
TL;DR
This paper discusses the potential of large-scale replication of spectrographs to address the challenges of scaling instruments for extremely large telescopes, highlighting current implementations and future prospects.
Contribution
It reviews the design principles, lessons learned, and future technologies for replicating spectrographs to enable cost-effective, scalable solutions for ELTs.
Findings
Replicated spectrographs like MUSE and VIRUS increase information gathering.
Replication reduces costs and engineering complexity.
Future technologies could further enhance replicated instrument capabilities.
Abstract
As telescope apertures increase, the challenge of scaling spectrographic astronomical instruments becomes acute. The next generation of extremely large telescopes (ELTs) strain the availability of glass blanks for optics and engineering to provide sufficient mechanical stability. While breaking the relationship between telescope diameter and instrument pupil size by adaptive optics is a clear path for small fields of view, survey instruments exploiting multiplex advantages will be pressed to find cost-effective solutions. In this review we argue that exploiting the full potential of ELTs will require the barrier of the cost and engineering difficulty of monolithic instruments to be broken by the use of large-scale replication of spectrographs. The first steps in this direction have already been taken with the soon to be commissioned MUSE and VIRUS instruments for the Very Large…
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