diff --git a/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml b/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml
index d4a5281cef08c2828b04229b0d6d67a28ae23426..811fe4b8cb12a18ae9641d163a96d0996136eecc 100644
--- a/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml
+++ b/examples/EAGLE_low_z/EAGLE_6/eagle_6.yml
@@ -199,6 +199,7 @@ EAGLEFeedback:
 EAGLEAGN:
   subgrid_seed_mass_Msun:             1.5e5      # Black hole subgrid mass at creation time in solar masses.
   multi_phase_bondi:                  0          # Compute Bondi rates per neighbour particle?
+  subgrid_bondi:                      0          # Compute Bondi rates using the subgrid extrapolation of the gas properties around the BH?
   with_angmom_limiter:                1          # Are we applying the Rosas-Guevara et al. (2015) viscous time-scale reduction term?
   viscous_alpha:                      1e6        # Normalisation constant of the viscous time-scale in the accretion reduction term
   radiative_efficiency:               0.1        # Fraction of the accreted mass that gets radiated.