The role played by the large-scale structures in the galaxy evolution is not quite well understood yet .
In this study , we investigate properties of galaxy in the range 0.1 < z < 0.3 from a value-added version of the WISExSCOS catalogue around cosmic filaments detected with DisPerSE .
We have fitted a profile of galaxy over-density around cosmic filaments and found a typical radius of r _ { \mathrm { m } } = 7.5 \pm 0.2 Mpc .
We have measured an excess of passive galaxies near the filament ’ s spine , higher than the excess of transitioning and active galaxies .
We have also detected SFR and \mathrm { M } _ { \star } gradients pointing towards the filament ’ s spine .
We have investigated this result and found an \mathrm { M } _ { \star } gradient for each type of galaxies : active , transitioning , and passive , and a positive SFR gradient for passive galaxies .
We also link the galaxy properties and the gas content in the Cosmic Web .
To do so , we have investigated the quiescent fraction f _ { \mathrm { Q } } profile of galaxies around the cosmic filaments .
Based on recent studies about the effect of the gas and of the Cosmic Web on galaxy properties , we have modelled f _ { \mathrm { Q } } with a \beta model of gas pressure .
The slope obtained here , \beta = 0.54 \pm 0.18 , is compatible with the scenario of projected isothermal gas in hydrostatic equilibrium ( \beta = 2 / 3 ) , and with the profiles of gas fitted in SZ .