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About

Tamal Mukherjee is an instrumental astronomer whose work centers on developing advanced fiber-optic positioning systems for next-generation giant telescopes. His primary research focuses on MANIFEST, a sophisticated fibre-fed system designed to dramatically enhance the observational capabilities of the 24.5-meter Giant Magellan Telescope (GMT). Mukherjee’s major contribution lies in engineering this system to feed GMT’s first-light instruments—the high-resolution echelle spectrograph G-CLEF and the low/mid-resolution spectrograph GMACS—across a 14 arcminute field-of-view. This innovation enables simultaneous multi-object spectroscopy, vastly increasing the telescope’s efficiency for large-scale astronomical surveys. While his most cited paper, “Enhancing astronomical exploration with the GMT/MANIFEST” (2024), has garnered 2 citations, its significance lies in laying the technical groundwork for transformative science, from exoplanet characterization to galactic archaeology. Mukherjee’s work represents a critical step in enabling GMT to achieve its full potential, positioning him as a key figure in the next era of ground-based observational astronomy.