Common Name: OV 591 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz: NRAO Archive
B1950 Name: 1954+513 2 cm VLBA Image map
J2000 Name: J1955+5131
R.A. and Dec. (J2000): 19h55m42.738s
+51d31'48.546"
AGN Class: LSP LPQ
Redshift: 1.223 (1996ApJS..107..541L)
Luminosity Distance: 8533 Mpc ; 8.37 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology: Two-sided
Jet Speed: Maximum: 260 16 μas/y ; 15.78 0.95 c
Median: N/A ;
based on 6 moving features
Lister et al. 2019, ApJ,874,43
Separation Versus Time Plot: PNG    PS
Stacked epoch 15 GHz VLBA images:
Uniform weight: [PDF]   [GIF]
Natural weight: [PDF]   [GIF]
Circular Beam : [PDF]   [GIF]
Tapered Beam: [PDF]   [GIF]
Pushkarev et al. 2017 :   FITS

Rotation Measure Map: | Not available |

Spectral Index Map: | Not available |


VLBA 23 GHz:
Kpc-scale: Kollgaard, Wardle, and Roberts 1990, AJ 100
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: Former 1.5 Jy candidate; 150 mJy of extended flux density at 15 GHz

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.
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
2016-11-12 BL193BL 1132 27 2.4 42 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2016-10-29 BL193BK 1199 31 2.6 42 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2016-08-09 BL193BI 1160 20 1.7 30 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2016-06-16 BL193BG 1292 48 3.7 24 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2016-06-03 BL193BE 1333 42 3.2 25 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2016-03-05 BL193BC 1380 36 2.6 14 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2015-11-25 BL193AY 1429 35 2.5 21 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2015-05-18 BL193AS 1215 9.9 0.8 24 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-08-26 BL149DP 1194 40 3.4 26 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-03-05 BL149DD 1218 56 4.6 35 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2010-10-15 BL149CS 1269 43 3.4 42 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-03-15 BG152B 688 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2002-08-02 BR077M 736 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1999-05-21 BK068A 947 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1998-03-19 BK052C 943 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1995-01-20 BP14 1191 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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