CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observation
By continuing our brief but intense observations of PSR J0437-4715, we intend to further increase our sensitivity to long-term effects such as the structure of the ISM, receiver stability and orbital
This proposal requests 4 hours to carry out regular monitoring an eclipsing binary millisecond pulsar in the globular cluster NGC 6397, which we discovered with the Parkes UWL.
Fast radio bursts (FRBs) continue to raise more questions than they answer. Until last year, only one burst – the only one known to repeat - had been localized to a bright radio nebula (either a young
SUPERBx looks at the highest Galactic latitudes in a search for pulsars and fast radio bursts (FRBs). We use optimised GPU codes and supercomputing to search for these, making discoveries in real time
