Cosmic evolution of radio selected active galactic nuclei in the cosmos field

V. Smolčić, G. Zamorani, E. Schinnerer, S. Bardelli, M. Bondi, L. Bîrzan, C. L. Carilli, P. Ciliegi, M. Elvis, Christopher D Impey, A. M. Koekemoer, A. Merloni, T. Paglione, M. Salvato, M. Scodeggio, N. Scoville, J. R. Trump

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Abstract

We explore the cosmic evolution of radio luminous active galactic nuclei (AGNs) with low radio powers (L1.4GHz ≲ 5×1025 W Hz-1) out to z = 1.3 using to date the largest sample of ∼600 low-luminosity radio AGN at intermediate redshift drawn from the VLA-COSMOS survey. We derive the radio-luminosity function for these AGNs, and its evolution with cosmic time assuming two extreme cases: (1) pure luminosity and (2) pure density evolution. The former and latter yield L* α (1+z)0.8±0.1 and φ* α (1+z)1.1±0.1, respectively, both implying a fairly modest change in properties of low-radio-power AGNs since z = 1.3. We show that this is in stark contrast with the evolution of powerful (L1.4GHz > 5 × 1025 W Hz-1) radio AGN over the same cosmic time interval, constrained using the 3CRR, 6CE, and 7CRS radio surveys by Willot et al. We demonstrate that this can be explained through differences in black hole fueling and triggering mechanisms, and a dichotomy in host galaxy properties of weak and powerful AGNs. Our findings suggest that high- and low-radio-power AGN activities are triggered in different stages during the formation of massive red galaxies. We show that weak radio AGN occur in the most massive galaxies already at z ∼ 1, and they may significantly contribute to the heating of their surrounding medium and thus inhibit gas accretion onto their host galaxies, as recently suggested for the "radio mode" in cosmological models.

Original languageEnglish (US)
Pages (from-to)24-39
Number of pages16
JournalAstrophysical Journal
Volume696
Issue number1
DOIs
StatePublished - 2009

Fingerprint

cosmos
active galactic nuclei
radio
galaxies
luminosity
dichotomies
refueling
intervals
heating
accretion

Keywords

  • Cosmology: Observations
  • Galaxies: Active
  • Galaxies: Evolution
  • Galaxies: Fundamental parameters
  • Radio continuum: Galaxies

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Smolčić, V., Zamorani, G., Schinnerer, E., Bardelli, S., Bondi, M., Bîrzan, L., ... Trump, J. R. (2009). Cosmic evolution of radio selected active galactic nuclei in the cosmos field. Astrophysical Journal, 696(1), 24-39. https://doi.org/10.1088/0004-637X/696/1/24

Cosmic evolution of radio selected active galactic nuclei in the cosmos field. / Smolčić, V.; Zamorani, G.; Schinnerer, E.; Bardelli, S.; Bondi, M.; Bîrzan, L.; Carilli, C. L.; Ciliegi, P.; Elvis, M.; Impey, Christopher D; Koekemoer, A. M.; Merloni, A.; Paglione, T.; Salvato, M.; Scodeggio, M.; Scoville, N.; Trump, J. R.

In: Astrophysical Journal, Vol. 696, No. 1, 2009, p. 24-39.

Research output: Contribution to journalArticle

Smolčić, V, Zamorani, G, Schinnerer, E, Bardelli, S, Bondi, M, Bîrzan, L, Carilli, CL, Ciliegi, P, Elvis, M, Impey, CD, Koekemoer, AM, Merloni, A, Paglione, T, Salvato, M, Scodeggio, M, Scoville, N & Trump, JR 2009, 'Cosmic evolution of radio selected active galactic nuclei in the cosmos field', Astrophysical Journal, vol. 696, no. 1, pp. 24-39. https://doi.org/10.1088/0004-637X/696/1/24
Smolčić V, Zamorani G, Schinnerer E, Bardelli S, Bondi M, Bîrzan L et al. Cosmic evolution of radio selected active galactic nuclei in the cosmos field. Astrophysical Journal. 2009;696(1):24-39. https://doi.org/10.1088/0004-637X/696/1/24
Smolčić, V. ; Zamorani, G. ; Schinnerer, E. ; Bardelli, S. ; Bondi, M. ; Bîrzan, L. ; Carilli, C. L. ; Ciliegi, P. ; Elvis, M. ; Impey, Christopher D ; Koekemoer, A. M. ; Merloni, A. ; Paglione, T. ; Salvato, M. ; Scodeggio, M. ; Scoville, N. ; Trump, J. R. / Cosmic evolution of radio selected active galactic nuclei in the cosmos field. In: Astrophysical Journal. 2009 ; Vol. 696, No. 1. pp. 24-39.
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