MOJAVE Sample: 0256+075

Common Name:	OD 94.7	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz: NRAO Archive
B1950 Name:	0256+075
J2000 Name:	J0259+0747
R.A. and Dec. (J2000):	2h59m27.077s +7d47'39.643"
AGN Class:	LSP HPQ
Redshift:	0.893 (1989A&AS...80..103S)
Luminosity Distance:	5762 Mpc ; 7.79 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	Core
Jet Speed:	Maximum: 241 ± 26 μas/y ; 11.6 ± 1.2 c Median: N/A ; based on 3 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:	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:	Robopol main 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, 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
2022-04-08 *	BL286AJ
2021-12-10	BL286AD	646	31	4.8	53	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2021-10-23	BL286AC	732	33	4.5	36	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2021-05-01	BL273K	618	30	4.8	52	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-12-01	BL229BK	595	18	3.0	31	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-10-21	BL273G1	783	11	1.4	49	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-05-25	BL229BE	696	37	5.4	36	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-12-31	BL229BD	745	38	5.1	55	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-10-11	BL273B	738	42	5.7	47	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-06-13	BL229AX	601	29	4.9	46	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2018-11-11	BL229AS	841	86	10.3	46	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2018-04-22	BL229AN	1035	88	8.5	49	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2017-01-28	BL229AE	598	34	5.8	41	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-12-10	BL229AC	698	68	9.8	43	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-11-06	BL229AB	810	96	11.8	41	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-09-26	BL229AA	853	91	10.6	47	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2008-12-05	BG192	465	12	2.6	24	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
2004-11-01	BG152A	386	17	4.4	47	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
2004-09-10	BG144D	395	14	3.6	53	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
2003-03-05	BG128B	351	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
1999-06-17	BG091	381	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS