2006A&A...454..729X


Query : 2006A&A...454..729X

2006A&A...454..729X - Astronomy and Astrophysics, volume 454, 729-740 (2006/8-2)

European VLBI network observations of fourteen GHz-peaked-spectrum radio sources at 5 GHz.

XIANG L., REYNOLDS C., STROM R.G. and DALLACASA D.

Abstract (from CDS):

We present the results of EVN polarization observations of fourteen GHz-Peaked-Spectrum (GPS) radio sources at 5GHz. These sources were selected from bright GPS source samples and we aimed at finding Compact Symmetric Objects (CSOs). We have obtained full polarization 5GHz VLBI observations of 14 sources providing information on their source structure and spectral indices. The results show that two core-jet sources 1433-040 and DA193, out of 14 GPS sources, exhibit integrated fractional polarizations of 3.6% and 1.0% respectively. The other 12 sources have no clear detection of pc-scale polarization. The results confirm that the GPS sources generally have very low polarization at 5GHz. The sources 1133+432, 1824+271 and 2121-014 are confirmed as CSOs. Three new CSOs 0914+114, 1518+046 and 2322-040 (tentative) have been classified on the basis of 5GHz images and spectral indices. The sources 1333+589, 1751+278 and 2323+790 can be classified either as compact doubles, and then they are likely CSO candidates or core-jet sources; further observations are needed for an appropriate classification; 0554-026, 1433-040 and 1509+054 are core-jet sources. In addition, we estimate that a component in the jet of quasar DA193 has superluminal motion of 3.3±0.6h–1c in 5.5=years.

Abstract Copyright:

Journal keyword(s): galaxies: active - quasars: general - radio continuum: galaxies

Nomenclature: Table 3: [XSD2002] HHMM+DDd A, [XSD2002] HHMM+DDd AN, [XSD2002] WW, N=19 added.

Simbad objects: 18

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Number of rows : 18
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2767 2
2 1WGA J0555.5+3948 X 05 55 30.5 +39 48 46           ~ 1 1
3 7C 055201.39+394824.00 QSO 05 55 30.80561419 +39 48 49.1649683     18.30 17.5   ~ 498 2
4 ICRF J055652.6-024105 Sy2 05 56 52.62300614 -02 41 05.5163562   20.968   19.533   ~ 33 1
5 87GB 091433.4+112607 G 09 17 16.4 +11 13 37           ~ 24 1
6 B3 1133+432 G 11 35 55.9948 +42 58 44.648           ~ 30 0
7 NVSS J133500+584305 rG 13 35 00.695 +58 43 05.59           ~ 11 1
8 4C 58.26 Bz? 13 35 25.92853561 +58 44 00.2912887       21.91   ~ 52 1
9 QSO B1404+286 BLL 14 07 00.39441712 +28 27 14.6901341   16.13 15.35 10.29   ~ 753 2
10 ICRF J143539.9-041455 QSO 14 35 39.9099617256 -04 14 55.270986900   18.14   17.38   ~ 31 1
11 1WGA J1511.6+0518 X 15 11 38.6 +05 18 29           ~ 1 0
12 ICRF J151141.2+051809 Sy1 15 11 41.26637844 +05 18 09.2590927   18.49 17.80 13.95   ~ 103 0
13 ICRF J152114.4+043021 AGN 15 21 14.41846935 +04 30 21.6366133   18.2       ~ 98 1
14 87GB 175104.0+275120 G 17 53 01.34610 +27 50 59.0160           ~ 21 1
15 NVSS J182632+270808 Rad 18 26 32.10 +27 08 08.0           ~ 14 0
16 AT20G J212339-011235 AGN 21 23 39.1 -01 12 35           ~ 35 1
17 ICRF J232503.1+791715 G 23 25 03.13217293 +79 17 15.6810424           ~ 13 1
18 AT20G J232510-034446 AGN 23 25 10.258047 -03 44 46.71563           ~ 31 0

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2023.10.04-09:04:24

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