| Common Name: | PKS 2356+196 | MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie] | VLBA 1.4 GHz: NRAO Archive |
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| B1950 Name: | 2356+196 |  |
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| J2000 Name: | J2358+1955 | ||||||||||||||
| R.A. and Dec. (J2000): | 23h58m46.085s +19d55'20.302" |
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| AGN Class: | LSP Quasar | ||||||||||||||
| Redshift: | 1.05814 (2025arXiv250314745D) | Luminosity Distance: | 7120 Mpc ; 8.15 pc/mas | ||||||||||||
| Radio Spectrum: | Flat | ||||||||||||||
| Gamma-ray Association | LAT: N, EGRET: Y, TeV: N | ||||||||||||||
| Kpc-scale morphology: | Core | ||||||||||||||
| Jet Speed: | Maximum: 29 ± 5 μas/y ; 1.57 ± 0.27 c Median: N/A ; based on 6 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: 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: | Not available | Spectral Index 8-15 GHz Map: | 2006_04_05 | 2006_10_06 Multifrequency MOJAVE VLBA Data:
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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: | EGRET MOJAVE-2 source; Peaked spectrum that does not satisfy GPS criteria | ||||||||||||||
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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