Common Name: OP 151 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz:
B1950 Name: 1331+170 2 cm VLBA Image map
J2000 Name: J1333+1649
R.A. and Dec. (J2000): 13h33m35.783s
+16d49'4.015"
AGN Class: LSP Quasar
Redshift: 2.08494 (LAMOSTDR6V2)
Luminosity Distance: 16564 Mpc ; 8.44 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: N, EGRET: Y, TeV: N
Kpc-scale morphology: Unknown
Jet Speed: Maximum: 64 6 μas/y ; 5.40 0.51 c
Median: N/A ;
based on 2 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: | Not available |

Spectral Index Map: | 2006_04_05 | 2006_12_01




Multifrequency MOJAVE VLBA Data:

Epoch
8.1 GHz
8.4 GHz
12.1 GHz
2006-12-01
uvf  
uvf  
uvf  
2006-04-05
uvf   FITS   PS   PNG  
uvf   FITS   PS   PNG  
uvf   FITS   PS   PNG  

VLBA 23 GHz:
Kpc-scale: di Serego-Alighieri et al. 1994, MNRAS, 269, 998
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: EGRET MOJAVE-2 source; Radio spectrum looks peaked at high frequencies but steep below 1 GHz; VC lists z as 2.097

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 346 2.9 0.8 155 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-07-23 BL149BQ 397 1.2 0.3 172 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-09-06 BL149AG 373 3.0 0.8 32 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-07-03 BL149AC 373 1.2 0.3 49 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-03-28 BL137P 369 3.9 1.1 24 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2006-12-01 BL137L 340 < 2.7 < 8.1 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2006-04-05 BL137C 309 4.0 1.3 22 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-06-05 BU026C 315 1.8 0.6 14 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2004-08-12 BU026B 304 1.8 0.6 145 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2003-08-27 BU026A 292 1.4 0.5 130 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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