FLARES iterative line-selection algorithm achieves 1.122 m/s RV RMS using 24 lines on 383 days of NEID solar data, better than full list or CCF.
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New instrument suite for ultra-high resolution solar spectroscopy with laser frequency comb calibration enabling precise Sun-as-a-star and spatially resolved line studies.
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Improving the Precision of Line-by-Line Radial Velocities: A Data-Driven Iterative Algorithm for Spectral Line Selection
FLARES iterative line-selection algorithm achieves 1.122 m/s RV RMS using 24 lines on 383 days of NEID solar data, better than full list or CCF.
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Observing the integrated and spatially resolved Sun with ultra-high spectral resolution
New instrument suite for ultra-high resolution solar spectroscopy with laser frequency comb calibration enabling precise Sun-as-a-star and spatially resolved line studies.