activity
20012023
most citedPyNeb: a new tool for analyzing emission lines. I. Code description and validation of results

664 citations · 2.3k across the 62 of their papers we have counts for

collaborators

61 papers

astro-ph.GA2023

On the origin of optical and IR emission lines in star forming galaxies

Mariela Martínez-Paredes, Gustavo Bruzual, Christophe Morisset +3

Combining the {\sc Cloudy} photoionization code with updated stellar population synthesis results, we simultaneously model the MIR $\neiii/\neii$ vs. $\oiv/\neiii$, the MIR-FIR $\n…

astro-ph.GA2023

A Machine Learning Approach to Galactic Emission-Line Region Classification

Carter Lee Rhea, Laurie Rousseau-Nepton, Ismael Moumen +13

Diagnostic diagrams of emission-line ratios have been used extensively to categorize extragalactic emission regions; however, these diagnostics are occasionally at odds with each o…

astro-ph.GA2023★ 18 cited

Atomic Data Assessment with PyNeb: Radiative and Electron Impact Excitation Rates for [Fe II] and [Fe III]

Claudio Mendoza, José E. Méndez-Delgado, Manuel Bautista +2

We use the PyNeb 1.1.16 Python package to evaluate the atomic datasets available for the spectral modeling of [Fe II] and [Fe III], which list level energies, A-values, and effecti…

astro-ph.GA2023★ 5 cited

On the computation of interstellar extinction in photoionized nebulae

Christophe Morisset, Romano L. M. Corradi, Jorge García-Rojas +5

Ueta & Otsuka (2021) proposed a method, named as the "Proper Plasma Analysis Practice", to analyze spectroscopic data of ionized nebulae. The method is based on a coherent and simu…

astro-ph.SR2023★ 2 cited

Shock shaping? Nebular Spectroscopy of Nova V906 Carinae

É. J. Harvey, E. Aydi, L. Izzo +7

V906 Carinae was one of the best observed novae of recent times. It was a prolific dust producer and harboured shocks in the early evolving ejecta outflow. Here, we take a close lo…

astro-ph.GA2023

The planetary nebula NGC 6153 through the eyes of MUSE

V. Gómez-Llanos, J. García-Rojas, C. Morisset +7

In this contribution, we present the results of a study on the high abundance discrepancy factor (ADF 10) planetary nebula (PN) NGC 6153 with MUSE. We have constructed flux…