Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. The role of galaxy mass on AGN emission: a view from the VANDELS survey
 

The role of galaxy mass on AGN emission: a view from the VANDELS survey

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2020
Author(s)
MAGLIOCCHETTI, MANUELA  
•
PENTERICCI, Laura  
•
Cirasuolo, M.
•
Zamorani, G.
•
Amorin, R.
•
Bongiorno, A.  
•
Cimatti, A.
•
FONTANA, Adriano  
•
GARILLI, BIANCA MARIA ROSA  
•
GARGIULO, ADRIANA  
•
Hathi, N. P.
•
McLeod, D. J.
•
McLure, R. J.
•
Brusa, M.
•
SAXENA, AAYUSH  
•
Talia, M.
DOI
10.1093/mnras/staa410
Abstract
We present a comparative analysis of the properties of active galactic nuclei (AGNs) emitting at radio and X-ray wavelengths. The study is performed on 907 X-ray AGNs and 100 radio AGNs selected on the CDFS and UDS fields and makes use of new and ancillary data available to the VANDELS collaboration. Our results indicate that the mass of the host galaxy is a fundamental quantity that determines the level of AGN activity at the various wavelengths. Indeed, large stellar masses are found to be connected with AGN radio emission, as virtually all radio-active AGNs reside within galaxies of M* > 1010 M⊙. Large stellar masses also seem to favour AGN activity in the X-ray, even though X-ray AGNs present a mass distribution that is more spread out and with a non-negligible tail at M* ≲ 109 M⊙. Stellar mass alone is also observed to play a fundamental role in simultaneous radio and X-ray emission: the percentage of AGNs active at both wavelengths increases from around 1 per cent of all X-ray AGNs residing within hosts of M* < 1011 M⊙ to ˜13 per cent in more massive galaxies. In the case of radio-selected AGNs, such a percentage moves from ˜15 per cent to ˜45 per cent (but up to ˜80 per cent in the deepest fields). Neither cosmic epoch, nor radio luminosity, X-ray luminosity, Eddington ratio or star formation rate of the hosts are found to be connected to an enhanced probability for joint radio + X-ray emission of AGN origin. Furthermore, only a loose relation is observed between X-ray and radio luminosity in those AGNs that are simultaneously active at both frequencies.
Volume
493
Issue
3
Start page
3838
Uri
http://hdl.handle.net/20.500.12386/30986
Url
https://academic.oup.com/mnras/article/493/3/3838/5734514
Issn Identifier
0035-8711
Ads BibCode
2020MNRAS.493.3838M
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

staa410.pdf

Description
Pdf editoriale
Size

2.46 MB

Format

Adobe PDF

Checksum (MD5)

f808b2d652ba19b149bf8bdd8a4baa0c

Loading...
Thumbnail Image
Name

2002.02980.pdf

Description
postprint
Size

2.52 MB

Format

Adobe PDF

Checksum (MD5)

74be48d3ac0c4d245b0db25d44f832db

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback