| Publication |
A cool and inflated progenitor candidate for the Type Ib supernova 2019yvr at 2.6 yr before explosion, Kilpatrick, Charles D.,Drout, Maria R.,Auchettl, Katie, Monthly Notices of the Royal Astronomical Society, 504, 2021-06-01 00:00:00, 2021MNRAS.504.2073K||An environmental analysis of the Type Ib SN 2019yvr and the possible presence of an inflated binary companion, Sun, Ning-Chen,Maund, Justyn,Crowther, Paul A., Monthly Notices of the Royal Astronomical Society, 510, 2022-03-01 00:00:00, 2022MNRAS.510.3701S||How much hydrogen is in Type Ib and IIb supernova progenitors?, Gilkis, Avishai,Arcavi, Iair, Monthly Notices of the Royal Astronomical Society, 511, 2022-03-01 00:00:00, 2022MNRAS.511..691G||Late-time Observations of ASASSN-14lp Strengthen the Case for a Correlation between the Peak Luminosity of Type Ia Supernovae and the Shape of Their Late-time Light Curves, Graur, Or,Zurek, David R.,Cara, Mihai, The Astrophysical Journal, 866, 2018-10-01 00:00:00, 2018ApJ...866...10G||Late-time Observations of the Type Ia Supernova SN 2014J with the Hubble Space Telescope Wide Field Camera 3, Graur, Or, The Astrophysical Journal, 870, 2019-01-01 00:00:00, 2019ApJ...870...14G||Observations of SN 2015F Suggest a Correlation between the Intrinsic Luminosity of Type Ia Supernovae and the Shape of Their Light Curves >900 Days after Explosion, Graur, Or,Zurek, David R.,Rest, Armin, The Astrophysical Journal, 859, 2018-06-01 00:00:00, 2018ApJ...859...79G||Progenitor, environment, and modelling of the interacting transient AT 2016jbu (Gaia16cfr), Brennan, S. J.,Fraser, M.,Johansson, Joel, Monthly Notices of the Royal Astronomical Society, 513, 2022-07-01 00:00:00, 2022MNRAS.513.5666B |
