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arXiv · 1909.09022

SNIF: The SuperNova Interactive Fitter

Leilani Baker·Sophia Green·V. Ashley Villar
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Abstract

We present an online application, the SuperNova Interactive Fitter (SNIF), which can be used to interactively fit one-zone, analytical models to optical transient light curves powered by (1) the radioactive decay of 56Ni, (2) the spin-down of newly born magnetars, or (3) the interaction between supernova ejecta and pre-existing circumstellar material. This application utilizes the Open Astronomy Catalogs API to connect the user to thousands of publicly available transient light curves from the literature.

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Leilani Baker, Sophia Green, V. Ashley Villar. 2019-09-18. SNIF: The SuperNova Interactive Fitter. https://arxiv.org/abs/1909.09022

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