مورد إلكتروني
Qubic: the q and u bolometric interferometer for cosmology
| العنوان: | Qubic: the q and u bolometric interferometer for cosmology |
|---|---|
| بيانات النشر: | SPIE 2022 |
| تفاصيل مُضافة: | Zmuidzinas, J Gao, JR Piat, M Battistelli, E De Bernardis, P Dalessandro, G De Petris, M Grandsire, L Hamilton, J Hoang, T Marnieros, S Masi, S Mennella, A Mousset, L Osullivan, C Prele, D Stankowiak, G Tartari, A Thermeau, J Torchinsky, S Voisin, F Zannoni, M Ade, P Alberro, J Almela, A Amico, G Arnaldi, L Auguste, D Aumont, J Azzoni, S Banfi, S Belier, B Bau, 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 Cobos Cerutti, A Columbro, F Coppolecchia, A De Gasperis, G De Leo, M Dheilly, S Duca, C Dumoulin, L Etchegoyen, A Fasciszewski, A Ferreyro, L Fracchia, D Franceschet, C Gamboa Lerena, M Ganga, K Garcia, B Garcia Redondo, M Gaspard, M Gayer, D Gervasi, M Giard, M Gilles, V Giraud-Heraud, Y Gomez Berisso, M Gonzalez, M Gradziel, M Hampel, M 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 Murphy, J Murphy, J Nati, F Olivicri, 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 Salum, J Schillaci, A Scoccola, C Scully, S Spinelli, S Stolpovskiy, M Supanitsky, A Timbie, P Tomasi, M Tucker, C Tucker, G Vigano, D Vittorio, N Wicek, F Wright, M Zullo, A Piat M. Battistelli E. S. De Bernardis P. Dalessandro G. De Petris M. Grandsire L. Hamilton J. -C. Hoang T. D. Marnieros S. Masi S. Mennella A. Mousset L. Osullivan C. Prele D. Stankowiak G. 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. Belier B. Bau A. Bennett D. Berge L. Bernard J. -Ph. Bersanelli M. Bigot-Sazy M. -A. 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. Garcia B. Garcia Redondo M. E. Gaspard M. Gayer D. Gervasi M. Giard M. Gilles V. Giraud-Heraud Y. Gomez Berisso M. Gonzalez M. 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. Olivicri 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. Scoccola C. G. Scully S. Spinelli S. Stolpovskiy M. Supanitsky A. D. Timbie P. Tomasi M. Tucker C. Tucker G. Vigano D. Vittorio N. Wicek F. Wright M. Zullo A. |
| نوع الوثيقة: | Electronic Resource |
| مستخلص: | QUBIC (Q and U bolometric interferometer for cosmology) is an international ground-based experiment dedicated to the measurement of the polarized fluctuations of the cosmic microwave background (CMB). It is based on bolometric interferometry, an original detection technique which combines the immunity to systematic effects of an interferometer with the sensitivity of low temperature incoherent detectors. QUBIC will be deployed in Argentina, at the Alto Chorrillos mountain site near San Antonio de los Cobres, in the Salta province. The QUBIC detection chain consists of 2048 NbSi transition edge sensors (TESs) cooled to 320 mK. The voltage-biased TESs are read out with time domain multiplexing based on superconducting quantum interference devices (SQUIDs) at 1 K and a novel SiGe application-specific integrated circuit (ASIC) at 60 K allowing an unprecedented multiplexing (MUX) factor equal to 128 to be reached. The current QUBIC version is based on a reduced number of detectors (1/4) in order to validate the detection technique. The QUBIC experiment is currently being validated in the lab in Salta (Argentina) before going to the site for observations. This paper presents the main results of the characterization phase with a focus on the detectors and readout system. |
| مصطلحات الفهرس: | LaTeX, Manuscript format, SPIE Proceeding, Template, FIS/05 - ASTRONOMIA E ASTROFISICA, info:eu-repo/semantics/conferenceObject |
| URL: | info:eu-repo/semantics/altIdentifier/isbn/9781510653610 info:eu-repo/semantics/altIdentifier/wos/WOS:000864182000100 ispartofbook:Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI 2022 Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI 2022 - 17 July 2022 through 22 July 2022 volume:12190 firstpage:186 serie:PROCEEDINGS OF SPIE, THE INTERNATIONAL SOCIETY FOR OPTICAL ENGINEERING alleditors:Zmuidzinas, J; Gao, JR |
| الإتاحة: | Open access content. Open access content |
| ملاحظة: | English |
| أرقام أخرى: | ITBAO oai:boa.unimib.it:10281/395897 10.1117/12.2642114 info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85140773665 1355267012 |
| المصدر المساهم: | BICOCCA OPEN ARCH From OAIster®, provided by the OCLC Cooperative. |
| رقم الأكسشن: | edsoai.on1355267012 |
| قاعدة البيانات: | OAIster |
| الوصف غير متاح. |