The aim of this project is to enable impactful research by deploying a new astronomical "movie mode" on the Huntsman Telescope. Movie mode is enabled by the same image sensor technology that is found in mobile phone cameras. Driven by considerable consumer demand, these sensors are now very sensitive and can take much higher data rates compared to sensors normally used in astronomical instrumentation.
Huntsman is one of the first professional astronomy facilities to use this new sensor technology. We have conducted 3 observational proof-of-concept studies in significant areas of astrophysics: exomoon and exoplanet ring detection, tracking a flare star breakout phase and detection of Betelgeuse flux variations during the daytime. Furthermore, we have trialed a daytime satellite monitoring mode, which has activated a Research Translation collaboration with an industry partner.
In the first semester of this project ADACS were able to use the proof-of-concept work to develop a new command line tool that would efficiently capture "move mode" observations from the Huntsman Cameras. Additionally, ADACS software developers undertook a review of the architecture of the telescope control and observing software and have made plans for a second semeser's work, in which the "movie mode" observations will be implemented into the telescope control software.
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ADACS provided a solid foundation on which the GOTO-XBs team could further build the web app, and provided instructional information to up-skill the team.
The CoCoNuT supernova simulation code has a 6-dimensional radiation solver module for simulating neutrino transport. This method is computationally expensive to run, so ADACS enhanced this module with MPI to run in parallel on supercomputers.
This project optimised the CELEBI pipeline for precise localisation of FRBs (Fast Radio Bursts) using ASKAP's CRAFT survey, adapting to recent infrastructure changes and preparing for increased detection capabilities with the CRACO upgrade.