Hajime Kawahara

Code Comprehensive Review

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Based on the reflections from Bug #414 , we will thoroughly inspect the calculations and implementations of the code up to now. ## emission spectrum comparison with PetitRadtrans, which was...

See https://arxiv.org/abs/2401.03056 related #279

In `tests/integration/unittests_long/twostream/twostream_spectrum_test.py` (emission w/ scattering) , flux-adding and LART agree well with each other, but in some case, I found they gave different results and I do not why. See...

I would compare the Earth's reflection spectrum (w/ clouds) with libradtrans, using the flux adding two-stream radiative transfer. #420 #428

See https://github.com/radis/radis/issues/597

Some additional features in transmission spectroscopy

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- [ ] Hill radius cut-off - [ ] Link to Rayleigh scattering - [ ] think about wind velocity inclusion... e.g. see https://arxiv.org/abs/2303.09376

Do we need dtauM_mmwl and dtauCIA_mmwl?

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As discussed with @chonma0ctopus, we will rethink the necessity of opacity computation with a mmw (mean molecular weight) profile because MMR profile and molecular mass are sufficient to construct the...

Consider implementing the algorithm of [RotBroadInt](https://github.com/Adolfo1519/RotBroadInt) as a rotational spectral operator. https://arxiv.org/abs/2305.09693

I would like to try `kernex` to compute the convolution of the instruments/rotation, and maybe PreSolar convolution algorithmm. https://github.com/ASEM000/kernex

Note: I'd like to try flowMC https://github.com/kazewong/flowMC as a sampler of ExoJAX posterior.