CCAT: A status update on the EoR-Spec instrument module for Prime-Cam
Rodrigo Freundt, Yaqiong Li, Doug Henke, Jason Austermann, James R., Burgoyne, Scott Chapman, Steve K. Choi, Cody J. Duell, Zach Huber, Michael, Niemack, Thomas Nikola, Lawrence Lin, Dominik A. Riechers, Gordon Stacey,, Anna K. Vaskuri, Eve M. Vavagiakis, Jordan Wheeler

TL;DR
EoR-Spec is a new instrument designed for the Prime-Cam receiver to map the early universe's star formation history through [CII] line observations, utilizing advanced MKID detectors and a spectral resolving system.
Contribution
This paper provides a detailed update on the mechanical, optical, and fabrication progress of the EoR-Spec instrument for the Prime-Cam system.
Findings
Final design of EoR-Spec's optical and mechanical components
Progress in fabrication, characterization, and testing phases
Expected first light in 2026
Abstract
The Epoch of Reionization Spectrometer (EoR-Spec) is an upcoming Line Intensity Mapping (LIM) instrument designed to study the evolution of the early universe (z = 3.5 to 8) by probing the redshifted [CII] 158 m fine-structure line from aggregates of galaxies. The [CII] emission is an excellent tracer of star formation since it is the dominant cooling line from neutral gas heated by OB star light and thus can be used to probe the reionization of the early Universe due to star formation. EoR-Spec will be deployed on Prime-Cam, a modular direct-detection receiver for the 6-meter Fred Young Submillimeter Telescope (FYST), currently under construction by CPI Vertex Antennentechnik GmbH and to be installed near the summit of Cerro Chajnantor in the Atacama Desert. This instrument features an image plane populated with more than 6500 Microwave Kinetic Inductance Detectors (MKIDs) that…
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