Table A.6: Times of primary (P) and secondary (S) minima for VZ Hya. O-C values are calculated for the ephemeris given in Eq. (5) adopting a circular orbit. Observing methods are: PG photographic; V visual; PE photoelectric or CCD. Times marked with an asterisk were published after we completed the ephemeris calculations; including them makes no significant changes.

HJD
rms rms O-C Type Observing Reference
- 2 400 000 publ. adopt. days   method  

21 925.8246
0.0008 0.0011 0.0018 P PG O32 (T0)
26 674.3410 0.0010 0.0120 -0.0127 P PG G53 (T0)
27 856.412   0.0063 0.0081 P V L49
29 604.794   0.0063 0.0014 P V W46
29 700.634   0.0063 -0.0006 P V -
30 034.626   0.0063 -0.0031 P V -
39 926.673   0.0063 -0.0027 P V BA74
40 254.8602 0.0005 0.0007 -0.0014 P PE W70
40 998.362   0.0028 -0.0004 P PE PS75
41 033.212   0.0028 -0.0020 P PE -
42 354.668   0.0063 -0.0026 P V B18(1974)
42 848.401   0.0063 -0.0007 P V B27(1976)
43 577.372   0.0063 -0.0090 P V B37(1978)
44 236.6532   0.0028 -0.0040 P PE W82
47 971.5876* 0.0003   0.0003 P PE SC07
48 267.8259 0.0001 0.0001 -0.0001 P PE This paper
48 270.7303 0.0001 0.0001 0.0000 P PE -
48 273.6346 0.0001 0.0001 0.0001 P PE -
51 253.4340   0.0063 -0.0125 P V BAV122(1999)
51 256.3520   0.0063 0.0012 P V -
52 702.6936* 0.0001   0.0012 P PE SC07
27 840.437   0.0063 0.0067 S V L49
29 681.751   0.0063 -0.0056 S V W46
29 748.556   0.0063 0.0005 S V -
30 015.742   0.0063 -0.0091 S V -
40 305.6848 0.0005 0.0015 -0.0020 S PE W70
40 654.201   0.0028 -0.0019 S PE PS75
40 686.154   0.0028 0.0038 S PE -
41 743.305   0.0063 -0.0104 S V B8(1973)
48 684.5934 0.0002 0.0006 0.0004 S PE This paper
References are: B = BBSAG Bulletin, followed by volume number and year of publication; BA74 = Baldwin (1974); BAV = B.A.V. Mitt., followed by volume number and year of publication; G53 = epoch given by Gaposchkin (1953); L49 = Lause (1949); O32 = epoch given by O'Connell (1932); PS75 = Padalia & Srivastava (1975); SC07 = Smith & Caton (2007); W46 = Wood (1946); W70 = redetermined from B and V data by Walker (1970); W82 = Wolf et al. (1982).

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