“…1,2,4‐linked Rha p was detected in ASP−I−I, which means that neutral side chains could be attached to O ‐4 of Rha p , such as arabinans (composed of terminal, 1,5‐ and 1,3,5‐linked Ara f ), type II arabinogalactans (AG‐II) (consisting of 1,3‐ and 1,3,6‐Gal p ), or minor amounts of β‐1,4‐galactans (1,4‐linked Gal p ) [33] . Branches at O ‐3 of GalA (1,3,4‐linked Gal p A) might be due to terminal Xyl p or methyl‐ or acetyl‐esterification [34] . The HG region in ASP−I−II seems to be longer than in ASP−I−I as it contains around 15 mol % more of 1,4‐linked Gal p A (Table 2), and more terminal Xyl p moieties could be attached to O ‐3 of Gal p A.…”