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Table 2:

Projected rotational velocities for the binary sdB systems from Table 1.

System 		$T_{\rm eff}$ mB S/N Seeing $N_{\rm lines}$ ${v_{\rm rot}~\sin~i}$ Instrument Reference
  [K] [mag]   [arcsec]   [ ${\rm km~s^{-1}}$]    
PG 1627+017l 23 500 11.3 64   11 <7.0 HRS  
GD 687 24 300         21.2 $\pm$ 2.0   Geier et al. (2010a)
JL 82l 25 000 12.2 55   57 10.4 $\pm$ 1.0 FEROS  
PB 7352 25 000 12.0 61   39 7.4 $\pm$ 1.0 FEROS  
HE 0532-4503 25 400 16.1 83 0.8 18 11.1 $\pm$ 1.0 UVES  
PG 0001+275l 25 400 12.8 129   24 12.6 $\pm$ 1.0 FOCES  
PG 1248+164 26 600 14.4 47   13 8.9 $\pm$ 1.3 HRS  
PG 1232-136 26 900 13.1 167   64 <5.0 UVES  
PG 1432+159 26 900 13.6 50   22 9.5 $\pm$ 1.0 HRS  
PG 1716+426l 27 400 13.7 61   24 10.9 $\pm$ 1.0 HRS  
PG 0101+039l 27 500         10.9 $\pm$ 1.1   Geier et al. (2008a)
CPD -64 481 27 500 11.0 152   38 4.1 $\pm$ 1.0 FEROS  
PG 2345+318 27 500 14.4 92   21 12.9 $\pm$ 1.0 HRS  
PG 1043+760l 27 600 13.4 15   H/He <88 Palomar  
PG 1743+477 27 600 13.6 57   27 <7.0 HRS  
TON S 183 27 600 12.4 55   57 6.7 $\pm$ 1.0 FEROS  
HD 171858 27 700 9.6 90   55 6.7 $\pm$ 1.0 FEROS  
HW Vir 28 500 10.3 130   H/He 78.3 $\pm$ 1.0 FEROS  
HS 0705+6700 28 800 14.2 28   H/He <170 HRS  
          H/He 110 $\pm$ 14   Drechsel et al. (2001)
PG 1329+159 29 100 13.3 52   26 10.7 $\pm$ 1.0 HRS  
Feige 48s 29 500 13.1 37   36 8.5 $\pm$ 1.0 HIRES  
HE 0929-0424 29 500 15.4 25 0.6 9 7.1 $\pm$ 1.0 UVES  
HE 1421-1206 29 600 15.1 21 0.5 18 6.7 $\pm$ 1.1 UVES  
PG 0133+114 29 600 10.7 194   17 <8.0 FOCES  
PG 1101+249 29 700 12.5 66   24 8.1 $\pm$ 1.0 HIRES  
PG 1512+244 29 900 13.0 87   17 <8.0 HRS  
HE 2135-3749 30 000 13.7 84 1.0 53 6.9 $\pm$ 1.0 UVES  
PHL 861 30 000 15.1 24 0.6 16 7.2 $\pm$ 1.3 UVES  
HE 1047-0436 30 200 14.7 37 0.6 37 6.2 $\pm$ 1.0 UVES  
HE 2150-0238 30 200 15.8 27 0.8 16 8.3 $\pm$ 1.5 UVES  
PG 1017+086 30 300       H/He 118 $\pm$ 5   Maxted et al. (2002)
HE 0230-4323s 31 100 13.8 59 0.9 40 12.7 $\pm$ 1.0 UVES  
PG 1336-018s 31 300 14.0 40   H/He <79.0 FEROS  
PG 1116+301 32 500 14.3 42   8 9.0 $\pm$ 1.7 HRS  
KPD 1946+4340 34 200 14.1 55   H/He 26.0 $\pm$ 1.0 HRS  
HE 1448-0510 34 700 15.0 27 0.6 8 7.2 $\pm$ 1.7 UVES  
KPD 1930+2752s 35 200         92.3 $\pm$ 1.5   Geier et al. (2007)
CD -24 731 35 400 11.6 42   8 12.1 $\pm$ 1.7 FEROS  
[CW83] 1735+22 38 000 11.5 230   H/He 44.0 $\pm$ 1.0 FOCES  
BPS CS 22169-0001 39 300 12.6 109   5 8.5 $\pm$ 1.5 FEROS  

Notes. For binaries with high ${v_{\rm rot}~\sin~i}$ helium lines and Balmer line cores (H/He) are used instead of metal lines. The average seeing is only given if the spectra were obtained with a wide slit in the course of the SPY survey. In all other cases the seeing should not influence the measurements. c Companion visible in the spectrum. s Pulsating subdwarf of V 361 Hya type. l Pulsating subdwarf of V 1093 Her type.


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