Common Name: CGRABS J0433+2905 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz:
B1950 Name: 0430+289 2 cm VLBA Image map
J2000 Name: J0433+2905
R.A. and Dec. (J2000): 4h33m37.830s
+29d5'55.477"
AGN Class: LSP BL Lac
Redshift: Unknown
Luminosity Distance: Unknown
Radio Spectrum: Flat
Gamma-ray Association LAT: Y, EGRET: Y, TeV: N
Kpc-scale morphology: Core
Jet Speed: Maximum: 121 19 μas/y ;
Median: N/A ;
based on 1 moving feature
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_04_28 |

Spectral Index Map: | 2006_04_28 | 2006_12_01




Multifrequency MOJAVE VLBA Data:

Epoch
8.1 GHz
8.4 GHz
12.1 GHz
2006-12-01
uvf  
uvf  
uvf  
2006-04-28
uvf   FITS   PS   PNG  
uvf   FITS   PS   PNG  
uvf   FITS   PS   PNG  

VLBA 23 GHz:
Kpc-scale: NVSS
23 GHz Image
Kpc Image

Fermi LAT and 15 GHz VLBA Light Curves

Fermi LAT and 15 GHz VLBA Light Curves
VLBA 43 GHz:
Multiepoch Radio Spectrum:
43 GHz Image
Radio Spectrum
Comments: NED/BZCAT z=0.97 incorrect; Meisner 2010 get z > 0.48; z < 1.66 from Shaw et al. 2013

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
2010-10-15 BL149CS 338 5.8 1.7 20 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-07-23 BL149BQ 314 5.7 1.8 32 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2008-06-25 BL149AJ 275 4.9 1.8 72 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-08-24 BL149AM 225 10 4.7 1 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-03-28 BL137P 216 6.6 3.0 109 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2006-12-01 BL137L 240 6.6 2.8 115 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2006-04-28 BL137D 327 16 4.8 106 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-06-05 BU026C 338 5.5 1.6 125 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2004-08-12 BU026B 292 10 3.6 125 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2003-08-27 BU026A 228 14 5.9 88 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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