Atomic Data Assessment with PyNeb

• Published in: Atoms 2020-12, Vol.8 (4), p.66
• Main Authors: Morisset, Christophe, Luridiana, Valentina, García-Rojas, Jorge, Gómez-Llanos, Verónica, Bautista, Manuel, Mendoza, Claudio
• Format: Article
• Language: English
• Subjects: astrophysical software; atomic data assessment; atomic databases; Atomic structure; Data analysis; Datasets; Electron density; Electron impact; Energy; Historical structures; Isoelectronic sequence; nebular modeling; Planetary nebulae; Plasma; plasma diagnostics; Position measurement; Temperature; Uncertainty
• ISSN: 2218-2004; 2218-2004
• DOI: 10.3390/atoms8040066

PyNeb is a Python package widely used to model emission lines in gaseous nebulae. We take advantage of its object-oriented architecture, class methods, and historical atomic database to structure a practical environment for atomic data assessment. Our aim is to reduce the uncertainties in the parameter space (line ratio diagnostics, electron density and temperature, and ionic abundances) arising from the underlying atomic data by critically selecting the PyNeb default datasets. We evaluate the questioned radiative-rate accuracy of the collisionally excited forbidden lines of the N- and P-like ions (O ii, Ne iv, S ii, Cl iii, and Ar iv), which are used as density diagnostics. With the aid of observed line ratios in the dense NGC 7027 planetary nebula and careful data analysis, we arrive at emissivity ratio uncertainties from the radiative rates within 10%, a considerable improvement over a previously predicted 50%. We also examine the accuracy of an extensive dataset of electron-impact effective collision strengths for the carbon isoelectronic sequence recently published. By estimating the impact of the new data on the pivotal [N ii] and [O iii] temperature diagnostics and by benchmarking the collision strength with a measured resonance position, we question their usefulness in nebular modeling. We confirm that the effective-collision-strength scatter of selected datasets for these two ions does not lead to uncertainties in the temperature diagnostics larger than 10%.