  Using EPS we present 13 refined Lick/IDS absorption-line indices for an
extensive set of instantaneous-burst binary stellar populations (BSPs) at high
resolution (0.3 \AA) of various age and metallicity (1-15Gyr, 0.004-0.03), and
38 indices at intermediate resolution (3 \AA). These indices are obtained by
two methods: (1) obtain them by using the empirical fitting functions (FFs
method); (2) measure them directly from the synthetic spectra (DC method).
Together with our previous paper a database of Lick/IDS spectral
absorption-line indices for BSPs at high and intermediate resolutions is
provided. This set of indices includes 21 indices of Worthey et al., four
Balmer indices defined by Worthey & Ottaviani and 13 indices with the new
passband definitions of Trager et al. The full set of synthetic indices and the
integrated pseudo-continuum are listed in the Appendix, which is only available
online or from our website (http://www.ast9. com/), or on request from the
first author. Moreover, the ISEDs can be obtained from our website.
  We compare the synthetic Lick/IDS indices obtained by FFs method and those by
DC method, and find that the discrepancies are significant: Ca4455 (index 6),
Fe4668 (8), Mg_b (13), Fe5709 (17), NaD (19), TiO_1 (20) and TiO_2 (21, except
for Z=0.02) in the W94 system, Ca4455^T (6^T), C_2 4668^T (8^T), NaD^T (19^T),
TiO_1^T (20^T) and TiO_2^T (21^T, except for Z=0.02) in the T98 system obtained
by DC method are less (bluer) than the corresponding ones obtained by FFs
method for all metallicities. Ca4227 (index 3), Fe5782 (18),Ca4227^T (3^T) and
Fe5782^T (18^T) are greater at Z=0.03 and become to be bluer at Z=0.004,
Fe5709^T (17^T) index is less at Z=0.03 and becomes to be redder at Z=0.004
than the corresponding ones obtained by FFs method.
