From 41cb2352c30802b7b49527066441e94be3ca18e2 Mon Sep 17 00:00:00 2001
From: =?UTF-8?q?M=C3=A9d=C3=A9ric=20Boquien?=
Date: Thu, 3 Dec 2015 15:45:05 -0300
Subject: [PATCH] Start a new development cycle
---
CHANGELOG.md | 8 +++++++-
1 file changed, 7 insertions(+), 1 deletion(-)
diff --git a/CHANGELOG.md b/CHANGELOG.md
index ce354049c..4faa23efc 100644
--- a/CHANGELOG.md
+++ b/CHANGELOG.md
@@ -1,6 +1,12 @@
# Change Log
-## 0.8.0 (2015-11-01)
+## Unreleased
+### Added
+### Changed
+### Fixed
+### Optimised
+
+## 0.8.0 (2015-12-01)
### Added
- The evaluation of the parameters is always done linearly. This can be a problem when estimating the SFR or the stellar mass for instance as it is usual to estimate their log rather. Because the log is non-linear, the likelihood-weigthed mean of the log is not the log of the likelihood-weighted mean. Therefore the estimation of the log of these parameters has to be done during the analysis step. This is now possible. The variables to be analysed in log just need to be indicated with the suffix "_log", for instance "stellar.m_star_log". (Médéric Boquien, idea suggested by Samir Salim)
--
2.26.2