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Photoemission spectra of underdoped and lightly-doped BiPbSrCa{\it R}CuO ( Pr, Er) (BSCCO) have been measured and compared with those of LaSrCuO (LSCO). The lower-Hubbard band of the insulating BSCCO, like CaCuOCl, shows a stronger dispersion than LaCuO from ${\bf k}\sim\pi/2,\pi/2\sim\pi,0{\bf k}\sim\pi,0$) is found generally deeper in BSCCO. These observations together with the Fermi-surface shapes and the chemical potential shifts indicate that the next-nearest-neighbor hopping of the single-band model is larger in BSCCO than in LSCO and that rather than the super-exchange influences the pseudogap energy scale.

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