Table A.1
Results of the analysis of the observed light curves without variations in the MUCHFUSS follow-up.
| Target. | Primary | σa |  |
 |
 |
 |
 |
 |
system excludedf | lnpg |
|---|---|---|---|---|---|---|---|---|---|---|
| o | h | ° | km s−1 | ° | km s−1 | km s−1 | d | |||
| J002323−002953h | sdB+WD | 4.00 | 1.90 | 5.40 | 8.77 | 2.76 | 7.48 | 168.0 ± 4.0 | J1622 & HW Vir | < −680 |
| J095238+625818h | sdB+WD | 3.76 | 1.54 | 5.05 | 8.14 | 2.54 | 6.75 | 154.0 ± 8.0 | J1622 & HW Vir | < −680 |
| J134632+281722h | sdB+WD | 5.57 | 3.47 | 7.03 | 11.78 | 3.83 | 10.93 | 191.0 ± 7.0 | J1622 & HW Vir | < −680 |
| J083006+475150h | sdB+WD | 6.30 | 2.14 | 7.80 | 13.18 | 4.32 | 12.53 | 164.0 ± 9.0 | J1622 & HW Vir | < −680 |
| J032138+053840h | sdB+? | 2.60 | 1.52 | 3.96 | 6.10 | 1.82 | 4.40 | 110.0 ± 9.0 | J1622 & HW Vir | < −680 |
| J204613−045418h | sdB+WD | 5.47 | 0.67 | 6.93 | 11.59 | 3.76 | 10.71 | 259.0 ± 16.0 | J1622 & HW Vir | − 480.28 |
| J011857−002546h | sdOB+? | 4.39 | 1.98 | 5.80 | 9.52 | 3.02 | 8.33 | 140.0 ± 8.0 | J1622 & HW Vir | − 386.64 |
| J191908+371423 | sdB | 10.60 | 2.00 | 12.49 | 21.49 | 7.31 | 22.00 | 237.0 ± 12.0 | J1622 & HW Vir | −526.21 |
| J072245+305233 | sdB | 7.51 | 1.50 | 9.10 | 15.51 | 5.16 | 15.19 | 123.0 ± 12.0 | J1622 & HW Vir | −62.09 |
| J093059+025032 | sdB | 3.52 | 2.04 | 4.90 | 7.85 | 2.44 | 6.42 | 91.0 ± 9.0 | J1622 & HW Vir | −49.22 |
| J115358+353929 | sdOB | 16.00 | 2.18 | 18.77 | 32.05 | 11.19 | 33.92 | 79.0 ± 9.5 | J1622 & HW Vir | −19.15 |
| J153411+543345 | sdOB | 13.87 | 1.17 | 16.23 | 27.86 | 9.64 | 29.21 | 83.0 ± 18.5 | J1622 & HW Vir | −12.52 |
| J224518+220746 | sdB | 5.73 | 1.93 | 7.20 | 12.09 | 3.93 | 11.28 | 70.0 ± 11.5 | J1622 & HW Vir | −12.28 |
| J074534+372718 | sdB | 7.45 | 2.55 | 9.03 | 15.40 | 5.12 | 15.06 | 64.0 ± 17.0 | J1622 & HW Vir | −9.74 |
| J030607+382335 | sdB | 6.40 | 1.74 | 7.91 | 13.37 | 4.39 | 12.75 | 48.0 ± 6.5 | J1622 & HW Vir | −8.85 |
| J185129+182358 | sdB | 8.00 | 1.40 | 9.63 | 16.46 | 5.50 | 16.27 | 105.0 ± 18.0 | J1622 & HW Vir | −7.33 |
| J171629+575121 | sdOB | 27.50 | 1.41 | 34.19 | 55.18 | 19.99 | 59.43 | 67.0 ± 15.5 | – | −6.14 |
| J112242+613758 | sdB | 2.87 | 1.50 | 4.24 | 6.61 | 2.00 | 5.00 | 83.0 ± 18.5 | J1622 & HW Vir | −5.80 |
| J065044+383133 | sdOB | 10.60 | 2.33 | 12.49 | 21.49 | 7.31 | 22.00 | 88.0 ± 13.5 | J1622 & HW Vir | −4.63 |
| J115716+612410 | sdB | 5.19 | 2.17 | 6.63 | 11.05 | 3.57 | 10.09 | 102.0 ± 27.0 | J1622 & HW Vir | −3.63 |
| J113304+290221 | sdB | 13.60 | 2.84 | 15.92 | 27.33 | 9.45 | 28.62 | 95.0 ± 30.0 | J1622 & HW Vir | −3.39 |
| J133639+111948 | sdB | 9.50 | 1.97 | 11.27 | 19.36 | 6.54 | 19.58 | 48.0 ± 14.0 | J1622 & HW Vir | −3.25 |
Notes. (a) Standard deviation of the normalized light curve in RB. (b) Length of the observed light curve. (c)Maximum inclination. (d) Expected semi-amplitude of the RV curve. (e)Maximal measured radial velocity shift. (F)Type of system that can be excluded. (g)False detection probability of radial velocity variability (taken from Geier et al. 2015); stars were classified as RV variable for ln p < −9.2 and RV-variable candidates for lnp < −3.0. (h) Stars with known periods from time-resolved spectroscopy (see Kupfer et al. 2015).
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