Top row. Evolution of m(b, z) from Eq. A.1 as a function of the redshift to estimate the TIR luminosity from the main WISE, Spitzer, Herschel, and JWST bands. Bottom row. Standard deviation of the residual of the TIR luminosity estimated from Eq. A.1. Fewer bands are available at higher redshifts as the computation is only carried out for λ/(1 + z) > 6 μm, with λ the pivot wavelength of the filter.