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1. The Simons Observatory: Design, integration, and testing of the small aperture telescopes

Author

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, and Zheng, Kaiwen

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

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 between 27 and 280 GHz to search for primordial B-modes to a sensitivity of $\sigma(r)=0.002$, with quantified systematic errors well below this value. Each SAT is a self-contained cryogenic telescope with a 35$^\circ$ field of view, 42 cm diameter optical aperture, 40 K half-wave plate, 1 K refractive optics, and $<0.1$ K focal plane that holds $>12,000$ TES detectors. We describe the nominal design of the SATs and present details about the integration and testing for one operating at 93 and 145 GHz.

Published
2024

2. Simons Observatory Microwave SQUID Multiplexing Readout -- Cryogenic RF Amplifier and Coaxial Chain Design

Author

Rao, Mayuri Sathyanarayana, Silva-Feaver, Maximiliano, Ali, Aamir, Arnold, Kam, Ashton, Peter, Dober, Bradley J., Duell, Cody J., Duff, Shannon M., Galitzki, Nicholas, Healy, Erin, Henderson, Shawn, Ho, Shuay-Pwu Patty, Hoh, Jonathan, Kofman, Anna M., Kusaka, Akito, Lee, Adrian T., Mangu, Aashrita, Mathewson, Justin, Mauskopf, Philip, McCarrick, Heather, Moore, Jenna, Niemack, Michael D., Raum, Christopher, Salatino, Maria, Sasse, Trevor, Seibert, Joseph, Simon, Sara M., Staggs, Suzanne, Stevens, Jason R., Teply, Grant, Thornton, Robert, Ullom, Joel, Vavagiakis, Eve M., Westbrook, Benjamin, Xu, Zhilei, and Zhu, Ningfeng

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Instrumentation and Detectors
Abstract

The Simons Observatory (SO) is an upcoming polarization-sensitive Cosmic Microwave Background (CMB) experiment on the Cerro Toco Plateau (Chile) with large overlap with other optical and infrared surveys (e.g., DESI, LSST, HSC). To enable the readout of \bigO(10,000) detectors in each of the four telescopes of SO, we will employ the microwave SQUID multiplexing technology. With a targeted multiplexing factor of \bigO{(1,000)}, microwave SQUID multiplexing has never been deployed on the scale needed for SO. Here we present the design of the cryogenic coaxial cable and RF component chain that connects room temperature readout electronics to superconducting resonators that are coupled to Transition Edge Sensor bolometers operating at sub-Kelvin temperatures. We describe design considerations including cryogenic RF component selection, system linearity, noise, and thermal power dissipation., Comment: 10 pages, 2 figures

Published
2020
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3. Small Aperture Telescopes for the Simons Observatory

Author

Ali, Aamir M., Adachi, Shunsuke, Arnold, Kam, Ashton, Peter, Bazarko, Andrew, Chinone, Yuji, Coppi, Gabriele, Corbett, Lance, Crowley, Kevin D, Crowley, Kevin T, Devlin, Mark, Dicker, Simon, Duff, Shannon, Ellis, Chris, Galitzki, Nicholas, Goeckner-Wald, Neil, Harrington, Kathleen, Healy, Erin, Hill, Charles A, Ho, Shuay-Pwu Patty, Hubmayr, Johannes, Keating, Brian, Kiuchi, Kenji, Kusaka, Akito, Lee, Adrian T, Ludlam, Michael, Mangu, Aashrita, Matsuda, Frederick, McCarrick, Heather, Nati, Federico, Niemack, Michael D., Nishino, Haruki, Orlowski-Scherer, John, Rao, Mayuri Sathyanarayana, Raum, Christopher, Sakurai, Yuki, Salatino, Maria, Sasse, Trevor, Seibert, Joseph, Sierra, Carlos, Silva-Feaver, Maximiliano, Spisak, Jacob, Simon, Sara M, Staggs, Suzanne, Tajima, Osamu, Teply, Grant, Tsan, Tran, Wollack, Edward, Westbrook, Bejamin, Xu, Zhilei, Zannoni, Mario, and Zhu, Ningfeng

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Simons Observatory (SO) is an upcoming cosmic microwave background (CMB) experiment located on Cerro Toco, Chile, that will map the microwave sky in temperature and polarization in six frequency bands spanning 27 to 285 GHz. SO will consist of one 6-meter Large Aperture Telescope (LAT) fielding $\sim$30,000 detectors and an array of three 0.42-meter Small Aperture Telescopes (SATs) fielding an additional 30,000 detectors. This synergy will allow for the extremely sensitive characterization of the CMB over angular scales ranging from an arcmin to tens of degrees, enabling a wide range of scientific output. Here we focus on the SATs targeting degree angular scales with successive dichroic instruments observing at Mid-Frequency (MF: 93/145 GHz), Ultra-High-Frequency (UHF: 225/285 GHz), and Low-Frequency (LF: 27/39 GHz). The three SATs will be able to map $\sim$10% of the sky to a noise level of 2 $\mu$K-arcmin when combining 93 and 145 GHz. The multiple frequency bands will allow the CMB to be separated from galactic foregrounds (primarily synchrotron and dust), with the primary science goal of characterizing the primordial tensor-to-scalar ratio, $r$, at a target level of $\sigma \left(r\right) \approx 0.003$.

Published
2020
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4. Characterization of Transition Edge Sensors for the Simons Observatory

Author

Stevens, Jason R., Cothard, Nicholas F., Vavagiakis, Eve M., Ali, Aamir, Arnold, Kam, Austermann, Jason E., Choi, Steve K., Dober, Bradley J., Duell, Cody, Duff, Shannon M., Hilton, Gene C., Ho, Shuay-Pwu Patty, Hoang, Thuong D., Hubmayr, Johannes, Lee, Adrian T., Mangu, Aashrita, Nati, Federico, Niemack, Michael D., Raum, Christopher, Renzullo, Mario, Salatino, Maria, Sasse, Trevor, Simon, Sara M., Staggs, Suzanne, Suzuki, Aritoki, Truitt, Patrick, Ullom, Joel, Vivalda, John, Vissers, Michael R., Walker, Samantha, Westbrook, Benjamin, Wollack, Edward J., Xu, Zhilei, and Yohannes, Daniel

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Simons Observatory is building both large (6 m) and small (0.5 m) aperture telescopes in the Atacama desert in Chile to observe the cosmic microwave background (CMB) radiation with unprecedented sensitivity. Simons Observatory telescopes in total will use over 60,000 transition edge sensor (TES) detectors spanning center frequencies between 27 and 285 GHz and operating near 100 mK. TES devices have been fabricated for the Simons Observatory by NIST, Berkeley, and HYPRES/SeeQC corporation. Iterations of these devices have been tested cryogenically in order to inform the fabrication of further devices, which will culminate in the final TES designs to be deployed in the field. The detailed design specifications have been independently iterated at each fabrication facility for particular detector frequencies. We present test results for prototype devices, with emphasis on NIST high frequency detectors. A dilution refrigerator was used to achieve the required temperatures. Measurements were made both with 4-lead resistance measurements and with a time domain Superconducting Quantum Interference Device (SQUID) multiplexer system. The SQUID readout measurements include analysis of current vs voltage (IV) curves at various temperatures, square wave bias step measurements, and detector noise measurements. Normal resistance, superconducting critical temperature, saturation power, thermal and natural time constants, and thermal properties of the devices are extracted from these measurements., Comment: 9 Pages, 5 figures, Low Temperature Detectors 19

Published
2019
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5. Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from POLARBEAR and Cosmic Shear from Subaru Hyper Suprime-Cam

Author

Namikawa, Toshiya, Chinone, Yuji, Miyatake, Hironao, Oguri, Masamune, Takahashi, Ryuichi, Kusaka, Akito, Katayama, Nobuhiko, Adachi, Shunsuke, Aguilar, Mario, Aihara, Hiroaki, Ali, Aamir, Armstrong, Robert, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beck, Dominic, Beckman, Shawn, Bianchini, Federico, Boettger, David, Borrill, Julian, Cheung, Kolen, Corbett, Lance, Crowley, Kevin T., Bouhargani, Hamza El, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Feng, Chang, Galitzki, Nicholas, Goeckner-Wald, Neil, Groh, John, Hamada, Takaho, Hasegawa, Masaya, Hazumi, Masashi, Hill, Charles, Howe, Logan, Jeong, Oliver, Kaneko, Daisuke, Keating, Brian, Lee, Adrian T., Leon, David, Linder, Eric, Lowry, Lindsay Ng, Mangu, Aashrita, Matsuda, Frederick, Minami, Yuto, Miyazaki, Satoshi, Murayama, Hitoshi, Navaroli, Martin, Nishino, Haruki, Nishizawa, Atsushi J., Pham, Anh Thi Phuong, Poletti, Davide, Puglisi, Giuseppe, Reichardt, Christian L., Sherwin, Blake D., Silva-Feaver, Maximiliano, Siritanasak, Praween, Speagle, Joshua S., Stompor, Radek, Suzuki, Aritoki, Tait, Philip J., Tajima, Osamu, Takada, Masahiro, Takakura, Satoru, Takatori, Sayuri, Tanabe, Daiki, Tanaka, Masayuki, Teply, Grant P., Tsai, Calvin, Verges, Clara, Westbrook, Ben, Zhou, Yuyang, Collaboration, The POLARBEAR, and Collaboration, the Subaru HSC SSP

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present the first measurement of cross-correlation between the lensing potential, reconstructed from cosmic microwave background (CMB) {\it polarization} data, and the cosmic shear field from galaxy shapes. This measurement is made using data from the POLARBEAR CMB experiment and the Subaru Hyper Suprime-Cam (HSC) survey. By analyzing an 11~deg$^2$ overlapping region, we reject the null hypothesis at 3.5$\sigma$\ and constrain the amplitude of the {\bf cross-spectrum} to $\widehat{A}_{\rm lens}=1.70\pm 0.48$, where $\widehat{A}_{\rm lens}$ is the amplitude normalized with respect to the Planck~2018{} prediction, based on the flat $\Lambda$ cold dark matter cosmology. The first measurement of this {\bf cross-spectrum} without relying on CMB temperature measurements is possible due to the deep POLARBEAR map with a noise level of ${\sim}$6\,$\mu$K-arcmin, as well as the deep HSC data with a high galaxy number density of $n_g=23\,{\rm arcmin^{-2}}$. We present a detailed study of the systematics budget to show that residual systematics in our results are negligibly small, which demonstrates the future potential of this cross-correlation technique., Comment: 16 pages, 5 figures, Accepted for publication in ApJ

Published
2019
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6. Machine Learning in High Energy Physics Community White Paper

Author

Albertsson, Kim, Altoe, Piero, Anderson, Dustin, Anderson, John, Andrews, Michael, Espinosa, Juan Pedro Araque, Aurisano, Adam, Basara, Laurent, Bevan, Adrian, Bhimji, Wahid, Bonacorsi, Daniele, Burkle, Bjorn, Calafiura, Paolo, Campanelli, Mario, Capps, Louis, Carminati, Federico, Carrazza, Stefano, Chen, Yi-fan, Childers, Taylor, Coadou, Yann, Coniavitis, Elias, Cranmer, Kyle, David, Claire, Davis, Douglas, De Simone, Andrea, Duarte, Javier, Erdmann, Martin, Eschle, Jonas, Farbin, Amir, Feickert, Matthew, Castro, Nuno Filipe, Fitzpatrick, Conor, Floris, Michele, Forti, Alessandra, Garra-Tico, Jordi, Gemmler, Jochen, Girone, Maria, Glaysher, Paul, Gleyzer, Sergei, Gligorov, Vladimir, Golling, Tobias, Graw, Jonas, Gray, Lindsey, Greenwood, Dick, Hacker, Thomas, Harvey, John, Hegner, Benedikt, Heinrich, Lukas, Heintz, Ulrich, Hooberman, Ben, Junggeburth, Johannes, Kagan, Michael, Kane, Meghan, Kanishchev, Konstantin, Karpiński, Przemysław, Kassabov, Zahari, Kaul, Gaurav, Kcira, Dorian, Keck, Thomas, Klimentov, Alexei, Kowalkowski, Jim, Kreczko, Luke, Kurepin, Alexander, Kutschke, Rob, Kuznetsov, Valentin, Köhler, Nicolas, Lakomov, Igor, Lannon, Kevin, Lassnig, Mario, Limosani, Antonio, Louppe, Gilles, Mangu, Aashrita, Mato, Pere, Meenakshi, Narain, Meinhard, Helge, Menasce, Dario, Moneta, Lorenzo, Moortgat, Seth, Neubauer, Mark, Newman, Harvey, Otten, Sydney, Pabst, Hans, Paganini, Michela, Paulini, Manfred, Perdue, Gabriel, Perez, Uzziel, Picazio, Attilio, Pivarski, Jim, Prosper, Harrison, Psihas, Fernanda, Radovic, Alexander, Reece, Ryan, Rinkevicius, Aurelius, Rodrigues, Eduardo, Rorie, Jamal, Rousseau, David, Sauers, Aaron, Schramm, Steven, Schwartzman, Ariel, Severini, Horst, Seyfert, Paul, Siroky, Filip, Skazytkin, Konstantin, Sokoloff, Mike, Stewart, Graeme, Stienen, Bob, Stockdale, Ian, Strong, Giles, Sun, Wei, Thais, Savannah, Tomko, Karen, Upfal, Eli, Usai, Emanuele, Ustyuzhanin, Andrey, Vala, Martin, Vasel, Justin, Vallecorsa, Sofia, Verzetti, Mauro, Vilasís-Cardona, Xavier, Vlimant, Jean-Roch, Vukotic, Ilija, Wang, Sean-Jiun, Watts, Gordon, Williams, Michael, Wu, Wenjing, Wunsch, Stefan, Yang, Kun, and Zapata, Omar

Subjects
Physics - Computational Physics, Computer Science - Machine Learning, High Energy Physics - Experiment, Statistics - Machine Learning
Abstract

Machine learning has been applied to several problems in particle physics research, beginning with applications to high-level physics analysis in the 1990s and 2000s, followed by an explosion of applications in particle and event identification and reconstruction in the 2010s. In this document we discuss promising future research and development areas for machine learning in particle physics. We detail a roadmap for their implementation, software and hardware resource requirements, collaborative initiatives with the data science community, academia and industry, and training the particle physics community in data science. The main objective of the document is to connect and motivate these areas of research and development with the physics drivers of the High-Luminosity Large Hadron Collider and future neutrino experiments and identify the resource needs for their implementation. Additionally we identify areas where collaboration with external communities will be of great benefit., Comment: Editors: Sergei Gleyzer, Paul Seyfert and Steven Schramm

Published
2018

7. The Simons Observatory: Design, Integration, and Current Status of Small Aperture Telescopes

Author

Mangu, Aashrita, primary, Corbett, Lance, additional, Bhimani, Sanah, additional, Carl, Fred, additional, Day-Weiss, Samuel, additional, DiGia, Brooke, additional, Errard, Josquin, additional, Galitzki, Nicholas, additional, Hazumi, Masashi, additional, Henderson, Shawn W., additional, Miller, Amber, additional, Moore, Jenna, additional, Song, Xue, additional, Tsan, Tran, additional, Wang, Yuhan, additional, and Zonca, Andrea, additional

Published
2024
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9. Simons Observatory Microwave SQUID Multiplexing Readout: Cryogenic RF Amplifier and Coaxial Chain Design

Author

Sathyanarayana Rao, Mayuri, Silva-Feaver, Maximiliano, Ali, Aamir, Arnold, Kam, Ashton, Peter, Dober, Bradley J., Duell, Cody J., Duff, Shannon M., Galitzki, Nicholas, Healy, Erin, Henderson, Shawn, Ho, Shuay-Pwu Patty, Hoh, Jonathan, Kofman, Anna M., Kusaka, Akito, Lee, Adrian T., Mangu, Aashrita, Mathewson, Justin, Mauskopf, Philip, McCarrick, Heather, Moore, Jenna, Niemack, Michael D., Raum, Christopher, Salatino, Maria, Sasse, Trevor, Seibert, Joseph, Simon, Sara M., Staggs, Suzanne, Stevens, Jason R., Teply, Grant, Thornton, Robert, Ullom, Joel, Vavagiakis, Eve M., Westbrook, Benjamin, Xu, Zhilei, and Zhu, Ningfeng

Published
2020
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10. Characterization of Transition Edge Sensors for the Simons Observatory

Author

Stevens, Jason R., Cothard, Nicholas F., Vavagiakis, Eve M., Ali, Aamir, Arnold, Kam, Austermann, Jason E., Choi, Steve K., Dober, Bradley J., Duell, Cody, Duff, Shannon M., Hilton, Gene C., Ho, Shuay-Pwu Patty, Hoang, Thuong D., Hubmayr, Johannes, Lee, Adrian T., Mangu, Aashrita, Nati, Federico, Niemack, Michael D., Raum, Christopher, Renzullo, Mario, Salatino, Maria, Sasse, Trevor, Simon, Sara M., Staggs, Suzanne, Suzuki, Aritoki, Truitt, Patrick, Ullom, Joel, Vivalda, John, Vissers, Michael R., Walker, Samantha, Westbrook, Benjamin, Wollack, Edward J., Xu, Zhilei, and Yohannes, Daniel

Published
2020
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11. Assembly and Integration Process of the High-Density Detector Array Readout Modules for the Simons Observatory

Author

Li, Yaqiong, Arnold, Kam, Atkins, Zachary, Bruno, Sarah Marie, Cothard, Nicholas F., Dober, Bradley, Duell, Cody J., Duff, Shannon M., Gallardo, Patricio A., Healy, Erin, Ho, Shuay-Pwu Patty, Hubmayr, Johannes, Keating, Brian, Lee, Adrian T., Mangu, Aashrita, McCarrick, Heather, Niemack, Michael D., Newburgh, Laura, Raum, Christopher, Salatino, Maria, Sasse, Trevor, Silva-Feaver, Maximiliano, Simon, Sara M., Staggs, Suzanne, Suzuki, Aritoki, Ullom, Joel, Vavagiakis, Eve M., Vissers, Michael R., Wang, Yuhan, Westbrook, Benjamin, Wollack, Edward J., Xu, Zhilei, Zheng, Kaiwen, and Zhu, Ningfeng

Published
2020
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13. Method for rapid performance validation of large TES bolometer array for POLARBEAR-2A using a coherent millimeter-wave source

Author

Segawa, Yuuko, primary, Hirose, Haruaki, additional, Kaneko, Daisuke, additional, Hasegawa, Masaya, additional, Adachi, Shunsuke, additional, Ade, Peter, additional, Faúndez, Mario Andrés Osvaldo Aguilar, additional, Akiba, Yoshiki, additional, Arnold, Kam, additional, Avva, Jessica, additional, Baccigalupi, Carlo, additional, Barron, Darcy, additional, Beck, Dominic, additional, Beckman, Shawn, additional, Bianchini, Federico, additional, Boettger, David, additional, Borrill, Julian, additional, Carron, Julien, additional, Chapman, Scott, additional, Cheung, Kolen, additional, Chinone, Yuji, additional, Crowley, Kevin, additional, Cukierman, Ari, additional, de Haan, Tijmen, additional, Dobbs, Matt, additional, Dunner, Rolando, additional, Bouhargani, Hamza El, additional, Elleflot, Tucker, additional, Errard, Josquin, additional, Fabbian, Giulio, additional, Feeney, Stephen, additional, Feng, Chang, additional, Fujino, Takuro, additional, Galitzki, Nicholas, additional, Goeckner-Wald, Neil, additional, Groh, John, additional, Hall, Grantland, additional, Halverson, Nils, additional, Hamada, Takaho, additional, Hazumi, Masashi, additional, Hill, Charles, additional, Howe, Logan, additional, Inoue, Yuki, additional, Ito, Jennifer, additional, Jaehnig, Greg, additional, Jeong, Oliver, additional, Katayama, Nobuhiko, additional, Keating, Brian, additional, Keskitalo, Reijo, additional, Kikuchi, Shuhei, additional, Kisner, Theodore, additional, Krachmalnicoff, Nicoletta, additional, Kusaka, Akito, additional, Lee, Adrian T., additional, Leon, David, additional, Linder, Eric, additional, Lowry, Lindsay Ng, additional, Mangu, Aashrita, additional, Matsuda, Frederick, additional, Minami, Yuto, additional, Montgomery, Josh, additional, Navaroli, Martin, additional, Nishino, Haruki, additional, Peloton, Julien, additional, Pham, Anh Thi Phuong, additional, Poletti, Davide, additional, Puglisi, Giuseppe, additional, Raum, Christopher, additional, Reichardt, Christian L., additional, Ross, Colin, additional, Silva-Feaver, Maximiliano, additional, Siritanasak, Praween, additional, Stompor, Radek, additional, Suzuki, Aritoki, additional, Tajima, Osamu, additional, Takakura, Satoru, additional, Takatori, Sayuri, additional, Tanabe, Daiki, additional, Teply, Grant P., additional, Tsai, Calvin, additional, Verges, Clara, additional, Westbrook, Ben, additional, and Zhou, Yuyang, additional

Published
2021
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14. Small Aperture Telescopes for the Simons Observatory

Author

Ali, Aamir M., primary, Adachi, Shunsuke, additional, Arnold, Kam, additional, Ashton, Peter, additional, Bazarko, Andrew, additional, Chinone, Yuji, additional, Coppi, Gabriele, additional, Corbett, Lance, additional, Crowley, Kevin D., additional, Crowley, Kevin T., additional, Devlin, Mark, additional, Dicker, Simon, additional, Duff, Shannon, additional, Ellis, Chris, additional, Galitzki, Nicholas, additional, Goeckner-Wald, Neil, additional, Harrington, Kathleen, additional, Healy, Erin, additional, Hill, Charles A., additional, Ho, Shuay-Pwu Patty, additional, Hubmayr, Johannes, additional, Keating, Brian, additional, Kiuchi, Kenji, additional, Kusaka, Akito, additional, Lee, Adrian T., additional, Ludlam, Michael, additional, Mangu, Aashrita, additional, Matsuda, Frederick, additional, McCarrick, Heather, additional, Nati, Federico, additional, Niemack, Michael D., additional, Nishino, Haruki, additional, Orlowski-Scherer, John, additional, Sathyanarayana Rao, Mayuri, additional, Raum, Christopher, additional, Sakurai, Yuki, additional, Salatino, Maria, additional, Sasse, Trevor, additional, Seibert, Joseph, additional, Sierra, Carlos, additional, Silva-Feaver, Maximiliano, additional, Spisak, Jacob, additional, Simon, Sara M., additional, Staggs, Suzanne, additional, Tajima, Osamu, additional, Teply, Grant, additional, Tsan, Tran, additional, Wollack, Edward, additional, Westbrook, Bejamin, additional, Xu, Zhilei, additional, Zannoni, Mario, additional, and Zhu, Ningfeng, additional

Published
2020
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15. Machine Learning in High Energy Physics Community White Paper

Author

Albertsson, Kim, primary, Altoe, Piero, additional, Anderson, Dustin, additional, Andrews, Michael, additional, Araque Espinosa, Juan Pedro, additional, Aurisano, Adam, additional, Basara, Laurent, additional, Bevan, Adrian, additional, Bhimji, Wahid, additional, Bonacorsi, Daniele, additional, Calafiura, Paolo, additional, Campanelli, Mario, additional, Capps, Louis, additional, Carminati, Federico, additional, Carrazza, Stefano, additional, Childers, Taylor, additional, Coniavitis, Elias, additional, Cranmer, Kyle, additional, David, Claire, additional, Davis, Douglas, additional, Duarte, Javier, additional, Erdmann, Martin, additional, Eschle, Jonas, additional, Farbin, Amir, additional, Feickert, Matthew, additional, Castro, Nuno Filipe, additional, Fitzpatrick, Conor, additional, Floris, Michele, additional, Forti, Alessandra, additional, Garra-Tico, Jordi, additional, Gemmler, Jochen, additional, Girone, Maria, additional, Glaysher, Paul, additional, Gleyzer, Sergei, additional, Gligorov, Vladimir, additional, Golling, Tobias, additional, Graw, Jonas, additional, Gray, Lindsey, additional, Greenwood, Dick, additional, Hacker, Thomas, additional, Harvey, John, additional, Hegner, Benedikt, additional, Heinrich, Lukas, additional, Hooberman, Ben, additional, Junggeburth, Johannes, additional, Kagan, Michael, additional, Kane, Meghan, additional, Kanishchev, Konstantin, additional, Karpiński, Przemysław, additional, Kassabov, Zahari, additional, Kaul, Gaurav, additional, Kcira, Dorian, additional, Keck, Thomas, additional, Klimentov, Alexei, additional, Kowalkowski, Jim, additional, Kreczko, Luke, additional, Kurepin, Alexander, additional, Kutschke, Rob, additional, Kuznetsov, Valentin, additional, Köhler, Nicolas, additional, Lakomov, Igor, additional, Lannon, Kevin, additional, Lassnig, Mario, additional, Limosani, Antonio, additional, Louppe, Gilles, additional, Mangu, Aashrita, additional, Mato, Pere, additional, Meinhard, Helge, additional, Menasce, Dario, additional, Moneta, Lorenzo, additional, Moortgat, Seth, additional, Narain, Meenakshi, additional, Neubauer, Mark, additional, Newman, Harvey, additional, Pabst, Hans, additional, Paganini, Michela, additional, Paulini, Manfred, additional, Perdue, Gabriel, additional, Perez, Uzziel, additional, Picazio, Attilio, additional, Pivarski, Jim, additional, Prosper, Harrison, additional, Psihas, Fernanda, additional, Radovic, Alexander, additional, Reece, Ryan, additional, Rinkevicius, Aurelius, additional, Rodrigues, Eduardo, additional, Rorie, Jamal, additional, Rousseau, David, additional, Sauers, Aaron, additional, Schramm, Steven, additional, Schwartzman, Ariel, additional, Severini, Horst, additional, Seyfert, Paul, additional, Siroky, Filip, additional, Skazytkin, Konstantin, additional, Sokoloff, Mike, additional, Stewart, Graeme, additional, Stienen, Bob, additional, Stockdale, Ian, additional, Strong, Giles, additional, Thais, Savannah, additional, Tomko, Karen, additional, Upfal, Eli, additional, Usai, Emanuele, additional, Ustyuzhanin, Andrey, additional, Vala, Martin, additional, Vallecorsa, Sofia, additional, Vasel, Justin, additional, Verzetti, Mauro, additional, Vilasís-Cardona, Xavier, additional, Vlimant, Jean-Roch, additional, Vukotic, Ilija, additional, Wang, Sean-Jiun, additional, Watts, Gordon, additional, Williams, Michael, additional, Wu, Wenjing, additional, Wunsch, Stefan, additional, and Zapata, Omar, additional

Published
2018
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