Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Savarese, Claudio"'
Autor:
Baxter, Daniel, Bunker, Raymond, Shaw, Sally, Westerdale, Shawn, Arnquist, Isaac, Akerib, Daniel S., Calkins, Rob, Cebrián, Susana, Dent, James B., di Vacri, Maria Laura, Dobson, Jim, Egana-Ugrinovic, Daniel, Erlandson, Andrew, Ghag, Chamkaur, Hall, Carter, Hall, Jeter, Haselschwardt, Scott, Hoppe, Eric, Jackson, Chris M., Kahn, Yonatan, Kamaha, Alvine, Kelsey, Mike, Kish, Alexander, Kurinsky, Noah, Laubenstein, Matthias, Miller, Eric H., Morrison, Eric, Mount, Brianna, Newstead, Jayden L., Nisi, Stefano, Olcina, Ibles, Orrell, John, Pereverzev, Sergey, Perry, Emily, Piepke, Andreas, Poudel, Sagar Sharma, Ramanathan, Karthik, Reichenbacher, Juergen, Saab, Tarek, Saldanha, Richard, Savarese, Claudio, Schnee, Richard, Scorza, Silvia, Singh, Rajeev, Stifter, Kelly, Suerfu, Burkhant, Szydagis, Matthew, Temples, Dylan J., Villano, Anthony, Woodward, David, Xu, Jingke
Future dark matter direct detection experiments will reach unprecedented levels of sensitivity. Achieving this sensitivity will require more precise models of signal and background rates in future detectors. Improving the precision of signal and back
Externí odkaz:
http://arxiv.org/abs/2203.07623
Autor:
D'Incecco, Marco, Galbiati, Cristiano, Giovanetti, Graham K., Korga, George, Li, Xinran, Mandarano, Andrea, Razeto, Alessandro, Sablone, Davide, Savarese, Claudio
Silicon Photomultipliers (SiPMs) are an excellent candidate for the development of large-area light sensors. Large SiPM-based detectors require low-noise pre-amplifiers to maximize the signal coupling between the sensor and the readout electronics. T
Externí odkaz:
http://arxiv.org/abs/1706.04213
Autor:
D'Incecco, Marco, Galbiati, Cristiano, Giovanetti, Graham K., Korga, George, Li, Xinran, Mandarano, Andrea, Razeto, Alessandro, Sablone, Davide, Savarese, Claudio
We report on the realization of a novel SiPM-based, cryogenic photosensor with an active area of 24 cm$^2$ that operates as a single-channel analog detector. The device is capable of single photon counting with a signal to noise ratio better than 13,
Externí odkaz:
http://arxiv.org/abs/1706.04220
Autor:
Acerbi, Fabio, Davini, Stefano, Ferri, Alessandro, Galbiati, Cristiano, Giovanetti, Graham, Gola, Alberto, Korga, George, Mandarano, Andrea, Marcante, Marco, Paternoster, Giovanni, Piemonte, Claudio, Razeto, Alessandro, Regazzoni, Veronica, Sablone, Davide, Savarese, Claudio, Zappalá, Gaetano, Zorzi, Nicola
Publikováno v:
IEEE Transactions on Electron Devices (Volume: 64, Issue: 2, Feb. 2017) Page(s): 521 - 526
We report on the characterization of near-ultraviolet high density silicon photomultiplier (\SiPM) developed at Fondazione Bruno Kessler (\FBK) at cryogenic temperature. A dedicated setup was built to measure the primary dark noise and correlated noi
Externí odkaz:
http://arxiv.org/abs/1610.01915
Autor:
Savarese, Claudio
Progress and plans for DARKSIDE dark-matter search and ionization-yield/quenching-factormeasurements in LAr. Presented at the 2019 Magnificent CEvNS workshop.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a86cffdf171c9df861c3cc338b3f57c5
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Autor:
Baxter, Daniel, Bunker, Raymond, Shaw, Sally, Westerdale, Shawn, Arnquist, Isaac, Akerib, Daniel S., Calkins, Rob, Cebrián, Susana, Dent, James B., Di Vacri, Maria Laura, Dobson, Jim, Egana-Ugrinovic, Daniel, Erlandson, Andrew, Ghag, Chamkaur, Hall, Carter, Hall, Jeter, Haselschwardt, Scott, Hoppe, Eric, Jackson, Chris M., Kahn, Yonatan, Kamaha, Alvine, Kelsey, Mike, Kish, Alexander, Kurinsky, Noah, Laubenstein, Matthias, Miller, Eric H., Morrison, Eric, Mount, Brianna, Jayden Newstead, Nisi, Stefano, Olcina, Ibles, Orrell, John, Pereverzev, Sergey, Perry, Emily, Piepke, Andreas, Poudel, Sagar Sharma, Ramanathan, Karthik, Reichenbacher, Juergen, Saab, Tarek, Saldanha, Richard, Savarese, Claudio, Schnee, Richard, Scorza, Silvia, Singh, Rajeev, Stifter, Kelly, Suerfu, Burkhant, Szydagis, Matthew, Temples, Dylan J., Villano, Anthony, Woodward, David, Xu, Jingke
Publikováno v:
INSPIRE-HEP
Future dark matter direct detection experiments will reach unprecedented levels of sensitivity. Achieving this sensitivity will require more precise models of signal and background rates in future detectors. Improving the precision of signal and back
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::72d0a657fe56a39afaa4fdc66242c2a5
http://inspirehep.net/record/2052575
http://inspirehep.net/record/2052575