TRUE VARIABILITY TYPES OF SOME CANDIDATES FOR CLASSICAL CEPHEIDS AFTER LIGHT CURVE VERIFICATION Star ID Other ID Period Variability type Comments V567__Sco ASAS J164951-4055.1 68.6106 RV Tau (RVb) V641__Cen ASAS J143908-5950.1 - SR V910__Car ASAS J095355-5849.7 1.52636 ROT (ACV) low amplitude IU____Cen ASAS J140731-5641.9 3.31930 BL Her (CWB) ASAS J094844-3921.4 ASASSN-V J094843.93-392129.4 1.20172 BL Her (CWB) ASAS J164507-4129.0 4.23892 ELL two minima of different depth BEST-II_lra2b_01286 OGLE GD1712.05.46 - SPOTTED mean brightness and amplitude variations BEST-II_lra2b_01100 OGLE GD1707.29.6094 7.34 SPOTTED light curve shape variations BEST-II_lra2a_01358 OGLE GD1712.26.3352 14.74 SPOTTED amplitude and shape variations CT____Sge ASASSN-V J201908.36+204249.2 1.71791 BL Her (CWB) ASAS J183934+1122.9 ASASSN-V J183934.36+112252.6 2.30604 CONST ASAS J185152-1333.6 ASASSN-V J185151.64-133332.2 1.26857 BL Her (CWB) VVV-29 OGLE BLG669.07.4833 - SPOTTED =Matsunaga+2016 #7=17321407−3323595, no variability signal NSVS14571823 ATLAS 104623434388001674 2.25341 ACEP F ASAS J210538+2005.0 ATLAS 132093164073508412 1.70864 ACEP F ASAS J193435-1921.7 ATLAS 84762936444506995 2.11943 ACEP F V565__Oph ATLAS 115042689260103692 1.89972 ACEP F SU____Sct OGLE-BLG-T2CEP-1080 1.467808 BL Her (CWB) BC____Aql ATLAS 97102893506503176 2.90528 BL Her (CWB) NGC6819-SHLP-2203 - SPOTTED NGC6819 is not a young cluster (2.6 Gyr), in Kepler C0 field V1307_Aql 0.283117 RRab cannot be a Galactic DCEP with V~17 mag at b=-9.5 deg V1083_Cas 4.0783 SPOTTED not a DCEP light curve HQ____Car OGLE-GD-T2CEP-0020 14.1138 W Vir (CWA) ASAS J174419-2313.7 OGLE-BLG-T2CEP-655 16.0763 W Vir (CWA) V1313_Aql ASASSN-V J185724.14+104233.6 8.04148 W Vir (CWA) IX____Cas ASASSN-V J000450.81+501405.5 9.15337 W Vir (CWA) V507__Sco OGLE-BLG-T2CEP-0988 11.8034 W Vir (CWA) V5626_Sgr OGLE-GAL-ACEP-023 1.33919 ACEP F reclassification from OGLE-BLG-CEP-025 OGLE-BLG-RRLYR-09105 OGLE-GAL-ACEP-020 0.97667 ACEP F V1529_Sco OGLE-GAL-ACEP-019 1.53176 ACEP F reclassification from OGLE-BLG-CEP-014 ATLAS J099.2347-05.3509 ASAS J063656-0521.0 5.02875 SPOTTED mean brightness and amplitude variations ASASSN-V J140149.83-572016.5 OGLE-GAL-ACEP-068 1.71560 ACEP F V2830_Ori ASASSN-V J045954.96+101718.5 6.44077 W Vir (CWB) V1087_Cas ASASSN-V J011908.28+580419.0 - SPOTTED not a DCEP light curve HK____Cas ASASSN-V J005720.05+552620.1 2.49951 BL Her (CWB) V933__Per ASASSN-V J035848.11+514258.9 - SPOTTED no variability signal V5560_Sgr ASASSN-V J175621.48-273755.6 11.5994 pW Vir (CWA) NSV13578 ASASSN-V J211037.69+323134.0 9.53094 W Vir (CWA) EK____Del ASASSN-V J205404.91+083305.3 2.04685 ACEP F AL____Cyg ASASSN-V J204715.57+311247.1 1.84193 EA PP____Aql ASASSN-V J195246.45+124008.7 48.1655 RV Tau (RVa) V979__Aql ASASSN-V J193207.20+030045.5 0.70288 RRab V526__Aql OGLE-GD-T2CEP-0321 4.20906 W Vir (CWB) BEST-lrcby_01008 ASASSN-V J184359.24+052146.7 - SPOTTED not a DCEP light curve, low amplitude BEST-lrca1a_1673 ASASSN-V J183744.79+073305.9 0.560484 VAR not a CEP light curve OGLE-GD-CEP-0013 OGLE GD1337.07.1029 5.24673 SPOTTED =ASASSN-V J113302.65-605204.5, amplitude and shape variations ATLAS J285.5187-04.1866 ZTF 436206400035772 4.699260 RS CVn eclipses and modulation due to spots ASAS-SN J190001.20+114228.9 OGLE-GD-T2CEP-0299 15.7687 W Vir (CWA) ASAS J162326-0941.0 1.378289 BL Her (CWB) ATLAS J262.2976+04.9065 ASASSN-V J172911.44+045423.8 4.512015 VAR mean brightness and shape variations ASASSN-V J172007.96-122045.3 3.685669 BL Her (CWB) ASASSN-V J181932.39+091737.5 1.115468 BL Her (CWB) ASASSN-V J194551.90-175602.9 1.550998 ACEP F V2830_Ori ASASSN-V J045954.96+101718.5 6.441784 W Vir (CWA) SZ____Tau AAVSO VAR (RS CVn?) close object with d~637 pc, high latitude ASASSN-V J195350.28-095621.4 2.04019 BL Her (CWB) ATLAS J084.6341-05.0676 ASASSN-V J053832.19-050403.6 1.601789 BL Her (CWB) ASASSN-V J180520.08-265854.0 1.513792 BL Her (CWB) ATLAS J268.4127-20.0239 AP29347748 43.227915 RV Tau ATLAS J277.4719-01.1104 ASASSN-V J182953.33-010638.0 10.439689 VAR not a DCEP light curve ATLAS J282.2041+05.2860 ASASSN-V J184848.99+051710.0 38.235122 RV Tau OTHER COMMENTS ASAS J070832-1454.5 has stable amplitude and mildly asymmetric phased light curve with P=6.387742 d. It is DCEP 1O, not ELL. V4257 Sgr = OGLE-BLG-CEP-196 - DCEP 1O with P = 0.2535572 d V440__Per is a fundamental-mode Cepheid, according to spectroscopic observations by Kovtyukh et al. (2012).