Based on Yunnan-II-BaSeL (models with and without BIs) and Yunnan-II-BaSeL-sdB (models with BIs) models, we present the stellar (Fste), nebular (Fneb), total (Ftot) spectra, luminosities of spectral lines (LHα, LHβ) and the number of ionizing photons Q(H) for CSP+nebula systems, these CSPs include E, S0, Sa-Sd and Irr galaxies and five galaxies with short e-folding timescales (from τ = 0.1 to 0.9Gyr). Age (90): from 1.e+6 to 1.5e+10 yr. Metallicity (7): from 1.e-4 to 0.03.

For the data of E, S0, Sa-Sd and Irr galaxies based on Yunnan-II-BaseL modes, those at solar metallicity have even been used in our papers (2012.MNRAS.421.743), and those at non-solar metallicity will be used in future paper (2013.MNRAS, in preparation).