From 33fb192eb228147bf268d753a27e15883f4774c8 Mon Sep 17 00:00:00 2001
From: Folkert Nobels <nobels@strw.leidenuniv.nl>
Date: Tue, 15 Oct 2019 10:28:03 +0100
Subject: [PATCH] Use the same epsilon for the Hernquist potential and the
 baryons.

---
 .../IsolatedGalaxy_starformation/isolated_galaxy.yml            | 2 +-
 1 file changed, 1 insertion(+), 1 deletion(-)

diff --git a/examples/IsolatedGalaxy/IsolatedGalaxy_starformation/isolated_galaxy.yml b/examples/IsolatedGalaxy/IsolatedGalaxy_starformation/isolated_galaxy.yml
index e828eb889d..86c3a469bd 100644
--- a/examples/IsolatedGalaxy/IsolatedGalaxy_starformation/isolated_galaxy.yml
+++ b/examples/IsolatedGalaxy/IsolatedGalaxy_starformation/isolated_galaxy.yml
@@ -83,7 +83,7 @@ HernquistPotential:
   diskfraction:              0.040   # Disk mass fraction
   bulgefraction:              0.014   # Bulge mass fraction
   timestep_mult:   0.01     # Dimensionless pre-factor for the time-step condition, basically determines the fraction of the orbital time we use to do the time integration
-  epsilon:         0.1      # Softening size (internal units)
+  epsilon:         0.2      # Softening size (internal units)
  
 # EAGLE star formation parameters
 EAGLEStarFormation:
-- 
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