Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-25T15:54:50.960Z Has data issue: false hasContentIssue false

PyNeb: a new software for the analysis of emission lines

Published online by Cambridge University Press:  30 August 2012

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: [email protected]; [email protected]; [email protected]
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 We are also updating the supporting atomic data where they have been superseded by superior calculations or measurements.

Type
Contributed Papers
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