From 9328e77503a60d04388365332bcc57aa76e54538 Mon Sep 17 00:00:00 2001 From: Jammy2211 Date: Thu, 8 Oct 2026 09:22:19 +0100 Subject: [PATCH] docs: replace removed PySwarms search example with Nautilus/dynesty/emcee Co-Authored-By: Claude Fable 5.1 --- docs/index.md | 4 ++-- 1 file changed, 2 insertions(+), 2 deletions(-) diff --git a/docs/index.md b/docs/index.md index 44d713d9a..fafc3018f 100644 --- a/docs/index.md +++ b/docs/index.md @@ -119,8 +119,8 @@ tracer_plotter.figures_2d(image=True) To perform lens modeling, **PyAutoLens** adopts the probabilistic programming language [PyAutoFit](https://github.com/PyAutoLabs/PyAutoFit). **PyAutoFit** allows users to compose a lens model from `LightProfile`, `MassProfile` and `Galaxy` objects, customize the model parameterization and -fit it to data via a non-linear search (e.g. [dynesty](https://github.com/joshspeagle/dynesty), -[emcee](https://github.com/dfm/emcee) or [PySwarms](https://pyswarms.readthedocs.io/en/latest/)). The example +fit it to data via a non-linear search (e.g. [Nautilus](https://github.com/johannesulf/nautilus), +[dynesty](https://github.com/joshspeagle/dynesty) or [emcee](https://github.com/dfm/emcee)). The example code below shows how to setup and fit a lens model to a dataset: ```python