Ultrasensitive TES bolometers for space-based FIR astronomy

D. Morozov, P. D. Mauskopf, P. Ade, M. Ridder, P. Khosropanah, M. Bruijn, J. Van Der Kuur, H. Hoevers, J. R. Gao, D. Griffin

Research output: Contribution to journalArticle

11 Scopus citations

Abstract

Results of study optical performance of single pixel transition edge sensor (TES) bolometer presented at wavelength band 30-60 μm are presented. FIR radiation is coupled into amultimode horn with entrance aperture of 450 μM, length 4.5 mm and exit aperture of 45 μm, which feeds a metal integrating cavity containing the detector. The radiation band is defined by a pair of lowpass and highpass mesh filters in front of the horn. Here we present measurements of optical noise equivalent power (NEP), optical efficiency, dynamic range and time constant. The results showthat measured TES detectors are close to meeting the requirementof the "Band S" of SAFARI FTS imaging instrument [1] on the SPICA mission [2].

Original languageEnglish (US)
Article number5634093
Pages (from-to)188-191
Number of pages4
JournalIEEE Transactions on Applied Superconductivity
Volume21
Issue number3 PART 1
DOIs
StatePublished - Jun 1 2011
Externally publishedYes

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Keywords

  • Far-IR detector
  • SiN thermal transport
  • Transition edge sensor

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Electrical and Electronic Engineering

Cite this

Morozov, D., Mauskopf, P. D., Ade, P., Ridder, M., Khosropanah, P., Bruijn, M., Kuur, J. V. D., Hoevers, H., Gao, J. R., & Griffin, D. (2011). Ultrasensitive TES bolometers for space-based FIR astronomy. IEEE Transactions on Applied Superconductivity, 21(3 PART 1), 188-191. [5634093]. https://doi.org/10.1109/TASC.2010.2089585