MOJAVE Sample: 0507+179

Common Name:	PKS 0507+17	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz: 2017MNRAS.467...83K
B1950 Name:	0507+179
J2000 Name:	J0510+1800
R.A. and Dec. (J2000):	5h10m2.369s +18d0'41.582"
AGN Class:	LSP Quasar
Redshift:	0.416 (1998AJ....115.1253P)
Luminosity Distance:	2264 Mpc ; 5.47 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	Core
Jet Speed:	Maximum: 200 ± 12 μas/y ; 5.04 ± 0.29 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: [PDF] [GIF] Natural weight: [PDF] [GIF] Circular Beam : [PDF] [GIF] Tapered Beam: [PDF] [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: Cheng et al. 2020	Multiepoch Radio Spectrum:
Fermi LAT and 15 GHz VLBA Light Curves
Comments:	LAT flaring April 2013 ATEL 5001

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
2022-03-18 *	BL286AI	1855	70	3.8	161	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2021-09-13	BL286AB	2042	26	1.3	12	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-07-02	BL229BG	1993	30	1.5	124	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-01-19	BL229AU	1961	31	1.6	112	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2018-10-06	BL229AR	1920	39	2.1	114	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2018-05-31	BL229AO	2185	65	3.0	151	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2017-08-25	BL229AK	1739	57	3.3	102	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2017-04-22	BL229AG	2701	20	0.8	148	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2017-03-11	BL229AF	2620	56	2.1	128	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2017-01-03	BL229AD	2389	18	0.7	125	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-12-10	BL229AC	2366	57	2.4	152	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-11-06	BL229AB	2495	53	2.1	152	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-09-26	BL229AA	2344	12	0.5	119	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2007-05-03	BK134D	862	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS