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Title: SPT-SLIM: A Line Intensity Mapping Pathfinder for the South Pole Telescope

Journal Article · · Journal of Low Temperature Physics
ORCiD logo [1];  [2];  [3];  [4];  [5];  [6];  [3];  [7];  [2];  [8];  [9];  [10];  [7];  [6];  [11];  [7];  [12];  [13]
  1. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP)
  2. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  3. Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Argonne National Lab. (ANL), Lemont, IL (United States); Univ. of Chicago, IL (United States)
  4. Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  5. Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP); Univ. of Chicago, IL (United States)
  6. Argonne National Lab. (ANL), Lemont, IL (United States)
  7. McGill Univ., Montreal, QC (Canada). McGill Space Inst.
  8. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
  9. Univ. of Arizona, Tucson, AZ (United States). Steward Observatory
  10. Univ. of Chicago, IL (United States)
  11. Cardiff Univ. (United Kingdom)
  12. Univ. of Chicago, IL (United States); Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP)
  13. Three-Speed Logic, Inc., Victoria, BC (Canada)

The South Pole Telescope Summertime Line Intensity Mapper (SPT-SLIM) is a pathfinder experiment that will demonstrate the use of on-chip filter-bank spectrometers for mm-wave line intensity mapping (LIM). The SPT-SLIM focal plane consists of 18 dual-polarization R=300 filter-bank spectrometers covering 120-180 GHz, coupled to aluminum kinetic inductance detectors. A compact cryostat holds the detectors at 100 mK and performs observations without removing the SPT-3G receiver. SPT-SLIM will be deployed to the 10-m South Pole Telescope for observations during the 2023-24 austral summer. Furthermore, we discuss the overall instrument design, expected detector performance and sensitivity to the LIM signal from CO at 0.5 < z < 2. The technology and observational techniques demonstrated by SPT-SLIM will enable next-generation LIM experiments that constrain cosmology beyond the redshift reach of galaxy surveys.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); USDOE Laboratory Directed Research and Development (LDRD) Program
Grant/Contract Number:
AC02-07CH11359; AST-2108763; AST-2001802
OSTI ID:
1834182
Report Number(s):
FERMILAB-PUB-21-649-PPD; arXiv:2111.04631; ISSN 1573-7357; oai:inspirehep.net:1963691; TRN: US2300143
Journal Information:
Journal of Low Temperature Physics, Vol. 209, Issue 5-6; ISSN 0022-2291
Publisher:
Springer NatureCopyright Statement
Country of Publication:
United States
Language:
English

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