Common Name: S5 0454+84 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz: NRAO Archive
B1950 Name: 0454+844 2 cm VLBA Image map
J2000 Name: J0508+8432
R.A. and Dec. (J2000): 5h8m42.364s
+84d32'4.544"
AGN Class: LSP BL Lac
Redshift: 0.112 (2012RMxA&A..48....9T)
Luminosity Distance: 514 Mpc ; 2.01 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology: Core
Jet Speed: Maximum: 109 25 μas/y ; 0.80 0.18 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: | 2006_03_09 |


Multifrequency MOJAVE VLBA Data:

Epoch
8.1 GHz
8.4 GHz
12.1 GHz
2006-03-09
uvf  
uvf  
uvf  

VLBA 23 GHz:
Kpc-scale: Rector and Stocke 2001, AJ 122, 565
23 GHz Image
Kpc Image

Fermi LAT and 15 GHz VLBA Light Curves

Fermi LAT and 15 GHz VLBA Light Curves
VLBA 43 GHz: Lister and Smith 2000, ApJ 541,66
Multiepoch Radio Spectrum:
43 GHz Image
Radio Spectrum
Comments: NED z =1.340 from Rector and Stocke 2001 is a lower limit; z=0.113 from Lawrence et al. 1996 is tentative; was unusual kinematics source

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
2009-12-17 BL149CE 185 5.5 3.0 32 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-06-03 BL149BM 202 7.2 3.6 41 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2008-09-12 BL149BC 215 5.6 2.6 59 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2006-03-09 BL137B 267 8.9 3.3 64 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2004-04-12 BG144B 317 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2002-08-24 BG121E 332 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2001-12-30 BR077E 330 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2001-03-04 BK068E 264 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2001-01-13 BM142A 250 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2000-06-15 BM123 227 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1999-07-26 BM114B 172 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1999-07-19 BK068B 193 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1997-08-28 BK052A 214 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1997-02-09 BG063 262 5.6 2.1 3 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1996-07-10 BK037C 236 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1996-05-16 BK037B 309 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
1994-08-31 BZ004 332 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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