On-sky performance of the SPT-3G frequency-domain multiplexed readout
arXiv:1907.10947 · doi:10.1007/s10909-019-02280-w
Abstract
Frequency-domain multiplexing (fMux) is an established technique for the readout of large arrays of transition edge sensor (TES) bolometers. Each TES in a multiplexing module has a unique AC voltage bias that is selected by a resonant filter. This scheme enables the operation and readout of multiple bolometers on a single pair of wires, reducing thermal loading onto sub-Kelvin stages. The current receiver on the South Pole Telescope, SPT-3G, uses a 68x fMux system to operate its large-format camera of 16,000 TES bolometers. We present here the successful implementation and performance of the SPT-3G readout as measured on-sky. Characterization of the noise reveals a median pair-differenced 1/f knee frequency of 33 mHz, indicating that low-frequency noise in the readout will not limit SPT-3G's measurements of sky power on large angular scales. Measurements also show that the median readout white noise level in each of the SPT-3G observing bands is below the expectation for photon noise, demonstrating that SPT-3G is operating in the photon-noise-dominated regime.
arXiv comment9 pages, 5 figures submitted to the Journal of Low Temperature Physics: LTD18 Special Edition
References in corpus (15)
- The Quest for B Modes from Inflationary Gravitational Waves
- Advanced ACTPol Cryogenic Detector Arrays and Readout
- The POLARBEAR-2 and the Simons Array Experiment
- Frequency Multiplexed SQUID Readout of Large Bolometer Arrays for Cosmic Microwave Background Measurements
- Measurements of Sub-degree B-mode Polarization in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
- Antenna-coupled TES bolometers used in BICEP2, Keck array, and SPIDER
- The Simons Observatory: Instrument Overview
- Measurements of E-Mode Polarization and Temperature-E-Mode Correlation in the Cosmic Microwave Background from 100 Square Degrees of SPTpol Data
- Improved Performance of TES Bolometers using Digital Feedback
- Microwave SQUID Multiplexer demonstration for Cosmic Microwave Background Imagers
- Year two instrument status of the SPT-3G cosmic microwave background receiver
- Code-division multiplexing for x-ray microcalorimeters
- Millimeter Wavelength Brightness Fluctuations of the Atmosphere Above the South Pole
- Digital frequency domain multiplexing readout electronics for the next generation of millimeter telescopes
- Development of the superconducting detectors and read-out for the X-IFU instrument on board of the X-ray observatory Athena
Cited by in corpus (10)
- A Review of X-ray Microcalorimeters Based on Superconducting Transition Edge Sensors for Astrophysics and Particle Physics
- Simons Observatory Microwave SQUID Multiplexing Readout -- Cryogenic RF Amplifier and Coaxial Chain Design
- Instrumental systematics biases in CMB lensing reconstruction: a simulation-based assessment
- Performance and characterization of the SPT-3G digital frequency-domain multiplexed readout system using an improved noise and crosstalk model
- Characterization of MKIDs for CMB observation at 220 GHz with the South Pole Telescope
- Demonstration of a 1820 channel multiplexer for transition-edge sensor bolometers
- Light Dark Matter Detection with Hydrogen-rich Crystals and Low-Tc TES Detectors
- Performance of a low-parasitic frequency-domain multiplexing readout
- Correlating Visual Characteristics and Cryogenic Performance of Superconducting Detectors
- The Design and Integrated Performance of SPT-3G