Common Name:	PKS 1124-186	MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie]	VLBA 1.4 GHz: University College Cork Program
B1950 Name:	1124-186
J2000 Name:	J1127-1857
R.A. and Dec. (J2000):	11h27m4.392s -18d57'17.442"
AGN Class:	LSP HPQ
Redshift:	1.048 (Drinkwater et al. 1997, MNRAS, 284, 85)
Luminosity Distance:	7035 Mpc ; 8.13 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	One-sided
Jet Speed:	Maximum: 152 ± 19 μas/y ; 8.3 ± 1.0 c Median: N/A ; based on 3 moving features Lister et al. 2013,AJ,146,120
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: | 2006_11_10 | 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   Univ. College Cork VLBA L Band Data: Epoch 1.35 GHz 1.4 GHz 1.5 GHz 1.7 GHz 2010-03-07 uvf   uvf		VLBA 23 GHz: RRIFD Database	Kpc-scale: Kharb, Lister, and Cooper 2010, ApJ 710, 764
Fermi LAT and 15 GHz VLBA Light Curves		VLBA 43 GHz: Cheng et al. 2020	Multiepoch Radio Spectrum:
Comments:	Dropped from MOJAVE-2 since too compact; Ratan spectrum looks like HFP; but NED and others say Flat

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
2011-04-11	BL149DF	1845	17	0.9	125	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2011-02-27	BL149DC	2447	16	0.6	95	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2010-11-04	BL149CV	2271	6.2	0.3	13	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2010-06-19	BL149CK	1883	30	1.6	82	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2009-10-27	BL149CC	1636	55	3.4	0	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2009-07-23	BL149BQ	1650	9.7	0.6	31	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2009-05-02	BL149BK	1739	35	2.0	105	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2009-02-25	BL149BI	1647	35	2.1	138	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2006-11-10	BL137K	1300	49	3.8	59	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2005-10-29	BL123L	2292	94	4.1	31	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2005-05-13	BL123F	1862	48	2.6	39	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2004-08-09	BL111N	1816	70	3.8	40	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2003-03-01	BL111F	1416	29	2.1	23	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2002-05-29	BR077P	1351	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS
1998-11-01	BK052E	2892	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS

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