MOJAVE Sample: 0110+318

Common Name:	4C +31.03	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz: VLBA Archive: BU015B
B1950 Name:	0110+318
J2000 Name:	J0112+3208
R.A. and Dec. (J2000):	1h12m50.333s +32d8'17.433"
AGN Class:	LSP Quasar
Redshift:	0.603 (Wills and Wills 1976, ApJS, 31, 143)
Luminosity Distance:	3546 Mpc ; 6.69 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	One-sided Halo
Jet Speed:	Maximum: 538 ± 29 μas/y ; 18.8 ± 1.0 c Median: N/A ; based on 3 moving features Lister et al. 2019, ApJ,874,43
Separation Versus Time Plot:	PNG PS
Stacked epoch 15 GHz VLBA images: Uniform weight: [PDF] [GIF] Natural weight: [PDF] [GIF] Circular Beam : [PDF] [GIF] Tapered Beam: [PDF] [GIF] Pushkarev et al. 2017 : FITS Rotation Measure Map: \| Not available \| Spectral Index Map: \| Not available \|		VLBA 23 GHz:	Kpc-scale: Wilkinson et al., 1998, MNRAS, 300 790

Fermi LAT and 15 GHz VLBA Light Curves		VLBA 43 GHz:	Multiepoch Radio Spectrum:
Fermi LAT and 15 GHz VLBA Light Curves
Comments:	LAT 1FM source; 6cm image also in HDC98

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
2013-08-20	BL178BI	767	3.4	0.4	39	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2013-03-31	BL178BB	589	2.8	0.5	6	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-09-02	BL178AO	427	11	2.6	26	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-01-14	BL178AF	820	12	1.4	7	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2011-04-11	BL149DF	678	17	2.6	29	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2010-10-15	BL149CS	644	13	2.0	118	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2010-03-10	BL149CI	560	16	2.9	8	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2009-08-19	BL149BR	572	1.3	0.2	17	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2009-06-03	BL149BM	709	11	1.5	119	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS