Synthetic observables from tECSN models show slower early red-color decline due to higher Ti/Cr and a late-time 12.8 μm Ne II line that strengthens over time, unlike comparable CO deflagration models.
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slicersim is a modular Python tool that simulates IFS observations including noise and instrumental effects, demonstrating that the Lazuli Space Observatory could observe 8000 SNe Ia (z=0–1.5) at S/N=25 per resolution element in 1.5 years of on-sky time.
Pantheon+ releases 1701 light curves from 1550 spectroscopically confirmed Type Ia supernovae across 18 surveys for cosmological inference.
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Observational signatures of thermonuclear electron-capture supernovae -- Ne II line strengthening and color evolution as traces of the explosion mechanism
Synthetic observables from tECSN models show slower early red-color decline due to higher Ti/Cr and a late-time 12.8 μm Ne II line that strengthens over time, unlike comparable CO deflagration models.
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slicersim: A python package to simulate image slicer spectroscopic observations -- application to the Lazuli Spectrograph
slicersim is a modular Python tool that simulates IFS observations including noise and instrumental effects, demonstrating that the Lazuli Space Observatory could observe 8000 SNe Ia (z=0–1.5) at S/N=25 per resolution element in 1.5 years of on-sky time.
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The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
Pantheon+ releases 1701 light curves from 1550 spectroscopically confirmed Type Ia supernovae across 18 surveys for cosmological inference.