Zobrazeno 1 - 10
of 1 874
pro vyhledávání: '"Lucas, P J"'
Autor:
Satterthwaite, Thomas P., Ahmed, Zeeshan, Bae, Kyuyoung, Devlin, Mark, Dicker, Simon, Duff, Shannon M., Dutcher, Daniel, Haridas, Saianeesh K., Henderson, Shawn W., Hubmayr, Johannes, Johnson, Bradley R., Kofman, Anna, Lashner, Jack, Link, Michael J., Lucas, Tammy J., Manduca, Alex, Niemack, Michael D., Orlowski-Scherer, John, Pinsonneault-Marotte, Tristan, Silva-Feaver, Max, Staggs, Suzanne, Vavagiakis, Eve M., Wang, Yuhan, Zheng, Kaiwen
Publikováno v:
Proc. SPIE 13102, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII. 1310223 (2024)
The Simons Observatory is a new ground-based cosmic microwave background experiment, which is currently being commissioned in Chile's Atacama Desert. During its survey, the observatory's small aperture telescopes will map 10% of the sky in bands cent
Externí odkaz:
http://arxiv.org/abs/2406.01844
Autor:
Sierra, Carlos E., Harrington, Kathleen, Sutariya, Shreya, Alford, Thomas, Kofman, Anna M., Chesmore, Grace E., Austermann, Jason E., Bazarko, Andrew, Beall, James A., Bhandarkar, Tanay, Devlin, Mark J., Dicker, Simon R., Dow, Peter N., Duff, Shannon M., Dutcher, Daniel, Galitzki, Nicholas, Golec, Joseph E., Groh, John C., Gudmundsson, Jon E., Haridas, Saianeesh K., Healy, Erin, Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Lessler, Claire S., Lew, Richard A., Link, Michael J., Lucas, Tammy J., McMahon, Jeffrey J., Moore, Jenna E., Nati, Federico, Niemack, Michael D., Schmitt, Benjamin L., Silva-Feaver, Max, Singh, Robinjeet, Sonka, Rita F., Thomas, Alex, Thornton, Robert J., Tsan, Tran, Ullom, Joel N., Van Lanen, Jeffrey L., Vavagiakis, Eve M., Vissers, Michael R., Wang, Yuhan, Zheng, Kaiwen
The Simons Observatory will map the temperature and polarization over half of the sky, at millimeter wavelengths in six spectral bands from the Atacama Desert in Chile. These data will provide new insights into the genesis, content, and history of ou
Externí odkaz:
http://arxiv.org/abs/2405.06868
Autor:
Galitzki, Nicholas, Tsan, Tran, Spisak, Jake, Randall, Michael, Silva-Feaver, Max, Seibert, Joseph, Lashner, Jacob, Adachi, Shunsuke, Adkins, Sean M., Alford, Thomas, Arnold, Kam, Ashton, Peter C., Austermann, Jason E., Baccigalupi, Carlo, Bazarko, Andrew, Beall, James A., Bhimani, Sanah, Bixler, Bryce, Coppi, Gabriele, Corbett, Lance, Crowley, Kevin D., Crowley, Kevin T., Day-Weiss, Samuel, Dicker, Simon, Dow, Peter N., Duell, Cody J., Duff, Shannon M., Gerras, Remington G., Groh, John C., Gudmundsson, Jon E., Harrington, Kathleen, Hasegawa, Masaya, Healy, Erin, Henderson, Shawn W., Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Keating, Brian, Keller, Ben, Kiuchi, Kenji, Kofman, Anna M., Koopman, Brian J., Kusaka, Akito, Lee, Adrian T., Lew, Richard A., Lin, Lawrence T., Link, Michael J, Lucas, Tammy J., Lungu, Marius, Mangu, Aashrita, McMahon, Jeffrey J, Miller, Amber D., Moore, Jenna E., Morshed, Magdy, Nakata, Hironobu, Nati, Federico, Newburgh, Laura B., Nguyen, David V., Niemack, Michael D., Page, Lyman A., Sakaguri, Kana, Sakurai, Yuki, Rao, Mayuri Sathyanarayana, Saunders, Lauren J., Shroyer, Jordan E., Sugiyama, Junna, Tajima, Osamu, Takeuchi, Atsuto, Bua, Refilwe Tanah, Teply, Grant, Terasaki, Tomoki, Ullom, Joel N., Van Lanen, Jeffrey L., Vavagiakis, Eve M., Vissers, Michael R, Walters, Liam, Wang, Yuhan, Xu, Zhilei, Yamada, Kyohei, Zheng, Kaiwen
The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of 5,200 m in the Atacama Desert in Chile. The SO SATs will cover six spectral bands betwee
Externí odkaz:
http://arxiv.org/abs/2405.05550
Autor:
Duff, Shannon M., Austermann, Jason, Beall, James A., Daniel, David P., Hubmayr, Johannes, Jaehnig, Greg C., Johnson, Bradley R., Jones, Dante, Link, Michael J., Lucas, Tammy J., Sonka, Rita F., Staggs, Suzanne T., Ullom, Joel, Wang, Yuhan
The Simons Observatory (SO) is a cosmic microwave background instrumentation suite in the Atacama Desert of Chile. More than 65,000 polarization-sensitive transition-edge sensor (TES) bolometers will be fielded in the frequency range spanning 27 to 2
Externí odkaz:
http://arxiv.org/abs/2403.18225
Over the last decades, many prognostic models based on artificial intelligence techniques have been used to provide detailed predictions in healthcare. Unfortunately, the real-world observational data used to train and validate these models are almos
Externí odkaz:
http://arxiv.org/abs/2311.08427
Autor:
Dutcher, Daniel, Duff, Shannon M., Groh, John C., Healy, Erin, Hubmayr, Johannes, Johnson, Bradley R., Jones, Dante, Keller, Ben, Lin, Lawrence T., Link, Michael J., Lucas, Tammy J., Morgan, Samuel, Seino, Yudai, Sonka, Rita F., Staggs, Suzanne T., Wang, Yuhan, Zheng, Kaiwen
The Simons Observatory (SO) is a cosmic microwave background instrumentation suite being deployed in the Atacama Desert in northern Chile. The telescopes within SO use three types of dichroic transition-edge sensor (TES) detector arrays, with the 90
Externí odkaz:
http://arxiv.org/abs/2311.05583
Autor:
Zanga, Alessio, Bernasconi, Alice, Lucas, Peter J. F., Pijnenborg, Hanny, Reijnen, Casper, Scutari, Marco, Stella, Fabio
Causal inference for testing clinical hypotheses from observational data presents many difficulties because the underlying data-generating model and the associated causal graph are not usually available. Furthermore, observational data may contain mi
Externí odkaz:
http://arxiv.org/abs/2305.10050
Autor:
Zanga, Alessio, Bernasconi, Alice, Lucas, Peter J. F., Pijnenborg, Hanny, Reijnen, Casper, Scutari, Marco, Stella, Fabio
Assessing the pre-operative risk of lymph node metastases in endometrial cancer patients is a complex and challenging task. In principle, machine learning and deep learning models are flexible and expressive enough to capture the dynamics of clinical
Externí odkaz:
http://arxiv.org/abs/2305.10041
Autor:
Healy, Erin, Ali, Aamir M., Arnold, Kam, Austermann, Jason E., Beall, James A., Bruno, Sarah Marie, Choi, Steve K., Connors, Jake, Cothar, Nicholas F., Dober, Bradley, Duff, Shannon M., Galitzki, Nicholas, Hilton, Gene, Ho, Shuay-Pwu Patty, Hubmayr, Johannes, Johnson, Bradley R., Li, Yaqiong, Link, Michael J., Lucas, Tammy J., McCarrick, Heather, Niemack, Michael D., Silva-Feaver, Maximiliano, Sonka, Rita F., Staggs, Suzanne, Vavagiakis, Eve M., Vissers, Michael R., Wang, Yuhan, Westbrook, Benjamin, Wollack, Edward J., Xu, Zhilei, Zheng, Kaiwen
Publikováno v:
Proc. SPIE 11453, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X, 1145317 (2020)
The Simons Observatory (SO) is a suite of instruments sensitive to temperature and polarization of the cosmic microwave background (CMB) to be located at Cerro Toco in the Atacama Desert in Chile. Five telescopes, one large aperture telescope and fou
Externí odkaz:
http://arxiv.org/abs/2204.05869
Autor:
McCarrick, Heather, Healy, Erin, Ahmed, Zeeshan, Arnold, Kam, Atkins, Zachary, Austermann, Jason E., Bhandarkar, Tanay, Beall, Jim A., Bruno, Sarah Marie, Choi, Steve K., Connors, Jake, Cothard, Nicholas F., Crowley, Kevin D., Dicker, Simon, Dober, Bradley, Duell, Cody J., Duff, Shannon M., Dutcher, Daniel, Frisch, Josef C., Galitzki, Nicholas, Gralla, Megan B., Gudmundsson, Jon E., Henderson, Shawn W., Hilton, Gene C., Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Kofman, Anna M., Kusaka, Akito, Lashner, Jack, Lee, Adrian T., Li, Yaqiong, Link, Michael J., Lucas, Tammy J., Lungu, Marius, Mates, J. A. B., McMahon, Jeffrey J., Niemack, Michael D., Orlowski-Scherer, John, Seibert, Joseph, Silva-Feaver, Maximiliano, Simon, Sara M., Staggs, Suzanne, Suzuki, Aritoki, Terasaki, Tomoki, Ullom, Joel N., Vavagiakis, Eve M., Vale, Leila R., Van Lanen, Jeff, Vissers, Michael R., Wang, Yuhan, Wollack, Edward J., Xu, Zhilei, Young, Edward, Yu, Cyndia, Zheng, Kaiwen, Zhu, Ningfeng
Publikováno v:
2021 ApJ 922 38
Advances in cosmic microwave background (CMB) science depend on increasing the number of sensitive detectors observing the sky. New instruments deploy large arrays of superconducting transition-edge sensor (TES) bolometers tiled densely into ever lar
Externí odkaz:
http://arxiv.org/abs/2106.14797