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J/MNRAS/455/4136
  Kepler triples (Borkovits+, 2016)
img(gal)
    J/MNRAS/455/4136/table2(c)Properties of the investigated systems (230 rows)
    J/MNRAS/455/4136/table3Orbital elements from LTTE solutions for systems, where more than two outer periods are covered, or/and triply eclipsing systems (38 rows)
    J/MNRAS/455/4136/table4Orbital elements from LTTE solutions which cover more than one but less than two outer periods (64 rows)
    J/MNRAS/455/4136/table5Orbital elements from LTTE solutions which cover less than a full period (58 rows)
    J/MNRAS/455/4136/table6Orbital elements from combined dynamical and LTTE solutions for systems, where more than two outer periods are covered, or/and triply eclipsing systems (31 rows)
    J/MNRAS/455/4136/table7Orbital elements from combined dynamical and LTTE solutions which cover more than one but less than two outer periods (14 rows)
    J/MNRAS/455/4136/table8Orbital elements from combined dynamical and LTTE solutions which cover less than a full outer period (17 rows)
    J/MNRAS/455/4136/table9Orbital elements from LTTE solutions for systems which probably are oscillating variables instead of binaries (i.e. false positive EBs) (16 rows)
    J/MNRAS/455/4136/table10Apsidal motion and/or orientation parameters from AME and dynamical fits (66 rows)

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       (c)  indicates tables which contain celestial coordinates 
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