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

被引:300
作者
Lister, M. L. [1 ]
Aller, H. D. [2 ]
Aller, M. F. [2 ]
Cohen, M. H. [3 ]
Homan, D. C. [4 ]
Kadler, M. [5 ,6 ,7 ,8 ]
Kellermann, K. I. [9 ]
Kovalev, Y. Y. [10 ,11 ]
Ros, E. [10 ]
Savolainen, T. [10 ]
Zensus, J. A. [10 ]
Vermeulen, R. C. [12 ]
机构
[1] Purdue Univ, Dept Phys, W Lafayette, IN 47907 USA
[2] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA
[3] CALTECH, Dept Astron, Pasadena, CA 91125 USA
[4] Denison Univ, Dept Phys & Astron, Granville, OH 43023 USA
[5] Univ Erlangen Nurnberg, D-96049 Bamberg, Germany
[6] Erlangen Ctr Astroparticle Phys, D-91058 Erlangen, Germany
[7] NASA, Goddard Space Flight Ctr, CRESST, Greenbelt, MD 20771 USA
[8] Univ Space Res Assoc, Columbia, MD 21044 USA
[9] Natl Radio Astron Observ, Charlottesville, VA 22903 USA
[10] Max Planck Inst Radioastron, D-53121 Bonn, Germany
[11] PN Lebedev Phys Inst, Ctr Astro Space, Moscow 117997, Russia
[12] ASTRON, NL-7990 AA Dwingeloo, Netherlands
基金
芬兰科学院; 美国国家科学基金会; 俄罗斯基础研究基金会;
关键词
BL Lacertae objects: general; galaxies: active; galaxies: jets; quasars: general; radio continuum: galaxies; surveys; SPECTRUM RADIO-SOURCES; BL-LACERTAE OBJECTS; DIGITAL SKY SURVEY; OPTICAL-IDENTIFICATION STATUS; COMPACT SYMMETRIC OBJECTS; QUASI-STELLAR OBJECTS; RAY BLAZAR CANDIDATES; BANK 966-MHZ SURVEY; PARSEC-SCALE JET; COMPLETE SAMPLE;
D O I
10.1088/0004-6256/137/3/3718
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:3718 / 3729
页数:12
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