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WP2: Synthetic XUV spectra

<p>Set of XUV (0.01 - 10 keV) spectra, computed from parameterized plasma Emission Measure Distributions vs. temperature, for stars with different activity levels and plasma metallicities. Read the Introduction for more details. These spectra are intended as input for models of photochemistry and photoevaporation of exoplanetary atmospheres.</p>

ShareScore

16/100

Overall dataset sharing score

Score breakdown

These five areas show where the dataset supports — or may limit — practical reuse.

Stewardship
8
Harmonization
4
Access
0
Reuse readiness
0
Engagement
4

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