Published April 2021 | Version Accepted Version + Published
Journal Article Open

Proof of concept for through silicon vias in application-specific integrated circuits for hard x-ray imaging detectors

  • 1. ROR icon Harvard-Smithsonian Center for Astrophysics
  • 2. ROR icon California Institute of Technology

Abstract

Application-specific integrated circuits (ASICs) are commonly used to efficiently process the signals from sensors and detectors in space. Wire bonding is a space-qualified technique of making interconnections between ASICs and their substrate packaging board for power, control, and readout of the ASICs. Wire bonding is nearly ubiquitous in modern space programs, but their exposed wires can be prone to damage during assembly and subject to electric interference during operations. Additional space around the ASICs needed for wire bonding also impedes efficient packaging of large arrays of detectors. Here, we introduce the through silicon vias (TSV) technology that replaces wire bonds and eliminates their shortcomings. We have successfully demonstrated the feasibility of implementing TSVs to existing ASIC wafers (a.k.a. a via-last process) developed for processing the x-ray signals from the x-ray imaging CdZnTe detectors on the Nuclear Spectroscopic Telescope Array small explorer telescope mission that was launched in 2012. While TSVs are common in the semiconductor industry, this is the first (to our knowledge) successful application for astrophysics imaging instrumentation. We expect that the TSV technology will simplify the detector assembly and thus will enable significant cost and schedule savings in assembly of large area CdZnTe detectors.

Additional Information

© 2021 Society of Photo-Optical Instrumentation Engineers (SPIE). Paper 20186 received Dec. 22, 2020; accepted for publication Mar. 12, 2021; published online Apr. 9, 2021. This work was supported by NASA APRA Grant No. NNX17AE62G.

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Published - 026001_1.pdf

Accepted Version - 2103.08749.pdf

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Additional details

Identifiers

Eprint ID
108496
Resolver ID
CaltechAUTHORS:20210318-162735516

Related works

Funding

NASA
NNX17AE62G

Dates

Created
2021-03-24
Created from EPrint's datestamp field
Updated
2021-08-24
Created from EPrint's last_modified field

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