The VMC survey - L. Type II Cepheids in the Magellanic Clouds: Period–luminosity relations in the near-infrared bands

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Table 12.

As in Table 10, but for the SMC.

Relation	Galaxy	Sample	α	σ_α	β	σ_β	RMS	#star	Reference
			(mag)	(mag)	(mag dex⁻¹)	(mag dex⁻¹)	(mag)
PLJ	SMC	BLHer+WVir	18.070	0.116	−2.147	0.154	0.34	25	M11
PLJ+	SMC	BLHer+WVir	17.993	0.092	−2.092	0.116	0.33	47	M11
PLJ	SMC	BLHer+WVir	18.202	0.044	−2.280	0.100	0.17	28	TW
PLK_s	SMC	BLHer+WVir	17.5874	0.109	−2.082	0.151	0.32	23	M11
PLK_s+	SMC	BLHer+WVir	17.5966	0.082	−2.113	0.105	0.29	45	M11
PLK_s	SMC	BLHer+WVir	17.927	0.024	−2.396	0.053	0.12	25	TW
PWVI	SMC	BLHer+WVir	17.554	0.083	−2.304	0.107	0.23	27	M11
PWVI	SMC	BLHer	17.630	0.104	−2.753	0.403		20	I18
PWVI	SMC	WVir	17.976	0.164	−2.688	0.156		15	I18
PWVI	SMC	BLHer+WVir	17.592	0.033	−2.351	0.074	0.19	34	TW

Notes. “M11” refers to Matsunaga et al. (2011), “I18” refers to Iwanek et al. (2018), “TW” (grey line) refers to this work. In M11, J+ and K_s+ refer to the combination of IRSF and NTT data sets.

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