Empirical determination of atomic line parameters of the 1.5 μm spectral region
Context. Both the quality and amount of astrophysical data are steadily increasing over time owing to the improvement of telescopes and their instruments. This requires corresponding evolution of the techniques used for obtaining and analyzing the resulting data. The infrared spectral range at 1.56 μm usually observed by the GRegor Infrared
Trelles Arjona, J. C. et al.
Fecha de publicación:
4
2021