Table 1.
Results of the least-squares fit in the form mag = α + β log P for the LMC and SMC, where mag is represented by the Wesehneit magnitudes W (calculated as in Eq. 2) or by the G, GBP, GRP magnitudes.
| Galaxy | α | β | σ | n | Method | Type | Note |
|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| LMC | 16.000±0.008 | −3.327 ± 0.012 | 0.104 | 1539 | PW | DCEP_F | |
| LMC | 15.518±0.004 | −3.471 ± 0.012 | 0.087 | 1148 | PW | DCEP_1O | |
| LMC | 17.326±0.014 | −2.765 ± 0.021 | 0.191 | 1545 | PL(G) | DCEP_F | |
| LMC | 16.860±0.010 | −3.159 ± 0.029 | 0.209 | 1158 | PL(G) | DCEP_1O | |
| LMC | 17.545±0.017 | −2.580 ± 0.025 | 0.229 | 1545 | PL(GBP) | DCEP_F | |
| LMC | 17.088±0.012 | −3.008 ± 0.035 | 0.258 | 1176 | PL(GBP) | DCEP_1O | |
| LMC | 16.859±0.012 | −2.892 ± 0.018 | 0.159 | 1542 | PL(GRP) | DCEP_F | |
| LMC | 16.384±0.008 | −3.204 ± 0.023 | 0.169 | 1157 | PL(GRP) | DCEP_1O | |
| SMC | 16.705±0.015 | −3.595 ± 0.057 | 0.209 | 1126 | PW | DCEP_F | P < 2.95 d |
| SMC | 16.608±0.021 | −3.400 ± 0.026 | 0.169 | 608 | PW | DCEP_F | P ≥ 2.95 d |
| SMC | 17.294±0.027 | −2.897 ± 0.034 | 0.219 | 613 | PW | DCEP_1O | |
| SMC | 16.823±0.008 | −3.160 ± 0.031 | 0.221 | 1259 | PL(G) | DCEP_F | P < 2.95 d |
| SMC | 16.137±0.006 | −3.555 ± 0.025 | 0.175 | 1226 | PL(G) | DCEP_F | P ≥ 2.95 d |
| SMC | 17.916±0.017 | −3.113 ± 0.063 | 0.231 | 1110 | PL(G) | DCEP_1O | |
| SMC | 17.722±0.030 | −2.764 ± 0.037 | 0.238 | 598 | PL(GBP) | DCEP_F | P < 2.95 d |
| SMC | 17.274±0.009 | −3.134 ± 0.037 | 0.262 | 1264 | PL(GBP) | DCEP_F | P ≥ 2.95 d |
| SMC | 18.066±0.016 | −2.892 ± 0.063 | 0.229 | 1102 | PL(GBP) | DCEP_1O | |
| SMC | 17.891±0.035 | −2.578 ± 0.043 | 0.275 | 607 | PL(GRP) | DCEP_F | P < 2.95 d |
| SMC | 17.431±0.010 | −2.944 ± 0.040 | 0.286 | 1287 | PL(GRP) | DCEP_F | P ≥ 2.95 d |
| SMC | 17.425±0.014 | −3.153 ± 0.054 | 0.201 | 1132 | PL(GRP) | DCEP_1O | |
| LMC | 16.725±0.033 | −2.625 ± 0.196 | 0.143 | 38 | PW | ACEP F | |
| LMC | 16.314±0.087 | −2.564 ± 0.506 | 0.166 | 13 | PW | ACEP 1O | |
| LMC | 17.948±0.034 | −2.516 ± 0.201 | 0.189 | 46 | PL(G) | ACEP F | |
| LMC | 17.355±0.074 | −2.749 ± 0.455 | 0.173 | 19 | PL(G) | ACEP 1O | |
| LMC | 18.115±0.052 | −2.119 ± 0.304 | 0.225 | 38 | PL(GBP) | ACEP F | |
| LMC | 17.561±0.111 | −2.401 ± 0.649 | 0.212 | 13 | PL(GBP) | ACEP 1O | |
| LMC | 17.496±0.036 | −2.354 ± 0.209 | 0.154 | 38 | PL(GRP) | ACEP F | |
| LMC | 16.992±0.056 | −2.486 ± 0.327 | 0.107 | 13 | PL(GRP) | ACEP 1O | |
| SMC | 17.185±0.042 | −2.931 ± 0.229 | 0.170 | 31 | PW | ACEP F | |
| SMC | 16.942±0.078 | −3.211 ± 0.659 | 0.213 | 13 | PW | ACEP 1O | |
| SMC | 18.380±0.041 | −2.669 ± 0.223 | 0.188 | 36 | PL(G) | ACEP F | |
| SMC | 17.836±0.096 | −2.943 ± 0.843 | 0.284 | 15 | PL(G) | ACEP 1O | |
| SMC | 18.569±0.052 | −2.598 ± 0.280 | 0.207 | 31 | PL(GBP) | ACEP F | |
| SMC | 17.966±0.111 | −2.883 ± 0.944 | 0.305 | 13 | PL(GBP) | ACEP 1O | |
| SMC | 17.954±0.039 | −2.754 ± 0.209 | 0.155 | 31 | PL(GRP) | ACEP F | |
| SMC | 17.489±0.088 | −3.017 ± 0.750 | 0.243 | 13 | PL(GRP) | ACEP 1O | |
| LMC | 17.376±0.049 | −2.356 ± 0.050 | 0.162 | 80 | PW | T2CEP | |
| LMC | 18.627±0.055 | −1.726 ± 0.061 | 0.251 | 112 | PL(G) | T2CEP | |
| LMC | 18.743±0.088 | −1.484 ± 0.093 | 0.303 | 82 | PL(GBP) | T2CEP | |
| LMC | 18.132±0.069 | −1.875 ± 0.072 | 0.238 | 83 | PL(GRP) | T2CEP | |
| SMC | 17.755±0.197 | −2.359 ± 0.183 | 0.233 | 15 | PW | T2CEP | |
| SMC | 19.063±0.147 | −1.893 ± 0.145 | 0.271 | 20 | PL(G) | T2CEP | |
Notes. The different columns show the: (1) studied galaxy; (2) and (3) coefficients of the linear regression and relative errors; (4) rms of the residuals; (5) number of objects used in the fit; (6) method (PL or PW); (7) type of pulsator; and (8) notes.
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