MOJAVE Sample: 1118+073

Common Name:	IVS B1118+073	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz:
B1950 Name:	1118+073
J2000 Name:	J1120+0704
R.A. and Dec. (J2000):	11h20m38.444s +7d4'47.173"
AGN Class:	LSP Quasar
Redshift:	1.336 (Shaw et al. 2012, ApJ, 748, 49)
Luminosity Distance:	9529 Mpc ; 8.47 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	Core
Jet Speed:	Maximum: 29 ± 5 μas/y ; 1.86 ± 0.34 c Median: N/A ; based on 2 moving features Lister et al. 2021, ApJ, in press, arXiv:2108.13358
Separation Versus Time Plot:	PNG PS
Stacked epoch 15 GHz VLBA images: Uniform weight: [PS] [GIF] Natural weight: [PS] [GIF] Circular Beam : [PS] [GIF] Tapered Beam: [PS] [GIF] Rotation Measure Map: \| Not available \| Spectral Index Map: \| Not available \|		VLBA 23 GHz:	Kpc-scale: Healey et al. 2007, ApJS 171, 61

Fermi LAT and 15 GHz VLBA Light Curves		VLBA 43 GHz:	Multiepoch Radio Spectrum:
Fermi LAT and 15 GHz VLBA Light Curves
Comments:	Hard spectrum MOJAVE_4; in 2FGL but not in 3FGL or FL8Y

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, has 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. All observations after that date have correlated flux densities that are between 10% and 20% too low. The MOJAVE team and NRAO are currently investigating the issue.

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
2020-11-21	BL273H	150	3.0	2.0	85	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2020-07-02	BL229BG	149	2.0	1.3	66	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2019-07-19	BL229AZ	132	1.7	1.3	111	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2018-08-19	BL229AQ	134	2.2	1.6	112	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-10-29	BL193BK	138	1.4	1.0	67	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2016-07-16	BL193BH	150	1.8	1.2	65	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2015-12-19	BL193AZ	164	2.2	1.3	39	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2015-05-08	BL193AR	188	1.4	0.7	21	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2014-06-05	BL193AJ	212	1.4	0.7	40	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2014-02-27	BL193AG	210	2.5	1.2	18	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2014-01-11	BL193AD	201	1.9	0.9	12	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS