Table B.1
Known BL stars where we did not detect the modulation.
| ID | PPuls [d] | S/N | Pliterature [d] | Ref. |
|
|
||||
| AL Eri | 0.656947(4) | 3.3 | − | K05 |
| ASAS J030534-3116.1 | 0.496453(2) | 3.2 | 6.67 | SF07 |
| V0461 Her | 0.513006(6) | 3.0 | − | B14 |
| V1162 Her | 0.547929(6) | 3.3 | − | B14 |
| GL Hya | 0.505932(4) | 3.4 | 157 | B14 |
| V0487 Hya | 0.561482(6) | 3.2 | 64.4 | B14 |
| ASAS J101200+1921.9 | 0.482830(10) | 3.3 | 1141.03 | SF07 |
| MS Lib | 0.441446(8) | 3.1 | 105 | B14 |
| AQ Lyr | 0.356809(4) | 3.2 | 64.9 | J09 |
| V0829 Oph | 0.569222(8) | 3.1 | 165 | Wa06 |
| V2683 Oph | 0.597012(4) | 2.9 | 26.28 | SF07 |
| V0606 Peg | 0.529658(4) | 2.9 | 26.7 | B14 |
| FI Psc | 0.531285(6) | 3.2 | >170 | B14 |
| CzeV0245 | 0.513328(4) | 3.0 | − | K12 |
| UZ Vir | 0.459394(4) | 3.3 | 68.24 | J09, S12 |
| ASAS J194502+2434.2 | 0.845945(22) | 3.2 | 37.56 | SF07 |
Notes. The column S/N gives information about S/N of the highest peak detected after removing significant pulsation components in the vicinity of f0 ± 0.2 c/d. Ref: K05 −Kovács (2005); SF07 −Szczygieł & Fabrycky (2007); B14 −Bramich et al. (2014); J09 – Jurcsik et al. (2009); Wa06 −Watson et al. (2006); K12 −Kocián et al. (2012); S12 −Sódor et al. (2012).
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