Common Name:	PKS 1504-167	MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie]	VLBA 1.4 GHz: University College Cork Program
B1950 Name:	1504-166
J2000 Name:	J1507-1652
R.A. and Dec. (J2000):	15h7m4.787s -16d52'30.267"
AGN Class:	LSP HPQ
Redshift:	0.876 (Hunstead et al. 1978, MNRAS 185, 149)
Luminosity Distance:	5625 Mpc ; 7.75 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: N, EGRET: P, TeV: N
Kpc-scale morphology:	Core
Jet Speed:	Maximum: 97 ± 4 μas/y ; 4.61 ± 0.20 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: | 2006_12_01 | Spectral Index Map: | 2006_12_01 | Multifrequency MOJAVE VLBA Data: Epoch 8.1 GHz 8.4 GHz 12.1 GHz 2006-12-01 uvf   uvf   uvf		VLBA 23 GHz:	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:	HB89 catalog lists it as 1504-166; sometimes called 1504-167

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
2010-10-25	BL149CT	736	4.9	0.7	118	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2008-09-12	BL149BC	1028	7.6	0.7	118	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2006-12-01	BL137L	1164	22	1.8	158	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2005-09-16	BL123M	1608	21	1.3	116	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2005-07-24	BL123J	1558	20	1.3	116	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2004-06-11	BL111M	1684	11	0.6	105	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2003-02-05	BL111E	1610	19	1.2	69	FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS	PNG   PS
2000-01-11	BK068D	2191	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS
1997-08-18	BZ022	1807	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS
1996-05-02	BE10B	1498	no data			FITS   PNG   PS	FITS   PNG   PS	PNG   PS	uvf	PNG   PS

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