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A python module used to model the shock cooling emission from a double-peaked core collapse supernova.

Project description

shock-cooling-curve

INTRODUCTION

This package can be used to fit double-peaked supernova light curves using the following shock cooling emission models:

  1. PIRO 2015

  2. Sapir-Waxman 2017

    A) For a blue supergiant (n = 3)

    B) For a red supergiant (n = 3/2)

  3. PIRO 2020

Using this package

There are two files that have to be prepared before using this package.

  1. The config file: A template for this file in provided under templates/config_template.ini. Simply make a copy of the file and fill out all the entries in the DEFAULT section. The BOUNDS section is optional.

  2. The data file: This file containing the photometry data must be a csv. The column headers and template is under templates/phot_template.csv.

Related Papers: The Circumstellar Environments of Double-Peaked, Calcium-strong Supernovae 2021gno and 2021inl

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