V, URSA |
| 52 898.4989 | ±0.0011 | S | Wolf et al. (2010) |
| 52 997.3708 | ±0.0028 | S | Hubscher (2005) |
| 53 045.4406 | ±0.0035 | P | Hubscher et al. (2005) |
| 54 438.66519 | ±0.00079 | P | V, URSA |
| 54 447.65487 | ±0.00098 | P | V, NFO |
| 54 447.65613 | ±0.00062 | P | u, SAT |
| 54 447.65604 | ±0.00073 | P | v, SAT |
| 54 447.65602 | ±0.00093 | P | b, SAT |
| 54 447.65617 | ±0.00130 | P | y, SAT |
| 55 157.75013 | ±0.00090 | P | V, NFO |
| 55 175.72858 | ±0.00062 | P | V, NFO |
| 55 181.59081 | ±0.00071 | S | V, URSA |
| 55 202.69394 | ±0.00086 | P | V, NFO |
| 55 208.55713 | ±0.00069 | S | V, URSA |
| 55 247.63640 | ±0.00086 | P | V, NFO |
| 55 274.60204 | ±0.00058 | P | V, URSA |
| 55 813.91459 | ±0.00101 | P | V, URSA |
| 55 831.89207 | ±0.00103 | P | V, URSA |
| 55 831.89275 | ±0.00073 | P | V, NFO |
| 55 849.8700 | ±0.0015 | P | Diethelm (2012a) |
| 55 855.73235 | ±0.00079 | S | V, URSA |
| 55 882.69860 | ±0.00057 | S | V, NFO |
| 55 894.81080 | ±0.00070 | P | V, URSA |
| 55 936.62917 | ±0.00085 | S | V, NFO |
| 55 945.61739 | ±0.00078 | S | V, NFO |
| 55 945.62050 | ±0.00080 | S | Diethelm (2012b) |
Notes. Times are given as UTC HJD and are labelled as primary (“P”) or secondary (“S”) eclipses. Note that the adopted standard errors used here are not those quoted in the original sources.
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