Detection chain and electronic readout of the QUBIC instrument

Stankowiak, G.; Piat, M.; Battistelli, E.S.; D'Alessandro, G.; De Bernardis, P.; Petris, M.D.; Gonzalez, M.; Grandsire, L.; Hamilton, J.C.; Hoang, T.D.; Masi, S.; Marnieros, S.; Mennella, A.; Mousset, L.; O'Sullivan, C.; Prele, 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.; Banff, S.; Belier, B.; Baffu, A.; Bennett, D.; Berge, 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.; Cerutti, A.C.C.; Columbro, F.; Coppolecchia, A.; De Gasperis, G.; Leo, M.D.; Dheilly, S.; Duca, C.; Dumoulin, L.; Etchegoyen, A.; Fasciszewski, A.; Ferreyro, L.P.; Fracchia, D.; Franceschet, C.; Lerena, M.M.G.; Ganga, K.M.; Garcia, B.; Redondo, M.E.G.; Gaspard, M.; Gayer, D.; Gervasi, M.; Giard, M.; Gilles, V.; Giraud-Heraud, Y.; Berisso, M.G.; Gradziel, M.; Hampel, M.R.; Harari, D.; Henrot-Versille, 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.; Ringegni, P.; Romero, G.E.; Rasztocky, E.; Salum, J.M.; Schillaci, A.; Scoccola, C.; Scully, S.; Spinelli, S.; Stolpovskiy, M.; Supanitsky, A.D.; Timbie, P.; Tomasi, M.; Tucker, G.; Tucker, C.; Vigano, D.; Vittorio, N.; Wicek, F.; Wright, M.; Zullo, A.

doi:10.1117/12.2561567

The Q and U Bolometric Interferometer for Cosmology (QUBIC) Technical Demonstrator (TD) aiming to shows the feasibility of the combination of interferometry and bolometric detection. The electronic readout system is based on an array of 128 NbSi Transition Edge Sensors cooled at 350mK readout with 128 SQUIDs at 1K controlled and amplified by an Application Specific Integrated Circuit at 40K. This readout design allows a 128:1 Time Domain Multiplexing. We report the design and the performance of the detection chain in this paper. The technological demonstrator unwent a campaign of test in the lab. Evaluation of the QUBIC bolometers and readout electronics includes the measurement of I-V curves, time constant and the Noise Equivalent Power. Currently the mean Noise Equivalent Power is ∼ 2 x 10-16W= p √Hz..

Detection chain and electronic readout of the QUBIC instrument / G. Stankowiak, M. Piat, E.S. Battistelli, G. D'Alessandro, P. De Bernardis, M.D. Petris, M. Gonzalez, L. Grandsire, J.C. Hamilton, T.D. Hoang, S. Masi, S. Marnieros, A. Mennella, L. Mousset, C. O'Sullivan, D. Prele, A. Tartari, J.P. 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. Banff, B. Belier, A. Baffu, D. Bennett, L. Berge, 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.C. Cerutti, F. Columbro, A. Coppolecchia, G. De Gasperis, M.D. Leo, S. Dheilly, C. Duca, L. Dumoulin, A. Etchegoyen, A. Fasciszewski, L.P. Ferreyro, D. Fracchia, C. Franceschet, M.M.G. Lerena, K.M. Ganga, B. Garcia, M.E.G. Redondo, M. Gaspard, D. Gayer, M. Gervasi, M. Giard, V. Gilles, Y. Giraud-Heraud, M.G. Berisso, M. Gradziel, M.R. Hampel, D. Harari, S. Henrot-Versille, 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, P. Ringegni, G.E. Romero, E. Rasztocky, J.M. Salum, A. Schillaci, C. Scoccola, S. Scully, S. Spinelli, M. Stolpovskiy, A.D. Supanitsky, P. Timbie, M. Tomasi, G. Tucker, C. Tucker, D. Vigano, N. Vittorio, F. Wicek, M. Wright, A. Zullo (PROCEEDINGS OF SPIE, THE INTERNATIONAL SOCIETY FOR OPTICAL ENGINEERING). - In: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X / [a cura di] J. Zmuidzinas, J.-R. Gao. - [s.l] : SPIE, 2020. - ISBN 9781510636934. - pp. 1-14 (( convegno Astronomical telescopes + instrumentation tenutosi a Virtual, Online nel 2020 [10.1117/12.2561567].

Detection chain and electronic readout of the QUBIC instrument

Stankowiak G.;Piat M.;Battistelli E. S.;D'Alessandro G.;De Bernardis P.;Petris M. D.;Gonzalez M.;Grandsire L.;Hamilton J. Ch.;Hoang T. D.;Masi S.;Marnieros S.;A. Mennella;Mousset L.;O'Sullivan C.;Prele 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.;Banff S.;Belier B.;Baffu A.;Bennett D.;Berge L.;Bernard J. -P.;M. Bersanelli;Bigot-Sazy M. -A.;Bonaparte J.;Bonis J.;Bunn E.;Burke D.;Buzi D.;F. Cavaliere;Chanial P.;Chapron C.;Charlassier R.;Cerutti A. C. C.;Columbro F.;Coppolecchia A.;De Gasperis G.;Leo M. D.;Dheilly S.;Duca C.;Dumoulin L.;Etchegoyen A.;Fasciszewski A.;Ferreyro L. P.;Fracchia D.;C. Franceschet;Lerena M. M. G.;Ganga K. M.;Garcia B.;Redondo M. E. G.;Gaspard M.;Gayer D.;Gervasi M.;Giard M.;Gilles V.;Giraud-Heraud Y.;Berisso M. G.;Gradziel M.;Hampel M. R.;Harari D.;Henrot-Versille S.;F. Incardona;Jules E.;Kaplan J.;Kristukat C.;Lamagna L.;Loucatos S.;Louis T.;Maffei B.;Marty W.;A. Mattei;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.;Ringegni P.;Romero G. E.;Rasztocky E.;Salum J. M.;Schillaci A.;Scoccola C.;Scully S.;Spinelli S.;Stolpovskiy M.;Supanitsky A. D.;Timbie P.;M. Tomasi;Tucker G.;Tucker C.;Vigano D.;Vittorio N.;Wicek F.;Wright M.;A. Zullo

2020

Abstract

The Q and U Bolometric Interferometer for Cosmology (QUBIC) Technical Demonstrator (TD) aiming to shows the feasibility of the combination of interferometry and bolometric detection. The electronic readout system is based on an array of 128 NbSi Transition Edge Sensors cooled at 350mK readout with 128 SQUIDs at 1K controlled and amplified by an Application Specific Integrated Circuit at 40K. This readout design allows a 128:1 Time Domain Multiplexing. We report the design and the performance of the detection chain in this paper. The technological demonstrator unwent a campaign of test in the lab. Evaluation of the QUBIC bolometers and readout electronics includes the measurement of I-V curves, time constant and the Noise Equivalent Power. Currently the mean Noise Equivalent Power is ∼ 2 x 10-16W= p √Hz..

Scheda breve

Scheda completa

Scheda completa (DC)

	Parole chiave
	
			CMB; SQUID; TDM; TES
		
	Settori scientifico-disciplinari del contributo
	
			Settore FIS/05 - Astronomia e Astrofisica
		
	Data di pubblicazione
	
			2020
		
	Enti collegati al convegno
	
			The Society of Photo-Optical Instrumentation Engineers (SPIE)
		
	DOI
	
			https://dx.doi.org/10.1117/12.2561567
		
	Tipologia
	
			Book Part (author)
		
	Appare nelle tipologie:
	
			03 - Contributo in volume

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