  We complement a previous work \cite{Fortuna:2020wwx} using an EFT framework
of dark matter and standard model interactions, with spin-one mediators,
exploring a wider dark matter mass range, up to $6.4$ TeV. We use again bounds
from different experiments: relic density, direct detection experiments and
indirect detection limits from the search of gamma-ray emissions and positron
fluxes. Besides, in this paper we add collider constraints by the ATLAS
Collaboration in monojet analysis. Moreover, here we tested our previous
results in the light of the aforementioned ATLAS data, which turn out to be the
most restrictive forlight dark matter masses (as expected), $m_{\rm DM}<M_Z/2$.
We obtain a larger range of solutions for the operators of dimension 5, OP1 and
OP4, where masses above $43$ GeV and $30$ GeV (but for the $Z$ resonance
region, $\sim (M_Z\pm\Gamma_Z)/2$), respectively, are allowed. In contrast, the
operator of dimension 6, OP3, has viable solutions for masses $\gtrsim 190$
GeV. For the combination of OP1\&OP3 we obtain solutions (for masses larger
than $140$ or $325$ GeV) that depend on the relative sign between the
operators.
