MOJAVE Sample: 0202-172

Common Name:	PKS 0202-17	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz: BG246
B1950 Name:	0202-172
J2000 Name:	J0204-1701
R.A. and Dec. (J2000):	2h4m57.674s -17d1'19.841"
AGN Class:	LSP Quasar
Redshift:	1.739 (Jones et al. 2009, MNRAS, 399, 683)
Luminosity Distance:	13234 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: 257 ± 57 μas/y ; 19.6 ± 4.4 c Median: N/A ; based on 3 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:	Kpc-scale: Kharb et al., in prep.

Fermi LAT and 15 GHz VLBA Light Curves	VLBA 43 GHz: Cheng et al. 2020	Multiepoch Radio Spectrum:

Comments:	MOJAVE 1.5 Jy; OVRO > 1.5 Jy

Common Name:

PKS 0202-17

MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie]

VLBA 1.4 GHz: BG246

R.A. and Dec. (J2000):

2h4m57.674s
-17d1'19.841"

AGN Class:

LSP Quasar

Redshift:

1.739 (Jones et al. 2009, MNRAS, 399, 683)

Luminosity Distance:

13234 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: 257 ± 57 μas/y ; 19.6 ± 4.4 c
Median: N/A ;
based on 3 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:

Kpc-scale: Kharb et al., in prep.

Fermi LAT and 15 GHz VLBA Light Curves

VLBA 43 GHz: Cheng et al. 2020

Multiepoch Radio Spectrum:

Comments:

MOJAVE 1.5 Jy; 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
2013-07-08	BL178BE	1853	33	1.8	116	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-03-04	BL178AH	1318	23	1.7	137	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2010-11-04	BL149CV	1199	36	3.0	111	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2010-01-16	BL149CG	1328	34	2.6	109	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2009-07-05	BL149BP	1451	66	4.5	97	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS