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our (4) vlba detections:
our (4) vlba detections:
radio quiet agn buried in star-forming galaxies
radio quiet agn buried in star-forming galaxies
Cutouts of our 4 VLBA detections (ID 338, 351, 408 and 498) found at signal-to-noise S/N>5.5
The deepest vlbi view of radio quiet agn
The deepest vlbi view of radio quiet agn
see Peluso, Delvecchio et al. 2025
AGN-CORRECTED INFRARED-RADIO CORRELATION (IRRC)
AGN-CORRECTED INFRARED-RADIO CORRELATION (IRRC)
Main result: Radio-faint AGN without radio-excess have a negligible impact to the evolving infrared-radio correlation.
Radio-SFR conversions calibrated after removing radio-excess AGN are robust.
Some of the main results are described in this presentation held at INAF-OAS on April 2025 (from slide 28).
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