A temperature- and pressure-stabilized Fabry-Perot etalon with Xenon arc lamp produces >10,000 lines across 62 echelle orders for PARAS-2 and yields a theoretical RV calibration stability of 10 cm/s.
TOI-6038 A b: A dense sub-Saturn in the transition regime between the Neptunian ridge and savanna,
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Design and development of Fabry-Perot based wavelength calibration system for PARAS-2 spectrograph
A temperature- and pressure-stabilized Fabry-Perot etalon with Xenon arc lamp produces >10,000 lines across 62 echelle orders for PARAS-2 and yields a theoretical RV calibration stability of 10 cm/s.