Common Name: TXS 0241+622 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz: BG246
B1950 Name: 0241+622 2 cm VLBA Image map
J2000 Name: J0244+6228
R.A. and Dec. (J2000): 2h44m57.697s
+62d28'6.516"
AGN Class: LSP Quasar
Redshift: 0.045 (Marziani et al. 2003)
Luminosity Distance: 197 Mpc ; 0.87 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: N, EGRET: N, TeV: N
Kpc-scale morphology: Core
Jet Speed: Maximum: 521 30 μas/y ; 1.549 0.088 c
Median: N/A ;
based on 2 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: | Not available |

Spectral Index Map: | 2006_04_05 |


Multifrequency MOJAVE VLBA Data:

Epoch
8.1 GHz
8.4 GHz
12.1 GHz
2006-04-05
uvf  
uvf  
uvf  

VLBA 23 GHz: RRIFD Database
Kpc-scale: Hutchings et al. 1982, ApJ 262, 48
23 GHz Image
Kpc Image

Fermi LAT and 15 GHz VLBA Light Curves

Fermi LAT and 15 GHz VLBA Light Curves
VLBA 43 GHz: Cheng et al. 2020
Multiepoch Radio Spectrum:
43 GHz Image
Radio Spectrum
Comments: Promoted 1.5 Jy; Low-L, low-b quasar, VCV classify as Sy1.2, Corbin 1997 finds broad Halpha

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
2012-12-23 BL178AX 1016 1.3 0.1 116 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2012-03-27 BL178AI 1040 1.1 0.1 1 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2011-04-11 BL149DF 1285 1.4 0.1 7 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2010-07-12 BL149CL 1841 2.8 0.2 171 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-10-27 BL149CC 1619 4.3 0.3 162 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-06-03 BL149BM 2086 3.3 0.2 157 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2008-08-06 BL149BA 2310 4.1 0.2 1 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-08-16 BL149AF 1688 4.6 0.3 148 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-06-10 BL149AB 1580 1.7 0.1 140 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2007-02-22 BA068F 1726 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2007-01-06 BL137R 1485 2.2 0.1 31 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2006-04-05 BL137C 604 4.7 0.8 169 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2005-10-19 BD105D 513 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2004-08-11 BA068E 1220 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2004-05-02 BA068D 1256 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2003-10-07 BA068B 752 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2003-07-13 BA068A 909 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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