MOJAVE Sample: 0044+566

Common Name:	GB6 J0047+5657	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz:
B1950 Name:	0044+566
J2000 Name:	J0047+5657
R.A. and Dec. (J2000):	0h47m0.429s +56d57'42.395"
AGN Class:	LSP BL Lac
Redshift:	0.747 (Sowards-Emmerd et al. 2005,ApJ,626,95)
Luminosity Distance:	4616 Mpc ; 7.33 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	Unknown
Jet Speed:	Maximum: 21 ± 3 μas/y ; 0.86 ± 0.13 c Median: N/A ; based on 4 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: \| Not available \|		VLBA 23 GHz:	Kpc-scale:

Fermi LAT and 15 GHz VLBA Light Curves		VLBA 43 GHz:	Multiepoch Radio Spectrum:
Fermi LAT and 15 GHz VLBA Light Curves
Comments:	z = 0.747 listed as uncertain in Sowards-Emmerd 2005

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
2020-11-21 *	BL273H	192	15	8.0	21	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-05-08 *	BL273E1	163	15	9.5	24	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-04-09 *	BL273E	160	12	7.7	23	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-12-17 *	BL273C	125	6.8	5.4	35	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-06-13	BL229AX	134	5.2	3.9	19	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-07-16	BL193BH	215	25	11.8	8	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2015-11-25	BL193AY	206	16	7.9	1	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2015-09-06	BL193AW	170	12	7.2	18	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2015-07-20	BL193AU	164	9.0	5.5	19	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2014-12-12	BL193AP	203	7.7	3.8	14	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2014-09-01	BL193AN	217	9.9	4.6	16	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2014-05-12	BL193AI	194	7.0	3.6	17	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2014-01-25	BL193AE	163	3.9	2.4	16	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS