Zobrazeno 1 - 10
of 135
pro vyhledávání: '"Zannoni, Mario"'
Autor:
Coppi, Gabriele, Astori, Federico, Cattaneo, Giulia Rancati, Errand, Josquin, Dunner-Planella, Rolando, Nati, Federico, Zannoni, Mario
Cosmic Microwave Background experiments need to measure polarization properties of the incoming radiation very accurately to achieve their scientific goals. As a result of that, it is necessary to properly characterize these instruments. However, the
Externí odkaz:
http://arxiv.org/abs/2407.13941
Autor:
Guarcello, Claudio, Ahrens, Felix, Avallone, Guerino, Barone, Carlo, Borghesi, Matteo, Callegaro, Luca, Carapella, Giovanni, Caricato, Anna Paola, Carusotto, Iacopo, Cian, Alessandro, D'Elia, Alessandro, Di Gioacchino, Daniele, Enrico, Emanuele, Falferi, Paolo, Fasolo, Luca, Faverzani, Marco, Ferri, Elena, Filatrella, Giovanni, Gatti, Claudio, Giachero, Andrea, Giubertoni, Damiano, Granata, Veronica, Leo, Angelo, Labranca, Danilo, Ligi, Carlo, Maccarrone, Giovanni, Mantegazzini, Federica, Margesin, Benno, Maruccio, Giuseppe, Mezzena, Renato, Monteduro, Anna Grazia, Moretti, Roberto, Nucciotti, Angelo, Oberto, Luca, Origo, Luca, Komnang, Alex Stephane Piedjou, Pagano, Sergio, Piersanti, Luca, Rettaroli, Alessio, Rizzato, Silvia, Tocci, Simone, Vinante, Andrea, Zannoni, Mario
Publikováno v:
IEEE TAS, 34 (3), 1, 1701105 (2024)
Recent advancements in quantum technologies and advanced detection experiments have underscored the pressing need for the detection of exceedingly weak signals within the microwave frequency spectrum. Addressing this challenge, the Josephson Travelin
Externí odkaz:
http://arxiv.org/abs/2403.01597
Autor:
Ahrens, Felix, Ferri, Elena, Avallone, Guerino, Barone, Carlo, Borghesi, Matteo, Callegaro, Luca, Carapella, Giovanni, Caricato, Anna Paola, Carusotto, Iacopo, Cian, Alessandro, D'Elia, Alessandro, Di Gioacchino, Daniele, Enrico, Emanuele, Falferi, Paolo, Fasolo, Luca, Faverzani, Marco, Filatrella, Giovanni, Gatti, Claudio, Giachero, Andrea, Giubertoni, Damiano, Granata, Veronica, Guarcello, Claudio, Labranca, Danilo, Leo, Angelo, Ligi, Carlo, Maccarrone, Giovanni, Mantegazzini, Federica, Margesin, Benno, Maruccio, Giuseppe, Mezzena, Renato, Monteduro, Anna Grazia, Moretti, Roberto, Nucciotti, Angelo, Oberto, Luca, Origo, Luca, Pagano, Sergio, Piedjou, Alex Stephane, Piersanti, Luca, Rettaroli, Alessio, Rizzato, Silvia, Tocci, Simone, Vinante, Andrea, Zannoni, Mario
Publikováno v:
IEEE Transactions on Applied Superconductivity, vol. 34, no. 3, pp. 1-5, May 2024, Art no. 1700605
Noise at the quantum limit over a broad bandwidth is a fundamental requirement for future cryogenic experiments for neutrino mass measurements, dark matter searches and Cosmic Microwave Background (CMB) measurements as well as for fast high-fidelity
Externí odkaz:
http://arxiv.org/abs/2402.12295
Autor:
Faverzani, Marco, Campana, Pietro, Carobene, Rodolfo, Gobbo, Marco, Ahrens, Felix, Avallone, Guerino, Barone, Carlo, Borghesi, Matteo, Capelli, Silvia, Carapella, Giovanni, Caricato, Anna Paola, Callegaro, Luca, Carusotto, Iacopo, Celotto, Andrea, Cian, Alessandro, D'Elia, Alessandro, Di Gioacchino, Daniele, Enrico, Emanuele, Falferi, Paolo, Fasolo, Luca, Ferri, Elena, Filatrella, Giovanni, Gatti, Claudio, Giubertoni, Damiano, Granata, Veronica, Guarcello, Claudio, Irace, Alessandro, Labranca, Danilo, Leo, Angelo, Ligi, Carlo, Maccarrone, Giovanni, Mantegazzini, Federica, Margesin, Benno, Maruccio, Giuseppe, Mezzena, Renato, Moneduro, Anna Grazia, Moretti, Roberto, Nucciotti, Angelo, Oberto, Luca, Origo, Luca, Pagano, Sergio, Komnang, Alex Stephane Piedjou, Piersanti, Luca, Rettaroli, Alessio, Rizzato, Silvia, Tocci, Simone, Vinante, Andrea, Zannoni, Mario, Giachero, Andrea
Superconducting parametric amplifiers offer the capability to amplify feeble signals with extremely low levels of added noise, potentially reaching quantum-limited amplification. This characteristic makes them essential components in the realm of hig
Externí odkaz:
http://arxiv.org/abs/2402.12045
Autor:
The BLAST Observatory Collaboration, Coppi, Gabriele, Dicker, Simon, Aguirre, James E., Austermann, Jason E., Beall, James A., Clark, Susan E., Cox, Erin G., Devlin, Mark J., Fissel, Laura M., Galitzki, Nicholas, Hensley, Brandon S., Hubmayr, Johannes, Molinari, Sergio, Nati, Federico, Novak, Giles, Schisano, Eugenio, Soler, Juan D., Tucker, Carole E., Ullom, Joel N., Vaskuri, Anna, Vissers, Michael R., Wheeler, Jordan D., Zannoni, Mario
Publikováno v:
2024 PASP 136 035003
Sensitive wide-field observations of polarized thermal emission from interstellar dust grains will allow astronomers to address key outstanding questions about the life cycle of matter and energy driving the formation of stars and the evolution of ga
Externí odkaz:
http://arxiv.org/abs/2401.14370
Autor:
Mantegazzini, Federica, Ahrens, Felix, Borghesi, Matteo, Falferi, Paolo, Fasolo, Luca, Faverzani, Marco, Ferri, Elena, Labranca, Danilo, Margesin, Benno, Mezzena, Renato, Moretti, Roberto, Nucciotti, Angelo, Origo, Luca, Vinante, Andrea, Zannoni, Mario, Giachero, Andrea
A wide-bandwidth and low-noise amplification chain in the microwave regime is crucial for the efficient read-out of quantum systems based on superconducting detectors, such as Microwave Kinetic Inductance Detectors (MKIDs), Transition Edge Sensors (T
Externí odkaz:
http://arxiv.org/abs/2310.11410
Autor:
Coppi, Gabriele, Conenna, Giulia, Savorgnano, Sofia, Carrero, Felipe, Dünner-Planella, Rolando, Galitzki, Nicholas, Nati, Federico, Zannoni, Mario
Cosmic Microwave Background experiments need to measure polarization properties of the incoming radiation very accurately to achieve their scientific goals. As a result of that, it is necessary to properly characterize these instruments. However, the
Externí odkaz:
http://arxiv.org/abs/2207.07595
In-flight polarization angle calibration for LiteBIRD: blind challenge and cosmological implications
Autor:
Krachmalnicoff, Nicoletta, Matsumura, Tomotake, de la Hoz, Elena, Basak, Soumen, Gruppuso, Alessandro, Minami, Yuto, Baccigalupi, Carlo, Komatsu, Eiichiro, Martínez-González, Enrique, Vielva, Patricio, Aumont, Jonathan, Aurlien, Ragnhild, Azzoni, Susanna, Banday, Anthony J., Barreiro, Rita B., Bartolo, Nicola, Bersanelli, Marco, Calabrese, Erminia, Carones, Alessandro, Casas, Francisco J., Cheung, Kolen, Chinone, Yuji, Columbro, Fabio, de Bernardis, Paolo, Diego-Palazuelos, Patricia, Errard, Josquin, Finelli, Fabio, Fuskeland, Unni, Galloway, Mathew, Genova-Santos, Ricardo T., Gerbino, Martina, Ghigna, Tommaso, Giardiello, Serena, Gjerløw, Eirik, Hazumi, Masashi, Henrot-Versillé, Sophie, Kisner, Theodore, Lamagna, Luca, Lattanzi, Massimiliano, Levrier, François, Luzzi, Gemma, Maino, Davide, Masi, Silvia, Migliaccio, Marina, Montier, Ludovic, Morgante, Gianluca, Mot, Baptiste, Nagata, Ryo, Nati, Federico, Natoli, Paolo, Pagano, Luca, Paiella, Alessandro, Paoletti, Daniela, Patanchon, Guillaume, Piacentini, Francesco, Polenta, Gianluca, Poletti, Davide, Puglisi, G., Remazeilles, Mathieu, Rubino-Martin, Jose Alberto, Sasaki, Manami, Shiraishi, Maresuke, Signorelli, Giovanni, Stever, Samantha, Tartari, Andrea, Tristram, Matthieu, Tsuji, Masatoshi, Vacher, Léo, Wehus, Ingunn K., Zannoni, Mario
We present a demonstration of the in-flight polarization angle calibration for the JAXA/ISAS second strategic large class mission, LiteBIRD, and estimate its impact on the measurement of the tensor-to-scalar ratio parameter, r, using simulated data.
Externí odkaz:
http://arxiv.org/abs/2111.09140
Autor:
Xu, Zhilei, Adachi, Shunsuke, Ade, Peter, Beall, J. A., Bhandarkar, Tanay, Bond, J. Richard, Chesmore, Grace E., Chinone, Yuji, Choi, Steve K., Connors, Jake A., Coppi, Gabriele, Cothard, Nicholas F., Crowley, Kevin D., Devlin, Mark, Dicker, Simon, Dober, Bradley, Duff, Shannon M., Galitzki, Nicholas, Gallardo, Patricio A., Golec, Joseph E., Gudmundsson, Jon E., Haridas, Saianeesh K., Harrington, Kathleen, Hervias-Caimapo, Carlos, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Iuliano, Jeffrey, Kaneko, Daisuke, Kofman, Anna M., Koopman, Brian J., Lashner, Jack, Limon, Michele, Link, Michael J., Lucas, Tammy J., Matsuda, Frederick, McCarrick, Heather, Nati, Federico, Niemack, Michael D., Orlowski-Scherer, John, Piccirillo, Lucio, Sarmiento, Karen Perez, Schaan, Emmanuel, Silva-Feaver, Maximiliano, Sonka, Rita, Sutariya, Shreya, Tajima, Osamu, Teply, Grant P., Terasaki, Tomoki, Thornton, Robert, Tucker, Carole, Ullom, Joel, Vavagiakis, Eve M., Vissers, Michael R., Walker, Samantha, Whipps, Zachary, Wollack, Edward J., Zannoni, Mario, Zhu, Ningfeng, Zonca, Andrea
Publikováno v:
Research Notes AAS, 5, 100 (2021)
The Simons Observatory (SO) is a Cosmic Microwave Background (CMB) experiment to observe the microwave sky in six frequency bands from 30GHz to 290GHz. The Observatory -- at $\sim$5200m altitude -- comprises three Small Aperture Telescopes (SATs) and
Externí odkaz:
http://arxiv.org/abs/2104.09511
Autor:
Zhu, Ningfeng, Bhandarkar, Tanay, Coppi, Gabriele, Kofman, Anna M., Orlowski-Scherer, John L., Xu, Zhilei, Adachi, Shunsuke, Ade, Peter, Aiola, Simone, Austermann, Jason, Bazarko, Andrew O., Beall, James A., Bhimani, Sanah, Bond, J. Richard, Chesmore, Grace E., Choi, Steve K., Connors, Jake, Cothard, Nicholas F., Devlin, Mark, Dicker, Simon, Dober, Bradley, Duell, Cody J., Duff, Shannon M., Dünner, Rolando, Fabbian, Giulio, Galitzki, Nicholas, Gallardo, Patricio A., Golec, Joseph E., Haridas, Saianeesh K., Harrington, Kathleen, Healy, Erin, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Keatin, Brian, Kiuchi, Kenji, Koopman, Brian J., Lashner, Jack, Lee, Adrian T., Li, Yaqiong, Limon, Michele, Link, Michael, Lucas, Tammy J, McCarrick, Heather, Moore, Jenna, Nati, Federico, Newburgh, Laura B., Niemack, Michael D., Pierpaoli, Elena, Randall, Michael J., Sarmiento, Karen Perez, Saunders, Lauren J., Seibert, Joseph, Sierra, Carlos, Sonka, Rita, Spisak, Jacob, Sutariya, Shreya, Tajima, Osamu, Teply, Grant P., Thornton, Robert J., Tsan, Tran, Tucker, Carole, Ullom, Joel, Vavagiakis, Eve M., Vissers, Michael R., Walker, Samantha, Westbrook, Benjamin, Wollack, Edward J., Zannoni, Mario
The Simons Observatory (SO) Large Aperture Telescope Receiver (LATR) will be coupled to the Large Aperture Telescope located at an elevation of 5,200 m on Cerro Toco in Chile. The resulting instrument will produce arcminute-resolution millimeter-wave
Externí odkaz:
http://arxiv.org/abs/2103.02747