star-line

Structure for accelerating line importance sampling
git clone git://git.meso-star.com/star-line.git
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commit 6c95f8e3f25e03a8b2e606cbb183cba1269f6b0c
parent a501a85b20aeb2bc70475664ec4f66597f7c7ab9
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Wed, 23 Sep 2026 11:31:54 +0200

Delete a comment

It was no longer relevant since the caller can evaluate a line at
thermodynamic properties other than those used to construct the tree.
It is therefore no longer possible to pre-calculate some of the lines
parameters, as suggested by the comment that this commit deletes.

Diffstat:
Msrc/sln_line.c | 2+-
1 file changed, 1 insertion(+), 1 deletion(-)

diff --git a/src/sln_line.c b/src/sln_line.c @@ -114,7 +114,7 @@ line_profile_factor density = density / (PERFECT_GAZ_CONSTANT * temperature); density = density * 1e-6; /* Convert in molec.cm^-3 */ - /* Compute the partition function. TODO precompute it for molid/isoid */ + /* Compute the partition function */ Q_Tref = isotope->Q296K; molid = shtr_line->molecule_id; isoid = shtr_line->isotope_id_local+1/*Local indices start at 1 in BD_TIPS*/;