Michael Ashley

Professor Michael Ashley is a faculty member at the University of New South Wales (UNSW), affiliated with the School of Physics. His primary research focuses on observational astronomy, particularly leveraging the unique conditions of the Antarctic plateau for astronomical observations. He is deeply involved in developing and deploying robotic telescopes and instrumentation for Antarctic sites like Dome A and Dome C.

His research interests encompass:

• Time-domain astronomy and infrared surveys (e.g., Palomar Gattini-IR)
• Exoplanet detection and characterization
• Stellar variability, transients, and binary systems
• Site testing and atmospheric conditions in Antarctica
• Telescope automation and wide-field imaging systems

Analysis of his recent articles reveals a strong emphasis on Antarctic astronomy infrastructure development (e.g., AST3-II/CHESPA, Cryoscope), large-scale infrared time-domain surveys (Palomar Gattini-IR), and the study of variable objects like R Coronae Borealis stars, Mira variables, Be/X-ray binaries, and transients. His work frequently involves public data releases and catalog construction.

Professor Ashley contributes to major collaborative projects including the Chinese Small Telescope ARray (CSTAR), the Antarctic Survey Telescopes (AST3), Kunlun Infrared Sky Survey (KISS), and the PLATO observatory. He has significant expertise in instrument design, data pipelines for automated surveys, and analyzing Antarctic meteorological data for astronomical site characterization.