MOJAVE Sample: 0238+711

Common Name:	S5 0238+711	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz:
B1950 Name:	0238+711
J2000 Name:	J0243+7120
R.A. and Dec. (J2000):	2h43m30.891s +71d20'17.904"
AGN Class:	ISP BL Lac
Redshift:	Unknown
Luminosity Distance:	Unknown
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	Core
Jet Speed:	Maximum: 124 ± 7 μas/y ; 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] Pushkarev et al. 2017 : FITS 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:	Hard spectrum LAT source added to MOJAVE_2

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
2022-06-11 *	BL286AL
2022-02-24 *	BL286AH	124	2.4	1.9	62	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2021-08-07	BL286AA	120	2.9	2.4	33	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2021-03-02	BL273J	112	2.5	2.2	38	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-08-30	BL229BI	126	5.3	4.2	40	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-05-08	BL273E1	119	1.3	1.1	86	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-04-09	BL273E	123	2.1	1.7	78	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-12-17	BL273C	127	1.1	0.9	76	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-04-15	BL229AV	145	4.0	2.8	40	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2018-10-06	BL229AR	165	3.2	1.9	80	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2017-11-18	BL229AL	122	2.8	2.3	57	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2017-06-17	BL229AI	114	1.4	1.2	39	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-11-18	BL193BM	124	1.4	1.1	40	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-06-09	BL193BF	116	4.2	3.6	80	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-01-22	BL193BB	128	3.5	2.7	71	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2015-08-11	BL193AV	121	< 0.5	< 4.5		FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2014-11-17	BL193AO	161	1.7	1.1	29	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2014-01-25	BL193AE	139	3.5	2.5	37	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2013-07-22	BL178BF	148	2.9	2.0	27	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2013-01-21	BL178AY	168	6.1	3.6	38	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-11-28	BL178AU	157	6.4	4.1	52	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-09-02	BL178AO	176	5.6	3.2	43	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-03-27	BL178AI	206	7.6	3.7	38	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS