Versatile light curve templates of Cepheids - Multi-band fitting of photometric time series

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Volume 698 (May 2025)

A&A, 698 (2025) A97

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Table 3.

Distribution of mean magnitudes errors in HST filters for the different samples (see also Fig. 15).

	F555W		F814W		F160W		W_H

	$\bar{Δ ⟨ m_{λ} ⟩}$ $\overline{\Delta \langle m_\lambda \rangle}$	σ_{Δ⟨m_λ⟩}	$\bar{Δ ⟨ m_{λ} ⟩}$ $\overline{\Delta \langle m_\lambda \rangle}$	σ_{Δ⟨m_λ⟩}	$\bar{Δ ⟨ m_{λ} ⟩}$ $\overline{\Delta \langle m_\lambda \rangle}$	σ_{Δ⟨m_λ⟩}	$\bar{Δ ⟨ m_{λ} ⟩}$ $\overline{\Delta \langle m_\lambda \rangle}$	σ_{Δ⟨m_λ⟩}
Gold	0.070	0.054	0.014	0.043	−0.031	0.043	−0.014	0.052
Silver	0.044	0.055	0.004	0.049	−0.062	0.021	−0.041	0.030
Bronze	0.044	0.053	0.006	0.037	−0.036	0.058	−0.058	0.065
Bronze+	0.063	0.080	0.017	0.057	−0.030	0.079	−0.054	0.083
Total	0.056	0.056	0.010	0.043	−0.039	0.047	−0.034	0.057
Total+	0.063	0.068	0.014	0.051	−0.035	0.062	−0.037	0.068

Notes. The ‘+’ indicates selections where the stars with no NIR photometry were included (excluded otherwise).

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