TY CrA
Casey1998 - Casey1998y (Stromgren y)
Table 2 from Casey et al. (1995)
Stellar Heliocentric Radial Velocities for TY CrA
Telescope HJD Phase Phase Primary Secondary Tertiary
(2400000+) orig. 2 HV dv N HV dv N HV dv N Shift
4m89 47671.889 0.318 0.069 -48.6 0.6 3 60.4 14.0 2 26.4 18.0 2 -7.7
4m89 47672.621 0.571 0.322 -86.5 0.6 4 142.0 2.3 4 18.4 2.4 4 -5.4
4m89 47672.916 0.675 0.424 -49.5 0.4 3 78.4 4.2 3 29.4 2.7 3 -6.2
4m89 47673.624 0.917 0.669 63.5 0.6 4 -156.4 1.5 4 22.8 2.6 4 -6.7
4m89 47673.934 0.023 0.777 73.4 0.5 4 -167.8 1.0 4 18.4 4.5 4 -6.1
4m92 48807.778 0.526 0.276 -86.8 0.4 4 157.2 3.0 4 8.4 2.4 4 1.8
4m94 49493.740 0.981 0.733 90.4 0.4 14 -157.5 2.1 4 -8.6 3.0 4 10.0
4m94 49493.756 0.989 0.732 91.2 0.3 14 -157.3 1.6 4 -5.8 1.9 4 10.6
BMES94 49528.576 0.042 0.793 79.3 0.8 3 -158.2 2.4 8 3.2 3.4 8 1.3
BMES94 49528.624 0.057 0.809 77.9 1.8 3 -150.4 4.5 8 5.8 3.1 8 1.3
BMES94 49528.678 0.077 0.828 72.6 1.1 3 -147.2 1.9 6 4.4 5.4 6 1.3
BMES94 49528.739 0.097 0.849 65.4 0.7 3 -146.9 1.4 4 8.3 4.9 4 1.3
BMES94 49528.794 0.115 0.868 59.6 0.2 3 -137.6 11.2 4 2.0 5.5 4 1.3
BMES94 49528.852 0.136 0.888 49.8 0.9 3 -108.5 11.2 7 -1.1 4.6 6 1.3
BMES94 49528.910 0.157 0.908 44.5 1.4 3 -98.2 12.9 2 0.0 0.0 0 1.3
BMES94 49529.580 0.388 0.140 -69.2 0.3 3 120.0 0.2 3 6.0 6.5 3 1.3
BMES94 49529.633 0.405 0.158 -74.8 0.7 3 137.9 3.9 3 2.2 4.7 3 1.3
BMES94 49529.685 0.427 0.176 -80.1 0.5 3 145.7 5.0 6 -4.3 5.7 4 1.3
BMES94 49529.743 0.443 0.197 -85.2 1.1 3 157.5 3.5 7 -1.2 6.4 4 1.3
BMES94 49529.801 0.465 0.216 -85.2 0.5 3 152.6 3.2 6 -10.9 3.0 5 1.3
BMES94 49529.854 0.483 0.235 -87.5 0.6 3 154.8 2.1 8 -4.1 3.7 6 1.3
BMES94 49529.912 0.503 0.255 -87.3 1.4 3 152.3 3.6 5 -1.1 4.5 6 1.3
BMES94 49530.664 0.762 0.515 1.9 0.1 3 0 0 1.3
BMES94 49530.748 0.794 0.544 21.2 0.3 3 0 0 1.3
BMES94 49530.801 0.811 0.563 27.0 0.3 3 0 0 1.3
BMES94 49530.867 0.835 0.586 42.4 0.3 3 0 0 1.3
BMES94 49530.923 0.853 0.605 49.6 0.1 3 0 0 1.3
Phase orig. was given in Casey et al. and calculated using their ephemeris.
Phase 2 was calculated by Bradstreet (2004) using the ephemeris given in
Vaz et al. (1998).
The Shift column is explained in Casey et al. (1995).