Common Name: 4C +05.64 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz: University College Cork Program
B1950 Name: 1548+056 2 cm VLBA Image map
J2000 Name: J1550+0527
R.A. and Dec. (J2000): 15h50m35.269s
+5d27'10.448"
AGN Class: LSP HPQ
Redshift: 1.417 (2010AJ....139.2360S)
Luminosity Distance: 10256 Mpc ; 8.51 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology: Core
Jet Speed: Maximum: 172 25 μas/y ; 11.6 1.7 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: [PS]   [GIF]
Natural weight: [PS]   [GIF]
Circular Beam : [PS]   [GIF]
Tapered Beam: [PS]   [GIF]
Pushkarev et al. 2017 :   FITS

Rotation Measure Map: | 2006_10_06 |

Spectral Index Map: | 2006_10_06 |


Multifrequency MOJAVE VLBA Data:

Epoch
8.1 GHz
8.4 GHz
12.1 GHz
2006-10-06
uvf  
uvf  
uvf  

VLBA 23 GHz: RRIFD Database
Kpc-scale: Kharb, Lister, and Cooper 2010, ApJ 710, 764
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: VLA data listed in Murphy et al. 1998 (no image)

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
2012-06-25 BL178AL 2442 80 3.3 132 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-08-26 BL149DP 2704 111 4.1 141 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2010-07-12 BL149CL 2599 65 2.5 136 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-01-30 BL149BH 2634 167 6.3 137 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-08-09 BL149AE 3071 162 5.3 146 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2006-10-06 BL137J 2814 176 6.3 147 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-10-29 BL123L 2765 135 4.9 151 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-05-13 BL123F 2486 136 5.5 142 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2004-09-11 BL111O 2381 52 2.2 168 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2003-03-01 BL111F 2919 88 3.0 99 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2001-06-20 BZ026 2641 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2001-01-21 BK068H 2402 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2000-08-25 BH068 2726 128 4.7 138 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1999-07-19 BK068B 2351 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1997-03-10 BK048A 2769 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1995-12-15 BK37A 2478 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1995-07-28 BZ014 2662 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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