| Common Name: | CTD 93 | MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie] | VLBA 1.4 GHz: |
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| B1950 Name: | 1607+268 |  |
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| J2000 Name: | J1609+2641 | ||||||||||
| R.A. and Dec. (J2000): | 16h9m13.321s +26d41'29.036" |
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| AGN Class: | G | ||||||||||
| Redshift: | 0.473 (2007A&A...463...97L) | Luminosity Distance: | 2640 Mpc ; 5.90 pc/mas | ||||||||
| Radio Spectrum: | GPS1 | ||||||||||
| Gamma-ray Association | LAT: N, EGRET: N, TeV: N | ||||||||||
| Kpc-scale morphology: | Core | ||||||||||
| Jet Speed: | Maximum: 8 ± 5 μas/y ; 0.23 ± 0.15 c Median: N/A ; based on 7 moving features Lister et al. 2021, ApJ,923,30 |
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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: |
Kpc-scale: Spencer 89, MNRAS 240,657 | |||||||||
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| Fermi LAT and 15 GHz VLBA Light Curves |
VLBA 43 GHz: |
Multiepoch Radio Spectrum: |
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| Comments: | GPS MOJAVE-2 source;Not listed in Veron-Cetty and Veron (2001) ;sometimes called CSS variable at high freqs;VLA data in SP89 | ||||||||||
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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