Common Name: TXS 0529+483 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz: University College Cork Program
B1950 Name: 0529+483 2 cm VLBA Image map
J2000 Name: J0533+4822
R.A. and Dec. (J2000): 5h33m15.866s
+48d22'52.808"
AGN Class: LSP Quasar
Redshift: 1.16 (Shaw et al. 2012, ApJ, 748, 49)
Luminosity Distance: 7987 Mpc ; 8.30 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: Y, EGRET: P, TeV: N
Kpc-scale morphology: One-sided Halo
Jet Speed: Maximum: 338 51 μas/y ; 19.8 3.0 c
Median: N/A ;
based on 4 moving features
Lister et al. 2019, ApJ, 874, 43
Separation Versus Time Plot: PNG    PS
Stacked epoch 15 GHz VLBA images:
Uniform weight: [PS]   [GIF]
Natural weight: [PS]   [GIF]
Circular Beam : [PS]   [GIF]
Tapered Beam: [PS]   [GIF]
Pushkarev et al. 2017 :   FITS

Rotation Measure Map: | 2006_05_24 |

Spectral Index Map: | 2006_05_24 |


Multifrequency MOJAVE VLBA Data:

Epoch
8.1 GHz
8.4 GHz
12.1 GHz
2006-05-24
uvf  
uvf  
uvf  

VLBA 23 GHz:
Kpc-scale: Cooper et al. 2007, ApJ Supl 171, 376
23 GHz Image
Kpc Image

Fermi LAT and 15 GHz VLBA Light Curves

Fermi LAT and 15 GHz VLBA Light Curves
VLBA 43 GHz: Cheng et al. 2018
Multiepoch Radio Spectrum:
43 GHz Image
Radio Spectrum
Comments: RATAN meas > 1.5 Jy at 15 Ghz; b = 8.2; redshift from Mattox et al. 2003:AJ 125 572; Sowers-Emmerd 03 lists EGRET id as highly probable

If you use these data in a publication, we ask that you please contact us so we can add a link to the list of external MOJAVE publications, and ask that you cite Lister et al., 2018, ApJS, 234, 12 and include the following acknowledgment: "This research has made use of data from the MOJAVE database that is maintained by the MOJAVE team (Lister et al. 2018)"

Important Note: The MOJAVE team, working with the OVRO 40m AGN monitoring group, has discovered a systematic error in the flux densities of all VLBA 15 GHz observations taking place after a date that lies between 2019 April 16 and 2019 May 16. All observations after that date have correlated flux densities that are between 10% and 20% too low. The MOJAVE team and NRAO are currently investigating the issue.

Asterisked entries below denote epochs that have not yet been corrected for the VLBA flux density scaling problem.
Epoch
(Y-M-D)
VLBA Code VLBA I
(mJy)
VLBA P
(mJy)
VLBA
P (%)
VLBA
EVPA (deg.)
I Image (Nat. Weight) Tapered I Image Tapered I Image (Widefield) Visibility
Data
Stokes I Radplot Pol.
Image
2013-03-31 BL178BB 2103 18 0.9 161 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2012-11-02 BL178AR 1666 7.1 0.4 163 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2012-05-24 BL178AK 1567 34 2.2 175 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-09-12 BL149DQ 1592 21 1.3 51 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2010-08-27 BL149CN 1264 21 1.7 115 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2008-10-03 BL149BD 864 11 1.3 3 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-08-16 BL149AF 1348 43 3.2 112 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2006-05-24 BL137E 790 16 2.0 38 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-09-19 BL123N 1463 53 3.6 162 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-06-15 BL123I 1237 24 1.9 1 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-06-05 BU026C 1215 18 1.5 2 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2005-02-05 BL123B 1130 25 2.2 156 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2004-08-12 BU026B 766 16 2.1 147 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2004-02-11 BL111K 638 10 1.6 157 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2003-08-27 BU026A 892 7.7 0.9 27 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2002-10-09 BL111C 1043 19 1.9 152 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
1995-01-20 BP14 1274 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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