All Tables

Table 1: Principle properties of the sample of 68 galaxies used in this study, ordered by increasing RA (see text).
Table 2: Fits to the local and distant K-band TFRs, using $M_K({\rm AB})=a+b\times \log{(V_{\rm flat})}$ .
Table A.1: Fits to the local and distant smTFRs, using $\log{(M_{\rm stellar}/M_\odot)}=a+b\times\log{(V_{\rm flat})}$ .
Table A.2: Identified systematic uncertainties that could impact the shift of zero point between the local and the distant smTFRs. Systematic uncertainties on $V_{\rm flat}$ have been converted into $M_{\rm stellar}$ using Eq. (A.1). Negative values tend to reduce the shift of zero point, while positive values have the opposite trend.