We report on the performance of lumped-elements Kinetic Inductance Detector (KID) arrays for mm and sub-mm wavelengths, operated at 0.3 K during the stratospheric flight of the OLIMPO payload, at an altitude of 37.8 km. We find that the detectors can be tuned in-flight, and their performance is robust against radiative background changes due to varying telescope elevation. We also find that the noise equivalent power of the detectors in flight is smaller by a factor of ~ 2, 8, 3.5, 4.5 at 150, 250, 350 and 460 GHz relative to the one measured in the laboratory, and is close to our calculated photon-noise-limited performance. The effect of primary cosmic rays crossing the detector is found to be consistent with the expected ionization energy loss with phonon-mediated energy transfer from the ionization sites to the resonators. In the OLIMPO detector arrays, at float, cosmic ray events affect less than 4% of the detector samplings for all the pixels of all the arrays, and less than 1% of the samplings for most of the pixels. These results are also representative of what one can expect from primary cosmic rays in a satellite mission with similar KIDs and instrument environment.

Kinetic Inductance Detectors for the OLIMPO experiment: in-flight operation and performance / Masi, S.; de Bernardis, P.; Paiella, A.; Piacentini, F.; Lamagna, L.; Coppolecchia, A.; Ade, P. A. R.; Battistelli, E. S.; Castellano, M. G.; Colantoni, I.; Columbro, F.; D'Alessandro, G.; Petris, M. De; Gordon, S.; Magneville, C.; Mauskopf, P.; Pettinari, G.; Pisano, G.; Polenta, G.; Presta, G.; Tommasi, E.; Tucker, C.; Vdovin, V.; Volpe, A.; Yvon, D.. - In: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. - ISSN 1475-7516. - 2019:07(2019), pp. 003-003. [10.1088/1475-7516/2019/07/003]

Kinetic Inductance Detectors for the OLIMPO experiment: in-flight operation and performance

Masi, S.;de Bernardis, P.;Paiella, A.;Piacentini, F.;Lamagna, L.;Coppolecchia, A.;Battistelli, E. S.;Colantoni, I.;Columbro, F.;D'Alessandro, G.;Petris, M. De;Gordon, S.;Mauskopf, P.;Pettinari, G.;Pisano, G.;Polenta, G.;Presta, G.;Tommasi, E.;Vdovin, V.;
2019

Abstract

We report on the performance of lumped-elements Kinetic Inductance Detector (KID) arrays for mm and sub-mm wavelengths, operated at 0.3 K during the stratospheric flight of the OLIMPO payload, at an altitude of 37.8 km. We find that the detectors can be tuned in-flight, and their performance is robust against radiative background changes due to varying telescope elevation. We also find that the noise equivalent power of the detectors in flight is smaller by a factor of ~ 2, 8, 3.5, 4.5 at 150, 250, 350 and 460 GHz relative to the one measured in the laboratory, and is close to our calculated photon-noise-limited performance. The effect of primary cosmic rays crossing the detector is found to be consistent with the expected ionization energy loss with phonon-mediated energy transfer from the ionization sites to the resonators. In the OLIMPO detector arrays, at float, cosmic ray events affect less than 4% of the detector samplings for all the pixels of all the arrays, and less than 1% of the samplings for most of the pixels. These results are also representative of what one can expect from primary cosmic rays in a satellite mission with similar KIDs and instrument environment.
2019
CMBR detectors; CMBR experiments; Sunyaev-Zeldovich effect
01 Pubblicazione su rivista::01a Articolo in rivista
Kinetic Inductance Detectors for the OLIMPO experiment: in-flight operation and performance / Masi, S.; de Bernardis, P.; Paiella, A.; Piacentini, F.; Lamagna, L.; Coppolecchia, A.; Ade, P. A. R.; Battistelli, E. S.; Castellano, M. G.; Colantoni, I.; Columbro, F.; D'Alessandro, G.; Petris, M. De; Gordon, S.; Magneville, C.; Mauskopf, P.; Pettinari, G.; Pisano, G.; Polenta, G.; Presta, G.; Tommasi, E.; Tucker, C.; Vdovin, V.; Volpe, A.; Yvon, D.. - In: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. - ISSN 1475-7516. - 2019:07(2019), pp. 003-003. [10.1088/1475-7516/2019/07/003]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1303719
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