diff --git a/BSEdyn.tex b/BSEdyn.tex
index 0e52be7..4b0178d 100644
--- a/BSEdyn.tex
+++ b/BSEdyn.tex
@@ -741,7 +741,8 @@ The $GW$ calculations performed to obtain the screened Coulomb operator and the
 Perturbative $GW$ (or {\GOWO}) \cite{Hybertsen_1985a, Hybertsen_1986} quasiparticle energies are employed as starting points to compute the BSE neutral excitations.
 These quasiparticle energies are obtained by linearizing the frequency-dependent quasiparticle equation, and the entire set of orbitals is corrected.
 Further details about our implementation of {\GOWO} can be found in Refs.~\onlinecite{Loos_2018b,Veril_2018}.
-\titou{Comment on evGW.}
+Note that, for the present (small) molecular systems, {\GOWO}@HF and ev$GW$@HF yield similar quasiparticle energies. 
+Moreover, {\GOWO} allows to avoid rather laborious iterations as well as the significant additional computational effort of ev$GW$.
 As one-electron basis sets, we employ the augmented Dunning family (aug-cc-pVXZ) defined with cartesian Gaussian functions. 
 Finally, the infinitesimal $\eta$ is set to $100$ meV for all calculations.
 
@@ -1072,6 +1073,7 @@ PFL thanks the European Research Council (ERC) under the European Union's Horizo
 This work was performed using HPC resources from GENCI-TGCC (Grant No.~2019-A0060801738) and CALMIP (Toulouse) under allocation 2020-18005.
 Funding from the \textit{``Centre National de la Recherche Scientifique''} is acknowledged.
 This study has been (partially) supported through the EUR grant NanoX No.~ANR-17-EURE-0009 in the framework of the \textit{``Programme des Investissements d'Avenir''.}
+\titou{The authors would like to thank Elisa Rebolini for insightful discussions.}
 
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 \section*{Data availability}