2024-A, Extended
- Venus Chico
Overview
Semester 2024A will run observations in the extended configuration from the 02 of June 2024 to around the end of September 2024 (nominal dates).
Approved Proposals
PI | Title | Science Theme | Triggered? (Y/N) | Visibility Time Requested (hours) | VCS Time Requested (hours) |
|---|---|---|---|---|---|
Anderson | Rapid-response triggering on binary neutron star mergers with the Murchison Widefield Array | Transients | Y | 0 | 11 |
Bhat | Low frequency radio beam of the neutron star-white dwarf binary PSR J1141-6545 | PFT | N | 2 | 6 |
Cook | Multi-Frequency All-Sky m-Mode Imaging With the MWA | EoR/GEG | N | 73.5 | 0 |
Das | Investigating ‘Main-sequence Radio Pulse emitters’ (MRPs) at MWA frequencies | Transients | N | 63 | 0 |
Hurley-Walker (1) | Monitoring the Galactic Plane for radio transients | Transients | N | 341 | 0 |
Hurley-Walker (2) | A white dwarf pulsar at low radio frequencies | Transients | N | 0 | 8 |
Hurley-Walker (3) | An ultra-long period radio transient in a binary orbit | Transients | N | 5.13 | 0 |
Kansabanik | Measurement of CME magnetic fields in the heliosphere using Faraday Rotation observations | SHI | Y | 60 | 0 |
Mondal | Coordinated solar and heliospheric observation campaign using the MWA with the Parker Solar Probe and Solar Orbiter | SHI | Y & N | 37 | 0 |
Morgan | An Interplanetary Scintillation Survey with the extended Phase II MWA | SHI | N | 205.3 | 0 |
Oberoi | MWA Observations of the Sun | SHI | Y & N | 100 | 0 |
Rankin | Exploring the Core/Cone Radio Emission-Beam Geometry of PSR B1451–68 at Metre Wavelengths | PFT | N | 1 | 5.5 |
Sokolowski (1) | SKA-Low station sensitivity measurements using pulsar co-observations with the MWA | PFT | N | 12 | 0 |
Sokolowski (2) | Commissioning the commensal FRB search pipeline using the MWAX real-timebeamformer | Transients | N | 30 | 0 |
Tan | Timing observations of SMART discovery PSR J1002-2044 | Transients | N | 0.5 | 2.5 |
Waszewski | Long-Duration Observation of Ambient Solar Wind with Interplanetary Scintillation | SHI | N | 6 | 0 |
Totals: | 936 | 33 | |||