Panoramic Radio Astronomy
  In this contribution we give a brief overview of the Panoramic Radio
Astronomy (PRA) conference held on 2-5 June 2009 in Groningen, the Netherlands.
The conference was motivated by the on-going development of a large number of
new radio telescopes and instruments which, within a few years, will bring a
major improvement over current facilities. Interferometers such as the EVLA,
ASKAP, ATA, MeerKAT, and APERTIF will provide a combination of larger field of
view and increased simultaneous bandwidth, while maintaining good collecting
area and angular resolution. They will achieve a survey speed 10-50 times
larger at 1-2 GHz than the current possibilities, allowing for the first time
optical-like all-sky extra-galactic surveys at these frequencies.
  Significant progress will be made in many fields of radio astronomy. In this
conference we focused on research into the evolution of galaxies over the past
few Gyr. In particular, wide-field observations at 1-2 GHz will provide an
unprecedented panoramic view of the gas properties and star formation in
galaxies, embedded in their environment, from z~0.2-0.5 to the present. Within
the framework of our current knowledge of the galaxy population at z<0.5, we
discussed: the key science questions that the new telescopes will permit us to
answer in combination with complimentary work at other wavelengths; the
observing modes and analysis strategies which will allow us to most efficiently
exploit the data; and the techniques for most effectively coping with the huge
volume of survey products, so far unusual for the radio community. Emphasis was
placed on the complementarity of the upcoming facilities and on their role in
paving the way for the technological development and science goals of the
Square Kilometre Array.
