star-line

Structure for accelerating line importance sampling
git clone git://git.meso-star.com/star-line.git
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commit 1e38fffc23e6ed3f0bf7d24d9378c9519764db06
parent 49a867d04cd05cc75ad131ed866c7552a4aeece0
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Wed, 23 Sep 2026 12:29:21 +0200

Prepare version 0.1

Write the release notes and increase the version number.

Diffstat:
MREADME.md | 13+++++++++++++
Mconfig.mk | 2+-
2 files changed, 14 insertions(+), 1 deletion(-)

diff --git a/README.md b/README.md @@ -21,6 +21,19 @@ Edit config.mk as needed, then run: ## Release notes +### Version 0.1 + +- Allow the caller to modify the thermodynamic properties at which it + evaluates the node of a tree or the lines it partitions, i.e., to use + others than those used to build the tree. + The same acceleration structure can therefore be used to sample lines + with different thermodynamic properties *as long as the sampling + criteria are met*; + such as the polylines of nodes that must be an upper limit of the + lines they encompass. +- Provide the `sln-stat` utility, which uses line importance sampling to + estimate the absorption coefficient of a spectrum, and its square. + ### Version 0.0 - Initial version of the library that structures a set of lines into an diff --git a/config.mk b/config.mk @@ -1,4 +1,4 @@ -VERSION = 0.0 +VERSION = 0.1 PREFIX = /usr/local BINPREFIX = $(PREFIX)/bin