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The MARTINI platform - I. Se I–X atomic calculation and expansion opacity for early stage kilonova spectral analysis | Astronomy & Astrophysics (A&A)
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Home All issues Volume 708 (April 2026) A&A, 708 (2026) A366 Full HTML
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Fig. A.1.

Fig. A.1. Refer to the following caption and surrounding text.

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Se I–X expansion opacity at T = 100 000 K. In the panels, it can be seen that the opacity contribution at T = 100 000 K only comes from the ionisation stages beyond Se VI. No significant contribution can be observed in the ionisation stages between Se I–VI.

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