MOJAVE Sample: 0502+049

Common Name:	PKS 0502+049	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz:
B1950 Name:	0502+049
J2000 Name:	J0505+0459
R.A. and Dec. (J2000):	5h5m23.185s +4d59'42.725"
AGN Class:	LSP Quasar
Redshift:	0.954 (Drinkwater et al. 1997, MNRAS, 284, 85)
Luminosity Distance:	6256 Mpc ; 7.94 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	Core
Jet Speed:	Maximum: 186 ± 21 μas/y ; 9.4 ± 1.1 c Median: N/A ; based on 5 moving features Lister et al. 2021, ApJ,923,30
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: RRIFD Database	Kpc-scale: Healey et al. 2007, ApJS 171, 61

Fermi LAT and 15 GHz VLBA Light Curves		VLBA 43 GHz:	Multiepoch Radio Spectrum:
Fermi LAT and 15 GHz VLBA Light Curves
Comments:	LAT_3FM source; LAT flaring Aug 2011 ATEL 3573, Mar 2013 ATEL 4858

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
2020-12-24 *	BL229BL	767	23	3.0	128	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-12-01	BL229BK	790	20	2.5	132	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-08-01	BL229BH	1035	40	3.9	126	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-05-25	BL229BE	927	17	1.8	135	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-07-19	BL229AZ	1086	21	1.9	150	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-04-15	BL229AV	658	20	3.1	141	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2018-11-11	BL229AS	731	20	2.8	134	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2018-08-19	BL229AQ	947	26	2.7	140	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2018-04-22	BL229AN	952	29	3.0	137	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2017-01-28	BL229AE	948	15	1.6	140	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-12-10	BL229AC	928	16	1.7	119	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-11-06	BL229AB	982	17	1.7	143	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-09-26	BL229AA	846	22	2.6	126	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS