From 6b6fb8cbb8e88ed4a582c6944b949d78519f8115 Mon Sep 17 00:00:00 2001 From: =?UTF-8?q?Pawe=C5=82?= Date: Mon, 16 Oct 2023 09:44:39 +0200 Subject: [PATCH] Update README.md --- README.md | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/README.md b/README.md index 0b07647..8ac6883 100644 --- a/README.md +++ b/README.md @@ -23,7 +23,7 @@ There are also several methods for fitting the clonal and subclonal components: - using Gaussian mixtures ([mclust](https://mclust-org.github.io/mclust/)) ([Scrucca et al., 2016](https://journal.r-project.org/archive/2016/RJ-2016-021/index.html)), - using binomial distributions ([BMix](https://github.com/caravagnalab/BMix)) ([Caravagna et al., 2020](https://www.nature.com/articles/s41588-020-0675-5)), -- and by penalizing pairwise differences ([CliP](https://github.com/wwylab/CliP)) ([Jiang et al., 2021](https://www.biorxiv.org/content/10.1101/2021.03.31.437383v1)). +- and by penalizing pairwise differences ([CliP](https://github.com/wwylab/CliP), via [Apptainer](https://apptainer.org/)) ([Jiang et al., 2021](https://www.biorxiv.org/content/10.1101/2021.03.31.437383v1)). See the model fitting details in the [Get Started](https://pawelqs.github.io/cevomod/articles/get_started.html) and [Fitting models](https://pawelqs.github.io/cevomod/articles/fitting_models.html) vignettes.