The CRS: a scalable full-stack control system for Microwave Kinetic Inductance Detectors
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| Main Authors: | , , , , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866929493791211520 |
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| author | Montgomery, Joshua Avelino, Wellington Dobbs, Matt Letang, Joseph Rouble, Maclean Savchyn, Sofiia Smecher, Graeme |
| author_facet | Montgomery, Joshua Avelino, Wellington Dobbs, Matt Letang, Joseph Rouble, Maclean Savchyn, Sofiia Smecher, Graeme |
| contents | The t0.technology Control and Readout System (CRS) is a modular microwave control and readout system for mm-wave and radio astronomy, THz imaging, noise radar, and superconducting qubit control. The configuration discussed in this work implements firmware for readout of microwave Kinetic Inductance Detector (KID) arrays. The CRS can operate 4,096 KIDs over 2.5 GHz of complex bandwidth between 0-10 GHz, typically allocated across four independent RF chains at 1,024x multiplexing and 625 MHz of complex bandwidth each. Every CRS can operate as a standalone unit or collectively within one or more backplane-enabled subracks that distribute power, clocking, and synchronization, scaling to an arbitrary number of channels. Each fully populated subrack supports arrays of more than 65,000 KIDs. The signal processing and control software supports recent innovations in multi-probe measurements and dynamic feedback modes, which are described in (Rouble et al. 2024). The CRS has recently been selected as the new baseline readout system for the proposed South Pole Telescope instrument, SPT-3G+. We present the hardware design, firmware capabilities, open-source control and data acquisition software, and the first laboratory characterization measurements. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_16266 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The CRS: a scalable full-stack control system for Microwave Kinetic Inductance Detectors Montgomery, Joshua Avelino, Wellington Dobbs, Matt Letang, Joseph Rouble, Maclean Savchyn, Sofiia Smecher, Graeme Instrumentation and Methods for Astrophysics The t0.technology Control and Readout System (CRS) is a modular microwave control and readout system for mm-wave and radio astronomy, THz imaging, noise radar, and superconducting qubit control. The configuration discussed in this work implements firmware for readout of microwave Kinetic Inductance Detector (KID) arrays. The CRS can operate 4,096 KIDs over 2.5 GHz of complex bandwidth between 0-10 GHz, typically allocated across four independent RF chains at 1,024x multiplexing and 625 MHz of complex bandwidth each. Every CRS can operate as a standalone unit or collectively within one or more backplane-enabled subracks that distribute power, clocking, and synchronization, scaling to an arbitrary number of channels. Each fully populated subrack supports arrays of more than 65,000 KIDs. The signal processing and control software supports recent innovations in multi-probe measurements and dynamic feedback modes, which are described in (Rouble et al. 2024). The CRS has recently been selected as the new baseline readout system for the proposed South Pole Telescope instrument, SPT-3G+. We present the hardware design, firmware capabilities, open-source control and data acquisition software, and the first laboratory characterization measurements. |
| title | The CRS: a scalable full-stack control system for Microwave Kinetic Inductance Detectors |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2406.16266 |