Common Name: PKS 0925-203 VLBA 2cm Image   | VLBA 1.4 GHz:
B1950 Name: 0925-203 2 cm VLBA Image map
J2000 Name: J0927-2034
R.A. and Dec. (J2000): 9h27m51.824s
AGN Class: LSP Quasar
Redshift: 0.348 (Eracleous and Halpern 1994, ApJS 90, 1)
Luminosity Distance: 1833 Mpc ; 4.89 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology: Core
Jet Speed: Maximum: Unknown ;
Median: Unknown ;
Separation Versus Time Plot: Not available   
Stacked epoch 15 GHz VLBA images:
Uniform weight: Not Available  
Natural weight: Not Available  
Circular Beam : Not Available  
Tapered Beam: Not Available  

Rotation Measure Map: | Not available |

Spectral Index Map: | Not available |

VLBA 23 GHz:
Kpc-scale: Healey et al. 2007, ApJS 171, 61
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. 2020
Multiepoch Radio Spectrum:
43 GHz Image
Radio Spectrum
Comments: new MOJAVE 1.5JyQC source

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, 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. Observations after that date have correlated flux densities that are between 10% and 20% too low. We have adjusted the flux density scaling of the MOJAVE VLBA data up to 2022 Jan 3 based on near-simultaneous OVRO 40m measurements at 15 GHz.

Asterisked entries below denote epochs that have not yet been corrected for the VLBA flux density scaling problem.
P (%)
EVPA (deg.)
I Image (Nat. Weight) Tapered I Image Tapered I Image (Widefield) Visibility
Stokes I Radplot Pol.
2022-06-11 * BL286AL
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