2005ApJS..159...27T


Query : 2005ApJS..159...27T

2005ApJS..159...27T - Astrophys. J., Suppl. Ser., 159, 27-40 (2005/July-0)

VLBA imaging polarimetry of active galactic nuclei: an automated approach.

TAYLOR G.B., FASSNACHT C.D., SJOUWERMAN L.O., MYERS S.T., ULVESTAD J.S., WALKER R.C., FOMALONT E.B., PEARSON T.J., READHEAD A.C.S., GEHRELS N. and MICHELSON P.F.

Abstract (from CDS):

We present full polarization Very Long Baseline Array (VLBA) observations at 5 and 15 GHz of 24 compact active galactic nuclei (AGNs). These sources were observed as part of a pilot project to demonstrate the feasibility of conducting a large VLBI survey to further our understanding of the physical properties and temporal evolution of AGN jets. The sample is drawn from the Cosmic Lens All-Sky Survey (CLASS) where it overlaps with the Sloan Digital Sky Survey at declinations north of 15°. There are 2100 CLASS sources brighter than 50 mJy at 8.4 GHz, of which we have chosen 24 for this pilot study. All 24 sources were detected and imaged at 5 GHz with a typical dynamic range of 500:1, and 21 of 24 sources were detected and imaged at 15 GHz. Linear polarization was detected in eight sources at both 5 and 15 GHz, allowing for the creation of Faraday rotation measure (RM) images. The core RMs for the sample were found to have an average absolute value of 390±100 rad/m2. We also present the discovery of a new compact symmetric object, J08553+5751. All data were processed automatically using pipelines created or adapted for the survey.

Abstract Copyright:

Journal keyword(s): Catalogs - Galaxies: Active - Galaxies: Jets - Galaxies: Nuclei - Radio Continuum: Galaxies - Surveys - Techniques: Polarimetric

Simbad objects: 27

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Number of rows : 27
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 ICRF J084728.0+572338 G 08 47 28.0579 +57 23 38.349           ~ 20 1
2 7C 084512.90+561507.00 QSO 08 49 00.8542674096 +56 03 50.111489520           ~ 11 1
3 ICRF J084957.9+510829 Sy1 08 49 57.97685916 +51 08 29.0238146   19.37 18.78 17.79   ~ 249 2
4 QSO J0850+5159 QSO 08 50 42.2440214784 +51 59 11.650187472   19.92 19.41     ~ 47 1
5 4C 58.17 QSO 08 54 41.99641612 +57 57 29.9391251   18.56 18.18 17.43   ~ 238 1
6 QSO J0854+2006 BLL 08 54 48.8749846272 +20 06 30.639583620   15.91 15.43 15.56   ~ 2331 1
7 BWE 0851+5803 G 08 55 21.35749 +57 51 44.0817           ~ 11 1
8 87GB 085340.6+583903 QSO 08 57 31.4511 +58 27 22.538           ~ 3 1
9 87GB 085444.0+560424 G 08 58 30.4786 +55 52 41.302           ~ 4 1
10 6C 085940+470301 QSO 09 03 03.99010563 +46 51 04.1374172   19.90 19.44 18.7   ~ 265 1
11 NVSS J094704+590741 Rad 09 47 04.8631 +59 07 41.467           ~ 9 1
12 SDSS J094920.21+603922.8 QSO 09 49 20.2278744960 +60 39 22.890294864           ~ 8 1
13 SDSS J094939.80+581912.9 QSO 09 49 39.8149 +58 19 12.933           ~ 8 1
14 3C 279 Bla 12 56 11.16657958 -05 47 21.5251510   18.01 17.75 15.87   ~ 3044 2
15 US 371 BLL 13 10 28.66385420 +32 20 43.7828340   15.61 15.24 17.91   ~ 852 1
16 ICRF J141414.8+455448 Sy2 14 14 14.8497 +45 54 48.730           ~ 34 1
17 7C 1539+5813 QSO 15 40 37.5782720568 +58 03 34.398790740   17.9 18.84 17.9   ~ 27 1
18 6C 154338+514423 QSO 15 45 02.8236292176 +51 35 00.878127144   17.96 17.77 17.57   ~ 78 1
19 7C 154427.19+540953.00 QSO 15 45 43.82588016 +54 00 42.7587127           ~ 22 1
20 SDSS J154633.61+514645.4 QSO 15 46 33.6208 +51 46 45.455           ~ 11 1
21 6C 155103+560124 QSO 15 52 10.8964666272 +55 52 43.192027848           ~ 6 1
22 7C 164252.79+392128.00 QSO 16 44 34.4739184440 +39 16 04.930873680   20.54 20.17     ~ 24 1
23 ICRF J164656.8+405917 Sy1 16 46 56.85870434 +40 59 17.1721176   19.34 19.20 19.38   ~ 56 1
24 6C 164650+410912 QSO 16 48 29.25803616 +41 04 05.5525848   19.18 18.90 19   ~ 63 1
25 SDSS J165233.20+401358.3 QSO 16 52 33.2136 +40 13 58.339           ~ 10 0
26 7C 165116.19+390743.00 QSO 16 52 58.50958176 +39 02 49.8221906   22.23 21.54 20.57   ~ 47 1
27 SDSS J165412.72+395005.6 QSO 16 54 12.7223 +39 50 05.681           ~ 8 1

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