Common Name: S5 0014+813 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz:
B1950 Name: 0014+813 2 cm VLBA Image map
J2000 Name: J0017+8135
R.A. and Dec. (J2000): 0h17m8.475s
+81d35'8.136"
AGN Class: LSP Quasar
Redshift: 3.382 (1987AZh....64..262V)
Luminosity Distance: 29874 Mpc ; 7.54 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: N, EGRET: N, TeV: N
Kpc-scale morphology: Core
Jet Speed: Maximum: 88 8 μas/y ; 9.47 0.91 c
Median: N/A ;
based on 3 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]

Rotation Measure Map: | Not available |

Spectral Index Map: | Not available |


VLBA 23 GHz:
Kpc-scale: Xu et al. 1995, ApJS 99, 297
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: Robopol control sample

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
2021-08-07 * BL286AA
2021-05-01 * BL273K
2021-01-11 * BL273I 1046 12 1.1 33 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2020-08-30 * BL229BI 925 5.7 0.6 21 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2020-06-13 * BL229BF 921 13 1.4 15 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2020-02-16 * BL273D 938 19 2.0 5 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2019-12-22 * BL229BC 923 20 2.2 176 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2019-12-17 * BL273C 872 11 1.3 20 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2019-06-29 BL229AY 1077 27 2.5 2 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2019-01-19 BL229AU 957 26 2.7 177 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2018-11-11 BL229AS 963 27 2.8 177 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2018-07-08 BL229AP 849 20 2.4 175 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2018-02-02 BL229AM 904 11 1.2 178 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2017-11-18 BL229AL 922 7.1 0.8 171 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2017-06-17 BL229AI 853 10 1.2 171 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2017-01-28 BL229AE 828 10 1.2 168 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2016-12-10 BL229AC 809 12 1.5 169 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2016-11-06 BL229AB 875 13 1.5 167 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2016-09-26 BL229AA 882 12 1.3 164 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
1999-01-02 BG077D 488 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1996-06-12 BK042 646 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1996-04-23 BE10A 643 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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