Abstract
The adaptive optics (AO) technology unfolds the capabilities of ground-based telescopes and opens new horizons. A cost-effective and resilient laser-guided single conjugated adaptive optics system offers the opportunity to a significant number of existing 1-4 meter telescopes. This opens the door for medium-sized telescopes to pursue cutting-edge scientific research that may be challenging to achieve with larger observatories due to a scarcity of time for various survey observations. The medium-class telescope, equipped with adaptive optics along with advanced image processing, provides unprecedented image quality in terms of spatial resolution (sub-arcsec), high cadence with high SNR.
Here, we present a robust Rayleigh scattered laser-guided single conjugated adaptive optics system called SALTO, which was designed, built, and tested in the Belgian countryside on a 1-meter class telescope and an automated robotic adaptive optics system called iRobo-AO for IUCAA 2m telescope. These projects aim to demonstrate the possibility of rejuvenating the scientific goals of medium-class telescopes with AO technology. This talk discusses the overall study of the design of the AO system, from the optics to the control system. It also includes a description of the integration and calibration of SALTO along with successful on-sky results at 1.55µm under 2-3'' seeing. We also present our recent work on non-common path aberration correction at the Subaru telescope and high-spectral resolution interferometry BIFROST/Asgard instrument. The Asgard instrument suite is being designed as a guest instrument for the VLTI, representing a new generation of instruments that leverage long-baseline interferometry to perform spectroscopy and nulling.
About Speaker
Dr. Jyotirmay Paul is a postdoctoral fellow at the University of Exeter, UK, where he is involved in research on the VLTI interferometric instrument BIFROST/Asgard.
Previously, he was a postdoctoral fellow at the University of Liege, Belgium, focusing on adaptive optics for medium-class telescopes and implementing focal plane wavefront sensing at the Subaru Telescope. He completed his PhD work at the IUCAA Instrumentation Laboratory, Pune, under the guidance of Prof. A. N. Ramaprakash (IUCAA) and Dr. A. Bhadra (University of North Bengal, Siliguri).
His research interests primarily revolve around astronomical instrumentation related to optical telescopes, with a specific focus on designing and developing high-resolution/high-contrast imaging systems.