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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
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Abstract

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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 We are also updating the supporting atomic data where they have been superseded by superior calculations or measurements.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

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