From e9e977f107b0549639a53ac98b2f740649c2069d Mon Sep 17 00:00:00 2001 From: Arun Kannawadi Date: Wed, 14 Oct 2026 00:15:22 -0400 Subject: [PATCH 1/2] Update reference to MCP working group conveners TJP WG no longer exists. The link to the DESC website particularly lets external contributors know who the conveners are to contact. --- README.md | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/README.md b/README.md index 5dfe46d87..57531026e 100644 --- a/README.md +++ b/README.md @@ -103,7 +103,7 @@ the code, which is open source and available under terms consistent with our ([BSD 3-Clause](https://opensource.org/licenses/BSD-3-Clause)). External contributors and DESC members wishing to use CCL for non-DESC projects -should consult with the TJP working group conveners, ideally before the work has +should consult with the [MCP working group conveners](https://lsstdesc.org/pages/organization.html#analysis-working-groups), ideally before the work has started, but definitely before any publication or posting of the work to the arXiv. For free use of the `CLASS` library, the `CLASS` developers require that the `CLASS` From 4cae02389f80f40d13eb73364adb5b71be82c99e Mon Sep 17 00:00:00 2001 From: Arun Kannawadi Date: Wed, 14 Oct 2026 00:16:14 -0400 Subject: [PATCH 2/2] Remove extraneous power --- README.md | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/README.md b/README.md index 57531026e..9351c30cf 100644 --- a/README.md +++ b/README.md @@ -26,7 +26,7 @@ The core functions of this package include: - Background quantities (Hubble parameter $H(z)$, distances etc.). - Linear growth factor $D(z)$ and growth rate $f(z)$. - Linear matter power spectra $P(k)$ from Boltzmann codes (CLASS, CAMB), emulators, and approximate fitting functions. - - Non-linear matter power power spectra using a variety of prescriptions, including emulators, and including the impact of baryonic effects. + - Non-linear matter power spectra using a variety of prescriptions, including emulators, and including the impact of baryonic effects. - Angular power spectra $C_\ell$ and correlation functions $\xi(\theta)$ for arbitrary combinations of tracers including number counts, shear, CMB lensing, ISW, thermal SZ, CIB, as well as custom-made tracers. - A comprehensive halo model framework able to combine different prescriptions for the halo mass function $dn/dM$, halo bias $b(M)$, concentration-mass relation $c(M)$, mass definitions, and halo profiles, as well as to provide predictions for summary statistics (power spectra, non-Gaussian covariances) of arbitrary quantities. - Support for $\Lambda$ CDM, and $w_0-w_a$CDM cosmologies with curvature and massive neutrinos, as well as simple modified gravity extensions (e.g. $\mu-\Sigma$ ).