MOJAVE Sample: 0640+090

Common Name:	TXS 0640+090	MOJAVE 15 GHz [Total intensity movie] \| [Polariz. movie]	VLBA 1.4 GHz:
B1950 Name:	0640+090
J2000 Name:	J0643+0857
R.A. and Dec. (J2000):	6h43m26.445s +8d57'38.012"
AGN Class:	LSP Quasar
Redshift:	0.882 (Ackermann et al. 2011, ApJ, 743, 171)
Luminosity Distance:	5673 Mpc ; 7.77 pc/mas
Radio Spectrum:	Flat
Gamma-ray Association	LAT: Y, EGRET: N, TeV: N
Kpc-scale morphology:	Unknown
Jet Speed:	Maximum: Unknown ; Median: Unknown ;
Separation Versus Time Plot:	Not available
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:	Kpc-scale: NVSS

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

Comments:	New LAT, low b, core id uncertain

Common Name:

TXS 0640+090

MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie]

VLBA 1.4 GHz:

R.A. and Dec. (J2000):

6h43m26.445s
+8d57'38.012"

AGN Class:

LSP Quasar

Redshift:

0.882 (Ackermann et al. 2011, ApJ, 743, 171)

Luminosity Distance:

5673 Mpc ; 7.77 pc/mas

Radio Spectrum:

Flat

Gamma-ray Association

LAT: Y, EGRET: N, TeV: N

Kpc-scale morphology:

Unknown

Jet Speed:

Maximum: Unknown ;
Median: Unknown ;

Separation Versus Time Plot:

Not available

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:

Kpc-scale: NVSS

Fermi LAT and 15 GHz VLBA Light Curves

VLBA 43 GHz:

Multiepoch Radio Spectrum:

Comments:

New LAT, low b, core id uncertain

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
2011-07-24	BL149DN	476	12	2.5	175	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2011-02-20	BL149DB	1142	14	1.3	151	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2010-10-25	BL149CT	744	17	2.3	152	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2010-03-10	BL149CI	962	29	3.0	171	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS
2009-08-19	BL149BR	842	16	1.9	151	FITS PNG PS	FITS PNG PS	PNG PS	uvf	PNG PS	PNG PS