CTAO | Australia Meeting #1 2026

Australia/Adelaide
Gavin Rowell (University of Adelaide), Sabrina Einecke (University of Adelaide)
Description

This will be a one-day online meeting, on Tuesday April 28th.

Start time is 11:00 CST, with a nominal 17:00 CST finish time.

Main topics: CTAO status and Australia's involvements (now & future).

For continuing updates on the CTAO, please visit the CTAO news website for more details.

Link to full timetable.

Zoom access: https://adelaide.zoom.us/j/84052035644?pwd=Jeaz7IVbDPbc5PJ46oZul4DMPNAQrZ.1

Please note that there is no registration fee for this event.

For those in Adelaide, we will use Room 121 in the Physics building, and we'll have a local morning tea at 10:30.

 

Scientific Organising Committee

Gavin Rowell, Adelaide University, Australia

Sabrina Einecke, Adelaide University, Australia

Local Organising Committee

Gavin Rowell, Adelaide University, Australia

Sabrina Einecke, Adelaide University, Australia

Simon Lee, Adelaide University, Australia

Paddy McGee, Adelaide University, Australia

 

Registration
Registration and Abstract Submission
Participants
    • 10:30
      Morning tea (for those in Adelaide)
    • 1
      CTAO Status and Update

      This talk will give a brief update on CTAO and Australia's involvements.

      Speaker: Prof. Gavin Rowell (University of Adelaide)
    • 2
      SSTCAM Updates

      In July 2025 the initial build of a quarter camera (QCAM-i) designed for the Cherenkov Telescope Array Observatory (CTAO) Small Sized Telescope (SST) was tested on Tenerife, Canary Islands. This was the first field test of the camera hardware which will be used for the SSTs at CTAO-South in Chile. Dark field observations and trigger threshold scans were taken, which can be compared with simulated cosmic ray shower images and night-sky background trigger rates. This talk will present an update on the progress comparing data taken on Tenerife with QCAM-i with Monte Carlo simulations.

      In addition, updates from the development of SSTCAM will be presented.

      Speaker: Simon Lee
    • 3
      CTAO's Science Data Challenge
      Speaker: Sabrina Einecke (University of Adelaide)
    • 4
      CTA-Pol Update

      TBD

      Speaker: Nick Tothill (Western Sydney University)
    • 12:30
      Lunch
    • 5
      AAL's Role in CTAO

      TBD

      Speaker: Grace Lawrence
    • 6
      SKAO Science Operations Update

      The Square Kilometre Array Observatory (SKAO) Science Operations Team is focused on the development and implementation of various workflows and procedures to ensure that SKA-Low and SKA-Mid will be operationally ready for transformational science. In this talk, I will give an update on the telescope capability rollout, as well as plans for the upcoming Science Verification phase.

      Speaker: Jess Broderick
    • 7
      An Australian Radio Transients Facility
      Speaker: James Miller-Jones
    • 14:30
      Afternoon tea
    • 8
      Searching for New Physics with CTAO

      TBD

      Speaker: Hayden James (The University of Adelaide)
    • 9
      Resolving point sources in diffuse backgrounds using Microcanonical Langevin Monte Carlo with Parametric Cataloging

      Using IceCube neutrino skies as an example, we show how this method can resolve large numbers of weak sources from high diffuse backgrounds.

      Speaker: Gary Hill (University of Adelaide)
    • 10
      Clustering the Interstellar Medium for Galactic Gamma-Ray Modelling

      In this update, we will present preliminary results from our 3D molecular hydrogen distributions of ISM cloud structures, derived over the entire Mopra Southern Galactic Plane CO Survey. We will introduce our novel cloud identification method used to create these distributions. This involves Gaussian decompositions and clustering, as well as combining measurements from different gas tracers (12CO and 13CO).

      Speaker: Imogen Barnsley (University of Adelaide)
    • 11
      Update: Searching for Escaped Cosmic Rays from Supernova Remnants

      The detection of gamma-ray emission outside the shell of a supernova remnant (SNR) can be critical evidence for cosmic-ray acceleration in, and escape from, SNRs. In this contribution, we present an analysis of the Fermi Large Area Telescope (LAT) gamma-ray data towards middle-aged Galactic SNR W51C. We perform both a morphological and spectral analysis to search for evidence of gamma-ray emission outside the SNR shell. We also look for a spatial correlation between the observed gamma rays and surrounding molecular clouds.

      Speaker: Jemma Pilossof (University of Adelaide)
    • 12
      Opportunities for Deep Learning With IACTs : Update

      TBD

      Speaker: Lydia Castellucci
    • 18:30
      Dinner (British Hotel) : Time TBC