MOJAVE Sample: 1150+497

Common Name:	4C +49.22	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz: BG246
B1950 Name:	1150+497
J2000 Name:	J1153+4931
R.A. and Dec. (J2000):	11h53m24.467s +49d31'8.830"
AGN Class:	LSP Quasar
Redshift:	0.333939 (2020ApJS..249....3A)
Luminosity Distance:	1746 Mpc ; 4.76 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	Two-sided
Jet Speed:	Maximum: 845 ± 98 μas/y ; 17.5 ± 2.0 c Median: 395 ± 29 μas/y ; 8.18 ± 0.61 c based on 6 moving features Lister et al. 2019, ApJ,874,43
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] Pushkarev et al. 2017 : FITS Rotation Measure Map: \| Not available \| Spectral Index Map: \| Not available \|		VLBA 23 GHz: RRIFD Database	Kpc-scale: Ulvestad et al. 1981, AJ 86, 1010

Fermi LAT and 15 GHz VLBA Light Curves		VLBA 43 GHz: Cheng et al. 2020	Multiepoch Radio Spectrum:
Fermi LAT and 15 GHz VLBA Light Curves
Comments:	RATAN ~2 Jy before 2010

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
2013-07-22	BL178BF	2259	5.1	0.2	52	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2013-02-28	BL178BA	1154	18	1.6	72	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-11-11	BL178AS	1462	47	3.2	21	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-08-03	BL178AN	1760	44	2.5	14	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2012-01-02	BL178AE	1880	35	1.8	161	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2011-08-15	BL149DO	1108	21	1.9	107	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2011-05-26	BL149DI	877	19	2.2	115	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2010-11-04	BL149CV	1182	8.2	0.7	86	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2010-03-10	BL149CI	744	19	2.5	97	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2009-10-27	BL149CC	857	21	2.4	116	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2009-05-28	BL149BL	893	11	1.2	117	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2009-02-25	BL149BI	944	11	1.1	121	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2008-10-03	BL149BD	968	4.9	0.5	135	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2008-05-30	BL149AI	1041	9.8	0.9	165	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS