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This article has an erratum: [https://doi.org/10.1051/0004-6361/202554679e]


Fig. A.1.

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Model specific intensities fλ (in Equation (3)) observed at Earth from RSGs (a) and BSGs (b) located at z = 0.03 hosted in a galaxy with extinction value EB − V (median value from Figure 1). Blue, green, and orange shaded regions show results for explosion energy E = 1051 erg, E = 1052 erg, and E = 1053 erg, respectively. (a) RSG progenitor: by fixing the ejected mass at Mej = 2.8 M (fiducial parameter), the shaded regions reflect the variation of the progenitor radius between 200 and 1500 R. (b) BSG progenitor: by fixing the ejected mass at Mej = 10 M (fiducial parameter), the shaded regions reflect the variation of the progenitor radius between 10 and 50 R. f λ lim $ f_{\lambda}^{\mathrm{lim}} $ of ULTRASAT and ZTF in their observational wavelength bands, obtained following Equation (7), are indicated with the grey and black dashed horizontal lines, respectively.

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