MOJAVE Sample: 1128+385

Common Name:	IVS B1128+385	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz: BG246
B1950 Name:	1128+385
J2000 Name:	J1130+3815
R.A. and Dec. (J2000):	11h30m53.283s +38d15'18.547"
AGN Class:	LSP Quasar
Redshift:	1.741 (2010AJ....139.2360S)
Luminosity Distance:	13252 Mpc ; 8.55 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	One-sided
Jet Speed:	Maximum: 61 ± 11 μas/y ; 4.66 ± 0.83 c Median: N/A ; based on 4 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: \| Not available \| Spectral Index Map: \| Not available \|		VLBA 23 GHz: RRIFD Database	Kpc-scale: Murphy, Browne and Perley 1993, MNRAS, 264, 298

Fermi LAT and 15 GHz VLBA Light Curves		VLBA 43 GHz: Cheng et al. 2018	Multiepoch Radio Spectrum:
Fermi LAT and 15 GHz VLBA Light Curves
Comments:	MOJAVE 1.5 Jy; Compact VLA (MPB93), OVRO > 1.5 Jy

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
2022-01-03 *	BL286AE	2014	21	1.0	134	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2013-02-10	BL178AZ	1330	58	4.4	174	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-11-21	BL178AT	1518	56	3.7	177	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-03-04	BL178AH	1334	50	3.7	175	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2011-08-26	BL149DP	1333	34	2.6	161	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2011-04-11	BL149DF	1375	30	2.2	168	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2010-10-15	BL149CS	1432	44	3.0	150	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2010-02-20	BD147B	1298	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
2001-03-04	BK068E	1129	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
1999-01-02	BG077D	761	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
1997-08-28	BK052A	691	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
1996-07-10	BK037C	1013	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
1996-05-16	BK037B	914	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
1995-12-15	BK37A	798	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
1995-04-07	BK016	874	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS
1995-01-20	BP14	728	no data			FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS