Commit e52b59dc authored by Laura Ketzer's avatar Laura Ketzer
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Tool to estimate the atmospheric mass loss of planets induced by the stellar X-ray and extreme UV irradiance.
## Our Model Assumptions
We do not make use of full-blown hydrodynamical simulations, but instead couple existing parametrizations of planetary mass-radius relations with an energy-limited hydrodynamic escape model to estimate the mass-loss rate over time.
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