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Sensor for mm and sub-mm wawelength range

Context evolution

  • CNES prospective 2014 : first priority : Detection of B-modes of the Cosmic Microwave Background (CMB) polarization (to constrain inflation models of the early Universe evolution, prior to recombination)
  • ESA cosmic vision 2015-2025 program M5 call end 2015 : Core+ ? SPICA (sub mm) ?

FOCUS progresses

Detector development along two axes :

  • High impedance bolometers
  • Kinetic Inductance Detector (KIDs)* (Choice was made not to develop Transistor Edge Sensors, well developed in US)

*superconducting devices using photon-assisted pair breaking to detect radiation

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SI-Grid bolometers : a new start thanks to FOCUS

Assets : all silicon technology,
benefits from LETI silicon platform (semi-industrial),
HERSCHEL-PACS heritage, www.herschel.fr

A novel conception

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Silicium report
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SI-Grid bolometers
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Type Bipol

Derived on bolometers developed for commercial use
> cost effective

Enhanced capability on the pixel two polarisations simultaneously measured, 
 multi colors (Patented)

  • New key technological processes successfully tested on test vehicles produced at Leti
  • New technological processes in synergies with R&D for large production industrial projects at CEA-Leti

> guarantee the continuity of the technology

KIDS : fast reacting developments thanks to FOCUS

Assets
• very few technological steps to make them.

FOCUS
• Improvement of detector arrays for the NIKA2 camera

Increase in complexity

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Matrice à 2000 pixels

30 pixels (2009) {JPEG}


to be installed by the end of 2015 at the 30 m IRAM telescope


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