| Common Name: | 3C 66A | MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie] | VLBA 1.4 GHz: |
||||||||||||
| B1950 Name: | 0219+428 |  |
 |
||||||||||||
| J2000 Name: | J0222+4302 | ||||||||||||||
| R.A. and Dec. (J2000): | 2h22m39.611s +43d2'7.799" |
||||||||||||||
| AGN Class: | HSP BL Lac | ||||||||||||||
| Redshift: | 0.34 (2018MNRAS.474.3162T) | Luminosity Distance: | 1784 Mpc ; 4.82 pc/mas | ||||||||||||
| Radio Spectrum: | Flat | ||||||||||||||
| Gamma-ray Association | LAT: Y, EGRET: Y, TeV: Y | ||||||||||||||
| Kpc-scale morphology: | Core Halo | ||||||||||||||
| Jet Speed: | Maximum: 544 ± 38 μas/y ; 11.46 ± 0.79 c Median: N/A ; based on 8 moving features Lister et al. 2021, ApJ,923,30 |
||||||||||||||
| Separation Versus Time Plot: | PNG PDF | ||||||||||||||
| Stacked 15 GHz Stokes I VLBA images: Natural weight: PNG PDF FITS Circular Beam: PNG PDF FITS Tapered Beam: PNG PDF FITS Stacking for 1994-2015: FITS Stacked 15 GHz Polarization VLBA images: Method I: Cumulative GIF, pol PNG, I FITS, P FITS, m FITS, EVPA FITS Method II: std EVPA PNG, FITS Rotation Measure 8-15 GHz Map: | 2006_04_05 | 2006_11_10 Spectral Index 8-15 GHz Map: | 2006_04_05 | 2006_11_10 Multifrequency MOJAVE VLBA Data:
|
VLBA 23 GHz: |
Kpc-scale: Taylor et al. 1996, ApJS 107, 37 | |||||||||||||
|
 |
||||||||||||||
Fermi LAT and 15 GHz VLBA Light Curves |
VLBA 43 GHz: Jorstad et al. 2017 |
Multiepoch Radio Spectrum: |
|||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
 |
 |
||||||||||||||
| Comments: | NED z=0.44 (Miller 78) uncertain; see Bramel 05; 0.3347 < z < 0.41 from Furniss 2013; z > 0.42 from host mag- Stadnik 2014; z=0.34 from cluster Torres-Zafra 2018 | ||||||||||||||
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 team checks and adjusts the flux density scaling of the MOJAVE VLBA data for possible systematics based on near-simultaneous OVRO 40m measurements at 15 GHz. Asterisked entries below denote epochs that have not yet been checked and corrected.
Important Note: The MOJAVE team, working with the OVRO 40m AGN monitoring team checks and adjusts the flux density scaling of the MOJAVE VLBA data for possible systematics based on near-simultaneous OVRO 40m measurements at 15 GHz. Asterisked entries below denote epochs that have not yet been checked and corrected.
| Home | Science | AGN Samples | Data Archive | Status | Publications | Movies | RM Maps | α Maps | People | Outreach |