Common Name: PKS 0539-057 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz: BG246
B1950 Name: 0539-057 2 cm VLBA Image map
J2000 Name: J0541-0541
R.A. and Dec. (J2000): 5h41m38.083s
-5d41'49.428"
AGN Class: LSP Quasar
Redshift: 0.838 (Shaw et al. 2012, ApJ, 748, 49)
Luminosity Distance: 5323 Mpc ; 7.64 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology: Unknown
Jet Speed: Maximum: 301 46 μas/y ; 13.8 2.1 c
Median: N/A ;
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: [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: NVSS
23 GHz Image
Kpc Image

Fermi LAT and 15 GHz VLBA Light Curves

Fermi LAT and 15 GHz VLBA Light Curves
VLBA 43 GHz:
Multiepoch Radio Spectrum:
43 GHz Image
Radio Spectrum
Comments: New 1.5 Jy; AT 20 GHz indicates > 1.5 Jy; in 1FGL but not 2FGL, 3FGL, FL8Y

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
2022-05-21 * BL286AK
2021-12-10 BL286AD 629 11 1.8 47 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-12-29 BL178AD 720 16 2.3 60 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-10-03 BL178AA 648 18 2.8 62 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-07-24 BL149DN 581 22 3.7 64 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-03-05 BL149DD 691 17 2.5 57 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2010-11-20 BL149CX 858 31 3.6 61 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2010-08-06 BL149CM 833 41 4.9 49 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2004-12-11 BB174E 975 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2004-10-15 BB174D 893 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2004-06-12 BB174C 863 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2004-04-08 BB174F 753 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2004-04-02 BB174B 811 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2003-12-22 BB174A 613 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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