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Table A.1

Orbital parameters of all known hot subdwarf binaries from literature.

Object P γ K Reference
[d] [km s-1] [km s-1]
PG 0850+170 27.815 32.2 ± 2.8 33.5 ± 3.3 Morales-Rueda et al. (2003a)
PG 1619+522 15.3578 −52.5 ± 1.1 35.2 ± 1.1 Morales-Rueda et al. (2003a)
PG 1110+294 9.4152 −15.2 ± 0.9 58.7 ± 1.2 Morales-Rueda et al. (2003a)
Feige 108 8.7465 45.8 ± 0.6 50.2 ± 1.0 Edelmann et al. (2004)
PG 0940+068 8.330 −16.7 ± 1.4 61.2 ± 1.4 Maxted et al. (2000b)
PHL 861 7.44 −26.5 ± 0.4 47.9 ± 0.4 Karl et al. (2006)
HE 1448−0510 7.159 −45.5 ± 0.8 53.7 ± 1.1 Karl et al. (2006)
PG 1032+406 6.7791 24.5 ± 0.5 33.7 ± 0.5 Morales-Rueda et al. (2003a)
PG 0907+123 6.11636 56.3 ± 1.1 59.8 ± 0.9 Morales-Rueda et al. (2003a)
HE 1115−0631 5.87 87.1 ± 1.3 61.9 ± 1.1 Napiwotzki et al. (in prep.)
CD −24 731 5.85 20.0 ± 5.0 63.0 ± 3.0 Edelmann et al. (2005)
PG 1244+113 5.75207 9.8 ± 1.2 55.6 ± 1.8 Morales-Rueda et al. (2003b)
PG 0839+399 5.6222 23.2 ± 1.1 33.6 ± 1.5 Morales-Rueda et al. (2003a)
TON S 135 4.1228 −3.7 ± 1.1 41.4 ± 1.5 Edelmann et al. (2005)
PG 0934+186 4.051 7.4 ± 2.9 60.2 ± 2.0 Morales-Rueda et al. (2003b)
PB 7352 3.62166 −2.1 ± 0.3 60.8 ± 0.3 Edelmann et al. (2005)
KPD 0025+5402 3.5711 −7.8 ± 0.7 40.2 ± 1.1 Morales-Rueda et al. (2003a)
TON 245 2.501 − 88.3 Morales-Rueda et al. (2003a)
PG 1300+2756 2.25931 −3.1 ± 0.9 62.8 ± 1.6 Morales-Rueda et al. (2003a)
NGC 188/II−91 2.15 − 22.0 Green et al. (2004)
V 1093 Herp 1.77732 −3.9 ± 0.8 70.8 ± 1.0 Morales-Rueda et al. (2003a)
HD 171858 1.63280 62.5 ± 0.1 60.8 ± 0.3 Edelmann et al. (2005)
KPD 2040+3954 1.48291 −11.5 ± 1.0 95.1 ± 1.7 Morales-Rueda et al. (2003b)
HE 2150−0238 1.321 −32.5 ± 0.9 96.3 ± 1.4 Karl et al. (2006)
 [CW83]  1735+22 1.278 20.6 ± 0.4 103.0 ± 1.5 Edelmann et al. (2005)
PG 1512+244 1.26978 −2.9 ± 1.0 92.7 ± 1.5 Morales-Rueda et al. (2003a)
PG 0133+114 1.23787 −0.3 ± 0.2 82.0 ± 0.3 Edelmann et al. (2005)
HE 1047−0436 1.21325 25.0 ± 3.0 94.0 ± 3.0 Napiwotzki et al. (2001)
HE 1421−1206 1.188 −86.2 ± 1.1 55.5 ± 2.0 Napiwotzki et al. (in prep.)
PG 1000+408 1.041145 41.9 72.4 Shimanskii et al. (2008)
PB 5333 0.92560 −95.3 ± 1.3 22.4 ± 0.8 Edelmann et al. (2004)
HE 2135−3749 0.9240 45.0 ± 0.5 90.5 ± 0.6 Karl et al. (2006)
EC 12408−1427 0.90243 −52.0 ± 1.2 58.9 ± 1.6 Morales-Rueda et al. (2006)
PG 0918+0258 0.87679 104.4 ± 1.7 80.0 ± 2.6 Morales-Rueda et al. (2003a)
PG 1116+301 0.85621 −0.2 ± 1.1 88.5 ± 2.1 Morales-Rueda et al. (2003a)
PG 1230+052 0.8372 −43.4 ± 0.8 41.5 ± 1.3 Morales-Rueda et al. (2003b)
V 2579 Ophp 0.8292056 −54.16 ± 0.27 70.10 ± 0.13 For et al. (2006)
TON S 183 0.8277 50.5 ± 0.8 84.8 ± 1.0 Edelmann et al. (2005)
EC 02200−2338 0.8022 20.7 ± 2.3 96.3 ± 1.4 Morales-Rueda et al. (2005)
PG 0849+319 0.74507 64.0 ± 1.5 66.3 ± 2.1 Morales-Rueda et al. (2003a)
JL 82r 0.73710 −1.6 ± 0.8 34.6 ± 1.0 Edelmann et al. (2005)
PG 1248+164 0.73232 −16.2 ± 1.3 61.8 ± 1.1 Morales-Rueda et al. (2003a)
HD 188112† 0.60658125 26.6 ± 0.3 188.4 ± 0.2 Edelmann et al. (2005)
PG 1247+554 0.602740 13.8 ± 0.6 32.2 ± 1.0 Maxted et al. (2000b)
PG 1725+252 0.601507 −60.0 ± 0.6 104.5 ± 0.7 Morales-Rueda et al. (2003a)
PG 0101+039el,p 0.569899 7.3 ± 0.2 104.7 ± 0.4 Geier et al. (2008)
HE 1059−2735 0.555624 −44.7 ± 0.6 87.7 ± 0.8 Napiwotzki et al. (in prep.)
PG 1519+640 0.54029143 0.1 ± 0.4 42.7 ± 0.6 Edelmann et al. (2004)
PG 0001+275 0.529842 −44.7 ± 0.5 92.8 ± 0.7 Edelmann et al. (2005)
PG 1743+477 0.515561 −65.8 ± 0.8 121.4 ± 1.0 Morales-Rueda et al. (2003a)
HE 1318−2111 0.487502 48.9 ± 0.7 48.5 ± 1.2 Napiwotzki et al. (in prep.)
PG 1544+488‡ 0.48 −23 ± 4 57 ± 4/97 ± 10 Ahmad et al. (2004)
GALEX J234947.7+384440 0.46249 2.0 ± 1.0 87.9 ± 2.2 Kawka et al. (2010)
HE 0230−4323r,p 0.45152 16.6 ± 1.0 62.4 ± 1.6 Edelmann et al. (2005)
HE 0929−0424 0.4400 41.4 ± 1.0 114.3 ± 1.4 Karl et al. (2006)
 [CW83]  1419−09 0.4178 42.3 ± 0.3 109.6 ± 0.4 Edelmann et al. (2005)
KPD 1946+4340ec,el 0.403739 −5.5 ± 1.0 167.0 ± 2.4 Morales-Rueda et al. (2003a)
KUV 04421+1416r,p 0.398 33 ± 3 90 ± 5 Reed et al. (2010)
Feige 48p 0.376 −47.9 ± 0.1 28.0 ± 0.2 O’Toole et al. (2004)
GD 687 0.37765 32.3 ± 3.0 118.3 ± 3.4 Geier et al. (2010a)
PG 1232−136 0.3630 4.1 ± 0.3 129.6 ± 0.04 Edelmann et al. (2005)
PG 1101+249 0.35386 −0.8 ± 0.9 134.6 ± 1.3 Moran et al. (1999)
PG 1438−029r 0.336 − 32.1 Green et al. (2005)
PG 1528+104 0.331 −49.9 ± 0.8 52.7 ± 1.3 Morales-Rueda et al. (2003b)
PG 0941+280ec 0.315 − − Green et al. (2004)
KBS 13r 0.2923 7.53 ± 0.08 22.82 ± 0.23 For et al. (2008)
CPD−64 481 0.2772 94.1 ± 0.3 23.8 ± 0.4 Edelmann et al. (2005)
GALEX J032139.8+472716 0.26584 70.5 ± 2.2 59.8 ± 4.5 Kawka et al. (2010)
HE 0532−4503 0.2656 8.5 ± 0.1 101.5 ± 0.2 Karl et al. (2006)
AA Dorec,r 0.2614 1.57 ± 0.09 40.15 ± 0.11 Müller et al. (2010)
PG 1329+159r 0.249699 −22.0 ± 1.2 40.2 ± 1.1 Morales-Rueda et al. (2003a)
PG 2345+318ec 0.2409458 −10.6 ± 1.4 141.2 ± 1.1 Moran et al. (1999)
PG 1432+159 0.22489 −16.0 ± 1.1 120.0 ± 1.4 Moran et al. (1999)
BPS CS 22169−0001r 0.1780 2.8 ± 0.3 14.9 ± 0.4 Edelmann et al. (2005)
HS 2333+3927r 0.1718023 −31.4 ± 2.1 89.6 ± 3.2 Heber et al. (2004)
2M 1533+3759ec,r 0.16177042 −3.4 ± 5.2 71.1 ± 1.0 For et al. (2010)
EC 00404−4429 0.12834 33.0 ± 2.9 152.8 ± 3.4 Morales-Rueda et al. (2005)
2M 1938+4603ec,r 0.1257653 20.1 ± 0.3 65.7 ± 0.6 Østensen et al. (2010)
BUL-SC 16 335ec,r 0.125050278 − − Polubek et al. (2007)
PG 1043+760 0.1201506 24.8 ± 1.4 63.6 ± 1.4 Morales-Rueda et al. (2003a)
HW Virec,r 0.115 −13.0 ± 0.8 84.6 ± 1.1 Edelmann (2008)
HS 2231+2441ec,r 0.1105880 − 49.1 ± 3.2 Østensen et al. (2007)
NSVS 14256825ec,r 0.110374102 − − Wils et al. (2007)
PG 1336−018ec,r,p 0.101015999 −25.0 78.7 ± 0.6 Vučković et al. (2007)
HS 0705+6700ec,r 0.09564665 −36.4 ± 2.9 85.8 ± 3.6 Drechsel et al. (2001)
KPD 1930+2752el,p 0.0950933 5.0 ± 1.0 341.0 ± 1.0 Geier et al. (2007)
KPD 0422+5421ec,el 0.09017945 −57.0 ± 12.0 237.0 ± 18.0 Orosz & Wade (1999)
NGC 6121−V46el† 0.087159 31.3 ± 1.6 211.6 ± 2.3 O’Toole et al. (2006)
PG 1017−086r 0.0729938 −9.1 ± 1.3 51.0 ± 1.7 Maxted et al. (2002)

Notes. The superscript p denotes sdB pulsators, r binaries where with reflection effect, ec eclipsing systems and el systems with light variations caused by ellipsoidal deformation.

†

Post-RGB stars without core helium-burning.

‡

Double-lined binary consisting of two helium rich sdBs. The RV semi-amplitudes of both components are given.

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