Common Name:	B3 1758+388B	MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie]	VLBA 1.4 GHz: University College Cork Program
B1950 Name:	1758+388
J2000 Name:	J1800+3848
R.A. and Dec. (J2000):	18h0m24.765s +38d48'30.697"
AGN Class:	LSP Quasar
Redshift:	2.092 (1994A&AS..103..349S)
Luminosity Distance:	16634 Mpc ; 8.43 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: N, EGRET: N, TeV: N
Kpc-scale morphology:	Core
Jet Speed:	Maximum: 25 ± 2 μas/y ; 2.11 ± 0.18 c Median: N/A ; based on 2 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: | 2006_11_10 | Multifrequency MOJAVE VLBA Data: Epoch 8.1 GHz 8.4 GHz 12.1 GHz 2006-11-10 uvf   uvf   uvf		VLBA 23 GHz:	Kpc-scale: Caltech-Jodrell Flat-Spectrum Survey
Fermi LAT and 15 GHz VLBA Light Curves		VLBA 43 GHz:	Multiepoch Radio Spectrum:
Comments:	D00 call it a HFP; Edelson 1987 fluxes confirm it; non-GPS based on variability and pol.

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	406	1.3	0.3	64	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2011-07-15	BL149DM	908	14	1.5	53	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2009-05-02	BL149BK	1205	20	1.7	36	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2008-06-25	BL149AJ	1120	28	2.5	43	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2006-11-10	BL137K	1139	18	1.5	47	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2006-01-05	BG161	1050	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS
2005-12-22	BL123Q	1109	23	2.1	42	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2005-06-03	BL123H	1064	23	2.2	38	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2004-12-02	BL111Q	1070	34	3.2	31	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2003-05-09	BL111H	1384	22	1.6	32	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2001-12-30	BR077H	1042	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS
1998-10-30	BK052D	1269	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS
1997-08-28	BK052A	1378	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS
1996-05-16	BK037B	1781	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS
1995-04-07	BK016	1433	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS
1995-01-20	BP14	1186	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS

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