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J/ApJ/837/96
  Rotation-Activity Correlations in K-M dwarfs II. (Houdebine+, 2017)
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    J/ApJ/837/96/table2(c)Equivalent width of the Ca II resonance doublet and Hα line for our sample of dK6 stars (127 rows)
    J/ApJ/837/96/table3(c)The values of vsin(i), P/sin(i) as well as [M/H] from Paper I (Houdebine+ 2016, J/ApJ/822/97) for our dM2 stars (108 rows)
    J/ApJ/837/96/table4(c)Equivalent width of the Ca II resonance doublet and Hα line for our sample of dM3 stars (see Houdebine & Mullan, 2015ApJ...801..106H) (83 rows)
    J/ApJ/837/96/table5(c)The values of vsin(i), P/sin(i) and [M/H] from Paper I (Houdebine+ 2016, J/ApJ/822/97) for our targets in our list of dM3 stars (97 rows)
    J/ApJ/837/96/table6(c)Equivalent width of the Ca II resonance doublet and Hα line for our sample of dM4 stars (103 rows)
    J/ApJ/837/96/table7(c)The values of vsin(i), P/sin(i) and [M/H] compiled from Paper I (Houdebine+ 2016, J/ApJ/822/97) for our targets in our list of dM4 stars (106 rows)
    J/ApJ/837/96/table8(c)The log(LHK), log(Lbol), R'HK and R0 for our samples of dK4, dK6, dM2, dM3 and dM4 stars (384 rows)

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       (c)  indicates tables which contain celestial coordinates 
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