2025-A
Overview
Semester 2025A will run observations from the end of June 2025 to around the end of March 2026 (nominal dates).
Approved Proposals:
PI | Title | Science Theme | Triggered? (Y/N) | Visibility Time Requested (hours) | VCS Time Requested (hours) |
|
|---|---|---|---|---|---|---|
Goodwin | Low-frequency radio emission from tidal disruption events | Transients | N | 12 |
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|
Hurley-Walker | Nightly Investigation of Galactic and High-latitude Transients | Transients | N | 1021 |
|
|
Hurley-Walker | Following up long-period radio transients | Transients | Y | 100 |
| 0 |
Hurley-Walker | Shadowing the LOTRUN Survey | Transients | N | 207 |
|
|
Kansabanik | Heliopolarimetry: Regular Monitoring of CME Magnetic Fields in the Heliosphere using Faraday Rotation Observations | SHI | N | 83 |
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Mondal | Coordinated Solar and Heliospheric Observing Campaign using the MWA with Parker Solar Probe, Solar Orbiter and PROBA-3 | SHI | Partially | 203 |
|
|
Morgan | An Interplanetary Scintillation Survey with the Extended Phase II MWA | SHI | N | 1753 |
|
|
Oberoi | Solar observations with the MWA | SHI | Partially | 160 |
|
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Trott | Epoch of Reionisation | EoR | N | 668 |
|
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Wang | Broadband Spectral Characterization of MeerKLASS HI Intensity Mapping Sources with MWA Observations | EoR | N | 60 |
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Zhang | Deep Imaging of One Selected EoR Candidate Field | EoR | N | 30 |
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Zheng | Deep Imaging of Cosmos Field | EoR | N | 30 |
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Totals: | 4327 |
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