The MaNGA Integral Field Unit Fiber Feed System for the Sloan 2.5 m Telescope
N. Drory (UT), N. MacDonald (UW), M.A. Bershady (UWisc), K. Bundy, (IPMU), J. Gunn (Princeton), D.R. Law (UofT), M. Smith (UWisc), R. Stoll, (C-Tech), C.A. Tremonti (UWisc), D.A. Wake (UWisc), R. Yan (UKY), A.M., Weijmans (St. Andrews), N. Byler (UW), B. Cherinka (UofT)

TL;DR
This paper details the design, manufacturing, and performance of high-throughput, dense-packed integral field units for the MaNGA survey on the Sloan telescope, enabling efficient spectroscopic observations of thousands of galaxies.
Contribution
It introduces a scalable, low-stress manufacturing process for high-multiplex IFUs with high packing density and throughput, suitable for large astronomical surveys.
Findings
Achieved 96%+/-0.5% throughput from 350 nm to 1 μm in lab tests.
On-sky throughput exceeds single-fiber feeds by 5%.
Maintained low focal-ratio degradation despite repeated mechanical stress.
Abstract
We describe the design, manufacture, and performance of bare-fiber integral field units (IFUs) for the SDSS-IV survey MaNGA (Mapping Nearby Galaxies at APO) on the the Sloan 2.5 m telescope at Apache Point Observatory (APO). MaNGA is a luminosity-selected integral-field spectroscopic survey of 10,000 local galaxies covering 360-1030 nm at R ~ 2200. The IFUs have hexagonal dense packing of fibers with packing regularity of 3 um (RMS), and throughput of 96+/-0.5% from 350 nm to 1 um in the lab. Their sizes range from 19 to 127 fibers (3-7 hexagonal layers) using Polymicro FBP 120:132:150 um core:clad:buffer fibers to reach a fill fraction of 56%. High throughput (and low focal-ratio degradation) is achieved by maintaining the fiber cladding and buffer intact, ensuring excellent surface polish, and applying a multi-layer AR coating of the input and output surfaces. In operations on-sky,…
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