A Novel Freeform Slicer IFU for the Magellan InfraRed Multi-Object Spectrograph (MIRMOS)
Maren Cosens (1), Nicholas P. Konidaris II (1), Gwen C. Rudie (1),, Andrew B. Newman (1), Gerrad Killion (1), Leon Aslan (1), Robert Barkhouser, (2), Andrea Bianco (3), Christoph Birk (1), Julia Brady (1), Michele, Frangiamore (3), Tyson Hare (1), Stephen C. Hope (4)

TL;DR
This paper introduces a new freeform slicer IFU design for MIRMOS, a next-generation infrared spectrograph, featuring a large field of view and innovative optical components to enhance astronomical observations.
Contribution
It presents a novel freeform surface design for the slicer IFU, enabling a large FoV and high image quality for the MIRMOS instrument, with detailed optical and mechanical concepts.
Findings
Design achieves a 20"x26" FoV with high image quality.
Use of freeform surfaces improves optical performance.
Manufacturing involves high-precision diamond milling.
Abstract
The Magellan InfraRed Multi-Object Spectrograph (MIRMOS) is a planned next generation multi-object and integral field spectrograph for the 6.5m Magellan telescopes at Las Campanas Observatory in Chile. MIRMOS will perform R3700 spectroscopy over a simultaneous wavelength range of 0.886 - 2.404m (Y,J,H,K bands) in addition to imaging over the range of 0.7 - 0.886m. The integral field mode of operation for MIRMOS will be achieved via an image slicer style integral field unit (IFU) located on a linear stage to facilitate movement into the beam during use or storage while operating in multi-object mode. The IFU will provide a field of view (FoV) made up of slices. This will be the largest FoV IFS operating at these wavelengths from either the ground or space, making MIRMOS an ideal instrument for a wide range of science cases…
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Astronomy and Astrophysical Research
