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Proceedings Paper

Fabricating transition-edge bolometers and the SQUID readout on one chip
Author(s): T. May; S. Anders; L. Fritzsch; R. Boucher; V. Zakosarenko; H.-G. Meyer; N. Jethava; E. Kreysa; G. Siringo
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Paper Abstract

Ever since the first proposal of the voltage-biased transition-edge bolometer the astrophysics community desired bolometer arrays with as many pixels as possible. With respect to the technical problem due to the need of lots of readout SQUID sensors only with multiplexing it is possible to go beyond a few hundred pixel. A technology which allows the manufacture of detector and readout on one chip would simplify this task substantially. Here we demonstrate the fabrication of a transition edge sensor based on a thermistor out of a molybdenum / gold-palladium bilayer. The alloy of gold-palladium (Au-Pd), which allows the tuning of molybdenum's critical temperature by one order of magnitude, is taken from our foundry process for SQUID manufacturing. Au-Pd can further be used for shunt resistances, absorber patterns and bond pads, and, therefore, it is a good choice for a combined technology. The thermistor is placed on a moderately patterned silicon nitride membrane in the shape of an 8-legged spider. The radiation band of interest is coupled via a conical feed horn to a simple grid of dipole-like antenna patterns. This removes the need for the poorly reproducible high-resistance absorption films for the matching of the free space impedance. The simple detector technology is compatible with the SQUID manufacturing. Hence, some of the SQUID layers can be merged with the corresponding detector layer, i.e. the thermistor wiring and the SQUID washer are made in a single niobium layer. The concept of feed horn coupling eases the design requirements, consequently the SQUID can be placed close to the detector, thereby allowing a simpler wiring to be used and in theory a better performance to be obtained.

Paper Details

Date Published: 27 June 2006
PDF: 8 pages
Proc. SPIE 6275, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III, 62751Q (27 June 2006); doi: 10.1117/12.671441
Show Author Affiliations
T. May, Institute for Physical High Technology (Germany)
S. Anders, Institute for Physical High Technology (Germany)
L. Fritzsch, Institute for Physical High Technology (Germany)
R. Boucher, Institute for Physical High Technology (Germany)
V. Zakosarenko, Institute for Physical High Technology (Germany)
H.-G. Meyer, Institute for Physical High Technology (Germany)
N. Jethava, Max Planck Institute for Radio Astronomy (Germany)
E. Kreysa, Max Planck Institute for Radio Astronomy (Germany)
G. Siringo, Max Planck Institute for Radio Astronomy (Germany)


Published in SPIE Proceedings Vol. 6275:
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III
Jonas Zmuidzinas; Wayne S. Holland; Stafford Withington; William D. Duncan, Editor(s)

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