diff --git a/CHANGELOG.md b/CHANGELOG.md
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--- a/CHANGELOG.md
+++ b/CHANGELOG.md
@@ -1,4 +1,13 @@
 # Changelog
+## [2.6.0] - 2024-02-01
+
+### Added
+
+- *TSModel:* An extremely fast transit model for transmission spectroscopy. The model is based on the RoadRunnerModel and can use any 
+  rotationally symmetric function to model stellar limb darkening.
+- *LDTkLDM:* A RoadRunnerModel limb darkening model that uses directly stellar intensity profiles created by the LDTk. The model is
+  parameterised by the effective stellar temperature, surface gravity, and metallicity. This should be quite valuable for transmission
+  spectroscopy since the number of limb darkening parameters is independent of the number of passbands.
 
 ## [2.4.0] - 2020-10-14
 
diff --git a/README.md b/README.md
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 PyTransit
 =========
 
-[![Travis](http://img.shields.io/travis/hpparvi/PyTransit/development.svg?style=flat)](https://travis-ci.org/hpparvi/PyTransit)
-[![Documentation Status](https://readthedocs.org/projects/pytransit/badge/?version=latest)](https://pytransit.readthedocs.io/en/latest/?badge=latest)
-[![codecov](https://codecov.io/gh/hpparvi/PyTransit/branch/master/graph/badge.svg)](https://codecov.io/gh/hpparvi/PyTransit)
 [![Licence](http://img.shields.io/badge/license-GPLv2-blue.svg?style=flat)](http://www.gnu.org/licenses/gpl-2.0.html)
 [![MNRAS](https://img.shields.io/badge/MNRAS-10.1093%2Fmnras%2Fstv894-blue.svg)](http://mnras.oxfordjournals.org/content/450/3/3233)
 [![arXiv](http://img.shields.io/badge/arXiv-1504.07433-blue.svg?style=flat)](http://arxiv.org/abs/1504.07433)