Common Name: S5 1044+71 MOJAVE 15 GHz [Total intensity movie]   | [Polariz. movie] VLBA 1.4 GHz: NRAO Archive
B1950 Name: 1044+719 2 cm VLBA Image map
J2000 Name: J1048+7143
R.A. and Dec. (J2000): 10h48m27.620s
+71d43'35.938"
AGN Class: LSP HPQ
Redshift: 1.15 (1996A&AS..115...11S)
Luminosity Distance: 7901 Mpc ; 8.29 pc/mas
Radio Spectrum: Flat
Gamma-ray Association LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology: Two-sided
Jet Speed: Maximum: 74 ± 24 μas/y ; 4.3 ± 1.4 c
Median: N/A ;
based on 1 moving feature
Lister et al. 2019, ApJ,874,43
Separation Versus Time Plot: PNG   
Stacked epoch 15 GHz VLBA images:
Uniform weight: [PDF]   [GIF]
Natural weight: [PDF]   [GIF]
Circular Beam : [PDF]   [GIF]
Tapered Beam: [PDF]   [GIF]
Animated Polarization: [GIF]
Pushkarev et al. 2017 :   FITS

Rotation Measure Map: | Not available |

Spectral Index Map: | Not available |


VLBA 23 GHz:
Kpc-scale: Caltech-Jodrell Flat-Spectrum Survey
23 GHz Image
Kpc Image

Fermi LAT and 15 GHz VLBA Light Curves

Fermi LAT and 15 GHz VLBA Light Curves
VLBA 43 GHz:
Multiepoch Radio Spectrum:
43 GHz Image
Radio Spectrum
Comments: 2FM source; z from Polatidis 1995 has no reference to any optical spectrum

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 group, discovered a systematic error in the flux densities of all VLBA 15 GHz observations taking place after a date that lies between 2019 April 16 and 2019 May 16. Observations after that date have correlated flux densities that are between 10% and 20% too low. We have adjusted the flux density scaling of the MOJAVE VLBA data up to 2022 Jan 3 based on near-simultaneous OVRO 40m measurements at 15 GHz.

Asterisked entries below denote epochs that have not yet been corrected for the VLBA flux density scaling problem.
Epoch
(Y-M-D)
VLBA Code VLBA I
(mJy)
VLBA P
(mJy)
VLBA
P (%)
VLBA
EVPA (deg.)
I Image (Nat. Weight) Tapered I Image Tapered I Image (Widefield) Visibility
Data
Stokes I Radplot Pol.
Image
2013-02-10 BL178AZ 1601 35 2.2 3 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2013-01-21 BL178AY 1612 45 2.8 175 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2012-11-21 BL178AT 1386 47 3.4 2 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2012-05-24 BL178AK 1202 54 4.5 4 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2012-02-06 BL178AG 1514 61 4.0 12 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2012-01-16 BH173 1615 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2011-08-15 BL149DO 1585 13 0.8 125 FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS PNG   PS
2009-10-04 BB277 1105 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2009-04-30 BB272 914 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2008-05-02 BB255A 1017 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2007-01-26 BB229A 1180 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
2003-04-26 BM185 1293 no data FITS   PNG   PS FITS   PNG   PS PNG   PS uvf   PNG   PS
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