| Common Name: | 4C +06.41 | MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie] | VLBA 1.4 GHz: University College Cork Program |
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| B1950 Name: | 1038+064 |  |
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| J2000 Name: | J1041+0610 | ||||||||||||||||||||
| R.A. and Dec. (J2000): | 10h41m17.162s +6d10'16.924" |
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| AGN Class: | LSP Quasar | ||||||||||||||||||||
| Redshift: | 1.265 (1991ApJ...382..433S) | Luminosity Distance: | 8901 Mpc ; 8.41 pc/mas | ||||||||||||||||||
| Radio Spectrum: | Flat | ||||||||||||||||||||
| Gamma-ray Association | LAT: N, EGRET: N, TeV: N | ||||||||||||||||||||
| Kpc-scale morphology: | One-sided | ||||||||||||||||||||
| Jet Speed: | Maximum: 158 ± 13 μas/y ; 9.85 ± 0.83 c Median: 81 ± 5 μas/y ; 5.02 ± 0.34 c based on 5 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, I FITS, P FITS, m FITS, EVPA FITS Method II: std EVPA 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:
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VLBA 23 GHz: |
Kpc-scale: Hintzen, Ulvestad and Owen 1983, AJ 88 , 709 | |||||||||||||||||||
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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: | 2LAC id likely incorrect, see Maselli 2015; possible neutrino assoc in 2019ApJ...880..103G | ||||||||||||||||||||
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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