| Common Name: | OK 492 | MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie] | VLBA 1.4 GHz: BG246 |
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| B1950 Name: | 0955+476 |  |
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| J2000 Name: | J0958+4725 | ||||||||||||||||||||
| R.A. and Dec. (J2000): | 9h58m19.672s +47d25'7.842" |
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| AGN Class: | LSP HPQ | ||||||||||||||||||||
| Redshift: | 1.88413 (2020ApJS..249....3A) | Luminosity Distance: | 14616 Mpc ; 8.52 pc/mas | ||||||||||||||||||
| Radio Spectrum: | Flat | ||||||||||||||||||||
| Gamma-ray Association | LAT: Y, EGRET: N, TeV: N | ||||||||||||||||||||
| Kpc-scale morphology: | One-sided | ||||||||||||||||||||
| Jet Speed: | Maximum: 90 ± 10 μas/y ; 7.25 ± 0.80 c Median: N/A ; based on 4 moving features Lister et al. 2019, ApJ,874,43 |
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| 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_11_10 | Spectral Index 8-15 GHz Map: | 2006_11_10 | Multifrequency MOJAVE VLBA Data:
Univ. College Cork VLBA L Band Data:
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VLBA 23 GHz: RRIFD Database |
Kpc-scale: Kharb et al., in prep. | |||||||||||||||||||
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Fermi LAT and 15 GHz VLBA Light Curves |
VLBA 43 GHz: |
Multiepoch Radio Spectrum: |
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| Comments: | Ratan spectrum looks like HFP | ||||||||||||||||||||
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.
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