| Common Name: | TXS 0106+612 | MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie] | VLBA 1.4 GHz: |
| B1950 Name: | 0106+612 |  |
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| J2000 Name: | J0109+6133 | ||
| R.A. and Dec. (J2000): | 1h9m46.344s +61d33'30.456" |
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| AGN Class: | LSP Quasar | ||
| Redshift: | 0.783 (Vandenbroucke et al. 2010, ApJ 718, L166) | Luminosity Distance: | 4893 Mpc ; 7.46 pc/mas |
| Radio Spectrum: | Flat | ||
| Gamma-ray Association | LAT: Y, EGRET: N, TeV: N | ||
| Kpc-scale morphology: | Unknown | ||
| Jet Speed: | Maximum: 468 ± 30 μas/y ; 20.3 ± 1.3 c Median: N/A ; based on 2 moving features Lister et al. 2019, ApJ,874,43 |
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| 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 | |
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Fermi LAT and 15 GHz VLBA Light Curves |
VLBA 43 GHz: |
Multiepoch Radio Spectrum: |
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| Comments: | LAT flaring, ATEL 2414 | ||
![[GIF]](../stackedimages/0106+612.u.stacked.icu.gif){kind=link}
![[GIF]](../stackedimages/0106+612.u.stacked.icd.gif){kind=link}
![[GIF]](../stackedimages/0106+612.u.stacked.icc.gif){kind=link}
![[GIF]](../stackedimages/0106+612.u.stacked.ict.gif){kind=link}
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.
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 |
2013-05-05 | BL178BC | 436 | 16 | 3.8 | 137 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2012-12-23 | BL178AX | 242 | 5.8 | 2.4 | 138 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2012-08-03 | BL178AN | 271 | 7.6 | 2.8 | 154 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2011-10-03 | BL178AA | 386 | 8.2 | 2.1 | 151 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2011-05-21 | BL149DH | 501 | 11 | 2.1 | 133 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2010-11-04 | BL149CV | 417 | 19 | 4.5 | 144 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2010-03-10 | BL149CI | 500 | 1.3 | 0.3 | 60 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS |
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