Table 1: XSS sources identified with ABs and CVs.
XSS source Name Classa Db $L_{\rm h}^{c}$ $L_{\rm x}^{d}$ Hardness $1/V_{\rm gen}$
(J2000.0)     pc erg/s erg/s ratio pc-3
02290-6931 RBS 324 P 250 1 31.88 31.70 0.41 $\pm$ 0.25 $4.9\times 10^{-8}$
02569+1931 XY Ari IP 270 2 32.43 32.12 0.88 $\pm$ 0.42 $1.2\times 10^{-8}$
03089+4101 $\beta$ Per AL 28 3 30.91 30.77 0.28 $\pm$ 0.06 $8.9\times 10^{-7}$
03385+0029 V711 Tau RS 29 3 30.23 30.15 0.10 $\pm$ 0.19 $8.2\times 10^{-6}$
05019+2444 V1062 Tau IP 1100 4 33.77 33.51 0.69 $\pm$ 0.12 $1.2\times 10^{-9}$
05295-3252 TV Col IP 370 5 33.08 32.80 0.77 $\pm$ 0.09 $3.1\times 10^{-9}$
05432-4116 TX Col IP 500 4 32.71 32.50 0.52 $\pm$ 0.21 $6.3\times 10^{-9}$
05450+6049 BY Cam P 190 6 31.96 31.74 0.55 $\pm$ 0.24 $3.9\times 10^{-8}$
06132+4755 SS Aur DN 280 7 32.17 31.97 0.48 $\pm$ 0.24 $2.2\times 10^{-8}$
07514+1442 PQ Gem IP 400 4 32.79 32.54 0.68 $\pm$ 0.20 $5.3\times 10^{-9}$
08010+6241 HT Cam IP 400 8 32.72 32.46 0.70 $\pm$ 0.29 $6.2\times 10^{-9}$
08142+6231 SU Uma DN 260 7 32.16 31.99 0.37 $\pm$ 0.17 $2.3\times 10^{-8}$
11474+7143 DO Dra IP 155 4 32.02 31.78 0.62 $\pm$ 0.10 $3.3\times 10^{-8}$
12392-3820 V1025 Cen IP 400 9 32.36 32.19 0.37 $\pm$ 0.14 $1.4\times 10^{-8}$
12529-2911 EX Hya IP 6510 31.79 31.62 0.40 $\pm$ 0.02 $6.2\times 10^{-8}$
13355+3714 BH CVn RS 45 3 31.15 31.07 0.11 $\pm$ 0.11 $4.2\times 10^{-7}$
14100-4500 V834 Cen P 15011 31.72 31.48 0.61 $\pm$ 0.12 $7.6\times 10^{-8}$
14241-4803 HD125599e ? 90 3 30.72 30.62 0.15 $\pm$ 0.15 $1.6\times 10^{-6}$
14527-2414 HD130693f ? 2712 30.07 29.93 0.28 $\pm$ 0.08 $1.4\times 10^{-5}$
16167-2817 V893 Sco DN 150 7 32.10 31.92 0.40 $\pm$ 0.08 $2.7\times 10^{-8}$
17309-0552 1RXS J173021.5-055933 IP 330013 34.28 34.06 0.54 $\pm$ 0.29 $8.1\times 10^{-10}$
17597+0821 V2301 Oph P 15014 31.90 31.67 0.56 $\pm$ 0.10 $4.6\times 10^{-8}$
18080+0622 V426 Oph DN 20015 32.07 31.85 0.56 $\pm$ 0.25 $2.9\times 10^{-8}$
18164+5004 AM Her P 79 7 31.77 31.50 0.74 $\pm$ 0.05 $6.6\times 10^{-8}$
18553-3111 V1223 Sgr IP 51016 33.73 33.45 0.76 $\pm$ 0.02 $1.2\times 10^{-9}$
19243+5041 CH Cyg SS 25017 32.26 31.87 1.25 $\pm$ 0.26 $1.8\times 10^{-8}$
21155-5836 CD Ind P 25018 31.90 31.64 0.70 $\pm$ 0.24 $4.6\times 10^{-8}$
22178-0822 FO Aqr IP 300 4 32.85 32.53 0.94 $\pm$ 0.09 $4.7\times 10^{-9}$
22526+1650 IM Peg RS 97 3 31.65 31.46 0.42 $\pm$ 0.03 $9.3\times 10^{-8}$
22551-0309 AO Psc IP 250 4 32.57 32.33 0.60 $\pm$ 0.10 $8.6\times 10^{-9}$
a Class: RS - RS CVn; AL - Algol; DN - dwarf nova; P - polar; IP - intermediate polar; SS - symbiotic star.
b Reference for distance: 1 - Schwope et al. (2002); 2 - Littlefair et al. (2001); 3 - Hipparcos; 4 - Patterson (1994); 5 - McArthur et al. (2001); 6 - Warner (1995); 7 - Thorstensen (2003); 8 - Tovmassian (1998); 9 - assumed; 10 - Eisenbart et al. (2002); 11 - Araujo-Betancor et al. (2005); 12 - Tycho; 13 - based on Gänsicke et al. (2005), see main text; 14 - Silber et al. (1994); 15 - Hessman (1998); 16 - Beuermann et al. (2004); 17 - Sokoloski & Kenyon (2003); 18 - lower limit (The MSSL Polar Page, http://www.mssl.ucl.ac.uk/www_astro/gal/polar.html).
c Log of 3-20 keV luminosity.
d Log of 2-10 keV luminosity.
e Bright (V=8.5) F7/8V star associated with the bright ROSAT source 1RXS J142148.7-480420.
f Bright (V=8.2) G6V star associated with the bright ROSAT source 1RXS J145017.6-242558 = RBS 1436 (Schwope et al. 2000).

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