In situ time constant and optical efficiency measurements of TRUCE pixels in the Atacama B-mode search

S. M. Simon, J. W. Appel, H. M. Cho, T. Essinger-Hileman, K. D. Irwin, A. Kusaka, M. D. Niemack, M. R. Nolta, L. A. Page, L. P. Parker, S. Raghunathan, J. L. Sievers, S. T. Staggs, K. Visnjic

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

Abstract

The Atacama B-mode Search (ABS) instrument, which began observation in February of 2012, is a crossed-Dragone telescope located at an elevation of 5,100 m in the Atacama Desert in Chile. The primary scientific goal of ABS is to measure the B-mode polarization spectrum of the Cosmic Microwave Background from multipole moments of about ℓ ≈ 50 to ℓ ≈ 500 (angular scales from ∼0.4° to ∼4°), a range that includes the primordial B-mode peak from inflationary gravitational waves. The ABS focal plane array consists of 240 pixels designed for observation at 145 GHz by the TRUCE collaboration. Each pixel has its own individual, single-moded feedhorn and contains two transition-edge sensor bolometers coupled to orthogonal polarizations that are read out using time domain multiplexing. We will report on the current status of ABS and discuss the time constants and optical efficiencies of the TRUCE detectors in the field.

Original languageEnglish (US)
Pages (from-to)712-718
Number of pages7
JournalJournal of Low Temperature Physics
Volume176
Issue number5-6
DOIs
StatePublished - Sep 2014

All Science Journal Classification (ASJC) codes

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

Keywords

  • Atacama B-mode Search
  • Cosmic Microwave Background
  • Polarization

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