| Cepheid | Period (d) | EB–V | MV | Cluster/Group2 | Reference3 |
| SU Cas (OT) | 1.95/(2.75) | 0.33 ±0.02 | –3.15 ±0.07 | Alessi 95 | Turner et al. 2012, MNRAS, 422, 2501 |
| EU Tau | 2.10 | Anon (HIP 27129) | Alessi: 2006, unpublished | ||
| DT Cyg | 2.50 | Anon (B-type stars) | Turner: 2006, unpublished | ||
| EV Sct | 3.09/(4.39) | NGC 6664 | Schmidt: 1982, AJ, 87, 1197 | ||
| SZ Tau (OT) | 3.15/(4.48) | 0.29 ±0.01 | –3.09 ±0.04 | NGC 1647 | Turner 1992, AJ, 104, 1865 |
| V1334 Cyg | 3.34 | Dolidze 45 | Turner & Majaess 2009, unpublished | ||
| V620 Pup (FM) | 2.59 | 0.64 ±0.02 | –2.74 ±0.11 | Turner 14 | Turner et al. 2012, AJ, 144, 187 |
| BD Cas | 3.65 | Czernik 1 ? | Turner: 2007, unpublished | ||
| QZ Nor | 3.79/(5.47) | NGC 6067 | Coulson & Caldwell: 1985, MNRAS, 216, 671 | ||
| SU Cyg (FM) | 3.85 | 0.15 ±0.01 | –3.19 ±0.07 | Turner 9 | Turner et al. 1998, JRASC, 92, 145 |
| α UMi (FM) | 3.97 | 0.02 ±0.01 | –3.07 ±0.01 | Harrington 1 | Turner et al. 2013, ApJL, 762, L8 |
| V1726 Cyg (FM) | 4.24 | 0.33 ±0.02 | –3.08 ±0.07 | Platais 1 | Turner et al. 2006, Observatory, 126, 207 |
| CG Cas (FM) | 4.37 | 0.64 ±0.02 | –3.06 ±0.12 | Berkeley 58 | Turner et al. 2008, MNRAS, 388, 444 |
| CE Cas B | 4.48 | NGC 7790 | Mateo & Madore: 1988, ASP Conf., 4, 174 | ||
| TV CMa | 4.67 | NGC 2345 | Moffat: 1974, A&AS, 16, 33 | ||
| CF Cas | 4.88 | NGC 7790 | Mateo & Madore: 1988, ASP Conf., 4, 174 | ||
| GSC3729-1127 | 5.07 | Tombaugh 5 | Majaess et al.: 2008, MNRAS, 390, 1539 | ||
| CE Cas A | 5.14 | NGC 7790 | Mateo & Madore: 1988, ASP Conf., 4, 174 | ||
| UY Per | 5.37 | Czernik 8 | Turner: 1977, PASP, 89, 277 | ||
| δ Cep | 5.37 | Cep OB6 | de Zeeuw et al.: 1999, AJ, 117, 354 | ||
| CV Mon (FM) | 5.38 | 0.75 ±0.02 | –3.37 ±0.08 | van den Bergh 1 | Turner et al. 1998, AJ, 115, 1958 |
| V Cen | 5.49 | NGC 5662b | Clariá et al.: 1991, MNRAS, 249, 193 | ||
| GH Car | 5.73 | Trumpler 18 | Vazquez & Feinstein: 1990, A&AS, 86, 209 | ||
| AB Cam | 5.79 | Tombaugh 5b? | Turner: 2007, unpublished | ||
| R Cru | 5.83 | NGC 4349 | Turner & Forbes: 1984, unpublished | ||
| T Ant | 5.90 | 0.02 ±0.01 | –3.07 ±0.01 | Anon (HD 82872) | Turner & Berdnikov: 2003, A&A, 407, 325 |
| CS Vel | 5.90 | Ruprecht 79 | Walker: 1987, MNRAS, 229, 31 | ||
| V367 Sct (DM, FM) | 4.38/6.29 | 1.27 ±0.02 | –3.58 ±0.07 | NGC 6649 | Turner 1981, AJ, 86, 231 |
| BB Sgr (FM) | 6.64 | 0.30 ±0.02 | –3.08 ±0.12 | Collinder 394 | Turner & Pedreros 1985, AJ, 90, 1231 |
| T Cru | 6.73 | NGC 4349 | Turner & Forbes 1984, unpublished | ||
| U Sgr | 6.74 | IC 4725 (M25) | Pel 1985, IAU Colloquium, 82, 1 | ||
| DL Cas (FM) | 8.00 | 0.47 ±0.01 | –3.80 ±0.05 | NGC 129 | Turner et al. 1992, AJ, 104, 1132 |
| S Nor (FM) | 9.75 | 0.17 ±0.01 | –3.95 ±0.04 | NGC 6087 | Turner: 1986, AJ, 92, 111 |
| ζ Gem | 10.15 | ADS 5742 | Turner & Fernie: 1978, IBVS, 1509 | ||
| TW Nor | 10.79 | Lyngå 6 | Walker: 1985, MNRAS, 213, 889 | ||
| V340 Nor | 11.29 | NGC 6067 | Coulson & Caldwell: 1985, MNRAS, 216, 671 | ||
| GT Car | 13.16 | 0.66 ±0.02 | –4.3 ±0.50? | Anon Car OB | Turner et al. 1993, ApJS, 85, 119 |
| X Cyg (FM) | 16.39 | 0.25 ±0.02 | –4.87 ±0.07 | Ruprecht 173/175 | Turner 1998, AJ, 116, 274 |
| VY Car | 18.99 | 0.36 ±0.03 | –4.90 ±0.13 | Turner 15/16 | Turner: 2017, in preparation |
| RU Sct | 19.70 | Trumpler 35b | Turner 1980, ApJ, 240, 137 | ||
| WZ Sgr (FM) | 21.85 | 0.56 ±0.01 | –5.07 ±0.10 | Turner 2 | Turner et al. 1993, ApJS, 85, 119 |
| SW Vel (FM) | 23.44 | 0.35 ±0.02 | –5.09 ±0.07 | Vel OB5 | Turner et al. 1993, ApJS, 85, 119 |
| T Mon | 27.02 | Mon OB2 | Turner: 1976, ApJ, 210, 65 | ||
| AQ Pup (FM) | 29.97 | 0.47 ±0.07 | –5.40 ±0.25 | Turner 14 | Turner et. al. 2012, AJ, 144, 187 |
| U Car | 38.77 | Anon Car OB | Turner: 1988, ASP Conf., 4, 178 | ||
| RS Pup | 41.38 | Pup R3 | Havlen: 1972, A&A, 16, 252 | ||
| SV Vul | 45.04 | Vul OB1 | Turner: 1984, JRASC, 78, 229 | ||
| GY Sge | 51.25 | Anon Sge OB | Forbes 1982, AJ, 87, 1022 | ||
| S Vul | 68.50 | Vul OB2 | Turner: 1980, ApJ, 235, 146 | ||
| V810 Cen (DM, FM) | 130.2/152.9 | 0.25 ±0.01 | –7.90 ±0.10 | Stock 14 | Turner 1982, PASP, 94, 655 |
| HD 18391 (DM, FM) | 123.0/177.8 | 1.02 ±0.09 | –7.76 ±0.10 | TKMLM 1 | Turner et al. 2009, AN, 330, 807 |
Notes:
1 The observed pulsational period is listed, with the periods for both modes listed for recognized overtone pulsators and the expected period for fundamental mode pulsation being indicated for suspected overtone pulsators.
2 The list includes only clusters or groups for which there are reasonably strong reasons to believe that the identified Cepheids are potential members, despite some controversy over individual objects. There is an equally long list of clusters that share the fields of Cepheids and that are less strongly indicated to share a physical association. Contact the author of this Web site for details.
3 Generally the most recent study of the associated cluster or group is listed.