Comparison of STIS and FUSE observations around H i L α–δ with our final model. Thick (red in the online version) photospheric + ISM line absorption model with N_H   i = 2.2 × 10¹⁸   cm^-2; thin (blue) pure photospheric model; dashed (green, L α only) N_H   i = 1.2 × 10¹⁸   cm^-2, 3.2 × 10¹⁸   cm^-2. The locations of the D i blends are marked. L β–δ are shifted in flux (0.7, 1.6, 2.7 × 10^-11   erg   cm^-2   s^-1  Å^-1) for clarity. A reddening of E_B − V = 0.0005 is applied following the law of Fitzpatrick (1999, with R_V = 3.1.