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Table 2

Best fits of the orbital parameters for the currently claimed planets around eclipsing PCEBs.

Name Msin(i) P asin(i) e Ref. Notes
[Mj] [yr] [AU]

HW Vir c 14.3    ±    1.0 12.7    ±    0.2 4.69    ±    0.06 0.40    ±    0.10 1
HW Vir d 30–120 55    ±    15 12.8    ±    0.2 0.05: 1 *
HS0705+6700 c 31.5    ±    1.0 8.41    ±    0.05 3.52 0.38    ±    0.05 2 *
HS2231+2441 c 13.94    ±    2.20 15.7  ~5.16 3
NSVS14256825 c 2.8    ±    0.3 3.49    ±    0.21 1.9    ±    0.3 0.00    ±    0.08 4
NSVS14256825 d 8.0    ±    0.8 6.86    ±    0.25 2.9    ±    0.6 0.52    ±    0.06 4
NY Vir c 2.3    ±    0.3 7.9 3.3    ±    0.8 5
NY Vir d 2.5:  >15  ≳5.08 5
NN Ser c 6.91    ±    0.54 15.50    ±    0.45 5.38    ±    0.20 0.0 6
NN Ser d 2.28    ±    0.38 7.75    ±    0.35 3.39    ±    0.10 0.20    ±    0.02 6
V471 Tau c 46-111 33.2    ±    0.2  ~12.6−12.8 0.26    ±    0.02 7 *
QS Vir c 9.01 14.4  ~6.32 0.62 8
QS Vir d 56.59 16.99  ~7.15 0.92 8 *
RR Cae c 4.2    ±    0.4 11.9    ±    0.1 5.3    ±    0.6 0 9
UZ For c 6.3    ±    1.5 16+3 5.9    ±    1.4 0.04    ±    0.05 10
UZ For d 7.7    ±    1.2 5.25    ±    0.25 2.8    ±    0.5 0.05    ±    0.05 10
HU Aqr c 7.1 9.00    ±    0.05 4.30 0.13    ±    0.04 11
DP Leo c 6.05    ±    0.47 28.01    ±    2.00 8.19    ±    0.39 0.39    ±    0.13 12

Notes.  Very uncertain values are followed by “:”.

(*)

The claimed third body is more consistent with a BD than with a planet.

References. (1) Beuermann et al. (2012b); (2) Beuermann et al. (2012a); (3) Qian et al. (2010c); (4) Almeida et al. (2012a); (5) Qian et al. (2012b); (6) Beuermann et al. (2010); (7) Kundra & Hric (2011); (8) Almeida & Jablonski (2011); (9) Qian et al. (2012a); (10) Potter et al. (2011); (11) Goździewski et al. (2012); (12) Beuermann et al. (2011).

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