Common Name: PKS 1036+054 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz: University College Cork Program
B1950 Name: 1036+054 2 cm VLBA Image map
J2000 Name: J1038+0512
R.A. and Dec. (J2000): 10h38m46.780s
+5d12'29.086"
AGN Class: LSP Quasar
Redshift: 0.473 (Healey et al. 2008, ApJS 175, 97)
Luminosity Distance: 2640 Mpc ; 5.90 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology: Two-sided
Jet Speed: Maximum: 223 46 μas/y ; 6.3 1.3 c
Median: N/A ;
based on 2 moving features
Lister et al. 2021, ApJ, in press
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_05_24 |


Multifrequency MOJAVE VLBA Data:

Epoch
8.1 GHz
8.4 GHz
12.1 GHz
2006-05-24
uvf  
uvf  
uvf  

VLBA 23 GHz:
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: Spectrum looks rather like a HFP but highly variable (RATAN); Arsioli 2018 claims LAT detection

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 1169 47 4.0 52 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-10-03 BL178AA 1133 59 5.2 61 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2010-09-27 BL149CQ 1158 39 3.4 31 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2010-06-27 BH152B 1512 14 1.0 5 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2008-10-03 BL149BD 1485 58 3.9 143 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2008-02-21 BG176F 1289 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2008-01-11 BG176E 1350 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2007-08-31 BG176B 1549 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2007-07-18 BG176A 1469 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2006-05-24 BL137E 1636 91 5.6 139 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-11-17 BH133 1660 51 3.1 123 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2005-09-23 BL123O 1674 40 2.4 113 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-06-03 BL123H 1548 16 1.0 143 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2004-10-18 BL111P 1533 69 4.5 132 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2003-05-09 BL111H 2631 66 2.5 146 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2002-05-31 BL111A 2664 37 1.4 74 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
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