| Common Name: | OE -280 | MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie] | VLBA 1.4 GHz: |
| B1950 Name: | 0347-211 |  |
 |
| J2000 Name: | J0349-2102 | ||
| R.A. and Dec. (J2000): | 3h49m57.827s -21d2'47.742" |
||
| AGN Class: | LSP Quasar | ||
| Redshift: | 2.944 (2001A&A...379..393E) | Luminosity Distance: | 25263 Mpc ; 7.87 pc/mas |
| Radio Spectrum: | Flat | ||
| Gamma-ray Association | LAT: Y, EGRET: N, TeV: N | ||
| Kpc-scale morphology: | One-sided | ||
| Jet Speed: | Maximum: 34 ± 15 μas/y ; 3.4 ± 1.5 c Median: N/A ; based on 2 moving features Lister et al. 2019, ApJ,874,43 |
||
| Separation Versus Time Plot: | PNG PS | ||
| Stacked epoch 15 GHz VLBA
images: Uniform weight: [PDF] [GIF] Natural weight: [PDF] [GIF] Circular Beam : [PDF] [GIF] Tapered Beam: [PDF] [GIF] Pushkarev et al. 2017 : FITS Rotation Measure Map: | Not available | Spectral Index Map: | Not available | |
VLBA 23 GHz: |
Kpc-scale: Kharb et al., in prep. | |
|
 |
||
Fermi LAT and 15 GHz VLBA Light Curves |
VLBA 43 GHz: |
Multiepoch Radio Spectrum: |
|
|---|---|---|---|
|
 |
||
| Comments: | LAT 1FM source | ||
![[GIF]](../stackedimages/0347-211.u.stacked.icu.gif){kind=link}
![[GIF]](../stackedimages/0347-211.u.stacked.icd.gif){kind=link}
![[GIF]](../stackedimages/0347-211.u.stacked.icc.gif){kind=link}
![[GIF]](../stackedimages/0347-211.u.stacked.ict.gif){kind=link}
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.
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 |
2013-08-20 | BL178BI | 554 | 13 | 2.4 | 94 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2012-06-25 | BL178AL | 520 | 12 | 2.3 | 121 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2011-06-06 | BL149DJ | 474 | 13 | 2.8 | 75 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2010-11-20 | BL149CX | 460 | 7.7 | 1.7 | 98 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2010-08-06 | BL149CM | 436 | 8.4 | 1.9 | 86 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2010-01-16 | BL149CG | 382 | 6.1 | 1.6 | 113 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2009-07-05 | BL149BP | 627 | 11 | 1.7 | 31 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS |
| Home | Science | AGN Samples | Data Archive | Status | Publications | Movies | RM Maps | α Maps | People | Outreach |