The WEAVE-TwiLight-Survey: expanding WEAVE's reach to bright and low-surface-density targets with a novel observing mode
Current-day multi-object spectroscopic surveys are often limited in their ability to observe bright stars due to their low surface densities, resulting in increased observational overheads and reduced efficiency. Addressing this, we have developed a novel observing mode for WEAVE (William Herschel Telescope Enhanced Area Velocity Explorer) that
Hajnik, Thomas et al.
Fecha de publicación:
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2025