MOJAVE Sample: 1328+254

Common Name:	3C 287	VLBA 2cm Image \|	VLBA 1.4 GHz:
B1950 Name:	1328+254
J2000 Name:	J1330+2509
R.A. and Dec. (J2000):	13h30m37.690s +25d9'10.879"
AGN Class:	Quasar
Redshift:	1.054 (2010AJ....139.2360S)
Luminosity Distance:	7086 Mpc ; 8.14 pc/mas
Radio Spectrum:	CSS
Gamma-ray Association	LAT: N, EGRET: N, TeV: N
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: Paragi, Frey and Sanghera 1998, AA 338, 840

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

Comments:	2cm survey source

Common Name:

3C 287

VLBA 2cm Image |

VLBA 1.4 GHz:

R.A. and Dec. (J2000):

13h30m37.690s
+25d9'10.879"

AGN Class:

Quasar

Redshift:

1.054 (2010AJ....139.2360S)

Luminosity Distance:

7086 Mpc ; 8.14 pc/mas

Radio Spectrum:

CSS

Gamma-ray Association

LAT: N, EGRET: N, TeV: N

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: Paragi, Frey and Sanghera 1998, AA 338, 840

Fermi LAT and 15 GHz VLBA Light Curves

VLBA 43 GHz:

Multiepoch Radio Spectrum:

Comments:

2cm survey 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
1996-05-16	BK037B	124	no data			FITS PNG PDF	UVF	PNG PDF		PNG