J/AJ/148/16          Updated 3CRR sample of radio sources         (Singal, 2014)

Discordance of the unified scheme with observed properties of quasars and high-excitation galaxies in the 3CRR sample. Singal A.K. <Astron. J., 148, 16 (2014)> =2014AJ....148...16S 2014AJ....148...16S
ADC_Keywords: QSOs ; Galaxies, radio ; Redshifts Keywords: galaxies: active - galaxies: nuclei - quasars: general Abstract: We examine the consistency of the unified scheme of Fanaroff-Riley type II radio galaxies and quasars with their observed number and size distributions in the 3CRR sample. We separate the low-excitation galaxies from the high-excitation ones, as the former might not harbor a quasar within and thus may not be partaking in the unified scheme models. In the updated 3CRR sample, at low redshifts (z<0.5), the relative number and luminosity distributions of high-excitation galaxies and quasars roughly match the expectations from the orientation-based unified scheme model. However, a foreshortening in the observed sizes of quasars, which is a must in the orientation-based model, is not seen with respect to radio galaxies even when the low-excitation galaxies are excluded. This dashes the hope that the unified scheme might still work if one includes only the high-excitation galaxies. Description: Our chosen 3CRR sample (Laing et al. 1983, cat. J/MNRAS/204/151) is radio complete in the sense that all radio sources stronger than its sensitivity limit S178=10.9Jy are included. The sample covers the sky north of declination, δ=10°, except for a zone of avoidance, a band of ±10° about the Galactic plane. Also it has a 100% optical identification content with detailed optical spectra to classify radio sources into radio galaxies and quasars. We have taken the updated optical and radio data from http://astroherzberg.org/people/chris-willott/research/3crr/. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 52 130 Radio and optical data for our sample -------------------------------------------------------------------------------- See also: VIII/14 : 87GB Catalog of radio sources (Gregory et al., 1991) VIII/3 : An Optical Catalogue of Radio Galaxies (Burbidge+ 1979) VIII/32 : Extragalactic sources at 5GHz (Jenkins+ 1977) VIII/4 : Fourth Cambridge Survey (4C) (Pilkington+ 1965; Gower+ 1967) VIII/1 : The 3C and 3CR Catalogues (Edge+ 1959-1962) J/MNRAS/204/151 : Bright radio sources at 178 MHz (3CRR) (Laing+ 1983) http://astroherzberg.org/people/chris-willott/research/3crr/ : 3CRR sample Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- IAU IAU source name (HHMM+DDd; B1950) 10- 17 A8 --- 3CRR 3CRR source name (3C or 4C name) 19- 23 F5.1 Jy S408 [4.3/115.3] Flux density at 408MHz 25- 27 F3.1 --- alpha [0.5/1.2] Spectral index α 29- 31 A3 --- Type Nature of the optical object (1) 33- 36 F4.2 --- z [0.03/2.01] Redshift 38- 41 I4 arcsec theta [3/2440] Largest angular size θ 43- 46 I4 kpc l [21/4408] Linear size 48- 52 E5.1 W/Hz P408 [6e+25/3e+29] Luminosity -------------------------------------------------------------------------------- Note (1): The optical objects are defined as follows: HEG = High-Excitation Galaxy; LEG = Low-Excitation Galaxy; Q = Quasar; WQ = Weak Quasar. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Sylvain Guehenneux [CDS] 13-Oct-2014
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line