Common Name: PKS B1345+125 MOJAVE 15 GHz [Total intensity movie]   | VLBA 1.4 GHz: NRAO Archive
B1950 Name: 1345+125 2 cm VLBA Image map
J2000 Name: J1347+1217
R.A. and Dec. (J2000): 13h47m33.362s
+12d17'24.240"
AGN Class: LSP G
Redshift: 0.121 (Adelman-McCarthy et al. 2006, ApJS, 162, 38)
Luminosity Distance: 558 Mpc ; 2.15 pc/mas
Radio Spectrum: Steep
Gamma-ray Association LAT: N, EGRET: N, TeV: N
Kpc-scale morphology: Two-sided
Jet Speed: Maximum: 118 21 μas/y ; 0.93 0.16 c
Median: N/A ;
based on 7 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_11_10 |


Multifrequency MOJAVE VLBA Data:

Epoch
8.1 GHz
8.4 GHz
12.1 GHz
2006-11-10
uvf  
uvf  
uvf  

VLBA 23 GHz:
Kpc-scale: Stanghellini et al. 2005, AA, 443, 891
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: Low-luminosity MOJAVE-2; GPS

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
2019-08-23 * BL229BA 814 7.5 0.9 139 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2013-07-30 BL178BG 743 1.8 0.2 2 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-07-24 BL149DN 870 10 1.2 143 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-07-23 BL149BQ 795 13 1.6 151 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2006-11-10 BL137K 656 14 2.1 153 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2001-03-28 BS085D 366 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2001-03-27 BS085B 288 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2001-01-04 BK078 704 5.7 0.8 148 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1999-11-06 BK068C 560 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1998-11-01 BK052E 450 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1997-08-28 BK052A 513 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1996-04-22 BS036 594 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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