PySpecKit: Python Spectroscopic Toolkit

Details PySpecKit: Python Spectroscopic Toolkit PySpecKit: Python Spectroscopic Toolkit

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ascl.soft09001g&link_type=abstract

Astrophysics Source Code Library, record ascl:1109.001

Astronomy and Astrophysics

Astrophysics

Scientific paper

PySpecKit is a Python spectroscopic analysis and reduction toolkit meant to be generally applicable to optical, infrared, and radio spectra. It is capable of reading FITS-standard and many non-standard file types including CLASS spectra. It contains procedures for line fitting including gaussian and voigt profile fitters, and baseline-subtraction routines. It is capable of more advanced line fitting using arbitrary model grids. Fitting can be done both in batch mode and interactively. PySpecKit also produces publication-quality plots with TeX axis labels and annotations. It is designed to be extensible, allowing user-written reader, writer, and fitting routines to be "plugged in." It is actively under development and currently in the 'alpha' phase, with plans for a beta release.

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