Atomic data needs for the modelling of stellar spectra

2015/09/30 by Monier, R.
#FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Solar and Stellar Astrophysics (astro-ph.SR)

paper · doi:10.48550/arxiv.1509.09165

Abstract

The current need for atomic data to model stellar spectra obtained in various wavelength ranges is described. The level of completeness and accuracy of these data is discussed.

Related

• Role of input atomic data in spectroscopic analyses of the Sun and metal-poor stars
• Atomic Data: Division B / Commission 14 / Working Group Atomic Data
• Atomic Data Needs for Modeling Photoionized Plasmas
• Handling of Atomic Data
• Atomic data for resonance absorption lines. I - Wavelengths longward of the Lyman limit