Table 2: Results of the IUE measurements for RS CVn stars.

HIP		 Name   $M_{\rm V}(IUE)$ $\Delta M_{\rm V}(IUE)$ ${\rm log}~W_{\circ}$ $\Delta {\rm log}~W_{\circ}$   ${\rm log}~L_{\mbox{Mg {\sc ii}}}$ $\Delta {\rm log}~L_{\mbox{Mg {\sc ii}}}$ N
4157 CF Tuc   2.76 0.17 2.16 0.15   30.41 0.30 8
9630 XX Tri   1.86   2.07     31.23   1
10280 TZ Tri   0.16 0.05 2.19 0.02   31.21 0.08 3
13118 VY Ari   3.59 0.17 1.91 0.01   30.13 0.06 5
16042 UX Ari   2.89 0.43 2.09 0.30   30.60 0.53 65
16846 V711 Tau   3.45 0.46 2.10 0.48   30.45 0.46 264
19431 EI Eri   3.29 0.16 2.12 0.23   30.23 0.18 28
23743 BM Cam   -0.32 0.10 2.23 0.01   31.77 0.08 2
24608 $\alpha$ Aur   -0.45 0.22 2.16 0.23   31.06 0.15 76
35600 AR Mon   1.43   2.41     30.99   1
37629 $\sigma$ Gem   1.36 0.26 2.13 0.30   31.09 0.33 27
46159 IL Hya   2.15   2.02     30.89   1
56851 V829 Cen       1.99     30.67   1
59600 HU Vir   3.25   2.04     30.46   1
59796 DK Dra   0.50 0.14 2.12 0.13   31.40 0.14 4
64293 RS CVn   2.98 0.14 2.05 0.05   29.96 0.08 3
65187 BM CVn       2.06     30.89   1
81519 WW Dra   3.10   2.28     29.97   1
82080 $\varepsilon$ UMi   -0.94 0.00 2.15 0.10   31.39 0.08 2
84586 V824 Ara   4.30 0.07 2.13 0.05   30.05 0.33 3
85852 DR Dra   1.62   2.05     30.88   1
87965 Z Her   2.29   1.82     29.92   1
88848 V815 Her   5.10 0.05 1.87 0.16   29.33 0.10 4
94013 V1762 Cyg   1.76 0.19 2.09 0.04   30.98 0.06 4
95244 V4138 Sgr   2.17   1.92     30.76   1
96003 V1817 Cyg   -1.23   2.22     32.11   1
96467 V1764 Cyg   0.35   2.34     31.53   1
109002 HK Lac   1.03 0.13 2.14 0.07   31.36 0.20 4
109303 AR Lac   3.08 0.90 2.28 0.33   30.19 0.47 198
111072 V350 Lac   1.03 0.05 2.16 0.09   30.97 0.11 2
112997 IM Peg   0.94 0.22 2.15 0.17   31.34 0.20 12
114639 SZ Psc   2.64 0.33 2.22 0.17   30.54 0.23 25
116584 $\lambda$ And   1.75 0.35 2.01 0.22   30.90 0.33 79
117915 II Peg   4.33 0.44 1.94 0.33   30.07 0.45 59
Notes: $M_{\rm V}(IUE)$ and $\Delta M_{\rm V}(IUE)$are the mean visual absolute magnitude and its maximum amplitude. ${\rm log}~W_{\circ}$ and $\Delta {\rm log}~W_{\circ}$ are, respectively, the logarithm of the mean full-width at half-maximum for the Mg II line and the corresponding spread. ${\rm log}~L_{\mbox{Mg {\sc ii}}}$ and $\Delta {\rm log}~L_{\mbox{Mg {\sc ii}}}$ are, respectively, the logarithm of the mean luminosity of the Mg II line and its spread. N is the number of the spectra used for each star. Units for the line widths $W_{\circ}$ and Mg II luminosities are in km s-1 and erg s-1, respectively.

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