Submilliarcsecond imaging of AGN with the Very Long Baseline Array at 2 centimeter wavelength

We are using the NRAO's Very Long Baseline Array for an imaging survey of compact radio sources at 15 GHz. Our primary scientific goals are: The observations are performed in a "snapshot" observing mode (1 scan per hour of 4-5 minute duration, over a 8 hour period). We achieve a dynamic range of typically exceeding 1000:1, with a typical noise limit (rms) of 0.35 milli-Jansky.

As a service to the scientific community, we are making the images from the survey available online for download on this website.

MOJAVE (Monitoring of Jets in Active Galaxies with VLBA Experiments) is the continuation of the 2cm Survey Effort, with a redefinition of the survey sample. As a service to the scientific community, we are making the images from the survey available online for download on this website.

People Involved (in alphabetical order)

M.H. Cohen (California Institute of Technology)
D.C. Homan (Denison University)
M. Kadler (NASA GSFC)
K.I. Kellermann (National Radio Astronomy Observatory)
Y.Y. Kovalev (Max-Planck-Institut für Radioastronomie)
M.L. Lister (Purdue University)
E. Ros (Max-Planck-Institut für Radioastronomie)
R.C. Vermeulen (Netherlands Foundation for Research in Astronomy)
J.A. Zensus (Max-Planck-Institut für Radioastronomie)


ros@mpifr-bonn.mpg.de