“…The absorption spectra encompass contributions of all chromophores in these complexes, namely Chls a (B xy ~435 nm, Q x ~ 625 nm, Q y ~ 668-672 nm), Pheos a (B xy ~ 416 nm, Q x ~ 540 nm, Q y ~ 669-681 nm) and b-Cars (~450-500 nm). Characteristic is the Soret (B xy ) absorption maximum of PSII RC at 416 nm (because of the higher Pheo a proportion; Tomo et al, 2008) and the higher energy Q y band of CP43 (668 nm; Alfonso et al, 1994;Dekker et al, 1995;Groot et al, 1999) relative to those in CP47 (671 nm;Alfonso et al, 1994;Chang et al,1994;Dekker et al, 1995;Groot et al, 1995) and in D1D2 (672 nm; Konermann and Holzwarth, 1996). At cryogenic temperatures, absorption bands become sharper and may split into two peaks.…”