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Curtin University
Curtin Institute of Radio Astronomy

Future Projects

Introduction

The Curtin Institute of Radio Astronomy at Curtin University of Technology is engaged in the following broad areas:

  1. Technology development for the next generation of radio astronomy instruments, including the Square Kilometre Array (SKA) and SKA pathfinder instruments, Very Long Baseline Interferomery (VLBI) and e-VLBI (using high speed optical fibre connections between telescopes), and the Murchison Widefield Array (MWA).
  2. Algorithm development for the calibration and operation of these telescopes.
  3. Fundamental studies in astronomy and astrophysics, using existing facilities such as VLBI arrays, the Australia Telescope Compact Array (ATCA), near Narrabri in NSW, and overseas radio and optical telescopes, including space-based instruments at high energies (i.e. SWIFT and GLAST). Areas such as supermassive black holes, supernova remnants, galactic X-ray binaries, active galactic nuclei, and pulsars will be covered, as well as new areas of radio astronomy targeting the transient radio sky. Research will be conducted in the radio, optical, and high energy photon regimes.

Upcoming projects are usually released by project supervisors during the second half of the year. Information on upcoming project opportunities may be found under individual supervisors.

For previous astronomy projects at Curtin, see cira.ivec.org/dokuwiki/doku.php/pastproj/start