Deriving the Lyα flux of LTT 1445A using a reconstruction from the wings of the Lyα profile observed with the STIS/G140M grating (orange 1σ band; Youngblood et al. 2016) and using UV-UV line correlations with other measured UV lines with the COS instrument (orange points with 1σ errors, and the average 1 σ gray band; Youngblood et al. 2017; Diamond-Lowe et al. 2021, 2022). In the case of LTT 1445A, we find that individual transition region lines agree with each other, and with the reconstructed value.