This is the code associated with The Cannon, a data-driven method for determining stellar labels (physical parameters and chemical abundances) from stellar spectra in the context of large spectroscopic surveys. It closely follows the method outlined in Ness et al. 2015, although some minor changes have been made. A description of these changes is outlined in Ho et al. 2016.
Documentation for The Cannon can be found here.
- Anna Ho (MPIA)
- Melissa Ness (MPIA)
- David W. Hogg (NYU CCPP)(MPIA)
- Hans-Walter Rix (MPIA)
Copyright 2015 the authors. TheCannon is open-source software released under
the MIT License. See the file LICENSE for details.
A condition on using this code for any academic purpose is citation of Ness et al. 2015 (arXiv:1501.07604) and Ho et al. 2016 (arXiv:1602.00303).
- Survey Cross-Calibration with The Cannon: Apogee-scale Stellar Labels from Lamost Spectra