Table 2: An X-ray and kinematic data ensemble for each star detailed in Table 1.
TARGET RASS X-raya,b,c Log $L^{d}_{\rm x}$ Log ($L_{\rm x}$/ $L_{\rm bol}$) $P_{\rm rot}$ $v \sin i$ HJD RV $v \sin i$ Commentse
  ct rate [ct s-1] [erg s-1]   [days] [kms-1] (+2450000) [kms-1] [kms-1]  
Lupus :                  
RX J1507.2-3505 $0.07 \pm 0.02$ 29.99 -4.09   15.0 2713.762 +2.1 13.0 RV = +1.4
            2718.766 +2.2 13.2  
RX J1507.4-4601 $0.06 \pm 0.02$ 29.93 -3.30     2718.790 +6.9 21.7  
RX J1515.7-3331 $0.10 \pm 0.02$ 30.15 -3.61 2.28 25.0 2713.860 +1.1 22.3  
            2718.925 +1.9 23.4  
RX J1518.4-3738 $0.13 \pm 0.02$ 30.26 -3.36 2.98 25.0 2718.746 +3.7 21.6 RV = +3.7
RX J1523.4-4055 $0.037 \pm 0.012$ 29.71 -3.62 4.15 9.9 2719.769 +5.6 11.7 RV = +6.8
RX J1524.5-3652 $0.06 \pm 0.02$ 29.93 -3.55 2.91 19.0 2713.826 +4.4 16.4 RV = +4.2
            2719.792 +4.6 17.6  
RX J1525.0-3604 $0.13 \pm 0.02$ 30.26 -3.44     2718.852 +4.8 23.2  
RX J1529.6-3546 $0.11 \pm 0.02$ 30.19       2718.879 +16.4 19.3 SB2
            2718.879 -11.3 19.5 SB2
RX J1529.7-3628 $0.06 \pm 0.02$ 29.93       2719.715 +3.2 14.5  
RX J1546.6-3618 $0.05 \pm 0.02$ 29.85 -3.69   7.1 2713.705 +7.2 $\leq$6 RV = +2.5
            2719.747 +7.3 $\leq$6  
RX J1547.6-4018 $0.06 \pm 0.01$ 29.93 -3.67   10.0 2713.737 +3.1 11.8 RV = +2.8
            2718.916 +3.2 12.9  
RX J1601.1-3320 $0.10 \pm 0.02$ 30.15 -3.62 3.78 21.9 2713.799 +2.3 18.8 RV = +3.0
RX J1605.7-3905 $0.16 \pm 0.02$ 30.35 -3.40     2713.780 +2.2 >50  
RX J1608.9-3905         $\sim49$ 2718.900 +9.7 30.4 RV = -0.6
            2718.900 -25.8 24.1 SB2
Chamaeleon I $\&$ II                  
RX J0850.1-7554 $0.17 \pm 0.02$ 30.68 -3.30   45 2712.590 +17.1 49.4 RV = +15.5
            2718.521 +35.0 26.5 SB2?
            2718.521 -0.8 23.3 SB2?
RX J0951.9-7901 $0.17 \pm 0.02$ 30.68 -3.54   73 2712.620 +39.8 49.0 RV = +12.2
            2712.620 -20.3 32.6 SB2?
            2718.533 +38.1 47.2 SB2?
            2718.533 -35.1 32.3 SB2?
RX J1112.7-7637 $0.08 \pm 0.02$ 30.36 -3.31   11 2712.694 +13.6 30.7 RV = +16.0
            2718.546 +15.2 28.4  
RX J1129.2-7546         20 2713.628 +15.9 20.8 RV = +11.4
            2719.528 +15.5 19.9  
RX J1140.3-8321 $0.11 \pm 0.02$ 30.50 -3.40   13 2718.563 +14.0 12.5 RV = +10.5
RX J1158.5-7754a $0.30 \pm 0.04$ 30.93 -3.45   11 2713.656 +10.4 15.1 RV = +13.1
            2718.614 +10.1 14.7  
RX J1159.7-7601 $0.10 \pm 0.02$ 30.46 -3.58   10 2718.636 +15.1 10.2 RV = +13.1
RX J1201.7-7859 $0.20 \pm 0.02$ 30.76 -3.96   21 2712.734 +12.3 22.2 RV = +10.0
            2718.678 +13.6 22.2 RV = +22.3
RX J1233.5-7523         7 2712.760 +14.8 7.2 RV = +14.0
            2718.716 +16.0 6.9 RV = +15.1
RX J1239.4-7502 $0.19 \pm 0.02$ 30.72 -3.47   19 2713.675 +14.5 20.2 RV = +13.1
            2718.726 +14.2 20.1  
RX J1303.5-7701           2712.779 -121.1   Early-Type
RX J1307.3-7708           2712.794 -25.3 $\leq$6  
Rho Ophiuchus :                  
RX J1627.1-2419           2712.852 -2.7    
RX J1625.6-2613           2712.886 -3.5 17.0  
CrA SFR :                  
CrAPMS 2 $0.08 \pm 0.02$ 29.93 -3.79 2.79 20 2713.909 -0.7 20.2 RV = -2.2,-1.2
            2719.923 0.0 20.4 RV = -2.6
RX J1839.0-3726         17.8 2719.869 -1.6 9.8 RV = -4.8
RX J1853.1-3609 $0.19 \pm 0.04$ 30.28 -3.68     2719.837 -3.2 24.0  
RX J1917.4-3756 $0.19 \pm 0.03$ 30.28 -3.82     2713.920 -0.9 28.1  
            2719.817 +0.5 28.3  
CrAPMS 4SE         <10 2719.901 -1.9 9.7 RV = -2.0
a The standard RASS conversion factor, for negligible interstellar absorption, of 6 $\times$ 10-12 erg cm-2 count-1 has been used.
b These fluxes are lower limits, as it is unlikely that these stars represent a sample of unabsorbed X-ray emitters (see text).
c For the ROSAT passband 0.1-2.4 keV.
d Distances used for luminosity calculations: Lupus, d= 140 pc (Hughes et al. 1993; Bertout et al. 1999; de Zeeuw et al. 1999); Chamaeleon, d= 160 pc (Bertout et al. 1999; Rebull et al. 2004, and references therein); CrA SFR, d= 120 pc (Morraco & Rydgren 1981; Casey et al. 1998).
e Lupus Vsini/Periods/RV data are taken from Wichmann et al. (1998, 1999); Chamaeleon Vsini/RV data are taken from Covino et al. (1997), Cutispoto et al. (2002) & Nordström et al. (2004); CrA SFR Vsini/RVs/Period data are taken from Neuhäuser et al. (2000), Franchini et al. (1992), Walter et al. (1997) & Shevchenko et al. (1995).


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