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  CASE. V. Three eclipsing binaries in M4 (Kaluzny+, 2013)
Post annotation
1.J/AJ/145/43/minimaTimes of minima for V65 (table1), V66 (table2), and V69 (table3)[timeSerie] (25 rows)
2.J/AJ/145/43/velocVelocity observations of V65 (table7), V66 (table8), and V69 (table9)[timeSerie] (92 rows)

Query by Constraints constraints help applied on Columns (Output Order: + - )
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (ALL)Star (char) V65 (table1), V66 (table2), V69 (table3) (;meta.main)
  (1)E  Eclipse (Note 1)   (meta.number;time.period)
  (1)f_E (char) [a] The orbit is eccentric, and the secondary minimum occurs at phase 0.6086052(±0.0000077) (meta.code)
   (ALL)HJD d Heliocentric Julian Date (HJD-2400000) (time.epoch)
  (1)e_HJD d 1σ uncertainty in HJD (stat.error;time.epoch)
  (1)O-C d The (O-C) residual (;
  (2)RV1 km/s Radial velocity of the primary component (spect.dopplerVeloc)
  (2)RV2 km/s Radial velocity of the secondary component (spect.dopplerVeloc)
  (2)RV3 km/s (n) Radial velocity of the contaminating star (Note 1)   (spect.dopplerVeloc)
  (2)Phase  Orbital phase (Note 2)   (time.phase)

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