@article{curtis_wolfe_frohlich_miller_wollaeger_ebinger_2021, title={Core-collapse Supernovae: From Neutrino-driven 1D Explosions to Light Curves and Spectra}, volume={921}, ISSN={["1538-4357"]}, url={http://dx.doi.org/10.3847/1538-4357/ac0dc5}, DOI={10.3847/1538-4357/ac0dc5}, abstractNote={Abstract}, number={2}, journal={ASTROPHYSICAL JOURNAL}, publisher={American Astronomical Society}, author={Curtis, Sanjana and Wolfe, Noah and Frohlich, Carla and Miller, Jonah M. and Wollaeger, Ryan and Ebinger, Kevin}, year={2021}, month={Nov} }
 @article{frohlich_curtis_ebinger_ghosh_menon_heger_perego_thielemann_2019, title={Nucleosynthesis for SN 1987A from single-star and binary-merger progenitors}, volume={46}, ISSN={["1361-6471"]}, url={https://doi.org/10.1088/1361-6471/ab1ff7}, DOI={10.1088/1361-6471/ab1ff7}, abstractNote={We apply the parametrized, spherically symmetric explosion method PUSH to two sets of pre-explosion models suitable for SN 1987A: blue supergiants (BSGs) resulting from the merger of a main sequence star with a giant and red supergiants (RSGs) representing the end point of single-star stellar evolution. For each model, we perform a calibration of the PUSH method to the observational properties of SN 1987A and calculate the detailed explosive nucleosynthesis yields. We find that such a calibration to SN 1987A is only possible for one of the BSG models. We compare the yields from this model with the yields from the best-fit RSG model. The largest differences are found for nuclei in the mass range of 20 ≤ A ≤ 40 which are mostly synthesized pre-explosion. We predict a neutron star with a gravitational mass of 1.48 M ⊙ from the BSG model and a neutron star of 1.41 M ⊙ from the RSG model.}, number={8}, journal={JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS}, author={Frohlich, C. and Curtis, S. and Ebinger, K. and Ghosh, S. and Menon, A. and Heger, A. and Perego, A. and Thielemann, F-K}, year={2019}, month={Aug} }
 @article{ebinger_curtis_froehlich_hempel_perego_liebendoerfer_thielemann_2019, title={PUSHing Core-collapse Supernovae to Explosions in Spherical Symmetry. II. Explodability and Remnant Properties}, volume={870}, ISSN={["1538-4357"]}, url={https://doi.org/10.3847/1538-4357/aae7c9}, DOI={10.3847/1538-4357/aae7c9}, abstractNote={Abstract}, number={1}, journal={ASTROPHYSICAL JOURNAL}, author={Ebinger, Kevin and Curtis, Sanjana and Froehlich, Carla and Hempel, Matthias and Perego, Albino and Liebendoerfer, Matthias and Thielemann, Friedrich-Karl}, year={2019}, month={Jan} }