Common Name:	S4 0003+38	MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie]	VLBA 1.4 GHz: BG246
B1950 Name:	0003+380
J2000 Name:	J0005+3820
R.A. and Dec. (J2000):	0h5m57.175s +38d20'15.149"
AGN Class:	LSP Quasar
Redshift:	0.229 (1994A&AS..103..349S)
Luminosity Distance:	1131 Mpc ; 3.63 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	Core
Jet Speed:	Maximum: 317 ± 25 μas/y ; 4.61 ± 0.36 c Median: N/A ; based on 5 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: | 2006_12_01 | Spectral Index Map: | 2006_03_09 | 2006_12_01 Multifrequency MOJAVE VLBA Data: Epoch 8.1 GHz 8.4 GHz 12.1 GHz 2006-12-01 uvf   uvf   uvf   2006-03-09 uvf   FITS   PS   PNG   uvf   FITS   PS   PNG   uvf   FITS   PS   PNG		VLBA 23 GHz:	Kpc-scale: Caltech-Jodrell Flat-Spectrum Survey
Fermi LAT and 15 GHz VLBA Light Curves		VLBA 43 GHz:	Multiepoch Radio Spectrum:
Comments:	Low-luminosity MOJAVE-2 source; Seyfert in NED; possible spiral host in Zhao et al. 2021

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
2013-08-12	BL178BH	669	9.7	1.5	139	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2011-06-06	BL149DJ	605	2.1	0.3	108	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2010-07-12	BL149CL	438	10	2.4	132	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2009-03-25	BL149BJ	435	10	2.3	145	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2008-07-17	BL149AK	726	17	2.3	175	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2008-05-01	BL149AO	807	12	1.5	178	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2007-08-24	BL149AM	554	7.3	1.3	166	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2007-03-28	BL137P	604	5.6	0.9	144	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2006-12-01	BL137L	512	9.2	1.8	146	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2006-03-09	BL137B	650	16	2.5	78	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS

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