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Data-driven stellar parameters and abundances from spectra

Project Description

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 (arXiv:1602.00303).

Documentation for The Cannon can be found here.

Authors

  • Anna Ho (MPIA)
  • Melissa Ness (MPIA)
  • David W. Hogg (SCDA NYU MPIA)
  • Hans-Walter Rix (MPIA)

License and Citation

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).

Projects

  • Label Transfer from APOGEE to LAMOST: Precise Stellar Parameters for 450,000 LAMOST Giants
  • Masses and Ages for 230,000 LAMOST Giants, via Their Carbon and Nitrogen Abundances
Release History

Release History

This version
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0.7.0

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0.6.9

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0.6.8

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0.6.7

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0.6.6

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0.6.5

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0.6.3

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0.6.2

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0.6.1

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0.6.0

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0.5.9

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0.5.8

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0.5.7

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0.5.0

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0.4.9

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0.3.9

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0.3.0

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0.2.9

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0.1

Download Files

Download Files

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File Name & Checksum SHA256 Checksum Help Version File Type Upload Date
TheCannon-0.7.0.tar.gz (50.4 kB) Copy SHA256 Checksum SHA256 Source May 21, 2017

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