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Table 1

Orbital parameters for the currently known eclipsing PCEBs.

System Alt. Name P orb M 1 M 2 References
[d] [M⊙] [M⊙]
Detached sdB+MS/BD PCEBs
HW Vir 2M J1244-0840 0.11671955 0.485    ±    0.013 0.142    ±    0.004 1, 2
HS 0705+6700 2M J0710+6655 0.095646625 0.483 0.134 3, 4
HS 2231+2441 2M J2234+2456 0.110588 0.47: 0.075: 5
NSVS 14256825 2M J2020+0437 0.11037423 0.419  ±  0.070 0.109  ±  0.023 6
NY Vir PG 1336-018 0.101015967 0.459    ±    0.005 0.122    ±    0.001 7, 8, 9
2M1938+4603 NSVS 05629361 0.1257653 0.48    ±    0.03 0.12    ±    0.01 10
NSVS 07826247 CSS06833 0.16177042 0.376    ±    0.055 0.113    ±    0.017 11
BUL-SC16 335 2M J1809-2641 0.12505028 0.5: 0.16: 12
PG 1621+4737 2M J1622+4730 0.075 – – 13
SDSS J0820+0008 GSC 0196.0617 0.097  ~0.25 0.045    ±    0.03 14, 15
 ~0.47 0.068    ±    0.03 15
ASAS 10232 2M J1023-3736 0.13927 0.461    ±    0.051 0.157    ±    0.017 16
AA Dor LB 3459 0.261539736 0.471    ±    0.005 17,18
EC 10246-2707 0.118507993 0.45    ±    0.17 0.12    ±    0.05 19
Detached WD+MS PCEBs
NN Ser 2M J1552+1254 0.13008014 0.535    ±    0.012 0.111    ±    0.004 20, 21
V471 Tau 2M J0350+1714 0.52118343 0.84    ±    0.05 0.93    ±    0.07 22, 23
QS Vir EC 13471-1258 0.1507575 0.78    ±    0.040 0.430    ±    0.040 24
RR Cae 2M J0421-4839 0.30370363 0.440    ±    0.022 0.183    ±    0.013 25
DE Cvn RX J1326.9+4532 0.364139315 0.41    ±    0.06 26, 27
GK Vir SDSS J1415+0117 0.344330833 0.564    ±    0.014 0.116    ±    0.003 28
RX J2130.6+4710 2M J2130+4710 0.52103562 0.554    ±    0.017 0.555    ±    0.023 29
SDSS J0110+1326 WD 0107+131 0.332687 0.47    ±    0.02 0.255–0.380 30
SDSS J0303+0054 0.1344377 0.878-0.946 0.224–0.282 30
SDSS J0857+0342 CSS03170 0.06509654 0.51    ±    0.05 0.09    ±    0.01 31
SDSS J1210+3347 0.12448976 0.415    ±    0.010 0.158    ±    0.006 32
SDSS J1212-0123 0.3358711 0.439    ±    0.002 0.273    ±    0.002 27
SDSS J1435+3733 0.125631 0.48-0.53 0.190–0.246 30
SDSS J1548+4057 0.1855177 0.614-0.678 0.146–0.201 30
CSS06653 SDSS J1329+1230 0.08096625 0.350    ±    0.081 – 33, 34
CSS07125 SDSS J1410-0202 0.363497 0.470    ±    0.055 0.380    ±    0.012 34, 35
CSS080408 SDSS J1423+2409 0.3820040 0.410    ±    0.024 0.255    ±    0.040 34, 35
CSS080502 SDSS J0908+0604 0.14943807 0.370    ±    0.018 0.319    ±    0.061 33, 34
CSS09704 SDSS J2208-0115 0.1565057 0.37 – 35
CSS09797 SDSS J1456+1611 0.229120 0.370    ±    0.016 0.196    ±    0.043 34, 35
CSS21357 SDSS J1348+1834 0.2484 0.590    ±    0.017 0.319    ±    0.061 34, 35
CSS21616 SDSS J1325+2338 0.1949589 – – 33
CSS25601 SDSS J1244+1017 0.227856 0.400    ±    0.026 0.319    ±    0.061 34, 35
CSS38094 SDSS J0939+3258 0.3309896 0.520    ±    0.026 0.319    ±    0.061 33, 34
CSS40190 SDSS J0838+1914 0.13011232 0.390    ±    0.035 0.255    ±    0.040 33, 34
CSS41631 SDSS J0957+2342 0.15087074 0.430    ±    0.025 0.431    ±    0.108 33, 34
WD 1333+005 SDSS J1336+0017 0.1219587 – – 33
PTFEB11.441 PTF1 J004546.0+415030.0 0.3587 0.51    ±    0.09 0.35    ±    0.05 36
PTFEB28.235 PTF1 J015256.6+384413.4 0.3861 0.65    ±    0.11 0.35    ±    0.05 36
PTFEB28.852 PTF1 J015524.7+373153.8 0.4615 0.52    ±    0.05 0.35    ±    0.05 36
KIC-10544976 USNO-B1.0 1377-0415424 0.35046872 0.61    ±    0.04 0.39    ±    0.03 37
SDSS J0821+4559 0.50909 0.66    ±    0.05 0.431    ±    0.108 34, 38
SDSS J0927+3329 2.30822 0.59    ±    0.05 0.380    ±    0.012 34, 38
SDSS J0946+2030 0.252861219 0.62    ±    0.10 0.255    ±    0.040 34, 38
SDSS J0957+3001 1.92612 0.42    ±    0.05 0.380    ±    0.012 34, 38
SDSS J1021+1744 0.14035907 0.50    ±    0.05 0.319    ±    0.061 34, 38
SDSS J1028+0931 0.23502576 0.42    ±    0.04 0.380    ±    0.012 34, 38
SDSS J1057+1307 0.1251621 0.34    ±    0.07 0.255    ±    0.040 34, 38
SDSS J1223-0056 0.09007 0.45    ±    0.06 0.196    ±    0.043 34, 38
SDSS J1307+2156 0.216322132 – 0.319    ±    0.061 34, 38
SDSS J1408+2950 0.1917902 0.49    ±    0.04 0.255    ±    0.040 34, 38
SDSS J1411+1028 0.167509 0.36    ±    0.04 0.380    ±    0.012 34, 38
SDSS J2235+1428 0.14445648 0.45    ±    0.06 0.319    ±    0.061 34, 38
CVs
UZ For 2M J0335-2544 0.08786542  ~0.71  ~0.14 39, 40
HU Aqr 2M J2107-0517 0.08682041 0.80    ±    0.04 0.18    ±    0.06 41, 42
DP Leo RX J2107.9-0518 0.06236286 1.2: 0.14: 43, 44
0.6: 0.09: 45

Notes. Systems with suspected planets are in bold. We distinguish between detached systems containing sdB primaries, detached systems with WD primaries, and CVs. For the case of CVs we only list those with suspected planets (see Sect. 2 for details). Very uncertain values are followed by “:”. It generally means that the mass was assumed and not derived. Systems with suspected planets are in bold. We distinguish between detached systems containing sdB primaries, detached systems with WD primaries, and CVs. For the case of CVs we only list those with suspected planets (see Sect. 2 for details).

References. (1) Lee et al. (2009); (2) Beuermann et al. (2012b); (3) Drechsel et al. (2001); (4) Beuermann et al. (2012a); (5) Østensen et al. (2007); (6) Almeida et al. (2012b); (7) Vučković et al. (2007); (8) Charpinet et al. (2008); (9) Qian et al. (2012b); (10) Østensen et al. (2010); (11) For et al. (2010); (12) Polubek et al. (2007); (13) Geier et al. (2010); (14) Geier et al. (2012); (15) Geier et al. (2011b); (16) Schaffenroth et al. (2011); (17) Kilkenny (2011); (18) Klepp & Rauch (2011); (19) Barlow et al. (2012); (20) Parsons et al. (2010a); (21) Beuermann et al. (2010); (22) O’Brien et al. (2001); (23) Kundra & Hric (2011); (24) O’Donoghue et al. (2003); (25) Maxted et al. (2007); (26) van den Besselaar et al. (2007); (27) Parsons et al. (2010b); (28) Parsons et al. (2012b); (29) Maxted et al. (2004); (30) Pyrzas et al. (2009); (31) Parsons et al. (2011a); (32) Pyrzas et al. (2012); (33) Backhaus et al. (2012); (34) Rebassa-Mansergas et al. (2012); (35) Drake et al. (2010); (36) Law et al. (2012); (37) Almenara et al. (2012); (38) Parsons et al. (2012a); (39) Bailey & Cropper (1991); (40) Potter et al. (2011); (41) Schwarz et al. (2009); (42) Schwope et al. (2011); (43) Pandel et al. (2002); (44) Beuermann et al. (2011); (45) Schwope et al. (2002).

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