ycamacho/SN-2014dt-TARDIS: zenodo.v1.0.0

integration_instructionsResearch softwarekeyboard_double_arrow_right Software 17 Apr 2023Publisher:ZenodoFunded by:NSF | CAREER: Supernova Cosmolo..., NSF | Graduate Research Fellows..., NSF | Revealing Supernova Proge...

Authors: Yssavo Camacho-Neves;

doi: 10.5281/zenodo.7838689 , 10.5281/zenodo.7838690

ycamacho/SN-2014dt-TARDIS: zenodo.v1.0.0

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Abstract

First release The input and output files used to model the spectra of Supernova 2014dt using the radiative transfer code TARDIS in Camacho-Neves et al. 2023. Each input file has a corresponding output file with a nearly identical name. The input files (TARDIS input file) are in the folder input_yml_files and are named as "UT-date_phase_telescope_model.yml". The output files (synthetic spectra) are in the folder output_synthetic_spectra and are named as "UT-date_phase_telescope_model_spec.dat". Each output file is a two-column text file with wavelength (Angstrom) and luminosity (erg/s/Angstrom).

Related Organizations

Rutgers, The State University of New Jersey
United States

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