Corrigendum: Improved He~I Emissivities in the Case B Approximation
R. L. Porter, G. J. Ferland, P. J. Storey, M. J. Detisch
TL;DR
This paper corrects previous errors in He I emissivity calculations under the Case B approximation, providing updated and more accurate emissivity values for astrophysical applications.
Contribution
It identifies and rectifies errors in prior He I emissivity calculations, offering revised data for improved astrophysical modeling.
Findings
Corrected He I emissivity values are presented.
Previous calculations contained errors that affected astrophysical interpretations.
Updated emissivities enhance the accuracy of nebular diagnostics.
Abstract
Errors were discovered in our recent calculations of HeI emissivities (Porter et al. 2012; arXiv:1206.4115). This corrigendum discusses the errors and reports corrected emissivities.
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