Table 1: Observations of six sdB stars using HST/STIS. Note that CPD  $-64^\circ 481$ was observed only in the FUV and using the E140H grating.

Target
$\alpha$ $\delta$ V $T_{{\rm eff}}$ $\log g$ log(He/H) Ref. Pulsator? $T_{\rm exp}^{\rm NUV}$ $T_{\rm exp}^{\rm FUV}$
  (2000) (2000) (mag) (K)         (s) (s)
PG 1219+534 12 21 29.1 +53 04 37 13.2 33 500 5.87 -1.6 4 yes 3100/3100 2160/3100
Feige 48 11 47 14.5 +61 15 32 13.5 29 500 5.54 -2.9 2 yes 3500/3511 3600/3600
CPD  $-64^\circ 481$ 05 47 59.3 -64 23 03 11.3 27 500 5.60 -2.5 3 no -- 1440
Feige 66 12 37 23.5 +25 03 60 10.6 34 500 5.83 -1.6 4 no 824 875
CD  $-24^\circ 731$ 01 43 48.6 -24 05 10 11.0 35 400 5.90 -2.9 4 no 800 878

References: (1) Heber et al. (1999); (2) Heber et al. (2000); (3) O'Toole et al. (2005); (4) this work.

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