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MOJAVE: MONITORING OF JETS IN ACTIVE GALACTIC NUCLEI WITH VLBA EXPERIMENTS. V. MULTI-EPOCH VLBA IMAGES

期刊

ASTRONOMICAL JOURNAL
卷 137, 期 3, 页码 3718-3729

出版社

IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/137/3/3718

关键词

BL Lacertae objects: general; galaxies: active; galaxies: jets; quasars: general; radio continuum: galaxies; surveys

资金

  1. NSF [AST-0406923, AST0807860]
  2. Purdue Research Foundation
  3. NRAO
  4. Alexander vonHumboldt fellowships at the MPIfR
  5. NASA Postdoctoral Program at the Goddard Space Flight Center
  6. Russian Foundation for Basic Research [01-02-16812, 05-02-17377, 08-02-00545]
  7. Max-Planck-Gesellschaft
  8. Academy of Finland [120516]
  9. National Science Foundation and by funds from the University of Michigan
  10. NASA's Astrophysics Data System
  11. NASA/IPAC Extragalactic Database (NED)
  12. Direct For Mathematical & Physical Scien [0807860] Funding Source: National Science Foundation

向作者/读者索取更多资源

We present images from a long-term program (MOJAVE: Monitoring of Jets in active galactic nuclei (AGNs) 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 Very Long Baseline Array (VLBA) images of a complete flux-density-limited sample of 135 AGNs 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 multiepoch 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.

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