diff --git a/README.md b/README.md index 5718b9c..0b687ac 100644 --- a/README.md +++ b/README.md @@ -1,7 +1,20 @@ # CLOE: Cosmology Likelihood for Observables in *Euclid* + +## ⚠️ CLOE is no longer maintained + +Please refer to the actively maintained repositories instead: + +- 👉 [cloelib](https://github.com/cloe-org/cloelib) +- 👉 [cloelike](https://github.com/cloe-org/cloelike) + +This code is no longer maintained by the Euclid Consortium (EC) and should not be used for future official EC publications or to reproduce Data Release 1 results. + +------------------------------------------------------------------------- + Logo + [![CI](https://github.com/cloe-org/cloe/actions/workflows/ci.yml/badge.svg)](https://github.com/cloe-org/cloe/actions/workflows/ci.yml) [![codecov](https://codecov.io/gh/cloe-org/cloe/branch/main/graph/badge.svg?token=26c55a1c-87b4-4666-be68-7c3269a5ce86)](https://codecov.io/gh/cloe-org/cloe) [![License: LGPL-3.0](https://img.shields.io/badge/License-LGPL%20v3-blue.svg)](https://www.gnu.org/licenses/lgpl-3.0.en.html) @@ -26,6 +39,8 @@ CLOE moreover allows the user to obtain the linear matter power spectrum and bac Further documentation is found in the [CLOE Read the Docs](https://cloe-euclid.readthedocs.io/). The full development history is available to EC members [here](https://gitlab.euclid-sgs.uk/pf-ist-likelihood/likelihood-implementation). +Synthetic data vectors and covariance matrices used for code validation and posterior exploration can be found [here](https://zenodo.org/records/10212464). +Scripts for posterior exploration can be found [here](https://github.com/gcanasherrera/Forecasting-Euclid/tree/main). ## Installation