| Publication |
New Fe I Level Energies and Line Identifications from Stellar Spectra. III. Initial Results from UV, Optical, and Infrared Spectra, Peterson, Ruth C.,Kurucz, Robert L., The Astrophysical Journal Supplement Series, 260, 2022-06-01 00:00:00, 2022ApJS..260...28P||Origins of Type Ibn SNe 2006jc/2015G in interacting binaries and implications for pre-SN eruptions, Sun, Ning-Chen,Maund, Justyn,Hirai, Ryosuke, Monthly Notices of the Royal Astronomical Society, 491, 2020-02-01 00:00:00, 2020MNRAS.491.6000S||The Candidate Progenitor Companion Star of the Type Ib/c SN 2013ge, Fox, Ori D.,Van Dyk, Schuyler D.,Williams, Benjamin F., The Astrophysical Journal, 929, 2022-04-01 00:00:00, 2022ApJ...929L..15F||The changing-type SN 2014C may come from an 11-M⊙ star stripped by binary interaction and violent eruption, Sun, Ning-Chen,Maund, Justyn,Crowther, Paul A., Monthly Notices of the Royal Astronomical Society, 497, 2020-08-01 00:00:00, 2020MNRAS.497.5118S||The interacting nature of dwarf galaxies hosting superluminous supernovae, Ørum, Simon Vanggaard,Ivens, David Lykke,Strandberg, Patrick, Astronomy and Astrophysics, 643, 2020-11-01 00:00:00, 2020A&A...643A..47O |
