Zobrazeno 1 - 10
of 758
pro vyhledávání: '"Stevens, Jason"'
Autor:
Fowler, Joseph W., Szypryt, Paul, Bunker, Raymond, Edwards, Ellen R., Florang, Ian Fogarty, Gao, Jiansong, Giachero, Andrea, Hoogerheide, Shannon F., Loer, Ben, Mumm, H. Pieter, Nakamura, Nathan, O'Neil, Galen C., Orrell, John L., Scott, Elizabeth M., Stevens, Jason, Swetz, Daniel S., VanDevender, Brent A., Vissers, Michael, Ullom, Joel N.
Publikováno v:
PRX Quantum, volume 5(4), page 040323 (2024)
Naturally occurring background radiation is a source of correlated decoherence events in superconducting qubits that will challenge error-correction schemes. To characterize the radiation environment in an unshielded laboratory, we performed broadban
Externí odkaz:
http://arxiv.org/abs/2404.10866
Autor:
Ebina, Haruki, Keskitalo, Reijo, Borrill, Julian, Choi, Steve K., Kisner, Theodore, Naess, Sigurd, Niemack, Michael, Stevens, Jason R.
Publikováno v:
SPIE Astronomical Telescopes + Instrumentation Proceedings Volume 12190, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI; 121902R (2022)
We present new wide field survey strategies for Chilean Large Aperture Telescopes (LAT) measuring the Cosmic Microwave Background (CMB), which we call Sinusoidal Modulated High Cadence Survey Strategies. The strategies were developed during the proce
Externí odkaz:
http://arxiv.org/abs/2208.10070
Autor:
Li, Yaqiong, Austermann, Jason E., Beall, James A., Bruno, Sarah Marie, Choi, Steve K., Cothard, Nicholas F., Crowley, Kevin T., Duff, Shannon M., Ho, Shuay-Pwu Patty, Golec, Joseph E., Hilton, Gene C., Hasselfield, Matthew, Hubmay, Johannes, Koopman, Brian J., Lungu, Marius, McMahon, Jeff, Niemack, Michael D., Page, LymanA., Salatino, Maria, Simon, Sara M., Staggs, Suzanne T., Stevens, Jason R., Ullom, Joel N., Vavagiakis, Eve M., Wang, Yuhan, Wollack, Edward J., Xu, Zhilei
The Advanced Atacama Cosmology Telescope Polarimeter (AdvACT) \cite{thornton} is an upgrade for the Atacama Cosmology Telescope using Transition Edge Sensor (TES) detector arrays to measure cosmic microwave background (CMB) temperature and polarizati
Externí odkaz:
http://arxiv.org/abs/2101.02658
Autor:
Stevens, Jason, author
Publikováno v:
Protestants on Screen : Religion, Politics and Aesthetics in European and American Movies, 2023, ill.
Externí odkaz:
https://doi.org/10.1093/oso/9780190058906.003.0021
Autor:
Espinosa, Gastón, author, Stevens, Jason, author
Publikováno v:
Protestants on Screen : Religion, Politics and Aesthetics in European and American Movies, 2023, ill.
Externí odkaz:
https://doi.org/10.1093/oso/9780190058906.003.0013
Autor:
Vavagiakis, Eve M., Ahmed, Zeeshan, Ali, Aamir, Arnold, Kam, Austermann, Jason, Bruno, Sarah Marie, Choi, Steve K., Connors, Jake, Cothard, Nicholas F., Dicker, Simon, Dober, Brad, Duff, Shannon, Fanfani, Valentina, Healy, Erin, Henderson, Shawn, Ho, Shuay-Pwu Patty, Hoang, Duc-Thuong, Hilton, Gene, Hubmayr, Johannes, Krachmalnicoff, Nicoletta, Li, Yaqiong, Mates, John, McCarrick, Heather, Nati, Federico, Niemack, Michael, Silva-Feaver, Maximiliano, Staggs, Suzanne, Stevens, Jason, Vissers, Michael, Ullom, Joel, Wagoner, Kasey, Xu, Zhilei, Zhu, Ningfeng
Publikováno v:
IEEE Transactions on Applied Superconductivity, vol. 31, issue 5, id. 3069294 (Aug 2021)
The Simons Observatory (SO) will be a cosmic microwave background (CMB) survey experiment with three small-aperture telescopes and one large-aperture telescope, which will observe from the Atacama Desert in Chile. In total, SO will field $\sim$70,000
Externí odkaz:
http://arxiv.org/abs/2012.04532
Autor:
Naess, Sigurd, Aiola, Simone, Austermann, Jason E., Battaglia, Nick, Beall, James A., Becker, Daniel T., Bond, Richard J., Calabrese, Erminia, Choi, Steve K., Cothard, Nicholas F., Crowley, Kevin T., Darwish, Omar, Datta, Rahul, Denison, Edward V., Devlin, Mark, Duell, Cody J., Duff, Shannon M., Duivenvoorden, Adriaan J., Dunkley, Jo, Dünner, Rolando, Fox, Anna E., Gallardo, Patricio A., Halpern, Mark, Han, Dongwon, Hasselfield, Matthew, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Hložek, Renée, Ho, Shuay-Pwu Patty, Hubmayr, Johannes, Huffenberger, Kevin, Hughes, John P., Kosowsky, Arthur B., Louis, Thibaut, Madhavacheril, Mathew S., McMahon, Jeff, Moodley, Kavilan, Nati, Federico, Nibarger, John P., Niemack, Michael D., Page, Lyman, Partridge, Bruce, Salatino, Maria, Schaan, Emmanuel, Schillaci, Alessandro, Schmitt, Benjamin, Sherwin, Blake D., Sehgal, Neelima, Sifón, Cristóbal, Spergel, David, Staggs, Suzanne, Stevens, Jason, Storer, Emilie, Ullom, Joel N., Vale, Leila R., Van Engelen, Alexander, Van Lanen, Jeff, Vavagiakis, Eve M., Wollack, Edward J., Xu, Zhilei
This paper presents a maximum-likelihood algorithm for combining sky maps with disparate sky coverage, angular resolution and spatially varying anisotropic noise into a single map of the sky. We use this to merge hundreds of individual maps covering
Externí odkaz:
http://arxiv.org/abs/2007.07290
Autor:
Aiola, Simone, Calabrese, Erminia, Maurin, Loïc, Naess, Sigurd, Schmitt, Benjamin L., Abitbol, Maximilian H., Addison, Graeme E., Ade, Peter A. R., Alonso, David, Amiri, Mandana, Amodeo, Stefania, Angile, Elio, Austermann, Jason E., Baildon, Taylor, Battaglia, Nick, Beall, James A., Bean, Rachel, Becker, Daniel T., Bond, J Richard, Bruno, Sarah Marie, Calafut, Victoria, Campusano, Luis E., Carrero, Felipe, Chesmore, Grace E., Cho, Hsiao-mei, Choi, Steve K., Clark, Susan E., Cothard, Nicholas F., Crichton, Devin, Crowley, Kevin T., Darwish, Omar, Datta, Rahul, Denison, Edward V., Devlin, Mark J., Duell, Cody J., Duff, Shannon M., Duivenvoorden, Adriaan J., Dunkley, Jo, Dünner, Rolando, Essinger-Hileman, Thomas, Fankhanel, Max, Ferraro, Simone, Fox, Anna E., Fuzia, Brittany, Gallardo, Patricio A., Gluscevic, Vera, Golec, Joseph E., Grace, Emily, Gralla, Megan, Guan, Yilun, Hall, Kirsten, Halpern, Mark, Han, Dongwon, Hargrave, Peter, Hasselfield, Matthew, Helton, Jakob M., Henderson, Shawn, Hensley, Brandon, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Hložek, Renée, Ho, Shuay-Pwu Patty, Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Infante, Leopoldo, Irwin, Kent, Jackson, Rebecca, Klein, Jeff, Knowles, Kenda, Koopman, Brian, Kosowsky, Arthur, Lakey, Victoria, Li, Dale, Li, Yaqiong, Li, Zack, Lokken, Martine, Louis, Thibaut, Lungu, Marius, MacInnis, Amanda, Madhavacheril, Mathew, Maldonado, Felipe, Mallaby-Kay, Maya, Marsden, Danica, McMahon, Jeff, Menanteau, Felipe, Moodley, Kavilan, Morton, Tim, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nibarger, John P., Nicola, Andrina, Niemack, Michael D., Nolta, Michael R., Orlowski-Sherer, John, Page, Lyman A., Pappas, Christine G., Partridge, Bruce, Phakathi, Phumlani, Pisano, Giampaolo, Prince, Heather, Puddu, Roberto, Qu, Frank J., Rivera, Jesus, Robertson, Naomi, Rojas, Felipe, Salatino, Maria, Schaan, Emmanuel, Schillaci, Alessandro, Sehgal, Neelima, Sherwin, Blake D., Sierra, Carlos, Sievers, Jon, Sifon, Cristobal, Sikhosana, Precious, Simon, Sara, Spergel, David N., Staggs, Suzanne T., Stevens, Jason, Storer, Emilie, Sunder, Dhaneshwar D., Switzer, Eric R., Thorne, Ben, Thornton, Robert, Trac, Hy, Treu, Jesse, Tucker, Carole, Vale, Leila R., Van Engelen, Alexander, Van Lanen, Jeff, Vavagiakis, Eve M., Wagoner, Kasey, Wang, Yuhan, Ward, Jonathan T., Wollack, Edward J., Xu, Zhilei, Zago, Fernando, Zhu, Ningfeng
We present new arcminute-resolution maps of the Cosmic Microwave Background temperature and polarization anisotropy from the Atacama Cosmology Telescope, using data taken from 2013-2016 at 98 and 150 GHz. The maps cover more than 17,000 deg$^2$, the
Externí odkaz:
http://arxiv.org/abs/2007.07288
Autor:
Choi, Steve K., Hasselfield, Matthew, Ho, Shuay-Pwu Patty, Koopman, Brian, Lungu, Marius, Abitbol, Maximilian H., Addison, Graeme E., Ade, Peter A. R., Aiola, Simone, Alonso, David, Amiri, Mandana, Amodeo, Stefania, Angile, Elio, Austermann, Jason E., Baildon, Taylor, Battaglia, Nick, Beall, James A., Bean, Rachel, Becker, Daniel T., Bond, J Richard, Bruno, Sarah Marie, Calabrese, Erminia, Calafut, Victoria, Campusano, Luis E., Carrero, Felipe, Chesmore, Grace E., Cho, Hsiao-mei, Clark, Susan E., Cothard, Nicholas F., Crichton, Devin, Crowley, Kevin T., Darwish, Omar, Datta, Rahul, Denison, Edward V., Devlin, Mark J., Duell, Cody J., Duff, Shannon M., Duivenvoorden, Adriaan J., Dunkley, Jo, Dünner, Rolando, Essinger-Hileman, Thomas, Fankhanel, Max, Ferraro, Simone, Fox, Anna E., Fuzia, Brittany, Gallardo, Patricio A., Gluscevic, Vera, Golec, Joseph E., Grace, Emily, Gralla, Megan, Guan, Yilun, Hall, Kirsten, Halpern, Mark, Han, Dongwon, Hargrave, Peter, Henderson, Shawn, Hensley, Brandon, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Hložek, Renée, Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Infante, Leopoldo, Irwin, Kent, Jackson, Rebecca, Klein, Jeff, Knowles, Kenda, Kosowsky, Arthur, Lakey, Victoria, Li, Dale, Li, Yaqiong, Li, Zack, Lokken, Martine, Louis, Thibaut, MacInnis, Amanda, Madhavacheril, Mathew, Maldonado, Felipe, Mallaby-Kay, Maya, Marsden, Danica, Maurin, Loïc, McMahon, Jeff, Menanteau, Felipe, Moodley, Kavilan, Morton, Tim, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nibarger, John P., Nicola, Andrina, Niemack, Michael D., Nolta, Michael R., Orlowski-Sherer, John, Page, Lyman A., Pappas, Christine G., Partridge, Bruce, Phakathi, Phumlani, Prince, Heather, Puddu, Roberto, Qu, Frank J., Rivera, Jesus, Robertson, Naomi, Rojas, Felipe, Salatino, Maria, Schaan, Emmanuel, Schillaci, Alessandro, Schmitt, Benjamin L., Sehgal, Neelima, Sherwin, Blake D., Sierra, Carlos, Sievers, Jon, Sifon, Cristobal, Sikhosana, Precious, Simon, Sara, Spergel, David N., Staggs, Suzanne T., Stevens, Jason, Storer, Emilie, Sunder, Dhaneshwar D., Switzer, Eric R., Thorne, Ben, Thornton, Robert, Trac, Hy, Treu, Jesse, Tucker, Carole, Vale, Leila R., Van Engelen, Alexander, Van Lanen, Jeff, Vavagiakis, Eve M., Wagoner, Kasey, Wang, Yuhan, Ward, Jonathan T., Wollack, Edward J., Xu, Zhilei, Zago, Fernando, Zhu, Ningfeng
We present the temperature and polarization angular power spectra of the CMB measured by the Atacama Cosmology Telescope (ACT) from 5400 deg$^2$ of the 2013-2016 survey, which covers $>$15000 deg$^2$ at 98 and 150 GHz. For this analysis we adopt a bl
Externí odkaz:
http://arxiv.org/abs/2007.07289