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Utilities for data taken with the Cosmic Origins Spectrograph on the Hubble Space Telescope

Project description

This package contains code useful for analysis of far-UV spectra taken with the Cosmic Origins Spectrograph (COS) on the Hubble Space Telescope. It allows fast convolution of synthetic spectra with the non-gaussian COS line spread function for the G130M, G160M and all near UV gratings. There are utilities for generating a wavelength-dependent line spread function for use with VPFIT, for reading and writing CalCOS pipeline output, and for estimating the significance of absorption features in reduced COS spectra. There is also a co-addition routine for combining COS spectra from multiple settings, and a script for running the CalCOS pipeline.

To install, download the tarball from the pypi website and then do:

python install

This package can also be easily installed using pip:

pip install COS

Project details

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Files for COS, version 0.1.1
Filename, size File type Python version Upload date Hashes
Filename, size COS-0.1.1-py2.7-macosx-10.6-x86_64.egg (239.8 kB) File type Egg Python version 2.7 Upload date Hashes View
Filename, size COS-0.1.1.tar.gz (98.0 kB) File type Source Python version None Upload date Hashes View

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