From 0dec185c5d2fa56e4f3f18caf7f2ed73fb6cd217 Mon Sep 17 00:00:00 2001 From: Camille Avestruz Date: Fri, 19 Jul 2024 05:39:39 -0400 Subject: [PATCH] added review contributions line :-) --- examples/demo_coordinate_system_datasets.ipynb | 1 + 1 file changed, 1 insertion(+) diff --git a/examples/demo_coordinate_system_datasets.ipynb b/examples/demo_coordinate_system_datasets.ipynb index 4f8dc867c..8e4410271 100644 --- a/examples/demo_coordinate_system_datasets.ipynb +++ b/examples/demo_coordinate_system_datasets.ipynb @@ -10,6 +10,7 @@ "\n", "Tested, modified, and documented by: Camille Avestruz, July 18, 2024\n", "\n", + "Reviewed by: Caio Lima de Oliveira, July 19, 2024\n", "\n", "This notebook illustrates the impact of having an incorrect coordinate system when calculating shear profiles. The default coordinate system for `CLMM` is the euclidean/pixel coordinate system. This is consistent with DC2 catalogs. However, if we input a catalog that assumes a celestial (sky) coordinate system and use the default euclidean (pixel) coordinate system (or vice versa), the signal of shear around a cluster disappears because the signal essentially looks random.\n", "\n",