Radio monitoring of gravitational wave events
The detection of gravitational waves and electromagnetic radiation from a neutron star merger was a scientific breakthrough, with important implications for physics and astronomy. We are using three Australian radio telescopes to search for and monitor radio waves from future gravitational wave events. These observations will provide key information to unlock the mystery of what causes some of the most energetic events in the Universe, their environment and how they evolve.
Some of our recent papers are:
- Dobie et al. A turnover in the radio light curve of GW170817
- Mooley et al. A mildly relativistic wide-angle outflow in the neutron-star merger event GW170817
- Hallinan et al. A radio counterpart to a neutron star merger
- Kasliwal et al. Illuminating gravitational waves: A concordant picture of photons from a neutron star merger
- Abbott et al. Multi-messenger Observations of a Binary Neutron Star Merger
Low frequency radio transients
Magnetised extrasolar planets are expected to emit strongly at low radio frequencies, in the same way that Jupiter does. So far, most exoplanets have been detected through indirect means such as radial velocity and transit searches but radio observations can provide another method of making direct detections.
We are searching for exoplanet emission, and studying other variable sources such as flare stars at low radio frequencies using the Murchison Widefield Array Telescope.
Some of our recent low frequency papers are:
- Lynch et al. The detectability of radio emission from exoplanets
- Murphy et al. Low-Frequency Spectral Energy Distributions of Radio Pulsars Detected with the Murchison Widefield Array
- Murphy et al. A search for long-time-scale, low-frequency radio transients
- Lynch et al. 154 MHz Detection of Faint, Polarized Flares from UV Ceti
ASKAP radio transients
Transients are astronomical objects that appear and disappear or change rapidly; they are our window to some of the most extreme processes in the Universe. Transient events can occur when black holes form, causing supernovae and gamma-ray bursts; when stars collide with black holes; or when hot, magnetised planets interact with their host stars. There are also mysterious transients of unknown origin, like fast radio bursts.
The Variables and Slow Transients project on the Australian SKA Pathfinder (ASKAP) telescope will investigate all of these phenomena through a suite of widefield surveys.
Some of our recent papers on gigahertz radio variability are:
- Bhandari et al. A pilot survey for transients and variables with the Australian Square Kilometre Array Pathfinder
- Hancock et al. Radio variability in the Phoenix Deep Survey at 1.4 GHz
- Hobbs et al.
A pilot ASKAP survey of radio transient events in the region around the intermittent pulsar PSR J1107-5907
- Murphy et al. VAST: An ASKAP Survey for Variables and Slow Transients