Design of the SPT-SLIM Focal Plane: A Spectroscopic Imaging Array for the South Pole Telescope

  • P. S. Barry
  • , A. Anderson
  • , B. Benson
  • , J. E. Carlstrom
  • , T. Cecil
  • , C. Chang
  • , M. Dobbs
  • , M. Hollister
  • , K. S. Karkare
  • , G. K. Keating
  • , D. Marrone
  • , J. McMahon
  • , J. Montgomery
  • , Z. Pan
  • , G. Robson
  • , M. Rouble
  • , E. Shirokoff
  • , G. Smecher

Research output: Contribution to journalArticlepeer-review

4 Scopus citations

Abstract

The Summertime Line Intensity Mapper (SLIM) is a mm-wave line-intensity mapping (mm-LIM) experiment for the South Pole Telescope (SPT). The goal of SPT-SLIM is to serve as a technical and scientific pathfinder for the demonstration of the suitability and in-field performance of multi-pixel superconducting filterbank spectrometers for future mm-LIM experiments. Scheduled to deploy in the 2023-24 austral summer, the SPT-SLIM focal plane will include 18 dual-polarisation pixels, each coupled to an R= λ/ Δ λ= 300 thin-film microstrip filterbank spectrometer that spans the 2 mm atmospheric window (120–180 GHz). Each individual spectral channel feeds a microstrip-coupled lumped-element kinetic inductance detector, which provides the highly multiplexed readout for the 10k detectors needed for SPT-SLIM. Here, we present an overview of the preliminary design of key aspects of the SPT-SLIM focal plane array, a description of the detector architecture and predicted performance, and initial test results that will be used to inform the final design of the SPT-SLIM spectrometer array.

Original languageEnglish (US)
Pages (from-to)879-888
Number of pages10
JournalJournal of Low Temperature Physics
Volume209
Issue number5-6
DOIs
StatePublished - Dec 2022

Keywords

  • Filterbank spectrometer
  • Kinetic inductance detectors
  • Line intensity mapping
  • SPT-SLIM
  • South pole telescope

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics
  • General Materials Science
  • Condensed Matter Physics

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