E_p–E_γ,iso plane for NDAF ﹩\nu \bar{\nu }﹩-annihilation jets. The colored sequences show the model tracks of ﹩\nu \bar{\nu }﹩-annihilation-powered baryonic jets in the dissipative-photosphere scenario. The different marker shapes indicate different initial black hole spin a_BH,0, while the color bar represents the accretion rate ﹩{\dot{m}}_{{\rm{acc}}}﹩. The calculation adopts η_γ = ϵ_ph = 0.03, f_± = 1, ϵ_P = 1, ϵ_W = 0.5, ﹩{{\rm{\Gamma }}}_{{\rm{P}}}={\rm{\max }}(\eta /2,1)﹩, and Γ_W = η.