WorldCat Identities

Yates, S. J. C.

Overview
Works: 7 works in 7 publications in 1 language and 12 library holdings
Roles: Contributor, Author, Other
Publication Timeline
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Most widely held works by S. J. C Yates
Superconducting Coplanar Waveguide Filters for Submillimeter Wave On-Chip Filterbank Spectrometers by A Endo( )

1 edition published in 2016 in English and held by 2 WorldCat member libraries worldwide

Large Angle Optical Access in a Sub-Kelvin Cryostat by S Hähnle( )

1 edition published in 2018 in English and held by 2 WorldCat member libraries worldwide

The Néel IRAM KID Arrays (NIKA) by A Monfardini( )

1 edition published in 2011 in English and held by 2 WorldCat member libraries worldwide

Calibration Scheme for Large Kinetic Inductance Detector Arrays Based on Readout Frequency Response by L Bisigello( )

1 edition published in 2016 in English and held by 2 WorldCat member libraries worldwide

A Time Domain Multiplexer for Large Arrays of High Impedance Low Temperature Bolometers by A Benoit( )

1 edition published in 2008 in English and held by 2 WorldCat member libraries worldwide

Antenna coupled kinetic inductance detectors for space based sub-mm astronomy: by S.J.C Yates( )

1 edition published in 2008 in English and held by 1 WorldCat member library worldwide

To achieve background limited detection, future space missions in the far infrared and sub-mm radiation bands will require large arrays (>1000 pixels) of very sensitive detectors. A typical requirement for the noise equivalent power is 10^-19 W/Hz^0.5 for a Fourier Transform Spectrometer, which is 100 to 1000 times more sensitive than the state of the art such as on HERSCHEL. Such low NEP is a significant technical challenge, both to achieve for the detectors and to demonstrate in the laboratory. Kinetic inductance detectors can theoretically achieve this performance and have significant advantages over other types of detectors, for example are well adapted to frequency domain multiplexing. We present antenna coupled kinetic inductance detectors, showing the loaded optical NEP measured with a well controlled narrow band black body radiation source. We will also discuss the optimization route required to reach the requirements for future missions, including the optical testing requirements
Antenna coupled kinetic inductance arrays for space and ground based imaging arrays: by S.J.C Yates( )

1 edition published in 2009 in English and held by 1 WorldCat member library worldwide

Very large arrays of Microwave Kinetic Inductance Detectors (MKIDs) have the potential to revolutionize ground and space based astronomy. They can offer in excess of 10000 pixels with large dynamic range and very high sensitivity in combination with very efficient frequency division multiplexing at GHz frequencies. In this paper we present the development for a ∼ 100 pixel MKID demonstration array based upon an single pixel consisting of an integrated MKID-antenna detector, with the antenna placed in the second focus of an elliptical Si lens. The design presented can be scaled to any frequency between 80 GHz and >5 THz because there is no need for superconducting structures that become lossy at frequencies above the gap frequency of the materials used. We present measurements of the optical coupling efficiency, sensitivity and discuss array development. We have obtained a dark sensitivity of 7 × 10<sup>-19</sup> W/Hz<sup>1/2</sup> using 100 nm thick Al devices and an optical coupling efficiency of 35 % referring to the power of a single polarization optical signal in front of the Si lens of the detector. © 2009 American Institute of Physics
 
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