Common Name: S5 0153+744 MOJAVE 15 GHz [Total intensity movie]   | VLBA 1.4 GHz:
B1950 Name: 0153+744 2 cm VLBA Image map
J2000 Name: J0157+7442
R.A. and Dec. (J2000): 1h57m34.965s
+74d42'43.229"
AGN Class: LSP Quasar
Redshift: 2.338 (1996A&AS..115...11S)
Luminosity Distance: 19070 Mpc ; 8.30 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: N, EGRET: N, TeV: N
Kpc-scale morphology: Core
Jet Speed: Maximum: 38 10 μas/y ; 3.47 0.95 c
Median: N/A ;
based on 4 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: Caltech-Jodrell Flat-Spectrum Survey
23 GHz Image
Kpc Image

Fermi LAT and 15 GHz VLBA Light Curves

Fermi LAT and 15 GHz VLBA Light Curves
VLBA 43 GHz: Lister and Smith 2000, ApJ 541,66
Multiepoch Radio Spectrum:
43 GHz Image
Radio Spectrum
Comments: Od91 list as candidate GPS; Hummell 88 show Flat spectrum; new z from McIntosh 1999

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
2020-07-02 BL229BG 275 1.9 0.7 146 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2010-12-18 BM300 169 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2002-06-12 BR077R 365 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2001-01-13 BM142A 280 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2000-12-28 BK068F 286 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2000-06-15 BM123 339 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1999-07-26 BM114B 351 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1999-07-20 BF050B 370 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1999-01-02 BG077D 416 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1998-03-19 BK052C 399 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1997-08-28 BK052A 377 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1996-07-10 BK037C 403 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1996-05-16 BK037B 372 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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