Common Name: PKS 1532+01 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz:
B1950 Name: 1532+016 2 cm VLBA Image map
J2000 Name: J1534+0131
R.A. and Dec. (J2000): 15h34m52.454s
+1d31'4.206"
AGN Class: LSP Quasar
Redshift: 1.425 (2010AJ....139.2360S)
Luminosity Distance: 10328 Mpc ; 8.51 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology: One-sided
Jet Speed: Maximum: 100 7 μas/y ; 6.72 0.46 c
Median: N/A ;
based on 3 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_03_09 |

Spectral Index Map: | 2006_03_09 |


Multifrequency MOJAVE VLBA Data:

Epoch
8.1 GHz
8.4 GHz
12.1 GHz
2006-03-09
uvf  
uvf  
uvf  

VLBA 23 GHz:
Kpc-scale: Browne et al., 1998, MNRAS 293, 257
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: LAT flare ATEL 7175; was unusual kinematics MOJAVE_2 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, 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
2010-08-27 BL149CN 896 13 1.4 113 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-12-26 BL149CF 610 10 1.7 96 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-07-05 BL149BP 576 19 3.3 102 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-02-25 BL149BI 612 3.0 0.5 76 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2008-10-03 BL149BD 606 13 2.1 101 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2008-05-30 BL149AI 586 9.7 1.7 115 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-08-16 BL149AF 1045 9.8 0.9 97 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-03-02 BL137O 1048 22 2.1 103 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2006-03-09 BL137B 1297 22 1.7 119 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2001-01-21 BK068H 430 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2000-01-11 BK068D 454 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1998-10-30 BK052D 535 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1997-03-10 BK048A 776 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1995-12-15 BK37A 540 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1995-07-28 BZ014 727 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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