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This study explores the implications of Dark Matter in Neutron Stars (DMANS)by focusing on two specific astronomical objects: HESS J1731-347 and PSRJ0952-0607. Varying the Fermi momentum k$f^{\rm DM}$ of DM, the study analyzesthe EOS for the INRS model with and without DM. Results show the robustness ofthe model, with most EOS curves within chiral Effective Field Theory bounds.Our model predicts a maximum mass of $2.343 \ M_\odot$ for PSR J0952-0607,satisfying NICER bounds. The analysis suggests HESS J1731-347 could be a DMANS.Constraints on DM within NSs are established, and tidal deformability lieswithin GW event limits. Nonradial $f$-mode oscillations increase with DM,concluding low mass stars pulsate at higher frequencies.

Dark Matter Admixed Neutron Star in the light of HESS J1731-347 and PSR J0952-0607