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Iron Project: atomic data for IR lines

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TLDR
A compilation of calculations of A-values and electron impact collision strengths for infrared transitions which will become useful in the spectral modelling of planetary nebulae is included.
Abstract
The Iron Project is an international consortium dedicated to the computation of atomic data for astrophysical applications. Although the project has been mainly concerned with ions in the iron group, the earlier papers gave priority to calculations of A-values and electron impact collision strengths for infrared transitions. In the present report we include a compilation of these data which will become useful in the spectral modelling of planetary nebulae. © 2006 International Astronomical Union.

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Milky Way and Magellanic Cloud Surveys for Planetary Nebulae

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Near-infrared studies of nova V1674 Herculis: A shocking record-breaker

TL;DR: In this article, the authors present near infrared spectroscopy of Nova Herculis 2021 (V1674 Her), obtained over the first 70 days of its evolution, and show that the vexing problem of whether collisional or photoionization is responsible for coronal emission in classical novae can be resolved by correlating the temporal sequence in which the X-ray supersoft phase and the near-infrared coronal line emission appear.
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Atomic Databases: Four of a Kind

Claudio Mendoza
- 19 Jun 2020 - 
TL;DR: AtomPy is a prototype for an open, distributed data-assessment environment to engage both producers and users and design strategies and implementation issues that may help in the undertaking of present and future scientific database projects are discussed.
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