A database of spectral energy distributions of progenitors of core-collapse supernovae*

This paper presents a database of the spectroscopic- and photometric- spectral energy distributions (spec-SEDs phot-SEDs) progenitors core-collapse supernovae (CCSNe). Both binary- single-star are included in database. The covers initial metallicity ($Z$) range 0.0001--0.03, mass 8--25 \dsm{}, binary ratio 0--1, orbital period 0.1--10000\,days. low-resolution spec-SEDs phot-SEDs single- binary-star CCSN These data can be used for studying basic parameters, e.g., metallicity, age, final masses progenitors. It also effects different factors on determination parameters When is fitting SEDs progenitors, it strongly suggested to determine advance, while not necessary