Jesse Cranney

Dr. Jesse Cranney is a Research Fellow at the Advanced Instrumentation Technology Centre (AITC) within the Research School of Astronomy and Astrophysics at the Australian National University (ANU). His work focuses on advanced instrumentation for astronomy, particularly in adaptive optics systems, telescope design, and precision astrometry. He contributes to cutting-edge projects such as MAVIS (Multi-conjugate Adaptive Optics Visionaries in Spectroscopy) and the Giant Magellan Telescope's adaptive optics systems. His research emphasizes optimizing optical performance, real-time control algorithms, and instrument calibration for ground-based telescopes.

Educational background: While specific academic degrees are not explicitly detailed, his postdoctoral role implies completion of a PhD in a relevant field like astrophysics or optical engineering.

Research Interests: Cranney specializes in adaptive optics, laser guide star systems, segmented telescope phasing, and high-precision astrometry. His work bridges theoretical control systems with practical astronomical instrumentation, aiming to enhance observational capabilities of large telescopes. Key applications include improving image resolution, reducing atmospheric turbulence effects, and enabling advanced scientific studies in astrophysics.

Key Projects: He leads or contributes to MAVIS (a visible-light adaptive optics instrument for the VLT), ULTIMATE-Subaru (next-gen wide-field AO system), and the Giant Magellan Telescope's laser tomography systems. These projects address challenges in optical stability, real-time processing, and multi-layer adaptive control.

Labs/Teams: Active in the AITC, collaborating with global teams on telescope instrumentation, including contributions to the European Southern Observatory's Very Large Telescope and Subaru Telescope projects.