Spectral flux densities from 50MHz to 50GHz : J/ApJS/230/7


Authors : Perley R.A. orcid , Butler B.J. (hide) , Butler B.J. et..al

Bibcode : 2017ApJS..230....7P (ADS) (Simbad) (Objects) (hide)

CDS Keywords : Interferometry; Radio sources
UAT : Interferometry, Radio sources

Observation (OC)

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Inserted into VizieR : 03-Aug-2017
Last modification : 04-Sep-2017

An accurate flux density scale from 50 MHz to 50 GHz. (2017)

Keywords : instrumentation interferometers; methods: data analysis; methods: observational; techniques: interferometric; telescopes

Abstract:The flux-density scale of Perley & Butler (2013ApJS..204...19P) is extended downward to ~50MHz by utilizing recent observations with the Karl G. Jansky Very Large Array (VLA) of 20 sources between 220MHz and 48.1GHz, and legacy VLA observations at 73.8MHz. The derived spectral flux densities are placed on an absolute scale by utilizing the Baars+ (1977A&A....61...99B) values for Cygnus A (3C405) for frequencies below 2GHz, and the Mars-based polynomials for 3C286, 3C295, and 3C196 from Perley & Butler above 2GHz. Polynomial expressions are presented for all 20 sources, with accuracy limited by the primary standards to 3%-5% over the entire frequency range. Corrections to the scales proposed by Perley & Butler, and by Scaife & Heald (2012MNRAS.423L..30S) ...(more)
Abstract: (hide)
The VLA observations were made in five observing sessions: 1998 Mar 07-08, 1998 Oct 04-05, 2014 Oct 11-12, 2016 Jan 25-26 and 2016 Jan 27. The first two of these sessions were taken under Project ID AK461. These data were taken with the original VLA correlator, with 1.6MHz bandwidth. All other data were taken with the new Jansky VLA system.

  • J/AJ/146/120 : MOJAVE. X. Parsec-scale kinematics of AGNs (Lister+, 2013)

                
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