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We make an in-depth analysis of different AGN jet models' signatures,inducing quiescence in galaxies with a halo mass of $10^{12} M_\odot$. Threejet models, including cosmic ray-dominant, hot thermal, and precessing kineticjets, are studied at two energy flux levels each, compared to a jet-free,stellar feedback-only simulation. We examine the distribution of Mg II, O VI,and O VIII ions, alongside gas temperature and density profiles. Low-energyions, like Mg II, concentrate in the ISM, while higher energy ions, e.g., OVIII, prevail at the AGN jet cocoon's edge. High-energy flux jets display anisotropic ion distribution with lower overall density. High-energy thermal orcosmic ray jets pressurize at smaller radii, significantly suppressing coredensity. The cosmic ray jet provides extra pressure support, extending cool andwarm gas distribution. A break in the ion-to-mass ratio slope in O VI and OVIII is demonstrated in the ISM-to-CGM transition (between 10-30 kpc), growingsmoothly towards the CGM at greater distances.

Observational Signatures of AGN Feedback in the Morphology and the Ionization States of Milky Way-like Galaxies