WP2: Synthetic XUV spectra
Authors/Creators
- 1. INAF Osservatorio Astronomico di Palermo
- 2. UNIPA Dipartimento di FIsica e Chimica
Description
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.
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Data produced in the framework of the ASI-INAF project THE StellaR PAth (ASI-INAF agreement n.2018-16-HH.0), available to members of the project and to reviewers, under request via email to Antonio Maggio.
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