MOJAVE Sample: 1229+290

Common Name:	B2 1229+29	MOJAVE 15 GHz \|	VLBA 1.4 GHz:
B1950 Name:	1229+290
J2000 Name:	J1231+2847
R.A. and Dec. (J2000):	12h31m43.573s +28d47'49.769"
AGN Class:	ISP BL Lac
Redshift:	0.236 (Shaw et al., 2013)
Luminosity Distance:	1170 Mpc ; 3.71 pc/mas
Radio Spectrum:	Steep
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	One-sided
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: E.Stanley Ph.D. Thesis 2017

Fermi LAT and 15 GHz VLBA Light Curves	VLBA 43 GHz:	Multiepoch Radio Spectrum:

Comments:	z=0.236 from Shaw et al. 2013 tentative; LAT_2FM weak sample; was a candidate MOJAVE_4 source

Common Name:

B2 1229+29

MOJAVE 15 GHz |

VLBA 1.4 GHz:

R.A. and Dec. (J2000):

12h31m43.573s
+28d47'49.769"

AGN Class:

ISP BL Lac

Redshift:

0.236 (Shaw et al., 2013)

Luminosity Distance:

1170 Mpc ; 3.71 pc/mas

Radio Spectrum:

Steep

Gamma-ray Association

LAT: Y, EGRET: N, TeV: N

Kpc-scale morphology:

One-sided

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: E.Stanley Ph.D. Thesis 2017

Fermi LAT and 15 GHz VLBA Light Curves

VLBA 43 GHz:

Multiepoch Radio Spectrum:

Comments:

z=0.236 from Shaw et al. 2013 tentative; LAT_2FM weak sample; was a candidate MOJAVE_4 source

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
2015-10-02	BL193AX	52	0.7	1.4	1	FITS PNG PDF	UVF	PNG PDF	p:PNG p:PDF f:PNG f:PDF	PNG
2015-08-11	BL193AV	40	12	31.2	132	FITS PNG PDF	UVF	PNG PDF	p:PNG p:PDF f:PNG f:PDF	PNG