O'Brien, John
Kerzendorf, Wolfgang
Fullard, Andrew
Williamson, Marc
Pakmor, Reudiger
Buchner, Johannes
Hachinger, Stephann
Vogl, Christian
Gillanders, James
Floers, Andreas
van der Smagt, Patrick
2021-06-21
<p><strong>SN2002bo_emulator_paper_data</strong></p>
<ul>
<li>The TARDIS configuration YAML file used as a template for the training spectra.</li>
<li>HDF5 file of posterior samples of model parameters and their associated weights from the nested sampler.</li>
</ul>
<p><strong>SN2002bo_emulator_paper_spectra</strong></p>
<ul>
<li>Input grid of model parameters and corresponding spectra produced by TARDIS used to generate the training grid of the emulator.</li>
</ul>
For further questions, please contact John O'Brien at obrie278@msu.edu
https://doi.org/10.5281/zenodo.5007378
oai:zenodo.org:5007378
eng
Zenodo
https://zenodo.org/communities/aas
https://doi.org/10.5281/zenodo.5007377
info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
radiative transfer
machine learning
spectroscopic analysis
Type Ia Supernova
SN2002bo
Probabilistic Reconstruction of Type Ia Supernova SN 2002bo
info:eu-repo/semantics/other