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Line broadening parameters of N2 by H2 and He for brown dwarf or exoplanet atmospheres spectral simulations are needed. #35

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Line broadening parameters of N2 by H2 and He for brown dwarf or exoplanet atmospheres spectral simulations are needed.#35
@Trovemaster

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@Trovemaster
Trovemaster
opened on Jun 7, 2025

Request from ATMO atmospheric modellers

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