| Common Name: | PKS 2126-158 | MOJAVE 15 GHz [Total intensity movie] | | VLBA 1.4 GHz: |
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| B1950 Name: | 2126-158 |  |
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| J2000 Name: | J2129-1538 | ||||||||||
| R.A. and Dec. (J2000): | 21h29m12.176s -15d38'41.042" |
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| AGN Class: | LSP Quasar | ||||||||||
| Redshift: | 3.291 (2022arXiv220712432K) | Luminosity Distance: | 28908 Mpc ; 7.61 pc/mas | ||||||||
| Radio Spectrum: | Flat | ||||||||||
| Gamma-ray Association | LAT: N, EGRET: N, TeV: N | ||||||||||
| Kpc-scale morphology: | Unknown | ||||||||||
| Jet Speed: | Maximum: 37 ± 4 μas/y ; 3.97 ± 0.45 c Median: N/A ; based on 1 moving feature 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: Rotation Measure 8-15 GHz Map: | Not available | Spectral Index 8-15 GHz Map: | 2006_04_28 | Multifrequency MOJAVE VLBA Data:
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VLBA 23 GHz: RRIFD Database |
Kpc-scale: di Serego-Alighieri et al. 1994, MNRAS, 269, 998 | |||||||||
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| Fermi LAT and 15 GHz VLBA Light Curves |
VLBA 43 GHz: Cheng et al. 2020 |
Multiepoch Radio Spectrum: |
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| Comments: | Added to MOJAVE since Jauncey says high CP; Torniainen 2008 claim GPS but has flux variability | ||||||||||
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.
| Epoch (YYYY-MM-DD) | VLBA Code | VLBA I (mJy) |
VLBA P (mJy) |
VLBA P (%) |
VLBA EVPA (deg.) |
I Image (Nat. Weight) | Visibility Data |
Stokes I Radplot | Polarization Image |
Full Montage |
2011-09-12 | BL149DQ | 728 | 0.9 | 0.1 | 119 | FITS PNG PDF | UVF | PNG PDF | p:PNG p:PDF f:PNG f:PDF | PNG | 2008-11-19 | BL149BE | 779 | 0.9 | 0.1 | 39 | FITS PNG PDF | UVF | PNG PDF | p:PNG p:PDF f:PNG f:PDF | PNG | 2006-04-28 | BL137D | 1233 | 2.9 | 0.2 | 104 | FITS PNG PDF | UVF | PNG PDF | p:PNG p:PDF f:PNG f:PDF | PNG | 2000-05-05 | BK074 | 1012 | no data | FITS PNG PDF | UVF | PNG PDF | PNG | 1998-12-05 | BG077C | 1142 | no data | FITS PNG PDF | UVF | PNG PDF | PNG | 1998-09-29 | BG077B | 1225 | no data | FITS PNG PDF | UVF | PNG PDF | PNG | 1996-04-22 | BS036 | 776 | no data | FITS PNG PDF | UVF | PNG PDF | PNG |
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