MOJAVE Sample: 2241+200

Common Name:	RGBJ2243+203	MOJAVE 15 GHz \|	VLBA 1.4 GHz:
B1950 Name:	2241+200
J2000 Name:	J2243+2021
R.A. and Dec. (J2000):	22h43m54.744s +20d21'3.778"
AGN Class:	HSP BL Lac
Redshift:	Unknown
Luminosity Distance:	Unknown
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: Y
Kpc-scale morphology:	Core
Jet Speed:	Maximum: Unknown ; Median: Unknown ;
Separation Versus Time Plot:	Not available
Stacked 15 GHz Stokes I VLBA images: Natural weight: Not Available Circular Beam: Not Available Tapered Beam: Not Available Stacked 15 GHz Polarization VLBA images: Rotation Measure 8-15 GHz Map: \| Not available \| Spectral Index 8-15 GHz 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:

Comments:	LAT_1FM weak sample, Rosa Gonzalez 2018 get z = 0.527 from cluster z

Common Name:

RGBJ2243+203

MOJAVE 15 GHz |

VLBA 1.4 GHz:

R.A. and Dec. (J2000):

22h43m54.744s
+20d21'3.778"

HSP BL Lac

Unknown

Unknown

Flat

Gamma-ray Association

LAT: Y, EGRET: N, TeV: Y

Kpc-scale morphology:

Core

Jet Speed:

Maximum: Unknown ;
Median: Unknown ;

Separation Versus Time Plot:

Not available

Stacked 15 GHz Stokes I VLBA images:
Natural weight: Not Available
Circular Beam: Not Available
Tapered Beam: Not Available

Stacked 15 GHz Polarization VLBA images:

Rotation Measure 8-15 GHz Map: | Not available |

Spectral Index 8-15 GHz 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:

Comments:

LAT_1FM weak sample, Rosa Gonzalez 2018 get z = 0.527 from cluster z

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.

Epoch (YYYY-MM-DD)	VLBA Code	VLBA I (mJy)	VLBA P (mJy)	VLBA P (%)	VLBA EVPA (deg.)	I Image (Nat. Weight)	Visibility Data	Stokes I Radplot	Polarization Image	Full Montage
2010-11-29	BL149CY	69	no data			FITS PNG PDF	UVF	PNG PDF		PNG