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Semester 2024A will run observations in the extended configuration from the 28 of October 2024 to around the end of March 2025 (nominal dates).
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Proposals currently being considered:
PI | Title | Science Theme | Triggered? (Y/N) | Visibility Time Requested (hours) | VCS Time Requested (hours) |
|---|---|---|---|---|---|
Anderson | Rapid-response triggering on gravitational wave-detected compact binary mergers with the Murchison Widefield Array | Transients | Y | 0 | 1.6 |
Bhat | Low frequency radio beam of the neutron star-white dwarf binary PSR J1141-6545 | Pulsars | N | 0.5 | 6.0 |
Burridge | Broadband studies of new X-ray binary transient outbursts | Transients | Y | 20 | 0 |
Chakraborty | Probing deeper into the curious case of sub-pulse drifting and nulling in PSR J0026-1955 using MWA | Pulsars | N | 0.3 | 3.5 |
Duchesne | Diffuse emission in the low-mass galaxy cluster Abell 194 | GEG | N | 31 | 0 |
Hurley-Walker (1) | Monitoring the Galactic Plane for radio transients | Transients | N | 229.5 | 0 |
Hurley-Walker (2) | Following up long-period radio transients | Transients | Somewhat | 99.5 | 0.5 |
Kansabanik | Heliopolarimetry: Measurement of CME Magnetic Fields using Faraday Rotation Observations | SHI | Y | 75 | 0 |
Lee | Precisely probing the interstellar medium towards the double pulsar | Pulsars | N | 0 | 5 |
Mondal | Coordinated solar and heliospheric observation campaign using the MWA with the Parker Solar Probe and Solar Orbiter | SHI | N | 66 | 0 |
Morgan | An Interplanetary Scintillation Survey with the extended Phase II MWA | SHI | N | 211 | 0 |
Oberoi | MWA Observations of the Sun | SHI | N | 100 | 0 |
Tan-1 | Timing observations of SMART discovery PSR J1002-2044 | Pulsars | N | 0 | 1.5 |
Tan-2 | Timing observations of the first binary pulsar discovered by SMART | Pulsars | N | 0 | 10 |
Totals: | 832.8 | 28.1 | |||