Common Name:	PMN J0405-1308	MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie]	VLBA 1.4 GHz: University College Cork Program
B1950 Name:	0403-132
J2000 Name:	J0405-1308
R.A. and Dec. (J2000):	4h5m34.003s -13d8'13.691"
AGN Class:	LSP HPQ
Redshift:	0.571 (Marziani et al. 1996, ApJS 104, 37)
Luminosity Distance:	3317 Mpc ; 6.52 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	One-sided
Jet Speed:	Maximum: 623 ± 19 μas/y ; 20.79 ± 0.62 c Median: 504 ± 32 μas/y ; 16.8 ± 1.1 c based on 7 moving features Lister et al. 2019, ApJ, 874, 43
Separation Versus Time Plot:	PNG    PS
Stacked epoch 15 GHz VLBA images: Uniform weight: [PS]   [GIF] Natural weight: [PS]   [GIF] Circular Beam : [PS]   [GIF] Tapered Beam: [PS]   [GIF] Pushkarev et al. 2017 :   FITS Rotation Measure Map: | 2006_05_24 | Spectral Index Map: | 2006_05_24 | Multifrequency MOJAVE VLBA Data: Epoch 8.1 GHz 8.4 GHz 12.1 GHz 2006-05-24 uvf   uvf   uvf		VLBA 23 GHz:	Kpc-scale: Cooper et al. 2007, ApJ Supl 171, 376
Fermi LAT and 15 GHz VLBA Light Curves		VLBA 43 GHz: Cheng et al. 2020	Multiepoch Radio Spectrum:
Comments:	UMRAO 2.5 Jy in 2002; VLA compact morph yet large UMRAO-VLB

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, has 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. All observations after that date have correlated flux densities that are between 10% and 20% too low. The MOJAVE team and NRAO are currently investigating the issue.

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
2012-03-27	BL178AI	783	15	1.9	172	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2010-11-13	BL149CW	887	42	4.7	19	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2010-01-16	BL149CG	738	13	1.8	100	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2009-06-15	BL149BN	941	5.4	0.6	56	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2009-01-07	BL149BG	752	4.2	0.6	33	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2008-07-17	BL149AK	933	58	6.2	9	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2007-07-03	BL149AC	946	52	5.5	48	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2007-02-05	BL137N	1453	71	4.9	76	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2006-05-24	BL137E	1812	57	3.2	29	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2005-09-19	BL123N	1347	16	1.2	48	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2005-02-05	BL123B	1627	14	0.9	136	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2004-12-02	BL111Q	1441	23	1.6	138	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2004-09-11	BL111O	1225	17	1.4	148	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2004-04-10	BL111L	1137	40	3.6	25	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2002-05-31	BL111A	1398	4.4	0.3	18	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
1998-06-05	BG077	1060	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS

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