r10_d4.0_Z_R_const_rad

Based on the r10_d4.0_Z pure deflagration model of Lach et al. (2022) but with treatment for a luminous central remnant included in the radiative transfer. The remnant has a temperature evolution consistent with a black body with a constant radius of 4.9x10^14 cm (which yields a temperature of 8000 K at 30 days after explosion). This model adopts a 56Ni mass of 0.054 Msun (the entire remnant 56Ni mass predicted by the Lach et al. 2022 hydrodynamic explosion simulations).

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r10_d4.0_Z_R_const_rad angle averaged light curves

  • Description: Light curve file format: Table with 15 columns. The first column gives the time since explosion in days, the second column gives the absolute bolometric magnitude and the remaining columns give the absolute magnitudes for the bands specified in the header line.
  • Date uploaded: April 9, 2024, 11:47 a.m.
    • r10_d4.0_Z_R_const_rad angle averaged light curves
    Interactive plot Download lightcurve file

    r10_d4.0_Z_R_const_rad angle averaged optical spectral time-series

  • Description: Optical spectral time-series file format: Table with 1+n columns and 1+m lines specifying the optical 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 since 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 10pc).
  • Date uploaded: April 9, 2024, 11:48 a.m.
    • r10_d4.0_Z_R_const_rad angle averaged optical spectral time-series
    Interactive plot Download spectrum file