Input files and simulation results for stellar evolution tracks computed for the paper "How much hydrogen is in Type Ib and IIb supernova progenitors?", as well as synthetic photometry generated and used in the analysis. Version 10398 of MESA was used for the simulations. More details in the README.txt file and in the paper
Linking supernovae to their progenitors is a powerful method for furthering our understanding of the...
We trace the formation and advection of several elements within a cosmological adaptive mesh refinem...
Core-collapse supernovae (CCSNe) are an important part of the stellar evolution of massive stars. Ce...
The inlist files for the paper "The formation of the stripped envelope type IIb Supernova progenit...
Context. The progenitor and explosion properties of type II supernovae (SNe II) are fundamental to u...
Context. The nature of type Ia supernova progenitors is still unclear. The outstanding characterist...
Inlists to reproduce the pre-SN simulations of the paper "Progenitor properties of type II supernova...
Context. The single degenerate model is the most widely accepted progenitor model of type Ia superno...
This is the dataset for the manuscript "Connecting the Light Curves of Type IIP Supernovae to the Pr...
The progenitors of core-collapse supernovae are stars with an initial mass greater than about 8M⊙. U...
The recent discovery of the accelerating expansion of the Universe and thus the existence of dark en...
We investigate the evolution of Type Ib/c supernova (SN Ib/c) progenitors in close binary systems, u...
Massive stars that lose their hydrogen-rich envelope down to a few tenths of a solar mass explode as...
The ever-expanding depth and quality of photometric and spectroscopic observations of stellar popula...
Aims. Our aim is to show how different hypotheses about type Ia supernova progenitors can affect Gal...
Linking supernovae to their progenitors is a powerful method for furthering our understanding of the...
We trace the formation and advection of several elements within a cosmological adaptive mesh refinem...
Core-collapse supernovae (CCSNe) are an important part of the stellar evolution of massive stars. Ce...
The inlist files for the paper "The formation of the stripped envelope type IIb Supernova progenit...
Context. The progenitor and explosion properties of type II supernovae (SNe II) are fundamental to u...
Context. The nature of type Ia supernova progenitors is still unclear. The outstanding characterist...
Inlists to reproduce the pre-SN simulations of the paper "Progenitor properties of type II supernova...
Context. The single degenerate model is the most widely accepted progenitor model of type Ia superno...
This is the dataset for the manuscript "Connecting the Light Curves of Type IIP Supernovae to the Pr...
The progenitors of core-collapse supernovae are stars with an initial mass greater than about 8M⊙. U...
The recent discovery of the accelerating expansion of the Universe and thus the existence of dark en...
We investigate the evolution of Type Ib/c supernova (SN Ib/c) progenitors in close binary systems, u...
Massive stars that lose their hydrogen-rich envelope down to a few tenths of a solar mass explode as...
The ever-expanding depth and quality of photometric and spectroscopic observations of stellar popula...
Aims. Our aim is to show how different hypotheses about type Ia supernova progenitors can affect Gal...
Linking supernovae to their progenitors is a powerful method for furthering our understanding of the...
We trace the formation and advection of several elements within a cosmological adaptive mesh refinem...
Core-collapse supernovae (CCSNe) are an important part of the stellar evolution of massive stars. Ce...
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