QUBIC IV:  Performance of TES bolometers and readout electronics

Piat, M.; Stankowiak, G.; Battistelli, E.S.; de Bernardis, P.; D'Alessandro, G.; De Petris, M.; Grandsire, L.; Hamilton, J.-.; Hoang, T.D.; Marnieros, S.; Masi, S.; Mennella, A.; Mousset, L.; O'Sullivan, C.; Prêle, D.; Tartari, A.; Thermeau, J.-.; Torchinsky, S.A.; Voisin, F.; Zannoni, M.; Ade, P.; Alberro, J.G.; Almela, A.; Amico, G.; Arnaldi, L.H.; Auguste, D.; Aumont, J.; Azzoni, S.; Banfi, S.; Baù, A.; Bélier, B.; Bennett, D.; Bergé, L.; Bernard, J.-.; Bersanelli, M.; Bigot-Sazy, M.-.; Bonaparte, J.; Bonis, J.; Bunn, E.; Burke, D.; Buzi, D.; Cavaliere, F.; Chanial, P.; Chapron, C.; Charlassier, R.; Cobos Cerutti, A.C.; Columbro, F.; Coppolecchia, A.; De Gasperis, G.; De Leo, M.; Dheilly, S.; Duca, C.; Dumoulin, L.; Etchegoyen, A.; Fasciszewski, A.; Ferreyro, L.P.; Fracchia, D.; Franceschet, C.; Gamboa Lerena, M.M.; Ganga, K.M.; García, B.; García Redondo, M.E.; Gaspard, M.; Gayer, D.; Gervasi, M.; Giard, M.; Gilles, V.; Giraud-Heraud, Y.; Gómez Berisso, M.; González, M.; Gradziel, M.; Hampel, M.R.; Harari, D.; Henrot-Versillé, S.; Incardona, F.; Jules, E.; Kaplan, J.; Kristukat, C.; Lamagna, L.; Loucatos, S.; Louis, T.; Maffei, B.; Marty, W.; Mattei, A.; May, A.; Mcculloch, M.; Mele, L.; Melo, D.; Montier, L.; Mundo, L.M.; Murphy, J.A.; Murphy, J.D.; Nati, F.; Olivieri, E.; Oriol, C.; Paiella, A.; Pajot, F.; Passerini, A.; Pastoriza, H.; Pelosi, A.; Perbost, C.; Perciballi, M.; Pezzotta, F.; Piacentini, F.; Piccirillo, L.; Pisano, G.; Platino, M.; Polenta, G.; Puddu, R.; Rambaud, D.; Rasztocky, E.; Ringegni, P.; Romero, G.E.; Salum, J.M.; Schillaci, A.; Scóccola, C.G.; Scully, S.; Spinelli, S.; Stolpovskiy, M.; Supanitsky, A.D.; Timbie, P.; Tomasi, M.; Tucker, C.; Tucker, G.; Viganò, D.; Vittorio, N.; Wicek, F.; Wright, M.; Zullo, A.

doi:10.1088/1475-7516/2022/04/037

A prototype version of the Q & U bolometric interferometer for cosmology (QUBIC) underwent a campaign of testing in the laboratory at Astroparticle Physics and Cosmology laboratory in Paris (APC). The detection chain is currently made of 256 NbSi transition edge sensors (TES) cooled to 320 mK. The readout system is a 128:1 time domain multiplexing scheme based on 128 SQUIDs cooled at 1K that are controlled and amplified by a SiGe application specific integrated circuit at 40 K. We report the performance of this readout chain and the characterization of the TES. The readout system has been functionally tested and characterized in the lab and in QUBIC. The low noise amplifier demonstrated a white noise level of 0.3 nV/root Hz. Characterizations of the QUBIC detectors and readout electronics includes the measurement of I-V curves, time constant and the noise equivalent power. The QUBIC TES bolometer array has approximately 80% detectors within operational parameters. It demonstrated a thermal decoupling compatible with a phonon noise of about 5 x 10(-1)7 W/root Hz at 410 mK critical temperature. While still limited by microphonics from the pulse tubes and noise aliasing from readout system, the instrument noise equivalent power is about 2 x 10(-16) W/root Hz, enough for the demonstration of bolometric interferometry.

QUBIC IV: Performance of TES bolometers and readout electronics / M. Piat, G. Stankowiak, E.S. Battistelli, P. de Bernardis, G. D'Alessandro, M. De Petris, L. Grandsire, J.-. Hamilton, T.D. Hoang, S. Marnieros, S. Masi, A. Mennella, L. Mousset, C. O'Sullivan, D. Prêle, A. Tartari, J.-. Thermeau, S.A. Torchinsky, F. Voisin, M. Zannoni, P. Ade, J.G. Alberro, A. Almela, G. Amico, L.H. Arnaldi, D. Auguste, J. Aumont, S. Azzoni, S. Banfi, A. Baù, B. Bélier, D. Bennett, L. Bergé, J.-. Bernard, M. Bersanelli, M.-. Bigot-Sazy, J. Bonaparte, J. Bonis, E. Bunn, D. Burke, D. Buzi, F. Cavaliere, P. Chanial, C. Chapron, R. Charlassier, A.C. Cobos Cerutti, F. Columbro, A. Coppolecchia, G. De Gasperis, M. De Leo, S. Dheilly, C. Duca, L. Dumoulin, A. Etchegoyen, A. Fasciszewski, L.P. Ferreyro, D. Fracchia, C. Franceschet, M.M. Gamboa Lerena, K.M. Ganga, B. García, M.E. García Redondo, M. Gaspard, D. Gayer, M. Gervasi, M. Giard, V. Gilles, Y. Giraud-Heraud, M. Gómez Berisso, M. González, M. Gradziel, M.R. Hampel, D. Harari, S. Henrot-Versillé, F. Incardona, E. Jules, J. Kaplan, C. Kristukat, L. Lamagna, S. Loucatos, T. Louis, B. Maffei, W. Marty, A. Mattei, A. May, M. Mcculloch, L. Mele, D. Melo, L. Montier, L.M. Mundo, J.A. Murphy, J.D. Murphy, F. Nati, E. Olivieri, C. Oriol, A. Paiella, F. Pajot, A. Passerini, H. Pastoriza, A. Pelosi, C. Perbost, M. Perciballi, F. Pezzotta, F. Piacentini, L. Piccirillo, G. Pisano, M. Platino, G. Polenta, R. Puddu, D. Rambaud, E. Rasztocky, P. Ringegni, G.E. Romero, J.M. Salum, A. Schillaci, C.G. Scóccola, S. Scully, S. Spinelli, M. Stolpovskiy, A.D. Supanitsky, P. Timbie, M. Tomasi, C. Tucker, G. Tucker, D. Viganò, N. Vittorio, F. Wicek, M. Wright, A. Zullo. - In: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. - ISSN 1475-7516. - 2022:4(2022 Apr), pp. 037.1-037.28. [10.1088/1475-7516/2022/04/037]

QUBIC IV: Performance of TES bolometers and readout electronics

Piat, M.;Stankowiak, G.;Battistelli, E. S.;de Bernardis, P.;D'Alessandro, G.;De Petris, M.;Grandsire, L.;Hamilton, J. -Ch.;Hoang, T. D.;Marnieros, S.;Masi, S.;A. Mennella;Mousset, L.;O'Sullivan, C.;Prêle, D.;Tartari, A.;Thermeau, J. -P.;Torchinsky, S. A.;Voisin, F.;Zannoni, M.;Ade, P.;Alberro, J. G.;Almela, A.;Amico, G.;Arnaldi, L. H.;Auguste, D.;Aumont, J.;Azzoni, S.;Banfi, S.;Baù, A.;Bélier, B.;Bennett, D.;Bergé, L.;Bernard, J. -Ph.;M. Bersanelli;Bigot-Sazy, M. -A.;Bonaparte, J.;Bonis, J.;Bunn, E.;Burke, D.;Buzi, D.;F. Cavaliere;Chanial, P.;Chapron, C.;Charlassier, R.;Cobos Cerutti, A. C.;Columbro, F.;Coppolecchia, A.;De Gasperis, G.;De Leo, M.;Dheilly, S.;Duca, C.;Dumoulin, L.;Etchegoyen, A.;Fasciszewski, A.;Ferreyro, L. P.;Fracchia, D.;C. Franceschet;Gamboa Lerena, M. M.;Ganga, K. M.;García, B.;García Redondo, M. E.;Gaspard, M.;Gayer, D.;Gervasi, M.;Giard, M.;Gilles, V.;Giraud-Heraud, Y.;Gómez Berisso, M.;González, M.;Gradziel, M.;Hampel, M. R.;Harari, D.;Henrot-Versillé, S.;Incardona, F.;Jules, E.;Kaplan, J.;Kristukat, C.;Lamagna, L.;Loucatos, S.;Louis, T.;Maffei, B.;Marty, W.;Mattei, A.;May, A.;McCulloch, M.;Mele, L.;Melo, D.;Montier, L.;Mundo, L. M.;Murphy, J. A.;Murphy, J. D.;Nati, F.;Olivieri, E.;Oriol, C.;Paiella, A.;Pajot, F.;Passerini, A.;Pastoriza, H.;Pelosi, A.;Perbost, C.;Perciballi, M.;F. Pezzotta;Piacentini, F.;Piccirillo, L.;Pisano, G.;Platino, M.;Polenta, G.;Puddu, R.;Rambaud, D.;Rasztocky, E.;Ringegni, P.;Romero, G. E.;Salum, J. M.;Schillaci, A.;Scóccola, C. G.;Scully, S.;Spinelli, S.;Stolpovskiy, M.;Supanitsky, A. D.;Timbie, P.;M. Tomasi;Tucker, C.;Tucker, G.;Viganò, D.;Vittorio, N.;Wicek, F.;Wright, M.;Zullo, A.

2022

Abstract

A prototype version of the Q & U bolometric interferometer for cosmology (QUBIC) underwent a campaign of testing in the laboratory at Astroparticle Physics and Cosmology laboratory in Paris (APC). The detection chain is currently made of 256 NbSi transition edge sensors (TES) cooled to 320 mK. The readout system is a 128:1 time domain multiplexing scheme based on 128 SQUIDs cooled at 1K that are controlled and amplified by a SiGe application specific integrated circuit at 40 K. We report the performance of this readout chain and the characterization of the TES. The readout system has been functionally tested and characterized in the lab and in QUBIC. The low noise amplifier demonstrated a white noise level of 0.3 nV/root Hz. Characterizations of the QUBIC detectors and readout electronics includes the measurement of I-V curves, time constant and the noise equivalent power. The QUBIC TES bolometer array has approximately 80% detectors within operational parameters. It demonstrated a thermal decoupling compatible with a phonon noise of about 5 x 10(-1)7 W/root Hz at 410 mK critical temperature. While still limited by microphonics from the pulse tubes and noise aliasing from readout system, the instrument noise equivalent power is about 2 x 10(-16) W/root Hz, enough for the demonstration of bolometric interferometry.

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Scheda completa

Scheda completa (DC)

	Parole chiave
	
			CMBR detectors; CMBR experiments; CMBR polarisation; cosmological parameters from CMBR
		
	Settori scientifico-disciplinari dell'articolo
	
			Settore FIS/05 - Astronomia e Astrofisica
		
	Data di pubblicazione
	
			apr-2022
		
	Rivista in ANCE
	
			JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
		
	DOI
	
			https://dx.doi.org/10.1088/1475-7516/2022/04/037
		
	Sostituita dalla registrazione
	
			hdl:2434/924630
		
	Tipologia
	
			Article (author)
		
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			01 - Articolo su periodico

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