Data for: Synthetic red supergiant explosion model grid for systematic characterization of Type II supernovae

This model grid contains 228,016 synthetic red supergiant explosion (Type
II supernova) models. Time evolution of spectral energy distributions from
1 Angstrom to 50,000 Angstrom (100 frequency bins in a log scale) up to
500 days after explosion is computed in each model. We provide light
curves for the filters of the Vera C. Rubin Observatory's Legacy
Survey of Space and Time (LSST), Zwicky Transient Facility (ZTF), Sloan
Digital Sky Servey (SDSS), and the Neil Gehrels Swift Observatory, but
light curves for any photometric filters with any extinctions at any
redshifts can be constructed based on the synthetic spectral energy
distributions. We also provide bolometric light curves and photosphere
information such as photospheric velocity evolution. The parameter space
covered by the model grid is five progenitor masses (10, 12, 14, 16, and
18 solar mass at the zero-age main sequence, solar metallicity), ten
explosion energies (0.5e51, 1.0e51, 1.5e51, 2.0e51, 2.5e51, 3.0e51,
3.5e51, 4.0e51, 4.5e51, and 5.0e51 erg), nine 56Ni masses (0.001, 0.01,
0.02, 0.04, 0.06, 0.08, 0.1, 0.2, and 0.3 solar mass), nine mass-loss
rates (10^-5.0, 10^-4.5, 10^-4.0, 10^-3.5, 10^-3.0, 10^-2.5, 10^-2.0,
10^-1.5, and 10^-1.0 Msun/yr with a wind velocity of 10 km/s), six
circumstellar matter radii (1e14, 2e14, 4e14, 6e14, 8e14, and 1e15 cm),
and ten circumstellar structures (beta = 0.5, 1.0, 1.5, 2.0, 2.5, 3.0,
3.5, 4.0, 4.5, and 5.0). 56Ni is assumed to be uniformly mixed up to the
half mass of a hydrogen-rich envelope.