A super-linear 'radio-AGN main sequence' links mean radio-AGN power and galaxy stellar mass since z~3

@article{Delvecchio2022AS,
  title={A super-linear 'radio-AGN main sequence' links mean radio-AGN power and galaxy stellar mass since z~3},
  author={Ivan Delvecchio and Emmanuele Daddi and Mark T. Sargent and James Aird and James R. Mullaney and B. Magnelli and David Elbaz and Laura Bisigello and L. Ceraj and S. Jin and Boris S. Kalita and D. Z. Liu and M. Novak and Isabella Prandoni and J. F. Radcliffe and Cristiana Spingola and Gianni Zamorani and Viola Allevato and Giulia Rodighiero and Vernesa Smol{\vc}i{\'c}},
  journal={Astronomy \& Astrophysics},
  year={2022}
}
Mapping the average AGN luminosity across galaxy populations and over time encapsulates important clues on the interplay between supermassive black hole (SMBH) and galaxy growth. This paper presents the demography, mean power and cosmic evolution of radio AGN across star-forming galaxies (SFGs) of di ff erent stellar masses ( M ∗ ). We exploit deep VLA-COSMOS 3 GHz data to build the rest-frame 1.4 GHz AGN luminosity functions at 0.1 ≤ z ≤ 4.5 hosted in SFGs. Splitting the AGN luminosity function… 

References

SHOWING 1-3 OF 3 REFERENCES

2017c) but identifying radio-excess AGN according to D21

  • 2017

2018) and Fig. 2 (grey dashed lines), we compute the AGN-related fraction at 1.4 GHz, f AGN

  • 2018

A128 A&A proofs: manuscript no

  • A&A
  • 2018