Computer Science – Performance
Scientific paper
May 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000pmagb..80..919g&link_type=abstract
Philisophical Magazine B, vol. 80, Issue 5, p.919-927
Computer Science
Performance
Scientific paper
A new generation of astronomical detectors has recently been developed, on the basis of superconducting tunnel junctions (STJs). STJs are capable of detecting photons in a wide range of wavelengths, from X-rays to infrared; also the counting of single photons in the optical range has been demonstrated. Since these detectors operate at very low temperature (down to 100mK), a natural candidate for the read-out electronics is the dc superconducting quantum interference device (SQUID), an extremely sensitive magnetometer that is fabricated with a similar technology to the STJ junctions. Biasing the STJ at a constant voltage, the current pulse caused by the incoming radiation is passed through the tightly coupled input coil of the SQUID and converted into a magnetic flux signal which can be detected. In this paper we present measurements on a home-made dc SQUID, showing the response of the device to current pulses, which simulate the real signals from a STJ. We show how the SQUID performance can be improved by using a superconducting flux transformer, which allows us to detect signal amplitudes of fraction of nanoamperes, such as the signals coming from irradiation of STJs in the nearinfrared range.
Carelli Pasquale
Castellano Maria Gabriella
Greco F. V.
Leoni Riccardo
Torrioli Guido
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