| Common Name: | PMN J0847-0703 | MOJAVE 15 GHz [Total intensity movie] | [Polariz. movie] | VLBA 1.4 GHz: |
| B1950 Name: | 0845-068 |  |
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| J2000 Name: | J0847-0703 | ||
| R.A. and Dec. (J2000): | 8h47m56.737s -7d3'16.902" |
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| AGN Class: | LSP BL Lac | ||
| Redshift: | Unknown | Luminosity Distance: | Unknown |
| Radio Spectrum: | Flat | ||
| Gamma-ray Association | LAT: Y, EGRET: N, TeV: N | ||
| Kpc-scale morphology: | Core | ||
| Jet Speed: | Maximum: 10 ± 20 μas/y ; Median: N/A ; based on 2 moving features Lister et al. 2021, ApJ,923,30 |
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| 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] Rotation Measure Map: | Not available | Spectral Index Map: | Not available | |
VLBA 23 GHz: |
Kpc-scale: Healey et al. 2007, ApJS 171, 61 | |
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Fermi LAT and 15 GHz VLBA Light Curves |
VLBA 43 GHz: |
Multiepoch Radio Spectrum: |
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| Comments: | Hard spectrum MOJAVE_4 source | ||
![[GIF]](../stackedimages/0845-068.u.stacked.icu.gif){kind=link}
![[GIF]](../stackedimages/0845-068.u.stacked.icd.gif){kind=link}
![[GIF]](../stackedimages/0845-068.u.stacked.icc.gif){kind=link}
![[GIF]](../stackedimages/0845-068.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 |
2020-12-01 | BL229BK | 253 | 6.9 | 2.7 | 118 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2018-11-11 | BL229AS | 428 | 11 | 2.7 | 109 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2016-08-09 | BL193BI | 216 | 3.6 | 1.7 | 132 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2016-06-03 | BL193BE | 267 | 9.8 | 3.7 | 128 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2015-09-06 | BL193AW | 363 | 6.4 | 1.8 | 82 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2015-06-16 | BL193AT | 424 | 7.3 | 1.7 | 104 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2014-12-12 | BL193AP | 452 | 19 | 4.2 | 119 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS | 2014-06-05 | BL193AJ | 370 | 4.8 | 1.3 | 128 | FITS PNG PS | FITS PNG PS | PNG PS | uvf | PNG PS | PNG PS |
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