Hostname: page-component-8448b6f56d-xtgtn Total loading time: 0 Render date: 2024-04-24T08:35:44.776Z Has data issue: false hasContentIssue false
  • English
  • Français

PyNeb: a new software for the analysis of emission lines

Published online by Cambridge University Press:  30 August 2012

Valentina Luridiana ,
Christophe Morisset  and
Richard A. Shaw
Valentina Luridiana
Affiliation:
Instituto de Astrofísica de Canarias, Vía Láctea s/n, La Laguna, E-38205, Spain Departamento de Astrofísica, Universidad de La Laguna, La Laguna, E-38205, Spain
Christophe Morisset
Affiliation:
Instituto de Astrofísica de Canarias, Vía Láctea s/n, La Laguna, E-38205, Spain Instituto de Astronomía, UNAM, Apartado Postal 70 - 264, México, D.F., 04510, Mexico
Richard A. Shaw
Affiliation:
NOAO, Tucson, AZ 85719, USA email: vale@iac.es; chris.morisset@gmail.com; shaw@noao.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We describe an ongoing project to migrate the emission-line analysis package nebular from its current environment, IRAF, to a modern programming environment where it can be used from command line, a local GUI, or the web. We are also updating the supporting atomic data where they have been superseded by superior calculations or measurements.

Keywords

Atomic dataISM: abundancesmethods: data analysis
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 422 - 423
Copyright
Copyright © International Astronomical Union 2012

References

Shaw, R. A., et al. 1998, in Albrecht, R. et al. , (Eds.), ADASS VII ASP Conf. Ser., 192, 145 Google Scholar
Shaw, R. A. & Dufour, R. J. 1995, PASP, 107, 896 CrossRefGoogle Scholar