MOJAVE: Monitoring of Jets in AGN with VLBA Experiments. V. Multi-epoch VLBA Images
By M. Lister, H. Aller, M. Aller, M. Cohen, D. Homan, M. Kadler, K. I. Kellermann, Y. Kovalev, E. Ros, T. Savolainen and 2 more. 2008
155 citations recorded by the source corpus.
We present images from a long term program (MOJAVE: Monitoring of Jets in AGN with VLBA Experiments) to survey the structure and evolution of parsec-scale jet phenomena associated with bright radio-loud active galaxies in the northern sky. The observations consist of 2424 15 GHz VLBA images of a complete flux-density limited sample of 135 AGN above declination -20 degrees, spanning the period 1994 August to 2007 September. These data were acquired as part of the MOJAVE and 2 cm Survey programs, and from the VLBA archive. The sample selection criteria are based on multi-epoch parsec-scale (VLBA) flux density, and heavily favor highly variable and compact blazars. The sample includes nearly all the most prominent blazars in the northern sky, and is well-suited for statistical analysis and comparison with studies at other wavelengths. Our multi-epoch and stacked-epoch images show 94% of the sample to have apparent one-sided jet morphologies, most likely due to the effects of relativistic beaming. Of the remaining sources, five have two-sided parsec-scale jets, and three are effectively unresolved by the VLBA at 15 GHz, with essentially all of the flux density contained within a few tenths of a milliarcsecond.
Subfields: Astronomy and Astrophysics, Communication, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/0dbabe1ca3fe0cb2e4c2b1da1dde15c5d9201280
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Citations in the corpus
- MOJAVE: Monitoring of Jets in Active galactic nuclei with VLBA Experiments (2012, methodology): “For a more detailed discussion of the data reduction and imaging process schemes, see Lister et al. (2009); Hovatta et al. (2012).”
- FERMI LARGE AREA TELESCOPE GAMMA-RAY DETECTION OF THE RADIO GALAXY M87 (2009, methodology): “This research has made use of data from the MOJAVE database that is maintained by the MOJAVE team (Lister et al. 2009).”
- FERMI DISCOVERY OF GAMMA-RAY EMISSION FROM NGC 1275 (2009, methodology): “In fact, the MOJAVE (Monitoring Of Jets in Active galactic nuclei with VLBA Experiments; Lister et al. 2009) 15 GHz VLBA observations of 3C 84, taken simultaneously withFermi on 2008 August 25, show a significant brightening of the centralsub-parsec-scale structure, indicating that a flare is happen”