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Tuesday, January 8, 2019 - 11:15 to 12:30 Auditorium
Following a review of G-CLEF – a first light High-R spectrograph for the Giant Magellan Telescope, I will present a concept extreme high resolution spectrograph optimized for molecular oxygen detection, a prominent biomarker in Earth atmosphere, using the transmission spectroscopy method. The instrument is based on the transmission properties of Fabry Perot Interferometers, and despite its modest dimensions is capable of achieving spectral resolution and sampling frequency in excess of R~300,000. I will discuss design parameters and the unique aspects that needs to be taken into account in the design of an FPI based instrument, and conclude with MC simulation results demonstrating the advantages of such a novel instrument.