Skip to main content

My code For Use with Supernova Spectropolarimetry

Project description

# For Use with Supernova Spectropolarimetry (FUSS)

[![astropy](http://img.shields.io/badge/powered%20by-AstroPy-orange.svg?style=flat)](http://www.astropy.org/) [![DOI](https://zenodo.org/badge/79924113.svg)](https://zenodo.org/badge/latestdoi/79924113)

Our code For Use with Supernova Spectropolarimetry was used to reduce and analyse the data for our paper on SN 2014ad, see https://arxiv.org/pdf/1704.06270.pdf.

If you want to use our code, or part of our code, we would be grateful if you could cite the aforementioned publication.

For documentation, see our wiki, or the pdf in the docs/FUSS folder.

## Installation ### Python pip install fussy

### IRAF scripts

Create tasks in your login.cl file for the .cl scripts (not the python scripts!) located in FUSS/iraf_scripts

e.g. task $ascii_f = [path_to_iraf_scripts]$toascii_flux.cl

You will also have to edit the path to the python scripts in arc_apertures.cl, create_id.cl, toascii_flux.cl and toascii_pol.cl manually to fit the location of your iraf_scripts folder.

## Licensed

This project is Copyright (c) H. F. Stevance and licensed under the terms of the MIT license. See the licenses folder for more information.

Project details


Download files

Download the file for your platform. If you're not sure which to choose, learn more about installing packages.

Filename, size & hash SHA256 hash help File type Python version Upload date
fusspy-2.0.0.tar.gz (467.7 kB) Copy SHA256 hash SHA256 Source None Jun 20, 2018

Supported by

Elastic Elastic Search Pingdom Pingdom Monitoring Google Google BigQuery Sentry Sentry Error logging AWS AWS Cloud computing DataDog DataDog Monitoring Fastly Fastly CDN SignalFx SignalFx Supporter DigiCert DigiCert EV certificate StatusPage StatusPage Status page