Design and Electrical Performance of the Kinetic Inductance Detectors of the OLIMPO Experiment

A. Paiella, E. S. Battistelli, F. Columbro, A. Coppolecchia, G. D'Alessandro, P. De Bernardis, L. Lamagna, S. Masi, F. Piacentini, M. G. Castellano, I. Colantoni, S. Gordon, Philip Mauskopf

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Citation (Scopus)

Abstract

We are going to describe the design and the electrical performance of the horn-coupled lumped element kinetic inductance detectors (LEKIDs) for the OLIMPO experiment. OLIMPO is a balloon-borne mission, devoted to the study of the largest structures in the Universe, by detecting the Sunyaev-Zel'dovich effect of the Cosmic Microwave Background (CMB) photons crossing clusters of galaxies. The multi-band focal planes (centered at 150, 200, 350 and 480 GHz), large aperture telescope (2.6 m), photometric and spectrometer configuration (OLIMPO is equipped with a plug-in differential Fourier transform spectrometer) make OLIMPO able to characaterise all the components of the Sunyaev-Zel'dovich effect with unprecedented precision. The design of the LEKIDs has been optimised to cope with a wide range of optical loadings (corresponding to both photometric and spectrometric configurations). The electrical characterisation of the LEKID arrays was performed in the OLIMPO cryostat, at a temperature around 300 mK and under a constant optical load lower than 500 fW. The readout electronics is a customised ROACH-2 coupled to a MUSIC DAC/ADC board. The averaged responsivities for the arrays, measured from the phase readout, are 1.18x1011 rad/W for the 150 GHz array, 4.10x1010 rad/W for the 200 GHz array, 1.09x1012 rad/W for the 350 GHz array, and 4.41x1011 rad/W for the 480 GHz array. Therefore, measuring the spectral noise density for each pixels of the arrays, whose average values are 2.5x10-5 rad/Hz(1/2) for the 150 GHz array, 3.6x10-5 rad/Hz(1/2) for the 200 GHz array, 5.1x10-5 rad/Hz(1/2) for the 350 GHz array, and 1.9x10-5 rad/Hz(1/2) for the 480 GHz array, we obtained the values of the averaged electrical noise equivalent power (NEP) over all the arrays: 2x10-16 W/Hz(1/2), 9x10-16 W/Hz(1/2), 5x10-17 W/Hz(1/2), and 4x10-17 W/Hz(1/2) respectively for the four OLIMPO arrays.

Original languageEnglish (US)
Title of host publication2017 16th International Superconductive Electronics Conference, ISEC 2017
PublisherInstitute of Electrical and Electronics Engineers Inc.
Pages1-3
Number of pages3
Volume2018-January
ISBN (Electronic)9781509058686
DOIs
StatePublished - Mar 9 2018
Event16th International Superconductive Electronics Conference, ISEC 2017 - Napoli, Italy
Duration: Jun 12 2017Jun 16 2017

Other

Other16th International Superconductive Electronics Conference, ISEC 2017
CountryItaly
CityNapoli
Period6/12/176/16/17

Fingerprint

inductance
Inductance
Detectors
Kinetics
Spectrometers
detectors
kinetics
Cryostats
Galaxies
Optical constants
Experiments
Balloons
Telescopes
Fourier transforms
Electronic equipment
Photons
Pixels
Microwaves
readout
spectrometers

Keywords

  • CMB radiation
  • kinetic inductance detectors
  • OLIMPO experiment
  • SZ effect

ASJC Scopus subject areas

  • Electrical and Electronic Engineering
  • Electronic, Optical and Magnetic Materials
  • Atomic and Molecular Physics, and Optics

Cite this

Paiella, A., Battistelli, E. S., Columbro, F., Coppolecchia, A., D'Alessandro, G., De Bernardis, P., ... Mauskopf, P. (2018). Design and Electrical Performance of the Kinetic Inductance Detectors of the OLIMPO Experiment. In 2017 16th International Superconductive Electronics Conference, ISEC 2017 (Vol. 2018-January, pp. 1-3). Institute of Electrical and Electronics Engineers Inc.. https://doi.org/10.1109/ISEC.2017.8314223

Design and Electrical Performance of the Kinetic Inductance Detectors of the OLIMPO Experiment. / Paiella, A.; Battistelli, E. S.; Columbro, F.; Coppolecchia, A.; D'Alessandro, G.; De Bernardis, P.; Lamagna, L.; Masi, S.; Piacentini, F.; Castellano, M. G.; Colantoni, I.; Gordon, S.; Mauskopf, Philip.

2017 16th International Superconductive Electronics Conference, ISEC 2017. Vol. 2018-January Institute of Electrical and Electronics Engineers Inc., 2018. p. 1-3.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Paiella, A, Battistelli, ES, Columbro, F, Coppolecchia, A, D'Alessandro, G, De Bernardis, P, Lamagna, L, Masi, S, Piacentini, F, Castellano, MG, Colantoni, I, Gordon, S & Mauskopf, P 2018, Design and Electrical Performance of the Kinetic Inductance Detectors of the OLIMPO Experiment. in 2017 16th International Superconductive Electronics Conference, ISEC 2017. vol. 2018-January, Institute of Electrical and Electronics Engineers Inc., pp. 1-3, 16th International Superconductive Electronics Conference, ISEC 2017, Napoli, Italy, 6/12/17. https://doi.org/10.1109/ISEC.2017.8314223
Paiella A, Battistelli ES, Columbro F, Coppolecchia A, D'Alessandro G, De Bernardis P et al. Design and Electrical Performance of the Kinetic Inductance Detectors of the OLIMPO Experiment. In 2017 16th International Superconductive Electronics Conference, ISEC 2017. Vol. 2018-January. Institute of Electrical and Electronics Engineers Inc. 2018. p. 1-3 https://doi.org/10.1109/ISEC.2017.8314223
Paiella, A. ; Battistelli, E. S. ; Columbro, F. ; Coppolecchia, A. ; D'Alessandro, G. ; De Bernardis, P. ; Lamagna, L. ; Masi, S. ; Piacentini, F. ; Castellano, M. G. ; Colantoni, I. ; Gordon, S. ; Mauskopf, Philip. / Design and Electrical Performance of the Kinetic Inductance Detectors of the OLIMPO Experiment. 2017 16th International Superconductive Electronics Conference, ISEC 2017. Vol. 2018-January Institute of Electrical and Electronics Engineers Inc., 2018. pp. 1-3
@inproceedings{a291c6670a0346de9c25e5b4a5756ad2,
title = "Design and Electrical Performance of the Kinetic Inductance Detectors of the OLIMPO Experiment",
abstract = "We are going to describe the design and the electrical performance of the horn-coupled lumped element kinetic inductance detectors (LEKIDs) for the OLIMPO experiment. OLIMPO is a balloon-borne mission, devoted to the study of the largest structures in the Universe, by detecting the Sunyaev-Zel'dovich effect of the Cosmic Microwave Background (CMB) photons crossing clusters of galaxies. The multi-band focal planes (centered at 150, 200, 350 and 480 GHz), large aperture telescope (2.6 m), photometric and spectrometer configuration (OLIMPO is equipped with a plug-in differential Fourier transform spectrometer) make OLIMPO able to characaterise all the components of the Sunyaev-Zel'dovich effect with unprecedented precision. The design of the LEKIDs has been optimised to cope with a wide range of optical loadings (corresponding to both photometric and spectrometric configurations). The electrical characterisation of the LEKID arrays was performed in the OLIMPO cryostat, at a temperature around 300 mK and under a constant optical load lower than 500 fW. The readout electronics is a customised ROACH-2 coupled to a MUSIC DAC/ADC board. The averaged responsivities for the arrays, measured from the phase readout, are 1.18x1011 rad/W for the 150 GHz array, 4.10x1010 rad/W for the 200 GHz array, 1.09x1012 rad/W for the 350 GHz array, and 4.41x1011 rad/W for the 480 GHz array. Therefore, measuring the spectral noise density for each pixels of the arrays, whose average values are 2.5x10-5 rad/Hz(1/2) for the 150 GHz array, 3.6x10-5 rad/Hz(1/2) for the 200 GHz array, 5.1x10-5 rad/Hz(1/2) for the 350 GHz array, and 1.9x10-5 rad/Hz(1/2) for the 480 GHz array, we obtained the values of the averaged electrical noise equivalent power (NEP) over all the arrays: 2x10-16 W/Hz(1/2), 9x10-16 W/Hz(1/2), 5x10-17 W/Hz(1/2), and 4x10-17 W/Hz(1/2) respectively for the four OLIMPO arrays.",
keywords = "CMB radiation, kinetic inductance detectors, OLIMPO experiment, SZ effect",
author = "A. Paiella and Battistelli, {E. S.} and F. Columbro and A. Coppolecchia and G. D'Alessandro and {De Bernardis}, P. and L. Lamagna and S. Masi and F. Piacentini and Castellano, {M. G.} and I. Colantoni and S. Gordon and Philip Mauskopf",
year = "2018",
month = "3",
day = "9",
doi = "10.1109/ISEC.2017.8314223",
language = "English (US)",
volume = "2018-January",
pages = "1--3",
booktitle = "2017 16th International Superconductive Electronics Conference, ISEC 2017",
publisher = "Institute of Electrical and Electronics Engineers Inc.",

}

TY - GEN

T1 - Design and Electrical Performance of the Kinetic Inductance Detectors of the OLIMPO Experiment

AU - Paiella, A.

AU - Battistelli, E. S.

AU - Columbro, F.

AU - Coppolecchia, A.

AU - D'Alessandro, G.

AU - De Bernardis, P.

AU - Lamagna, L.

AU - Masi, S.

AU - Piacentini, F.

AU - Castellano, M. G.

AU - Colantoni, I.

AU - Gordon, S.

AU - Mauskopf, Philip

PY - 2018/3/9

Y1 - 2018/3/9

N2 - We are going to describe the design and the electrical performance of the horn-coupled lumped element kinetic inductance detectors (LEKIDs) for the OLIMPO experiment. OLIMPO is a balloon-borne mission, devoted to the study of the largest structures in the Universe, by detecting the Sunyaev-Zel'dovich effect of the Cosmic Microwave Background (CMB) photons crossing clusters of galaxies. The multi-band focal planes (centered at 150, 200, 350 and 480 GHz), large aperture telescope (2.6 m), photometric and spectrometer configuration (OLIMPO is equipped with a plug-in differential Fourier transform spectrometer) make OLIMPO able to characaterise all the components of the Sunyaev-Zel'dovich effect with unprecedented precision. The design of the LEKIDs has been optimised to cope with a wide range of optical loadings (corresponding to both photometric and spectrometric configurations). The electrical characterisation of the LEKID arrays was performed in the OLIMPO cryostat, at a temperature around 300 mK and under a constant optical load lower than 500 fW. The readout electronics is a customised ROACH-2 coupled to a MUSIC DAC/ADC board. The averaged responsivities for the arrays, measured from the phase readout, are 1.18x1011 rad/W for the 150 GHz array, 4.10x1010 rad/W for the 200 GHz array, 1.09x1012 rad/W for the 350 GHz array, and 4.41x1011 rad/W for the 480 GHz array. Therefore, measuring the spectral noise density for each pixels of the arrays, whose average values are 2.5x10-5 rad/Hz(1/2) for the 150 GHz array, 3.6x10-5 rad/Hz(1/2) for the 200 GHz array, 5.1x10-5 rad/Hz(1/2) for the 350 GHz array, and 1.9x10-5 rad/Hz(1/2) for the 480 GHz array, we obtained the values of the averaged electrical noise equivalent power (NEP) over all the arrays: 2x10-16 W/Hz(1/2), 9x10-16 W/Hz(1/2), 5x10-17 W/Hz(1/2), and 4x10-17 W/Hz(1/2) respectively for the four OLIMPO arrays.

AB - We are going to describe the design and the electrical performance of the horn-coupled lumped element kinetic inductance detectors (LEKIDs) for the OLIMPO experiment. OLIMPO is a balloon-borne mission, devoted to the study of the largest structures in the Universe, by detecting the Sunyaev-Zel'dovich effect of the Cosmic Microwave Background (CMB) photons crossing clusters of galaxies. The multi-band focal planes (centered at 150, 200, 350 and 480 GHz), large aperture telescope (2.6 m), photometric and spectrometer configuration (OLIMPO is equipped with a plug-in differential Fourier transform spectrometer) make OLIMPO able to characaterise all the components of the Sunyaev-Zel'dovich effect with unprecedented precision. The design of the LEKIDs has been optimised to cope with a wide range of optical loadings (corresponding to both photometric and spectrometric configurations). The electrical characterisation of the LEKID arrays was performed in the OLIMPO cryostat, at a temperature around 300 mK and under a constant optical load lower than 500 fW. The readout electronics is a customised ROACH-2 coupled to a MUSIC DAC/ADC board. The averaged responsivities for the arrays, measured from the phase readout, are 1.18x1011 rad/W for the 150 GHz array, 4.10x1010 rad/W for the 200 GHz array, 1.09x1012 rad/W for the 350 GHz array, and 4.41x1011 rad/W for the 480 GHz array. Therefore, measuring the spectral noise density for each pixels of the arrays, whose average values are 2.5x10-5 rad/Hz(1/2) for the 150 GHz array, 3.6x10-5 rad/Hz(1/2) for the 200 GHz array, 5.1x10-5 rad/Hz(1/2) for the 350 GHz array, and 1.9x10-5 rad/Hz(1/2) for the 480 GHz array, we obtained the values of the averaged electrical noise equivalent power (NEP) over all the arrays: 2x10-16 W/Hz(1/2), 9x10-16 W/Hz(1/2), 5x10-17 W/Hz(1/2), and 4x10-17 W/Hz(1/2) respectively for the four OLIMPO arrays.

KW - CMB radiation

KW - kinetic inductance detectors

KW - OLIMPO experiment

KW - SZ effect

UR - http://www.scopus.com/inward/record.url?scp=85046968832&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85046968832&partnerID=8YFLogxK

U2 - 10.1109/ISEC.2017.8314223

DO - 10.1109/ISEC.2017.8314223

M3 - Conference contribution

AN - SCOPUS:85046968832

VL - 2018-January

SP - 1

EP - 3

BT - 2017 16th International Superconductive Electronics Conference, ISEC 2017

PB - Institute of Electrical and Electronics Engineers Inc.

ER -