M08_03_neg_z_1D_no_He

Optical and NIR spectral time series file format: Table with 1+n columns and 1+m lines specifying the spectral time series for n epochs on m wavelength bins. -The first line defines the time of the n epochs for which spectra have been calculated (time in days relative to B-band peak which occurs at 16.8 days after explosion, the first 0.00 is a dummy value). -The following m lines contain the fluxes for the various time steps for a given wavelength bin. The first column gives the wavelength in A, followed by n columns giving the fluxes (in units of erg/cm^2/s/A assuming a distance of 1 MPc). Comparing this model (M08_03_neg_z_1D_no_He) with the full model spectra series (M08_03_neg_z_1D) illustrates the impact of He absorption in the simulation. The spectral series is made up of all the spectra which appear for this model in Callan et al. (2025) Figures 2, 3 and A1.

This file is part of the M08_03_neg_z_1D_no_He model.