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Table 5.

Comparison between present results for ACs in the LMC, the SMC, and the literature.

Relation Galaxy Mode α σα α0 σα0 β σβ RMS n.stars Author
mag mag mag mag mag/dex mag/dex mag
PLG LMC F 17.78 0.04 −0.69 0.05 −2.99 0.20 0.24 83 TW
PLV theory F −0.69 0.14 −2.73 0.14 Marconi et al. (2004)
PLV LMC F −0.56 0.04 −3.21 0.21 0.20 32 Ripepi et al. (2014)
PLV LMC F 17.80 0.04 −0.68 0.05 −2.82 0.19 0.22 80 TW
PLV theory 1O −1.56 0.25 −2.95 0.25 Marconi et al. (2004)
PLV LMC 1O −1.26 0.09 −3.14 0.37 0.23 10 Ripepi et al. (2014)
PLV LMC 1O 17.10 0.04 −1.38 0.05 −3.31 0.32 0.22 35 TW
PLK LMC F 16.74 0.02 −3.54 0.15 0.10 32 Ripepi et al. (2014)
PLK LMC F 16.69 0.03 −1.79 0.04 −3.12 0.13 0.16 78 TW
PLK LMC 1O 16.06 0.07 −4.18 0.33 0.10 10 Ripepi et al. (2014)
PLK LMC 1O 16.13 0.02 −2.35 0.04 −3.41 0.18 0.13 33 TW
PWVI theory F −1.93 −3.34 0.20 Marconi et al. (2004)
PWVI LMC F 16.59 0.02 −3.41 0.16 0.15 32 Ripepi et al. (2014)
PWVI LMC F 16.61 0.02 −3.16 0.14 0.15 62 Groenewegen & Jurkovic (2017)
PWVI LMC F 16.59 0.02 −2.96 0.12 94 Iwanek et al. (2018)
PWVI LMC F 16.60 0.02 −1.88 0.04 −3.12 0.12 0.14 79 TW
PWVI SMC F 16.95 0.02 −2.89 0.14 72 Iwanek et al. (2018)
PWVI SMC F 16.95 0.03 −3.03 0.17 0.14 44 TW
PWVI LMC 1O 16.03 0.06 −3.37 0.25 0.14 19 Groenewegen & Jurkovic (2017)
PWVI LMC 1O 16.05 0.05 −3.44 0.22 0.13 10 Ripepi et al. (2014)
PWVI LMC 1O 16.04 0.04 −3.30 0.20 39 Iwanek et al. (2018)
PWVI LMC 1O 16.10 0.03 −2.38 0.03 −3.10 0.21 0.15 32 TW
PWVI SMC 1O 16.55 0.05 −3.69 0.28 39 Iwanek et al. (2018)
PWVI SMC 1O 16.38 0.02 −4.30 0.23 0.10 22 TW
PWVK theory F −1.71−1.83logM −2.93 0.04 Marconi et al. (2004)
PWVK LMC F 16.58 0.02 −3.58 0.15 0.10 32 Ripepi et al. (2014)
PWVK LMC F 16.54 0.02 −1.94 0.04 −3.17 0.12 0.14 75 TW
PWVK LMC 1O 15.93 0.07 −4.14 0.33 0.10 10 Ripepi et al. (2014)
PWVK LMC 1O 15.99 0.03 −2.49 0.04 −3.42 0.20 0.14 33 TW

Notes. The different columns report (1) the type of relationship and the band of interest; (2) the galaxy or the theory where the relation was tested; (3) the pulsating mode; (4)–(5) the α coefficient (relative intercept) and relative uncertainty; (6)–(7) the α0 coefficient (absolute intercept) and relative uncertainty; (8)–(9) the β coefficient (slope) and relative uncertainty; (10) the root mean square (RMS) of the relation; (11) the number of stars used in the fit; (12) the authors. The term “TW” (gray shading) refers to “this work”.

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