| Common Name: | OH 471 | MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie] | VLBA 1.4 GHz: University College Cork Program |
||||||||||||||||||
| B1950 Name: | 0642+449 |  |
 |
||||||||||||||||||
| J2000 Name: | J0646+4451 | ||||||||||||||||||||
| R.A. and Dec. (J2000): | 6h46m32.026s +44d51'16.590" |
||||||||||||||||||||
| AGN Class: | LSP Quasar | ||||||||||||||||||||
| Redshift: | 3.396 (Osmer et al. 1994, ApJ 436, 678) | Luminosity Distance: | 30023 Mpc ; 7.53 pc/mas | ||||||||||||||||||
| Radio Spectrum: | Flat | ||||||||||||||||||||
| Gamma-ray Association | LAT: , EGRET: N, TeV: N | ||||||||||||||||||||
| Kpc-scale morphology: | Core | ||||||||||||||||||||
| Jet Speed: | Maximum: 79 ± 4 μas/y ; 8.52 ± 0.42 c Median: N/A ; based on 4 moving features Lister et al. 2019, ApJ,874,43 |
||||||||||||||||||||
| Separation Versus Time Plot: | PNG PDF | ||||||||||||||||||||
| Stacked 15 GHz Stokes I VLBA images: Uniform weight: PNG PDF Natural weight: PNG PDF Circular Beam: PNG PDF Tapered Beam: PNG PDF 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_10_06 | Spectral Index 8-15 GHz Map: | 2006_10_06 | Multifrequency MOJAVE VLBA Data:
Univ. College Cork VLBA L Band Data:
|
VLBA 23 GHz: RRIFD Database |
Kpc-scale: Cooper et al. 2007, ApJ Supl 171, 376 | |||||||||||||||||||
 |
 |
||||||||||||||||||||
Fermi LAT and 15 GHz VLBA Light Curves |
VLBA 43 GHz: |
Multiepoch Radio Spectrum: |
|||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
 |
 |
||||||||||||||||||||
| Comments: | HFP; non-GPS based on variability and pol; Arsioli 2018 claims LAT detection | ||||||||||||||||||||
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 |