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Table 4:

Physical parameters and spectral types for the stars with Hectochelle or literature spectra.

Id
2MASS P R $v\sin i$ $T_{\rm eff}$ Sp. Type $EW_{\rm H\alpha}^{g}$ $EW_{\rm Li}$ $\sin i$
    (days) ($R_{\odot}$) (km s-1) (K)     (Å)   (Å)  
2 05352029-0546399 7.751 1.24 7.0 $\pm$ 1.0 3710 $\pm$ 110 M2.5a   7.5   0.864
4 05352007-0545526     30 $\pm$ 5 5720 $\pm$ 100 G2a   0.0    
5 05351981-0545409 0.60 1.33     M3.5b      
9 05352281-0544428 0.5627 1.98 126 $\pm$ 6 3480 $\pm$ 170 M3a   3.6 0.72c 0.674
10 05352617-0545084 5.816 1.25 11.0 $\pm$ 1.0 4110 $\pm$ 170 K8a   7.0 0.52d $\simeq$1
13 05351621-0547201     4.0 $\pm$ 2.0 5800 $\pm$ 200 G1a   0.0    
14 05351192-0545379 4.047 1.89 22.5 $\pm$ 1.5 4250 $\pm$ 170 K7a, K8b   3.8 0.41d 0.952
17 05350614-0545311 8.435 1.26     M0b      
18 05353222-0544265 12.461 2.16     M3b      
19 05352973-0548450 0.605 2.29     K8b      
21 05351033-0546335   4.72 12.0 $\pm$ 2.0 4830 $\pm$ 250 K0a   3.9    
23 05351011-0548342   0.84 1.0 $\pm$ 0.5 3690 $\pm$ 70 M2.5a   9.0    
28 05351423-0543175   3.28 20.0 $\pm$ 1.5 4260 $\pm$ 270 K7a, K7ee 13.7    
29 05351236-0543184 8.468 1.87     K7ed      
47 05353023-0551169 10.02 1.21     K8b      
48 05353047-0549037 7.721 1.04 7.5 $\pm$ 1.5 3830 $\pm$ 220 M2a, M2b   8.6   $\simeq$1
51 05353316-0547074 2.763 0.92 16.0 $\pm$ 0.5 3690 $\pm$ 100 M3a, M3.5b   2.6   0.949
52 05352930-0545381 1.696 1.03 25.0 $\pm$ 2.0 3740 $\pm$ 90 M2.5a, M3.5b   6.6 0.41c 0.813
56 05353092-0543053 3.80 1.38 13.5 $\pm$ 1.5 3920 $\pm$ 260 M1.5a, M2b   4.9 0.50c 0.734
60 05351643-0542396 4.11 1.40     K5b   0.45c  
62 05351715-0541538 2.05 1.18     M5b      
65 05345908-0544303   2.07 13.0 $\pm$ 1.5 3990 $\pm$ 260 M1.5a   8.6    
70 05350054-0548591   1.50 12.0 $\pm$ 2.0 4600 $\pm$ 500 K5a   8.2    
93 05351790-0542340 5.70: 3.33 34f 4775f K3f     $\simeq$1


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