A new radio loudness diagnostic for active galaxies: a radio-to-mid-infrared parameter

Record Type
Journal Articles
Full Title
A new radio loudness diagnostic for active galaxies: a radio-to-mid-infrared parameter
Author(s)
Melendez M, Kraemer S, Schmitt H
Publication Title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Publication Title (abbreviated)
MON NOTIC ROY ASTRON SOC
Publication Date
2010 Jul 21
DOI
10.1111/j.1365-2966.2010.16679.x
ISSN
0035-8711
Volume
406
Issue
1
Page Count
12
First Page
493
Last Page
504
Keyword(s)
Astronomy & Astrophysics, Galaxy: stellar content, galaxies: Seyfert, infrared: galaxies, BLACK-HOLE MASS, SPITZER-SPACE-TELESCOPE, EXTENDED 12-MU-M SAMPLE, X-RAY LUMINOSITY, SEYFERT-GALAXIES, GALACTIC NUCLEI, STAR-FORMATION, LIMITED SAMPLE, MU-M, ENERGY-DISTRIBUTIONS
Citation
Melendez M, Kraemer S, Schmitt H. A new radio loudness diagnostic for active galaxies: a radio-to-mid-infrared parameter. MON NOTIC ROY ASTRON SOC. 2010;406 (1):493-504.
Permissions
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society c: 2010 Monthly Notices of the Royal Astronomical Society. Published by Oxford University Press. All rights reserved.
Conditions of Use
  • Author can archive pre-print (i.e., pre-refereeing)
  • Author can archive post-print (i.e., final draft post-refereeing)
  • Pre-print can only be posted prior to acceptance
  • Pre-print on author's personal website, employer website, free public server or pre-prints in subject area
  • Pre-print must be accompanied by set statement (see link)
  • Pre-print set statement must be amended upon publication (see policy)
  • Publisher's version/PDF may be used
  • Author's Post-print and Publisher's version/PDF on Institutional repositories or Central repositories
  • Published source must be acknowledged
  • Must link to publisher version
  • Set phrase to accompany archived copy (see policy)

More usage information may be available at SHERPA/RoMEO