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164 results on '"Halverson, Nils"'

1. Development of the Low Frequency Telescope focal plane detector arrays for LiteBIRD

Author

Ghigna, Tommaso, Suzuki, Aritoki, Westbrook, Benjamin, Raum, Christopher, Akamatsu, Hiroki, Beckman, Shawn, Farias, Nicole, de Haan, Tijmen, Halverson, Nils, Hazumi, Masashi, Hubmayr, Johannes, Jaehnig, Greg, Lee, Adrian T., Stever, Samantha L., and Zhou, Yu

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

LiteBIRD, a forthcoming JAXA mission, aims to accurately study the microwave sky within the 40-400 GHz frequency range divided into 15 distinct nominal bands. The primary objective is to constrain the CMB inflationary signal, specifically the primordial B-modes. LiteBIRD targets the CMB B-mode signal on large angular scales, where the primordial inflationary signal is expected to dominate, with the goal of reaching a tensor-to-scalar ratio sensitivity of $\sigma_r\sim0.001$. LiteBIRD frequency bands will be split among three telescopes, with some overlap between telescopes for better control of systematic effects. Here we report on the development status of the detector arrays for the Low Frequency Telescope (LFT), which spans the 34-161 GHz range, with 12 bands subdivided between four types of trichroic pixels consisting of lenslet-coupled sinuous antennas. The signal from the antenna is bandpass filtered and sensed by AlMn Transition-Edge Sensors (TES). We provide an update on the status of the design and development of LiteBIRD's LFT LF1 (40-60-78 GHz), LF2 (50-68-89 GHz) pixels. We discuss design choices motivated by LiteBIRD scientific goals. In particular we focus on the details of the optimization of the design parameters of the sinuous antenna, on-chip bandpass filters, cross-under and impedance transformers and all the RF components that define the LF1 and LF2 pixel detection chain. We present this work in the context of the technical challenges and physical constraints imposed by the finite size of the instrument., Comment: 12 pages, 10 figures, 1 table, SPIE 2024

Published
2024

3. Development of the Low Frequency Telescope Focal Plane Detector Modules for LiteBIRD

Author

Westbrook, Benjamin, Raum, Christopher, Beckman, Shawn, Lee, Adrian T., Farias, Nicole, Bogdan, Andrew, Hornsby, Amber, Suzuki, Aritoki, Rotermund, Kaja, Elleflot, Tucker, Austermann, Jason E., Beall, James A., Duff, Shannon M., Hubmayr, Johannes, Vissers, Michael R., Link, Michael J., Jaehnig, Greg, Halverson, Nils, Ghigna, Tomasso, Hazumi, Masashi, Stever, Samantha, Minami, Yuto, Thompson, Keith L., Russell, Megan, Arnold, Kam, and Silva-Feaver, Maximiliano

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

LiteBIRD is a JAXA-led strategic large-class satellite mission designed to measure the polarization of the cosmic microwave background and Galactic foregrounds from 34 to 448 GHz across the entire sky from L2 in the late 2020s. The scientific payload includes three telescopes which are called the low-, mid-, and high-frequency telescopes each with their own receiver that covers a portion of the mission's frequency range. The low frequency telescope will map synchrotron radiation from the Galactic foreground and the cosmic microwave background. We discuss the design, fabrication, and characterization of the low-frequency focal plane modules for low-frequency telescope, which has a total bandwidth ranging from 34 to 161 GHz. There will be a total of 4 different pixel types with 8 overlapping bands to cover the full frequency range. These modules are housed in a single low-frequency focal plane unit which provides thermal isolation, mechanical support, and radiative baffling for the detectors. The module design implements multi-chroic lenslet-coupled sinuous antenna arrays coupled to transition edge sensor bolometers read out with frequency-domain mulitplexing. While this technology has strong heritage in ground-based cosmic microwave background experiments, the broad frequency coverage, low optical loading conditions, and the high cosmic ray background of the space environment require further development of this technology to be suitable for LiteBIRD. In these proceedings, we discuss the optical and bolometeric characterization of a triplexing prototype pixel with bands centered on 78, 100, and 140 GHz., Comment: SPIE Astronomical Telescope + Instrumentation (AS22)

Published
2022
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4. Snowmass2021 Cosmic Frontier: Cosmic Microwave Background Measurements White Paper

Author

Chang, Clarence L., Huffenberger, Kevin M., Benson, Bradford A., Bianchini, Federico, Chluba, Jens, Delabrouille, Jacques, Flauger, Raphael, Hanany, Shaul, Jones, William C., Kogut, Alan J., McMahon, Jeffrey J., Meyers, Joel, Sehgal, Neelima, Simon, Sara M., Umilta, Caterina, Abazajian, Kevork N., Ahmed, Zeeshan, Akrami, Yashar, Anderson, Adam J., Ansarinejad, Behzad, Austermann, Jason, Baccigalupi, Carlo, Barkats, Denis, Barron, Darcy, Barry, Peter S., Battaglia, Nicholas, Baxter, Eric, Beck, Dominic, Bender, Amy N., Bennett, Charles, Beringue, Benjamin, Bischoff, Colin, Bleem, Lindsey, Bock, James, Bolliet, Boris, Bond, J Richard, Borrill, Julian, Brinckmann, Thejs, Brown, Michael L., Calabrese, Erminia, Carlstrom, John, Challinor, Anthony, Chang, Chihway, Chinone, Yuji, Clark, Susan E., Coulton, William, Cukierman, Ari, Cyr-Racine, Francis-Yan, Duff, Shannon M., Dvorkin, Cora, van Engelen, Alexander, Errard, Josquin, Eskilt, Johannes R., Essinger-Hileman, Thomas, Fabbian, Giulio, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey, Freese, Katherine, Galitzki, Nicholas, Gawiser, Eric, Grin, Daniel, Grohs, Evan, Gruppuso, Alessandro, Gudmundsson, Jon E., Halverson, Nils W., Hamilton, Jean-Christophe, Harrington, Kathleen, Henrot-Versillé, Sophie, Hensley, Brandon, Hill, J. Colin, Hincks, Adam D., Hlozek, Renee, Holzapfel, William, Hotinli, Selim C., Hui, Howard, Ibitoye, Ayodeji, Johnson, Matthew, Johnson, Bradley R., Kang, Jae Hwan, Karkare, Kirit S., Knox, Lloyd, Kovac, John, Lau, Kenny, Legrand, Louis, Loverde, Marilena, Lubin, Philip, Ma, Yin-Zhe, Mroczkowski, Tony, Mukherjee, Suvodip, Münchmeyer, Moritz, Nagai, Daisuke, Nagy, Johanna, Niemack, Michael, Novosad, Valentine, Omori, Yuuki, Orlando, Giorgio, Pan, Zhaodi, Perotto, Laurence, Petroff, Matthew A., Pogosian, Levon, Pryke, Clem, Rahlin, Alexandra, Raveri, Marco, Reichardt, Christian L., Remazeilles, Mathieu, Rephaeli, Yoel, Ruhl, John, Schaan, Emmanuel, Shandera, Sarah, Shimon, Meir, Soliman, Ahmed, Stark, Antony A., Starkman, Glenn D., Stompor, Radek, Thakur, Ritoban Basu, Trendafilova, Cynthia, Tristram, Matthieu, Trivedi, Pranjal, Tucker, Gregory, Di Valentino, Eleonora, Vieira, Joaquin, Vieregg, Abigail, Wang, Gensheng, Watson, Scott, Wenzl, Lukas, Wollack, Edward J., Wu, W. L. Kimmy, Xu, Zhilei, Zegeye, David, and Zhang, Cheng

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, General Relativity and Quantum Cosmology, High Energy Physics - Experiment, High Energy Physics - Phenomenology
Abstract

This is a solicited whitepaper for the Snowmass 2021 community planning exercise. The paper focuses on measurements and science with the Cosmic Microwave Background (CMB). The CMB is foundational to our understanding of modern physics and continues to be a powerful tool driving our understanding of cosmology and particle physics. In this paper, we outline the broad and unique impact of CMB science for the High Energy Cosmic Frontier in the upcoming decade. We also describe the progression of ground-based CMB experiments, which shows that the community is prepared to develop the key capabilities and facilities needed to achieve these transformative CMB measurements., Comment: contribution to Snowmass 2021

Published
2022

5. Snowmass 2021 CMB-S4 White Paper

Author

Abazajian, Kevork, Abdulghafour, Arwa, Addison, Graeme E., Adshead, Peter, Ahmed, Zeeshan, Ajello, Marco, Akerib, Daniel, Allen, Steven W., Alonso, David, Alvarez, Marcelo, Amin, Mustafa A., Amiri, Mandana, Anderson, Adam, Ansarinejad, Behzad, Archipley, Melanie, Arnold, Kam S., Ashby, Matt, Aung, Han, Baccigalupi, Carlo, Baker, Carina, Bakshi, Abhishek, Bard, Debbie, Barkats, Denis, Barron, Darcy, Barry, Peter S., Bartlett, James G., Barton, Paul, Thakur, Ritoban Basu, Battaglia, Nicholas, Beall, Jim, Bean, Rachel, Beck, Dominic, Belkner, Sebastian, Benabed, Karim, Bender, Amy N., Benson, Bradford A., Besuner, Bobby, Bethermin, Matthieu, Bhimani, Sanah, Bianchini, Federico, Biquard, Simon, Birdwell, Ian, Bischoff, Colin A., Bleem, Lindsey, Bocaz, Paulina, Bock, James J., Bocquet, Sebastian, Boddy, Kimberly K., Bond, J. Richard, Borrill, Julian, Bouchet, Francois R., Brinckmann, Thejs, Brown, Michael L., Bryan, Sean, Buza, Victor, Byrum, Karen, Calabrese, Erminia, Calafut, Victoria, Caldwell, Robert, Carlstrom, John E., Carron, Julien, Cecil, Thomas, Challinor, Anthony, Chan, Victor, Chang, Clarence L., Chapman, Scott, Charles, Eric, Chauvin, Eric, Cheng, Cheng, Chesmore, Grace, Cheung, Kolen, Chinone, Yuji, Chluba, Jens, Cho, Hsiao-Mei Sherry, Choi, Steve, Clancy, Justin, Clark, Susan, Cooray, Asantha, Coppi, Gabriele, Corlett, John, Coulton, Will, Crawford, Thomas M., Crites, Abigail, Cukierman, Ari, Cyr-Racine, Francis-Yan, Dai, Wei-Ming, Daley, Cail, Dart, Eli, Daues, Gregorg, de Haan, Tijmen, Deaconu, Cosmin, Delabrouille, Jacques, Derylo, Greg, Devlin, Mark, Di Valentino, Eleonora, Dierickx, Marion, Dober, Brad, Doriese, Randy, Duff, Shannon, Dutcher, Daniel, Dvorkin, Cora, Dünner, Rolando, Eftekhari, Tarraneh, Eimer, Joseph, Bouhargani, Hamza El, Elleflot, Tucker, Emerson, Nick, Errard, Josquin, Essinger-Hileman, Thomas, Fabbian, Giulio, Fanfani, Valentina, Fasano, Alessandro, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey P., Flauger, Raphael, Flaugher, Brenna, Fraisse, Aurelien A., Frisch, Josef, Frolov, Andrei, Galitzki, Nicholas, Gallardo, Patricio A., Galli, Silvia, Ganga, Ken, Gerbino, Martina, Giannakopoulos, Christos, Gilchriese, Murdock, Gluscevic, Vera, Goeckner-Wald, Neil, Goldfinger, David, Green, Daniel, Grimes, Paul, Grin, Daniel, Grohs, Evan, Gualtieri, Riccardo, Guarino, Vic, Gudmundsson, Jon E., Gullett, Ian, Guns, Sam, Habib, Salman, Haller, Gunther, Halpern, Mark, Halverson, Nils W., Hanany, Shaul, Hand, Emma, Harrington, Kathleen, Hasegawa, Masaya, Hasselfield, Matthew, Hazumi, Masashi, Heitmann, Katrin, Henderson, Shawn, Hensley, Brandon, Herbst, Ryan, Hervias-Caimapo, Carlos, Hill, J. Colin, Hills, Richard, Hivon, Eric, Hlozek, Renée, Ho, Anna, Holder, Gil, Hollister, Matt, Holzapfel, William, Hood, John, Hotinli, Selim, Hryciuk, Alec, Hubmayr, Johannes, Huffenberger, Kevin M., Hui, Howard, nez, Roberto Ibá, Ibitoye, Ayodeji, Ikape, Margaret, Irwin, Kent, Jacobus, Cooper, Jeong, Oliver, Johnson, Bradley R., Johnstone, Doug, Jones, William C., Joseph, John, Jost, Baptiste, Kang, Jae Hwan, Kaplan, Ari, Karkare, Kirit S., Katayama, Nobuhiko, Keskitalo, Reijo, King, Cesiley, Kisner, Theodore, Klein, Matthias, Knox, Lloyd, Koopman, Brian J., Kosowsky, Arthur, Kovac, John, Kovetz, Ely D., Krolewski, Alex, Kubik, Donna, Kuhlmann, Steve, Kuo, Chao-Lin, Kusaka, Akito, Lähteenmäki, Anne, Lau, Kenny, Lawrence, Charles R., Lee, Adrian T., Legrand, Louis, Leitner, Matthaeus, Leloup, Clément, Lewis, Antony, Li, Dale, Linder, Eric, Liodakis, Ioannis, Liu, Jia, Long, Kevin, Louis, Thibaut, Loverde, Marilena, Lowry, Lindsay, Lu, Chunyu, Lubin, Phil, Ma, Yin-Zhe, Maccarone, Thomas, Madhavacheril, Mathew S., Maldonado, Felipe, Mantz, Adam, Marques, Gabriela, Matsuda, Frederick, Mauskopf, Philip, May, Jared, McCarrick, Heather, McCracken, Ken, McMahon, Jeffrey, Meerburg, P. Daniel, Melin, Jean-Baptiste, Menanteau, Felipe, Meyers, Joel, Millea, Marius, Miranda, Vivian, Mitchell, Don, Mohr, Joseph, Moncelsi, Lorenzo, Monzani, Maria Elena, Moshed, Magdy, Mroczkowski, Tony, Mukherjee, Suvodip, Münchmeyer, Moritz, Nagai, Daisuke, Nagarajappa, Chandan, Nagy, Johanna, Namikawa, Toshiya, Nati, Federico, Natoli, Tyler, Nerval, Simran, Newburgh, Laura, Nguyen, Hogan, Nichols, Erik, Nicola, Andrina, Niemack, Michael D., Nord, Brian, Norton, Tim, Novosad, Valentine, O'Brient, Roger, Omori, Yuuki, Orlando, Giorgio, Osherson, Benjamin, Osten, Rachel, Padin, Stephen, Paine, Scott, Partridge, Bruce, Patil, Sanjaykumar, Petravick, Don, Petroff, Matthew, Pierpaoli, Elena, Pilleux, Mauricio, Pogosian, Levon, Prabhu, Karthik, Pryke, Clement, Puglisi, Giuseppe, Racine, Benjamin, Raghunathan, Srinivasan, Rahlin, Alexandra, Raveri, Marco, Reese, Ben, Reichardt, Christian L., Remazeilles, Mathieu, Rizzieri, Arianna, Rocha, Graca, Roe, Natalie A., Rotermund, Kaja, Roy, Anirban, Ruhl, John E., Saba, Joe, Sailer, Noah, Salatino, Maria, Saliwanchik, Benjamin, Sapozhnikov, Leonid, Rao, Mayuri Sathyanarayana, Saunders, Lauren, Schaan, Emmanuel, Schillaci, Alessandro, Schmitt, Benjamin, Scott, Douglas, Sehgal, Neelima, Shandera, Sarah, Sherwin, Blake D., Shirokoff, Erik, Shiu, Corwin, Simon, Sara M., Singari, Baibhav, Slosar, Anze, Spergel, David, Germaine, Tyler St., Staggs, Suzanne T., Stark, Antony A., Starkman, Glenn D., Steinbach, Bryan, Stompor, Radek, Stoughton, Chris, Suzuki, Aritoki, Tajima, Osamu, Tandoi, Chris, Teply, Grant P., Thayer, Gregg, Thompson, Keith, Thorne, Ben, Timbie, Peter, Tomasi, Maurizio, Trendafilova, Cynthia, Tristram, Matthieu, Tucker, Carole, Tucker, Gregory, Umiltà, Caterina, van Engelen, Alexander, van Marrewijk, Joshiwa, Vavagiakis, Eve M., Vergès, Clara, Vieira, Joaquin D., Vieregg, Abigail G., Wagoner, Kasey, Wallisch, Benjamin, Wang, Gensheng, Wang, Guo-Jian, Watson, Scott, Watts, Duncan, Weaver, Chris, Wenzl, Lukas, Westbrook, Ben, White, Martin, Whitehorn, Nathan, Wiedlea, Andrew, Williams, Paul, Wilson, Robert, Winch, Harrison, Wollack, Edward J., Wu, W. L. Kimmy, Xu, Zhilei, Yefremenko, Volodymyr G., Yu, Cyndia, Zegeye, David, Zivick, Jeff, and Zonca, Andrea

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, General Relativity and Quantum Cosmology, High Energy Physics - Experiment, High Energy Physics - Phenomenology
Abstract

This Snowmass 2021 White Paper describes the Cosmic Microwave Background Stage 4 project CMB-S4, which is designed to cross critical thresholds in our understanding of the origin and evolution of the Universe, from the highest energies at the dawn of time through the growth of structure to the present day. We provide an overview of the science case, the technical design, and project plan., Comment: Contribution to Snowmass 2021. arXiv admin note: substantial text overlap with arXiv:1908.01062, arXiv:1907.04473

Published
2022

6. CMB-S4: Forecasting Constraints on Primordial Gravitational Waves

Author

Abazajian, Kevork, Addison, Graeme E, Adshead, Peter, Ahmed, Zeeshan, Akerib, Daniel, Ali, Aamir, Allen, Steven W, Alonso, David, Alvarez, Marcelo, Amin, Mustafa A, Anderson, Adam, Arnold, Kam S, Ashton, Peter, Baccigalupi, Carlo, Bard, Debbie, Barkats, Denis, Barron, Darcy, Barry, Peter S, Bartlett, James G, Thakur, Ritoban Basu, Battaglia, Nicholas, Bean, Rachel, Bebek, Chris, Bender, Amy N, Benson, Bradford A, Bianchini, Federico, Bischoff, Colin A, Bleem, Lindsey, Bock, James J, Bocquet, Sebastian, Boddy, Kimberly K, Bond, J Richard, Borrill, Julian, Bouchet, François R, Brinckmann, Thejs, Brown, Michael L, Bryan, Sean, Buza, Victor, Byrum, Karen, Caimapo, Carlos Hervias, Calabrese, Erminia, Calafut, Victoria, Caldwell, Robert, Carlstrom, John E, Carron, Julien, Cecil, Thomas, Challinor, Anthony, Chang, Clarence L, Chinone, Yuji, Cho, Hsiao-Mei Sherry, Cooray, Asantha, Coulton, Will, Crawford, Thomas M, Crites, Abigail, Cukierman, Ari, Cyr-Racine, Francis-Yan, de Haan, Tijmen, Delabrouille, Jacques, Devlin, Mark, Di Valentino, Eleonora, Dierickx, Marion, Dobbs, Matt, Duff, Shannon, Dvorkin, Cora, Eimer, Joseph, Elleflot, Tucker, Errard, Josquin, Essinger-Hileman, Thomas, Fabbian, Giulio, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey P, Flauger, Raphael, Flaugher, Brenna, Fraisse, Aurelien A, Frolov, Andrei, Galitzki, Nicholas, Gallardo, Patricio A, Galli, Silvia, Ganga, Ken, Gerbino, Martina, Gluscevic, Vera, Goeckner-Wald, Neil, Green, Daniel, Grin, Daniel, Grohs, Evan, Gualtieri, Riccardo, Gudmundsson, Jon E, Gullett, Ian, Gupta, Nikhel, Habib, Salman, Halpern, Mark, Halverson, Nils W, Hanany, Shaul, Harrington, Kathleen, Hasegawa, Masaya, Hasselfield, Matthew, Hazumi, Masashi, Heitmann, Katrin, and Henderson, Shawn

Subjects
Particle and High Energy Physics, Physical Sciences, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics, Space sciences
Abstract

CMB-S4 - the next-generation ground-based cosmic microwave background (CMB) experiment - is set to significantly advance the sensitivity of CMB measurements and enhance our understanding of the origin and evolution of the universe. Among the science cases pursued with CMB-S4, the quest for detecting primordial gravitational waves is a central driver of the experimental design. This work details the development of a forecasting framework that includes a power-spectrum-based semianalytic projection tool, targeted explicitly toward optimizing constraints on the tensor-to-scalar ratio, r, in the presence of Galactic foregrounds and gravitational lensing of the CMB. This framework is unique in its direct use of information from the achieved performance of current Stage 2-3 CMB experiments to robustly forecast the science reach of upcoming CMB-polarization endeavors. The methodology allows for rapid iteration over experimental configurations and offers a flexible way to optimize the design of future experiments, given a desired scientific goal. To form a closed-loop process, we couple this semianalytic tool with map-based validation studies, which allow for the injection of additional complexity and verification of our forecasts with several independent analysis methods. We document multiple rounds of forecasts for CMB-S4 using this process and the resulting establishment of the current reference design of the primordial gravitational-wave component of the Stage-4 experiment, optimized to achieve our science goals of detecting primordial gravitational waves for r > 0.003 at greater than 5σ, or in the absence of a detection, of reaching an upper limit of r < 0.001 at 95% CL.

Published
2022

7. Design and experimental investigation of a planar metamaterial Silicon based lenslet

Author

Gascard, Thomas, Pisano, Giampaolo, Doyle, Simon, Shitvov, Alexey, Austermann, Jason, Beall, James, Hubmayr, Johannes, Raymond, Benjamin, Halverson, Nils, Jaehnig, Gregory, McKenney, Christopher M., and Suzuki, Aritoki

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

The next generations of ground-based cosmic microwave background experiments will require polarisation sensitive, multichroic pixels of large focal planes comprising several thousand detectors operating at the photon noise limit. One approach to achieve this goal is to couple light from the telescope to a polarisation sensitive antenna structure connected to a superconducting diplexer network where the desired frequency bands are filtered before being fed to individual ultra-sensitive detectors such as Transition Edge Sensors. Traditionally, arrays constituted of horn antennas, planar phased antennas or anti-reflection coated micro-lenses have been placed in front of planar antenna structures to achieve the gain required to couple efficiently to the telescope optics. In this paper are presented the design concept and a preliminary analysis of the measured performances of a phase-engineered metamaterial flat-lenslet. The flat lens design is inherently matched to free space, avoiding the necessity of an anti-reflection coating layer. It can be fabricated lithographically, making scaling to large format arrays relatively simple. Furthermore, this technology is compatible with the fabrication process required for the production of large-format lumped element kinetic inductance detector arrays which have already demonstrated the required sensitivity along with multiplexing ratios of order 1000 detectors/channel., Comment: 10 pages, 8 figures, published in SPIE Proceedings Volume 11453, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X (https://nanolithography.spiedigitallibrary.org/conference-proceedings-of-spie/11453/1145307/Design-and-experimental-investigation-of-a-planar-metamaterial-silicon-based/10.1117/12.2562692.full)

Published
2021
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8. Detector fabrication development for the LiteBIRD satellite mission

Author

Westbrook, Benjamin, Raum, Christopher, Beckman, Shawn, Lee, Adrian T., Farias, Nicole, Sasse, Trevor, Suzuki, Aritoki, Kane, Elijah, Austermann, Jason E., Beall, James A, Duff, Shannon M., Hubmayr, Johannes, Hilton, Gene C., Van Lanen, Jeff, Vissers, Michael R., Link, Michael R., Jaehnig, Greg, Halverson, Nils, Ghinga, Tommaso, Stever, Samantha, Minami, Yuto, Thompson, Keith L., Russell, Megan, Arnold, Kam, Siebert, Joseph, Silva-Feaver, Maximiliano, and Group, the LiteBIRD Joint Study

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

LiteBIRD is a JAXA-led strategic Large-Class satellite mission designed to measure the polarization of the cosmic microwave background and cosmic foregrounds from 34 to 448 GHz across the entire sky from L2 in the late 2020's. The primary focus of the mission is to measure primordially generated B-mode polarization at large angular scales. Beyond its primary scientific objective LiteBIRD will generate a data-set capable of probing a number of scientific inquiries including the sum of neutrino masses. The primary responsibility of United States will be to fabricate the three flight model focal plane units for the mission. The design and fabrication of these focal plane units is driven by heritage from ground based experiments and will include both lenslet-coupled sinuous antenna pixels and horn-coupled orthomode transducer pixels. The experiment will have three optical telescopes called the low frequency telescope, mid frequency telescope, and high frequency telescope each of which covers a portion of the mission's frequency range. JAXA is responsible for the construction of the low frequency telescope and the European Consortium is responsible for the mid- and high- frequency telescopes. The broad frequency coverage and low optical loading conditions, made possible by the space environment, require development and adaptation of detector technology recently deployed by other cosmic microwave background experiments. This design, fabrication, and characterization will take place at UC Berkeley, NIST, Stanford, and Colorado University, Boulder. We present the current status of the US deliverables to the LiteBIRD mission., Comment: SPIE, Cosmology, LiteBIRD, Detectors, TES, Bolometers, Inflation, Sinuous Antenna, Horn Coupled, DfMUX

Published
2021

9. Planar Silicon Metamaterial Lenslet Arrays for Millimeter-wavelength Imaging

Author

McKenney, Christopher M., Austermann, Jason E., Beall, James A., Halverson, Nils W., Hubmayr, Johannes, Jaehnig, Gregory, Pisano, Giampaolo, Stevenson, Sarah A., Suzuki, Aritoki, and Thompson, Jonathan A.

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

Large imaging arrays of detectors at millimeter and submillimeter wavelengths have applications that include measurements of the faint polarization signal in the Cosmic Microwave Background (CMB), and submillimeter astrophysics. We are developing planar lenslet arrays for millimeter-wavelength imaging using metamaterials microlithically fabricated using silicon wafers. This metamaterial technology has many potential advantages compared to conventional hemispherical lenslet arrays, including high precision and homogeneity, planar integrated anti-reflection layers, and a coefficient of thermal expansion matched to the silicon detector wafer. Here we describe the design process for a gradient-index (GRIN) metamaterial lenslet using metal-mesh patterned on silicon and a combination of metal-mesh and etched-hole metamaterial anti-reflection layers. We optimize the design using a bulk-material model to rapidly simulate and iterate on the lenslet design. We fabricated prototype GRIN metamaterial lenslet array and mounted it on a Polarbear/Simons Array 90/150~GHz band transition edge sensor (TES) bolometer detector array with sinuous planar antennas. Beam measurements of a prototype lenslet array agree reasonably well with the model simulations. We plan to further optimize the design and combine it with a broadband anti-reflection coating to achieve operation over 70--350~GHz bandwidth., Comment: Presented at SPIE Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X, December 13-18, 2020

Published
2020

10. CMB-S4: Forecasting Constraints on Primordial Gravitational Waves

Author

Collaboration, CMB-S4, Abazajian, Kevork, Addison, Graeme E., Adshead, Peter, Ahmed, Zeeshan, Akerib, Daniel, Ali, Aamir, Allen, Steven W., Alonso, David, Alvarez, Marcelo, Amin, Mustafa A., Anderson, Adam, Arnold, Kam S., Ashton, Peter, Baccigalupi, Carlo, Bard, Debbie, Barkats, Denis, Barron, Darcy, Barry, Peter S., Bartlett, James G., Thakur, Ritoban Basu, Battaglia, Nicholas, Bean, Rachel, Bebek, Chris, Bender, Amy N., Benson, Bradford A., Bianchini, Federico, Bischoff, Colin A., Bleem, Lindsey, Bock, James J., Bocquet, Sebastian, Boddy, Kimberly K., Bond, J. Richard, Borrill, Julian, Bouchet, François R., Brinckmann, Thejs, Brown, Michael L., Bryan, Sean, Buza, Victor, Byrum, Karen, Caimapo, Carlos Hervias, Calabrese, Erminia, Calafut, Victoria, Caldwell, Robert, Carlstrom, John E., Carron, Julien, Cecil, Thomas, Challinor, Anthony, Chang, Clarence L., Chinone, Yuji, Cho, Hsiao-Mei Sherry, Cooray, Asantha, Coulton, Will, Crawford, Thomas M., Crites, Abigail, Cukierman, Ari, Cyr-Racine, Francis-Yan, de Haan, Tijmen, Delabrouille, Jacques, Devlin, Mark, Di Valentino, Eleonora, Dierickx, Marion, Dobbs, Matt, Duff, Shannon, Dunkley, Jo, Dvorkin, Cora, Eimer, Joseph, Elleflot, Tucker, Errard, Josquin, Essinger-Hileman, Thomas, Fabbian, Giulio, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey P., Flauger, Raphael, Flaugher, Brenna, Fraisse, Aurelien A., Frolov, Andrei, Galitzki, Nicholas, Gallardo, Patricio A., Galli, Silvia, Ganga, Ken, Gerbino, Martina, Gluscevic, Vera, Goeckner-Wald, Neil, Green, Daniel, Grin, Daniel, Grohs, Evan, Gualtieri, Riccardo, Gudmundsson, Jon E., Gullett, Ian, Gupta, Nikhel, Habib, Salman, Halpern, Mark, Halverson, Nils W., Hanany, Shaul, Harrington, Kathleen, Hasegawa, Masaya, Hasselfield, Matthew, Hazumi, Masashi, Heitmann, Katrin, Henderson, Shawn, Hensley, Brandon, Hill, Charles, Hill, J. Colin, Hlozek, Renée, Ho, Shuay-Pwu Patty, Hoang, Thuong, Holder, Gil, Holzapfel, William, Hood, John, Hubmayr, Johannes, Huffenberger, Kevin M., Hui, Howard, Irwin, Kent, Jeong, Oliver, Johnson, Bradley R., Jones, William C., Kang, Jae Hwan, Karkare, Kirit S., Katayama, Nobuhiko, Keskitalo, Reijo, Kisner, Theodore, Knox, Lloyd, Koopman, Brian J., Kosowsky, Arthur, Kovac, John, Kovetz, Ely D., Kuhlmann, Steve, Kuo, Chao-lin, Kusaka, Akito, Lähteenmäki, Anne, Lawrence, Charles R., Lee, Adrian T., Lewis, Antony, Li, Dale, Linder, Eric, Loverde, Marilena, Lowitz, Amy, Lubin, Phil, Madhavacheril, Mathew S., Mantz, Adam, Marques, Gabriela, Matsuda, Frederick, Mauskopf, Philip, McCarrick, Heather, McMahon, Jeffrey, Meerburg, P. Daniel, Melin, Jean-Baptiste, Menanteau, Felipe, Meyers, Joel, Millea, Marius, Mohr, Joseph, Moncelsi, Lorenzo, Monzani, Maria, Mroczkowski, Tony, Mukherjee, Suvodip, Nagy, Johanna, Namikawa, Toshiya, Nati, Federico, Natoli, Tyler, Newburgh, Laura, Niemack, Michael D., Nishino, Haruki, Nord, Brian, Novosad, Valentine, O'Brient, Roger, Padin, Stephen, Palladino, Steven, Partridge, Bruce, Petravick, Don, Pierpaoli, Elena, Pogosian, Levon, Prabhu, Karthik, Pryke, Clement, Puglisi, Giuseppe, Racine, Benjamin, Rahlin, Alexandra, Rao, Mayuri Sathyanarayana, Raveri, Marco, Reichardt, Christian L., Remazeilles, Mathieu, Rocha, Graca, Roe, Natalie A., Roy, Anirban, Ruhl, John E., Salatino, Maria, Saliwanchik, Benjamin, Schaan, Emmanuel, Schillaci, Alessandro, Schmitt, Benjamin, Schmittfull, Marcel M., Scott, Douglas, Sehgal, Neelima, Shandera, Sarah, Sherwin, Blake D., Shirokoff, Erik, Simon, Sara M., Slosar, Anze, Spergel, David, Germaine, Tyler St., Staggs, Suzanne T., Stark, Antony, Starkman, Glenn D., Stompor, Radek, Stoughton, Chris, Suzuki, Aritoki, Tajima, Osamu, Teply, Grant P., Thompson, Keith, Thorne, Ben, Timbie, Peter, Tomasi, Maurizio, Tristram, Matthieu, Tucker, Gregory, Umiltà, Caterina, van Engelen, Alexander, Vavagiakis, Eve M., Vieira, Joaquin D., Vieregg, Abigail G., Wagoner, Kasey, Wallisch, Benjamin, Wang, Gensheng, Watson, Scott, Westbrook, Ben, Whitehorn, Nathan, Wollack, Edward J., Wu, W. L. Kimmy, Xu, Zhilei, Yang, H. Y. Eric, Yasini, Siavash, Yefremenko, Volodymyr G., Yoon, Ki Won, Young, Edward, Yu, Cyndia, and Zonca, Andrea

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

CMB-S4---the next-generation ground-based cosmic microwave background (CMB) experiment---is set to significantly advance the sensitivity of CMB measurements and enhance our understanding of the origin and evolution of the Universe, from the highest energies at the dawn of time through the growth of structure to the present day. Among the science cases pursued with CMB-S4, the quest for detecting primordial gravitational waves is a central driver of the experimental design. This work details the development of a forecasting framework that includes a power-spectrum-based semi-analytic projection tool, targeted explicitly towards optimizing constraints on the tensor-to-scalar ratio, $r$, in the presence of Galactic foregrounds and gravitational lensing of the CMB. This framework is unique in its direct use of information from the achieved performance of current Stage 2--3 CMB experiments to robustly forecast the science reach of upcoming CMB-polarization endeavors. The methodology allows for rapid iteration over experimental configurations and offers a flexible way to optimize the design of future experiments given a desired scientific goal. To form a closed-loop process, we couple this semi-analytic tool with map-based validation studies, which allow for the injection of additional complexity and verification of our forecasts with several independent analysis methods. We document multiple rounds of forecasts for CMB-S4 using this process and the resulting establishment of the current reference design of the primordial gravitational-wave component of the Stage-4 experiment, optimized to achieve our science goals of detecting primordial gravitational waves for $r > 0.003$ at greater than $5\sigma$, or, in the absence of a detection, of reaching an upper limit of $r < 0.001$ at $95\%$ CL., Comment: 24 pages, 8 figures, 9 tables, submitted to ApJ. arXiv admin note: text overlap with arXiv:1907.04473

Published
2020
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11. CMB-S4 Decadal Survey APC White Paper

Author

Abazajian, Kevork, Addison, Graeme, Adshead, Peter, Ahmed, Zeeshan, Allen, Steven W., Alonso, David, Alvarez, Marcelo, Amin, Mustafa A., Anderson, Adam, Arnold, Kam S., Baccigalupi, Carlo, Bailey, Kathy, Barkats, Denis, Barron, Darcy, Barry, Peter S., Bartlett, James G., Thakur, Ritoban Basu, Battaglia, Nicholas, Baxter, Eric, Bean, Rachel, Bebek, Chris, Bender, Amy N., Benson, Bradford A., Berger, Edo, Bhimani, Sanah, Bischoff, Colin A., Bleem, Lindsey, Bock, James J., Bocquet, Sebastian, Boddy, Kimberly, Bonato, Matteo, Bond, J. Richard, Borrill, Julian, Bouchet, François R., Brown, Michael L., Bryan, Sean, Burkhart, Blakesley, Buza, Victor, Byrum, Karen, Calabrese, Erminia, Calafut, Victoria, Caldwell, Robert, Carlstrom, John E., Carron, Julien, Cecil, Thomas, Challinor, Anthony, Chang, Clarence L., Chinone, Yuji, Cho, Hsiao-Mei Sherry, Cooray, Asantha, Crawford, Thomas M., Crites, Abigail, Cukierman, Ari, Cyr-Racine, Francis-Yan, de Haan, Tijmen, de Zotti, Gianfranco, Delabrouille, Jacques, Demarteau, Marcel, Devlin, Mark, Di Valentino, Eleonora, Dobbs, Matt, Duff, Shannon, Duivenvoorden, Adriaan, Dvorkin, Cora, Edwards, William, Eimer, Joseph, Errard, Josquin, Essinger-Hileman, Thomas, Fabbian, Giulio, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey P., Flauger, Raphael, Flaugher, Brenna, Fraisse, Aurelien A., Frolov, Andrei, Galitzki, Nicholas, Galli, Silvia, Ganga, Ken, Gerbino, Martina, Gilchriese, Murdock, Gluscevic, Vera, Green, Daniel, Grin, Daniel, Grohs, Evan, Gualtieri, Riccardo, Guarino, Victor, Gudmundsson, Jon E., Habib, Salman, Haller, Gunther, Halpern, Mark, Halverson, Nils W., Hanany, Shaul, Harrington, Kathleen, Hasegawa, Masaya, Hasselfield, Matthew, Hazumi, Masashi, Heitmann, Katrin, Henderson, Shawn, Henning, Jason W., Hill, J. Colin, Hlozek, Renée, Holder, Gil, Holzapfel, William, Hubmayr, Johannes, Huffenberger, Kevin M., Huffer, Michael, Hui, Howard, Irwin, Kent, Johnson, Bradley R., Johnstone, Doug, Jones, William C., Karkare, Kirit, Katayama, Nobuhiko, Kerby, James, Kernovsky, Sarah, Keskitalo, Reijo, Kisner, Theodore, Knox, Lloyd, Kosowsky, Arthur, Kovac, John, Kovetz, Ely D., Kuhlmann, Steve, Kuo, Chao-lin, Kurita, Nadine, Kusaka, Akito, Lahteenmaki, Anne, Lawrence, Charles R., Lee, Adrian T., Lewis, Antony, Li, Dale, Linder, Eric, Loverde, Marilena, Lowitz, Amy, Madhavacheril, Mathew S., Mantz, Adam, Matsuda, Frederick, Mauskopf, Philip, McMahon, Jeff, Meerburg, P. Daniel, Melin, Jean-Baptiste, Meyers, Joel, Millea, Marius, Mohr, Joseph, Moncelsi, Lorenzo, Mroczkowski, Tony, Mukherjee, Suvodip, Münchmeyer, Moritz, Nagai, Daisuke, Nagy, Johanna, Namikawa, Toshiya, Nati, Federico, Natoli, Tyler, Negrello, Mattia, Newburgh, Laura, Niemack, Michael D., Nishino, Haruki, Nordby, Martin, Novosad, Valentine, O'Connor, Paul, Obied, Georges, Padin, Stephen, Pandey, Shivam, Partridge, Bruce, Pierpaoli, Elena, Pogosian, Levon, Pryke, Clement, Puglisi, Giuseppe, Racine, Benjamin, Raghunathan, Srinivasan, Rahlin, Alexandra, Rajagopalan, Srini, Raveri, Marco, Reichanadter, Mark, Reichardt, Christian L., Remazeilles, Mathieu, Rocha, Graca, Roe, Natalie A., Roy, Anirban, Ruhl, John, Salatino, Maria, Saliwanchik, Benjamin, Schaan, Emmanuel, Schillaci, Alessandro, Schmittfull, Marcel M., Scott, Douglas, Sehgal, Neelima, Shandera, Sarah, Sheehy, Christopher, Sherwin, Blake D., Shirokoff, Erik, Simon, Sara M., Slosar, Anze, Somerville, Rachel, Staggs, Suzanne T., Stark, Antony, Stompor, Radek, Story, Kyle T., Stoughton, Chris, Suzuki, Aritoki, Tajima, Osamu, Teply, Grant P., Thompson, Keith, Timbie, Peter, Tomasi, Maurizio, Treu, Jesse I., Tristram, Matthieu, Tucker, Gregory, Umiltà, Caterina, van Engelen, Alexander, Vieira, Joaquin D., Vieregg, Abigail G., Vogelsberger, Mark, Wang, Gensheng, Watson, Scott, White, Martin, Whitehorn, Nathan, Wollack, Edward J., Wu, W. L. Kimmy, Xu, Zhilei, Yasini, Siavash, Yeck, James, Yoon, Ki Won, Young, Edward, and Zonca, Andrea

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

We provide an overview of the science case, instrument configuration and project plan for the next-generation ground-based cosmic microwave background experiment CMB-S4, for consideration by the 2020 Decadal Survey., Comment: Project White Paper submitted to the 2020 Decadal Survey, 10 pages plus references. arXiv admin note: substantial text overlap with arXiv:1907.04473

Published
2019

12. CMB-S4 Science Case, Reference Design, and Project Plan

Author

Abazajian, Kevork, Addison, Graeme, Adshead, Peter, Ahmed, Zeeshan, Allen, Steven W., Alonso, David, Alvarez, Marcelo, Anderson, Adam, Arnold, Kam S., Baccigalupi, Carlo, Bailey, Kathy, Barkats, Denis, Barron, Darcy, Barry, Peter S., Bartlett, James G., Thakur, Ritoban Basu, Battaglia, Nicholas, Baxter, Eric, Bean, Rachel, Bebek, Chris, Bender, Amy N., Benson, Bradford A., Berger, Edo, Bhimani, Sanah, Bischoff, Colin A., Bleem, Lindsey, Bocquet, Sebastian, Boddy, Kimberly, Bonato, Matteo, Bond, J. Richard, Borrill, Julian, Bouchet, François R., Brown, Michael L., Bryan, Sean, Burkhart, Blakesley, Buza, Victor, Byrum, Karen, Calabrese, Erminia, Calafut, Victoria, Caldwell, Robert, Carlstrom, John E., Carron, Julien, Cecil, Thomas, Challinor, Anthony, Chang, Clarence L., Chinone, Yuji, Cho, Hsiao-Mei Sherry, Cooray, Asantha, Crawford, Thomas M., Crites, Abigail, Cukierman, Ari, Cyr-Racine, Francis-Yan, de Haan, Tijmen, de Zotti, Gianfranco, Delabrouille, Jacques, Demarteau, Marcel, Devlin, Mark, Di Valentino, Eleonora, Dobbs, Matt, Duff, Shannon, Duivenvoorden, Adriaan, Dvorkin, Cora, Edwards, William, Eimer, Joseph, Errard, Josquin, Essinger-Hileman, Thomas, Fabbian, Giulio, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey P., Flauger, Raphael, Flaugher, Brenna, Fraisse, Aurelien A., Frolov, Andrei, Galitzki, Nicholas, Galli, Silvia, Ganga, Ken, Gerbino, Martina, Gilchriese, Murdock, Gluscevic, Vera, Green, Daniel, Grin, Daniel, Grohs, Evan, Gualtieri, Riccardo, Guarino, Victor, Gudmundsson, Jon E., Habib, Salman, Haller, Gunther, Halpern, Mark, Halverson, Nils W., Hanany, Shaul, Harrington, Kathleen, Hasegawa, Masaya, Hasselfield, Matthew, Hazumi, Masashi, Heitmann, Katrin, Henderson, Shawn, Henning, Jason W., Hill, J. Colin, Hlozek, Renée, Holder, Gil, Holzapfel, William, Hubmayr, Johannes, Huffenberger, Kevin M., Huffer, Michael, Hui, Howard, Irwin, Kent, Johnson, Bradley R., Johnstone, Doug, Jones, William C., Karkare, Kirit, Katayama, Nobuhiko, Kerby, James, Kernovsky, Sarah, Keskitalo, Reijo, Kisner, Theodore, Knox, Lloyd, Kosowsky, Arthur, Kovac, John, Kovetz, Ely D., Kuhlmann, Steve, Kuo, Chao-lin, Kurita, Nadine, Kusaka, Akito, Lahteenmaki, Anne, Lawrence, Charles R., Lee, Adrian T., Lewis, Antony, Li, Dale, Linder, Eric, Loverde, Marilena, Lowitz, Amy, Madhavacheril, Mathew S., Mantz, Adam, Matsuda, Frederick, Mauskopf, Philip, McMahon, Jeff, McQuinn, Matthew, Meerburg, P. Daniel, Melin, Jean-Baptiste, Meyers, Joel, Millea, Marius, Mohr, Joseph, Moncelsi, Lorenzo, Mroczkowski, Tony, Mukherjee, Suvodip, Münchmeyer, Moritz, Nagai, Daisuke, Nagy, Johanna, Namikawa, Toshiya, Nati, Federico, Natoli, Tyler, Negrello, Mattia, Newburgh, Laura, Niemack, Michael D., Nishino, Haruki, Nordby, Martin, Novosad, Valentine, O'Connor, Paul, Obied, Georges, Padin, Stephen, Pandey, Shivam, Partridge, Bruce, Pierpaoli, Elena, Pogosian, Levon, Pryke, Clement, Puglisi, Giuseppe, Racine, Benjamin, Raghunathan, Srinivasan, Rahlin, Alexandra, Rajagopalan, Srini, Raveri, Marco, Reichanadter, Mark, Reichardt, Christian L., Remazeilles, Mathieu, Rocha, Graca, Roe, Natalie A., Roy, Anirban, Ruhl, John, Salatino, Maria, Saliwanchik, Benjamin, Schaan, Emmanuel, Schillaci, Alessandro, Schmittfull, Marcel M., Scott, Douglas, Sehgal, Neelima, Shandera, Sarah, Sheehy, Christopher, Sherwin, Blake D., Shirokoff, Erik, Simon, Sara M., Slosar, Anze, Somerville, Rachel, Spergel, David, Staggs, Suzanne T., Stark, Antony, Stompor, Radek, Story, Kyle T., Stoughton, Chris, Suzuki, Aritoki, Tajima, Osamu, Teply, Grant P., Thompson, Keith, Timbie, Peter, Tomasi, Maurizio, Treu, Jesse I., Tristram, Matthieu, Tucker, Gregory, Umiltà, Caterina, van Engelen, Alexander, Vieira, Joaquin D., Vieregg, Abigail G., Vogelsberger, Mark, Wang, Gensheng, Watson, Scott, White, Martin, Whitehorn, Nathan, Wollack, Edward J., Wu, W. L. Kimmy, Xu, Zhilei, Yasini, Siavash, Yeck, James, Yoon, Ki Won, Young, Edward, and Zonca, Andrea

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies, High Energy Physics - Experiment
Abstract

We present the science case, reference design, and project plan for the Stage-4 ground-based cosmic microwave background experiment CMB-S4., Comment: 287 pages, 82 figures

Published
2019

13. CMB-S4: Forecasting Constraints on Primordial Gravitational Waves

Author

Collaboration, The CMB-S4, :, Abazajian, Kevork, Addison, Graeme E, Adshead, Peter, Ahmed, Zeeshan, Akerib, Daniel, Ali, Aamir, Allen, Steven W, Alonso, David, Alvarez, Marcelo, Amin, Mustafa A, Anderson, Adam, Arnold, Kam S, Ashton, Peter, Baccigalupi, Carlo, Bard, Debbie, Barkats, Denis, Barron, Darcy, Barry, Peter S, Bartlett, James G, Thakur, Ritoban Basu, Battaglia, Nicholas, Bean, Rachel, Bebek, Chris, Bender, Amy N, Benson, Bradford A, Bianchini, Federico, Bischoff, Colin A, Bleem, Lindsey, Bock, James J, Bocquet, Sebastian, Boddy, Kimberly K, Bond, J Richard, Borrill, Julian, Bouchet, François R, Brinckmann, Thejs, Brown, Michael L, Bryan, Sean, Buza, Victor, Byrum, Karen, Caimapo, Carlos Hervias, Calabrese, Erminia, Calafut, Victoria, Caldwell, Robert, Carlstrom, John E, Carron, Julien, Cecil, Thomas, Challinor, Anthony, Chang, Clarence L, Chinone, Yuji, Cho, Hsiao-Mei Sherry, Cooray, Asantha, Coulton, Will, Crawford, Thomas M, Crites, Abigail, Cukierman, Ari, Cyr-Racine, Francis-Yan, de Haan, Tijmen, Delabrouille, Jacques, Devlin, Mark, Di Valentino, Eleonora, Dierickx, Marion, Dobbs, Matt, Duff, Shannon, Dunkley, Jo, Dvorkin, Cora, Eimer, Joseph, Elleflot, Tucker, Errard, Josquin, Essinger-Hileman, Thomas, Fabbian, Giulio, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey P, Flauger, Raphael, Flaugher, Brenna, Fraisse, Aurelien A, Frolov, Andrei, Galitzki, Nicholas, Gallardo, Patricio A, Galli, Silvia, Ganga, Ken, Gerbino, Martina, Gluscevic, Vera, Goeckner-Wald, Neil, Green, Daniel, Grin, Daniel, Grohs, Evan, Gualtieri, Riccardo, Gudmundsson, Jon E, Gullett, Ian, Gupta, Nikhel, Habib, Salman, Halpern, Mark, Halverson, Nils W, Hanany, Shaul, Harrington, Kathleen, Hasegawa, Masaya, and Hasselfield, Matthew

Subjects
astro-ph.CO
Abstract

CMB-S4---the next-generation ground-based cosmic microwave background (CMB)experiment---is set to significantly advance the sensitivity of CMBmeasurements and enhance our understanding of the origin and evolution of theUniverse, from the highest energies at the dawn of time through the growth ofstructure to the present day. Among the science cases pursued with CMB-S4, thequest for detecting primordial gravitational waves is a central driver of theexperimental design. This work details the development of a forecastingframework that includes a power-spectrum-based semi-analytic projection tool,targeted explicitly towards optimizing constraints on the tensor-to-scalarratio, $r$, in the presence of Galactic foregrounds and gravitational lensingof the CMB. This framework is unique in its direct use of information from theachieved performance of current Stage 2--3 CMB experiments to robustly forecastthe science reach of upcoming CMB-polarization endeavors. The methodologyallows for rapid iteration over experimental configurations and offers aflexible way to optimize the design of future experiments given a desiredscientific goal. To form a closed-loop process, we couple this semi-analytictool with map-based validation studies, which allow for the injection ofadditional complexity and verification of our forecasts with severalindependent analysis methods. We document multiple rounds of forecasts forCMB-S4 using this process and the resulting establishment of the currentreference design of the primordial gravitational-wave component of the Stage-4experiment, optimized to achieve our science goals of detecting primordialgravitational waves for $r > 0.003$ at greater than $5\sigma$, or, in theabsence of a detection, of reaching an upper limit of $r < 0.001$ at $95\%$ CL.

Published
2020

14. Development of Flat Silicon-Based Mesh Lens Arrays for Millimeter and Sub-millimeter Wave Astronomy

Author

Pisano, Giampaolo, Austermann, Jason, Beall, James, Halverson, Nils, Hubmayr, Johannes, Jaehnig, Gregory, McKenney, Christopher M, Raymond, Benjamin, and Suzuki, Aritoki

Subjects
Physical Sciences, Classical Physics, Condensed Matter Physics, Cosmic microwave background, Focal plane arrays, Millimeter waves, Optical coupling, Quasioptical systems, Mathematical Physics, General Physics, Classical physics, Condensed matter physics
Abstract

The high sensitivity requirements set by future cosmic microwave background instruments are pushing the current technologies to produce highly performant focal plane arrays with thousands of detectors. The coupling of the detectors to the telescope optics is a challenging task. Current implemented solutions include phased-array antenna-coupled detectors, platelet horn arrays, and lenslet-coupled planar antennas. There are also recent developments of flat graded-index lenses based on etched silicon. However, there are strong requirements in terms of electromagnetic performance, such as coupling efficiency and bandwidth, as well as requirements in terms of easy manufacturing and scalability, and it is very challenging to meet all these requirements with one of the above solutions. Here, we present a novel approach for producing flat metal-mesh lenslet arrays based on devices previously realized using the mesh-filter technology. We have now adapted the polypropylene-based mesh lens design to silicon substrates, thus providing a good mechanical match to the silicon-based detector arrays. The measured performance of prototype pixels operating at millimeter wavelengths is presented.

Published
2020

15. Optical Characterization of the SPT-3G Focal Plane

Author

Pan, Zhaodi, Ade, Peter, Ahmed, Zeeshan, Adam, Anderson, Austermann, Jason, Avva, Jessica, Thakur, Ritoban Basu, Amy, Bender, Benson, Bradford, Carlstrom, John, Carter, Faustin, Cecil, Thomas, Chang, Clarence, Cliche, Jean-Francois, Cukierman, Ariel, Denison, Edward, de Haan, Tijmen, Ding, Junjia, Dobbs, Matt, Dutcher, Daniel, Everett, Wendeline, Foster, Allen, Gannon, Renae, Gilbert, Adam, Groh, John, Halverson, Nils, Harke-Horsemann, Angelina, Harrington, Nicholas, Henning, Jaosn, Hilton, Gene, Holzapfel, William, Huang, Nicholas, Irwin, Kent, Jeong, Oliver, Jonas, Michalle, Khaire, Trupti, Kofman, Anna, Korman, Milo, Kubik, Donna, Kuhlmann, Steve, Kuo, Chaolin, Lee, Adrian, Lowitz, Amy, Meyer, Stephan, Michalik, Daniel, Montgomery, Joshua, Nadolski, Andrew, Natoli, Tyler, Nguyen, Hogan, Noble, Gavin, Novosad, Valentyn, Padin, Stephan, Pearson, John, Posada, Chrystian, Rahlin, Alexandra, Ruhl, John, Saunders, Lauren, Sayre, James, Shirley, Ian, Shirokoff, Erik, Smecher, Graeme, Sobrin, Joshua, Stark, Antony, Story, Kyle, Suzuki, Aritoki, Tang, Qingyang, Thompson, Keith, Tucker, Carole, Vale, Leila, Vanderlinde, Keith, Vieira, Joaquin, Wang, Gensheng, Whitehorn, Nathan, Yefremenko, Volodymyr, Yoon, Ki Won, and Young, Matt

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

The third-generation South Pole Telescope camera is designed to measure the cosmic microwave background across three frequency bands (95, 150 and 220 GHz) with ~16,000 transition-edge sensor (TES) bolometers. Each multichroic pixel on a detector wafer has a broadband sinuous antenna that couples power to six TESs, one for each of the three observing bands and both polarization directions, via lumped element filters. Ten detector wafers populate the focal plane, which is coupled to the sky via a large-aperture optical system. Here we present the frequency band characterization with Fourier transform spectroscopy, measurements of optical time constants, beam properties, and optical and polarization efficiencies of the focal plane. The detectors have frequency bands consistent with our simulations, and have high average optical efficiency which is 86%, 77% and 66% for the 95, 150 and 220 GHz detectors. The time constants of the detectors are mostly between 0.5 ms and 5 ms. The beam is round with the correct size, and the polarization efficiency is more than 90% for most of the bolometers, Comment: Conference proceeding for Low Temperature Detectors 2017

Published
2018
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16. CMB-S4 Technology Book, First Edition

Author

Abitbol, Maximilian H., Ahmed, Zeeshan, Barron, Darcy, Thakur, Ritoban Basu, Bender, Amy N., Benson, Bradford A., Bischoff, Colin A., Bryan, Sean A., Carlstrom, John E., Chang, Clarence L., Chuss, David T., Crowley, Kevin T., Cukierman, Ari, de Haan, Tijmen, Dobbs, Matt, Essinger-Hileman, Tom, Filippini, Jeffrey P., Ganga, Ken, Gudmundsson, Jon E., Halverson, Nils W., Hanany, Shaul, Henderson, Shawn W., Hill, Charles A., Ho, Shuay-Pwu P., Hubmayr, Johannes, Irwin, Kent, Jeong, Oliver, Johnson, Bradley R., Kernasovskiy, Sarah A., Kovac, John M., Kusaka, Akito, Lee, Adrian T., Maria, Salatino, Mauskopf, Philip, McMahon, Jeff J., Moncelsi, Lorenzo, Nadolski, Andrew W., Nagy, Johanna M., Niemack, Michael D., O'Brient, Roger C., Padin, Stephen, Parshley, Stephen C., Pryke, Clement, Roe, Natalie A., Rostem, Karwan, Ruhl, John, Simon, Sara M., Staggs, Suzanne T., Suzuki, Aritoki, Switzer, Eric R., Tajima, Osamu, Thompson, Keith L., Timbie, Peter, Tucker, Gregory S., Vieira, Joaquin D., Vieregg, Abigail G., Westbrook, Benjamin, Wollack, Edward J., Yoon, Ki Won, Young, Karl S., and Young, Edward Y.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

CMB-S4 is a proposed experiment to map the polarization of the Cosmic Microwave Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible from the ground. The science goals and capabilities of CMB-S4 in illuminating cosmic inflation, measuring the sum of neutrino masses, searching for relativistic relics in the early universe, characterizing dark energy and dark matter, and mapping the matter distribution in the universe have been described in the CMB-S4 Science Book. This Technology Book is a companion volume to the Science Book. The ambitious science goals of CMB-S4, a "Stage-4" experiment, require a step forward in experimental capability from the current Stage=II experiments. To guide this process, we summarize the current state of CMB instrumentation technology, and identify R&D efforts necessary to advance it for use in CMB-S4. The book focuses on technical challenges in four broad areas: Telescope Design; Receiver Optics; Focal-Plane Optical Coupling; and Focal-Plane Sensor and Readout., Comment: 191 pages

Published
2017

17. Performance of a continuously rotating half-wave plate on the POLARBEAR telescope

Author

Takakura, Satoru, Aguilar, Mario, Akiba, Yoshiki, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beckman, Shawn, Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Cukierman, Ari, Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Fujino, Takuro, Galitzki, Nicholas, Goeckner-Wald, Neil, Halverson, Nils W., Hasegawa, Masaya, Hattori, Kaori, Hazumi, Masashi, Hill, Charles, Howe, Logan, Inoue, Yuki, Jaffe, Andrew H., Jeong, Oliver, Kaneko, Daisuke, Katayama, Nobuhiko, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Krachmalnicoff, Nicoletta, Kusaka, Akito, Lee, Adrian T., Leon, David, Lowry, Lindsay, Matsuda, Frederick, Matsumura, Tomotake, Navaroli, Martin, Nishino, Haruki, Paar, Hans, Peloton, Julien, Poletti, Davide, Puglisi, Giuseppe, Reichardt, Christian L., Ross, Colin, Siritanasak, Praween, Suzuki, Aritoki, Tajima, Osamu, Takatori, Sayuri, and Teply, Grant

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

A continuously rotating half-wave plate (CRHWP) is a promising tool to improve the sensitivity to large angular scales in cosmic microwave background (CMB) polarization measurements. With a CRHWP, single detectors can measure three of the Stokes parameters, $I$, $Q$ and $U$, thereby avoiding the set of systematic errors that can be introduced by mismatches in the properties of orthogonal detector pairs. We focus on the implementation of CRHWPs in large aperture telescopes (i.e. the primary mirror is larger than the current maximum half-wave plate diameter of $\sim$0.5 m), where the CRHWP can be placed between the primary mirror and focal plane. In this configuration, one needs to address the intensity to polarization ($I{\rightarrow}P$) leakage of the optics, which becomes a source of 1/f noise and also causes differential gain systematics that arise from CMB temperature fluctuations. In this paper, we present the performance of a CRHWP installed in the POLARBEAR experiment, which employs a Gregorian telescope with a 2.5 m primary illumination pattern. The CRHWP is placed near the prime focus between the primary and secondary mirrors. We find that the $I{\rightarrow}P$ leakage is larger than the expectation from the physical properties of our primary mirror, resulting in a 1/f knee of 100 mHz. The excess leakage could be due to imperfections in the detector system, i.e. detector non-linearity in the responsivity and time-constant. We demonstrate, however, that by subtracting the leakage correlated with the intensity signal, the 1/f noise knee frequency is reduced to 32 mHz ($\ell \sim$39 for our scan strategy), which is very promising to probe the primordial B-mode signal. We also discuss methods for further noise subtraction in future projects where the precise temperature control of instrumental components and the leakage reduction will play a key role., Comment: 27 pages, 5 figures, 3 tables, published version in JCAP. Includes some minor corrections

Published
2017
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19. POLARBEAR Constraints on Cosmic Birefringence and Primordial Magnetic Fields

Author

POLARBEAR Collaboration, Ade, Peter A. R., Arnold, Kam, Atlas, Matt, Baccigalupi, Carlo, Barron, Darcy, Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Cukierman, Ari, Dobbs, Matt, Ducout, Anne, Dunner, Rolando, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Feeney, Stephen, Feng, Chang, Gilbert, Adam, Goeckner-Wald, Neil, Groh, John, Hall, Grantland, Halverson, Nils W., Hasegawa, Masaya, Hattori, Kaori, Hazumi, Masashi, Hill, Charles, Holzapfel, William L., Hori, Yasuto, Howe, Logan, Inoue, Yuki, Jaehnig, Gregory C., Jaffe, Andrew H., Jeong, Oliver, Katayama, Nobuhiko, Kaufman, Jonathan P., Keating, Brian, Kermish, Zigmund, Keskitalo, Reijo, Kisner, Theodore, Kusaka, Akito, Jeune, Maude Le, Lee, Adrian T., Leitch, Erik M., Leon, David, Li, Yun, Linder, Eric, Lowry, Lindsay, Matsuda, Frederick, Matsumura, Tomotake, Miller, Nathan, Montgomery, Josh, Myers, Michael J., Navaroli, Martin, Nishino, Haruki, Okamura, Takahiro, Paar, Hans, Peloton, Julien, Pogosian, Levon, Poletti, Davide, Puglisi, Giuseppe, Raum, Christopher, Rebeiz, Gabriel, Reichardt, Christian L., Richards, Paul L., Ross, Colin, Rotermund, Kaja M., Schenck, David E., Sherwin, Blake D., Shimon, Meir, Shirley, Ian, Siritanasak, Praween, Smecher, Graeme, Stebor, Nathan, Steinbach, Bryan, Suzuki, Aritoki, Suzuki, Jun-ichi, Tajima, Osamu, Takakura, Satoru, Tikhomirov, Alexei, Tomaru, Takayuki, Whitehorn, Nathan, Wilson, Brandon, Yadav, Amit, Zahn, Alex, and Zahn, Oliver

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We constrain anisotropic cosmic birefringence using four-point correlations of even-parity $E$-mode and odd-parity $B$-mode polarization in the cosmic microwave background measurements made by the POLARization of the Background Radiation (POLARBEAR) experiment in its first season of observations. We find that the anisotropic cosmic birefringence signal from any parity-violating processes is consistent with zero. The Faraday rotation from anisotropic cosmic birefringence can be compared with the equivalent quantity generated by primordial magnetic fields if they existed. The POLARBEAR nondetection translates into a 95% confidence level (C.L.) upper limit of 93 nanogauss (nG) on the amplitude of an equivalent primordial magnetic field inclusive of systematic uncertainties. This four-point correlation constraint on Faraday rotation is about 15 times tighter than the upper limit of 1380 nG inferred from constraining the contribution of Faraday rotation to two-point correlations of $B$-modes measured by Planck in 2015. Metric perturbations sourced by primordial magnetic fields would also contribute to the $B$-mode power spectrum. Using the POLARBEAR measurements of the $B$-mode power spectrum (two-point correlation), we set a 95% C.L. upper limit of 3.9 nG on primordial magnetic fields assuming a flat prior on the field amplitude. This limit is comparable to what was found in the Planck 2015 two-point correlation analysis with both temperature and polarization. We perform a set of systematic error tests and find no evidence for contamination. This work marks the first time that anisotropic cosmic birefringence or primordial magnetic fields have been constrained from the ground at subdegree scales., Comment: 10 pages, 5 figures. Phys. Rev. D Editors' Suggestion

Published
2015
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20. Horn Coupled Multichroic Polarimeters for the Atacama Cosmology Telescope Polarization Experiment

Author

Datta, Rahul, Hubmayr, Johannes, Munson, Charles, Austermann, Jason, Beall, James, Becker, Dan, Cho, Hsiao-Mei, Halverson, Nils, Hilton, Gene, Irwin, Kent, Li, Dale, McMahon, Jeff, Newburgh, Laura, Nibarger, John, Niemack, Michael, Schmitt, Benjamin, Smith, Harrison, Staggs, Suzanne, Van Lanen, Jeff, and Wollack, Edward

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

Multichroic polarization sensitive detectors enable increased sensitivity and spectral coverage for observations of the Cosmic Microwave Background (CMB). An array optimized for dual frequency detectors can provide 1.7 times gain in sensitivity compared to a single frequency array. We present the design and measurements of horn coupled multichroic polarimeters encompassing the 90 and 150 GHz frequency bands and discuss our plans to field an array of these detectors as part of the ACTPol project.

Published
2014
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21. POLARBEAR constraints on cosmic birefringence and primordial magnetic fields

Author

Ade, Peter AR, Arnold, Kam, Atlas, Matt, Baccigalupi, Carlo, Barron, Darcy, Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Cukierman, Ari, Dobbs, Matt, Ducout, Anne, Dunner, Rolando, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Feeney, Stephen, Feng, Chang, Gilbert, Adam, Goeckner-Wald, Neil, Groh, John, Hall, Grantland, Halverson, Nils W, Hasegawa, Masaya, Hattori, Kaori, Hazumi, Masashi, Hill, Charles, Holzapfel, William L, Hori, Yasuto, Howe, Logan, Inoue, Yuki, Jaehnig, Gregory C, Jaffe, Andrew H, Jeong, Oliver, Katayama, Nobuhiko, Kaufman, Jonathan P, Keating, Brian, Kermish, Zigmund, Keskitalo, Reijo, Kisner, Theodore, Kusaka, Akito, Le Jeune, Maude, Lee, Adrian T, Leitch, Erik M, Leon, David, Li, Yun, Linder, Eric, Lowry, Lindsay, Matsuda, Frederick, Matsumura, Tomotake, Miller, Nathan, Montgomery, Josh, Myers, Michael J, Navaroli, Martin, Nishino, Haruki, Okamura, Takahiro, Paar, Hans, Peloton, Julien, Pogosian, Levon, Poletti, Davide, Puglisi, Giuseppe, Raum, Christopher, Rebeiz, Gabriel, Reichardt, Christian L, Richards, Paul L, Ross, Colin, Rotermund, Kaja M, Schenck, David E, Sherwin, Blake D, Shimon, Meir, Shirley, Ian, Siritanasak, Praween, Smecher, Graeme, Stebor, Nathan, Steinbach, Bryan, Suzuki, Aritoki, Suzuki, Jun-ichi, Tajima, Osamu, Takakura, Satoru, Tikhomirov, Alexei, Tomaru, Takayuki, Whitehorn, Nathan, Wilson, Brandon, Yadav, Amit, Zahn, Alex, and Zahn, Oliver

Subjects
Particle and High Energy Physics, Astronomical Sciences, Physical Sciences, astro-ph.CO, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Astronomical sciences, Particle and high energy physics
Abstract

We constrain anisotropic cosmic birefringence using four-point correlations of even-parity E-mode and odd-parity B-mode polarization in the cosmic microwave background measurements made by the POLARization of the Background Radiation (POLARBEAR) experiment in its first season of observations. We find that the anisotropic cosmic birefringence signal from any parity-violating processes is consistent with zero. The Faraday rotation from anisotropic cosmic birefringence can be compared with the equivalent quantity generated by primordial magnetic fields if they existed. The POLARBEAR nondetection translates into a 95% confidence level (C.L.) upper limit of 93 nanogauss (nG) on the amplitude of an equivalent primordial magnetic field inclusive of systematic uncertainties. This four-point correlation constraint on Faraday rotation is about 15 times tighter than the upper limit of 1380 nG inferred from constraining the contribution of Faraday rotation to two-point correlations of B-modes measured by Planck in 2015. Metric perturbations sourced by primordial magnetic fields would also contribute to the B-mode power spectrum. Using the POLARBEAR measurements of the B-mode power spectrum (two-point correlation), we set a 95% C.L. upper limit of 3.9 nG on primordial magnetic fields assuming a flat prior on the field amplitude. This limit is comparable to what was found in the Planck 2015 two-point correlation analysis with both temperature and polarization. We perform a set of systematic error tests and find no evidence for contamination. This work marks the first time that anisotropic cosmic birefringence or primordial magnetic fields have been constrained from the ground at subdegree scales.

Published
2015

22. Millimeter-wave bolometer array receiver for the Atacama pathfinder experiment Sunyaev-Zel'dovich (APEX-SZ) instrument

Author

Schwan, Daniel, Ade, Peter A. R., Basu, Kaustuv, Bender, Amy N., Bertoldi, Frank, Cho, Hsaio-Mei, Chon, Guyong., Clarke, John, Dobbs, Matt, Ferrusca, Daniel, Gusten, Rolfe, Halverson, Nils W., Holzapfel, William L., Horellou, Cathy, Johansson, Daniel, Johnson, Bradley R., Kennedy, James, Kermish, Zigmund, Kneissl, Ruediger, Lanting, Trevor, Lee, Adrian T., Lueker, Martin, Mehl, Jared, Menten, Karl M., Muders, Dirk, Pacaud, Florian, Plagge, Thomas, Reichardt, Christian L., Richards, Paul L., Schaaf, Rienhold, Schilke, Peter, Sommer, Martin W., Spieler, Helmuth, Tucker, Carole, Weiss, Axel, Westbrook, Benjamin, and Zahn, Oliver

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

The Atacama pathfinder experiment Sunyaev-Zel'dovich (APEX-SZ) instrument is a millimeter-wave cryogenic receiver designed to observe galaxy clusters via the Sunyaev-Zel'dovich effect from the 12 m APEX telescope on the Atacama plateau in Chile. The receiver contains a focal plane of 280 superconducting transition-edge sensor (TES) bolometers instrumented with a frequency-domain multiplexed readout system. The bolometers are cooled to 280 mK via a three-stage helium sorption refrigerator and a mechanical pulse-tube cooler. Three warm mirrors, two 4 K lenses, and a horn array couple the TES bolometers to the telescope. APEX-SZ observes in a single frequency band at 150 GHz with 1' angular resolution and a 22' field-of-view, all well suited for cluster mapping. The APEX-SZ receiver has played a key role in the introduction of several new technologies including TES bolometers, the frequency-domain multiplexed readout, and the use of a pulse-tube cooler with bolometers. As a result of these new technologies, the instrument has a higher instantaneous sensitivity and covers a larger field-of-view than earlier generations of Sunyaev-Zel'dovich instruments. The TES bolometers have a median sensitivity of 890 uKcmb-sqrt(s) (NEy of 3.5e-4 sqrt(s)). We have also demonstrated upgraded detectors with improved sensitivity of 530 uKcmb-sqrt(s) (NEy of 2.2e-4 sqrt(s)). Since its commissioning in April 2007, APEX-SZ has been used to map 48 clusters. We describe the design of the receiver and its performance when installed on the APEX telescope., Comment: 27 pages, 20 figures, prepared with revtex 4.1

Published
2010
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23. Impact of Electrical Contacts Design and Materials on the Stability of Ti Superconducting Transition Shape

Author

Yefremenko, Volodymyr, Ade, Peter A. R., Ahmed, Zeeshan, Anderson, Adam J., Austermann, Jason E., Avva, Jessica S., Basu Thakur, Robitan, Bender, Amy N., Benson, Bradford A., Carlstrom, John E., Carter, Faustin W., Cecil, Thomas, Chang, Clarence L., Cliche, Jean-Francois, Cukierman, Ariel, Denison, Edward V., de Haan, Tijmen, Ding, Junjia, Divan, Ralu N. S., Dobbs, Matt A., Dutcher, Daniel, Everett, Wenderline, Foster, Allen, Gannon, Renae N., Gilbert, Adam, Groh, John, Halverson, Nils W., Harke-Hosemann, Angelina H., Harrington, Nicholas L., Henning, Jason W., Hilton, Gene C., Holzapfel, William L., Huang, Nicholas, Irwin, Kent D., Jeong, Oliver B., Jonas, Michelle, Khaire, Trupti, Kofman, Anna M., Korman, Milo, Kubik, Donna L., Kuhlmann, Steve, Kuo, Chao-Lin, Lee, Adrian T., Lowitz, Amy E., Meyer, Stephen S., Michalik, Daniel, Miller, Christina Suzanne, Montgomery, Joshua, Nadolski, Andrew, Natoli, Tyler J., Nguyen, Hogan, Noble, Gavin, Novosad, Valentine, Padin, Stephen, Pan, Zhaodi, Pearson, John, Posada, Chrystian M., Rahlin, Alexandra, Ruhl, John E., Saunders, L. J., Sayre, James T., Shirley, Ian, Shirokoff, Erik D., Smecher, Graeme, Sobrin, Joshua A., Stan, Liliana, Stark, Antony A., Story, Kyle T., Suzuki, Aritoki, Tang, Qing Yang, Thompson, Keith L., Tucker, Carole E., Vale, Leila R., Vanderlinde, Keith, Vieira, Joaquin D., Wang, Gensheng, Whitehorn, Nathan, Yoon, Ki Won, and Young, Matt

Published
2018
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24. The POLARBEAR experiment

Author

Kermish, Zigmund D, Ade, Peter, Anthony, Aubra, Arnold, Kam, Barron, Darcy, Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Dobbs, Matt A, Errard, Josquin, Fabbian, Giulio, Flanigan, Daniel, Fuller, George, Ghribi, Adnan, Grainger, Will, Halverson, Nils, Hasegawa, Masaya, Hattori, Kaori, Hazumi, Masashi, Holzapfel, William L, Howard, Jacob, Hyland, Peter, Jaffe, Andrew, Keating, Brian, Kisner, Theodore, Lee, Adrian T, Le Jeune, Maude, Linder, Eric, Lungu, Marius, Matsuda, Frederick, Matsumura, Tomotake, Meng, Xiaofan, Miller, Nathan J, Morii, Hideki, Moyerman, Stephanie, Myers, Mike J, Nishino, Haruki, Paar, Hans, Quealy, Erin, Reichardt, Christian L, Richards, Paul L, Ross, Colin, Shimizu, Akie, Shimon, Meir, Shimmin, Chase, Sholl, Mike, Siritanasak, Praween, Spieler, Helmuth, Stebor, Nathan, Steinbach, Bryan, Stompor, Radek, Suzuki, Aritoki, Tomaru, Takayuki, Tucker, Carole, and Zahn, Oliver

Subjects
Cosmic Microwave Background, Inflation, Polarization, Bolometer, astro-ph.IM
Abstract

We present the design and characterization of the polarbear experiment. polarbear will measure the polarization of the cosmic microwave background (CMB) on angular scales ranging from the experiment's 3.5′ beam size to several degrees. The experiment utilizes a unique focal plane of 1,274 antenna-coupled, polarization sensitive TES bolometers cooled to 250 milliKelvin. Employing this focal plane along with stringent control over systematic errors, polarbear has the sensitivity to detect the expected small scale B-mode signal due to gravitational lensing and search for the large scale B-mode signal from inflationary gravitational waves. polarbear was assembled for an engineering run in the Inyo Mountains of California in 2010 and was deployed in late 2011 to the Atacama Desert in Chile. An overview of the instrument is presented along with characterization results from observations in Chile. © 2012 SPIE.

Published
2012

25. The Impact of Atmospheric Fluctuations on Degree-scale Imaging of the Cosmic Microwave Background

Author

Lay, Oliver P. and Halverson, Nils W.

Subjects
Astrophysics
Abstract

Fluctuations in the brightness of the Earth's atmosphere originating from water vapor are an important source of noise for ground-based instruments attempting to measure anisotropy in the Cosmic Microwave Background. This paper presents a model for the atmospheric fluctuations and derives simple expressions to predict the contribution of the atmosphere to experimental measurements. Data from the South Pole and from the Atacama Desert in Chile, two of the driest places on Earth, are used to assess the level of fluctuations at each site., Comment: 29 pages, 7 figures, 1 table, appears in The Astrophysical Journal

Published
1999
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26. Experimental characterization of a planar phase-engineered metamaterial lenslet for millimeter astronomy

Author

Gascard, Thomas, primary, Pisano, Giampaolo, additional, Doyle, Simon, additional, Thompson, Jonathan, additional, Shitvov, Alexey, additional, Austermann, Jason, additional, Beall, James, additional, Hubmayr, Johannes, additional, Raymond, Benjamin, additional, Halverson, Nils, additional, Jaehnig, Gregory, additional, McKenney, Christopher M., additional, and Suzuki, Aritoki, additional

Published
2023
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29. SPT-3G+: mapping the high-frequency cosmic microwave background using kinetic inductance detectors

Author

Anderson, Adam J., primary, Barry, Peter, additional, Bender, Amy N., additional, Benson, Bradford, additional, Bleem, Lindsey, additional, Carlstrom, John E., additional, Cecil, Tom W., additional, Chang, Clarence L., additional, Crawford, Tom M., additional, Dibert, Karia R., additional, Dobbs, Matt A., additional, Fichman, Kyra, additional, Halverson, Nils W., additional, Holzapfel, William L., additional, Hryciuk, Alec, additional, Karkare, Kirit S., additional, Li, Juliang, additional, Lisovenko, Marharyta, additional, Marrone, Daniel, additional, McMahon, Jeff, additional, Montgomery, Joshua, additional, Natoli, Tyler, additional, Pan, Zhaodi, additional, Raghunathan, Srinivasan, additional, Reichardt, Christian L., additional, Rouble, Maclean, additional, Shirokoff, Erik, additional, Smecher, Graeme, additional, Stark, Antony A., additional, Vieira, Joaquin D., additional, and Young, Matt R., additional

Published
2022
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30. LiteBIRD Low- and mid-frequency detectors: design and status

Author

Jaehnig, Gregory, primary, Arnold, Kam S., additional, Austermann, Jason E., additional, Beall, James A., additional, Becker, Dan T., additional, Connors, Jake A., additional, Duff, Shannon M., additional, Halverson, Nils W., additional, Hazumi, Masashi, additional, Hilton, Gene C., additional, Hubmayr, Johannes, additional, Kuo, Chao-Lin, additional, Lee, Adrian T., additional, Link, Michael J., additional, Raum, Christopher R., additional, Stevenson, Sarah A., additional, Suzuki, Aritoki, additional, Thompson, Keith L., additional, Van Lanen, Jeff, additional, Vissers, Michael R., additional, Walker, S., additional, and Westbrook, Benjamin, additional

Published
2022
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31. Development of the low frequency telescope focal plane detector modules for LiteBIRD

Author

Westbrook, Benjamin, primary, Raum, Christopher, additional, Beckman, Shawn, additional, Lee, Adrian T., additional, Farias, Nicole, additional, Bogdan, Andrew, additional, Hornsby, Amber, additional, Suzuki, Aritoki, additional, Rotermund, Kaja, additional, Elleflot, Tucker, additional, Austerman, Jason E., additional, Beall, James A., additional, Duff, Shannon M., additional, Hubmayr, Johannes, additional, Vissers, Michael R., additional, Link, Michael J., additional, Jaehnig, Greg, additional, Halverson, Nils, additional, Ghigna, Tomasso, additional, Stever, Samantha, additional, Minami, Yuto, additional, Thompson, Keith L., additional, Russell, Megan, additional, Arnold, Kam, additional, and Silva-Feaver, Maximiliano, additional

Published
2022
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32. CMB-S4

Author

Collaboration, The CMB-S4, Abazajian, Kevork, Addison, Graeme E., Adshead, Peter, Ahmed, Zeeshan, Akerib, Daniel, Ali, Aamir, Allen, Steven W., Alonso, David, Alvarez, Marcelo, Amin, Mustafa A., Anderson, Adam, Arnold, Kam S., Ashton, Peter, Baccigalupi, Carlo, Bard, Debbie, Barkats, Denis, Barron, Darcy, Barry, Peter S., Bartlett, James G., Thakur, Ritoban Basu, Battaglia, Nicholas, Bean, Rachel, Bebek, Chris, Bender, Amy N., Benson, Bradford A., Bianchini, Federico, Bischoff, Colin A., Bleem, Lindsey, Bock, James J., Bocquet, Sebastian, Boddy, Kimberly K., Bond, J. Richard, Borrill, Julian, Bouchet, François R., Brinckmann, Thejs, Brown, Michael L., Bryan, Sean, Buza, Victor, Byrum, Karen, Caimapo, Carlos Hervias, Calabrese, Erminia, Calafut, Victoria, Caldwell, Robert, Carlstrom, John E., Carron, Julien, Cecil, Thomas, Challinor, Anthony, Chang, Clarence L., Chinone, Yuji, Cho, Hsiao-Mei Sherry, Cooray, Asantha, Coulton, Will, Crawford, Thomas M., Crites, Abigail, Cukierman, Ari, Cyr-Racine, Francis-Yan, de Haan, Tijmen, Delabrouille, Jacques, Devlin, Mark, Di Valentino, Eleonora, Dierickx, Marion, Dobbs, Matt, Duff, Shannon, Dunkley, Jo, Dvorkin, Cora, Eimer, Joseph, Elleflot, Tucker, Errard, Josquin, Essinger-Hileman, Thomas, Fabbian, Giulio, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey P., Flauger, Raphael, Flaugher, Brenna, Fraisse, Aurelien A., Frolov, Andrei, Galitzki, Nicholas, Gallardo, Patricio A., Galli, Silvia, Ganga, Ken, Gerbino, Martina, Gluscevic, Vera, Goeckner-Wald, Neil, Green, Daniel, Grin, Daniel, Grohs, Evan, Gualtieri, Riccardo, Gudmundsson, Jon E., Gullett, Ian, Gupta, Nikhel, Habib, Salman, Halpern, Mark, Halverson, Nils W., Hanany, Shaul, Harrington, Kathleen, Hasegawa, Masaya, Hasselfield, Matthew, Hazumi, Masashi, Heitmann, Katrin, Henderson, Shawn, Hensley, Brandon, Hill, Charles, Hill, J. Colin, Hlozek, Renée, Ho, Shuay-Pwu Patty, Hoang, Thuong, Holder, Gil, Holzapfel, William, Hood, John, Hubmayr, Johannes, Huffenberger, Kevin M., Hui, Howard, Irwin, Kent, Jeong, Oliver, Johnson, Bradley R., Jones, William C., Kang, Jae Hwan, Karkare, Kirit S., Katayama, Nobuhiko, Keskitalo, Reijo, Kisner, Theodore, Knox, Lloyd, Koopman, Brian J., Kosowsky, Arthur, Kovac, John, Kovetz, Ely D., Kuhlmann, Steve, Kuo, Chao-lin, Kusaka, Akito, Lähteenmäki, Anne, Lawrence, Charles R., Lee, Adrian T., Lewis, Antony, Li, Dale, Linder, Eric, Loverde, Marilena, Lowitz, Amy, Lubin, Phil, Madhavacheril, Mathew S., Mantz, Adam, Marques, Gabriela, Matsuda, Frederick, Mauskopf, Philip, McCarrick, Heather, McMahon, Jeffrey, Meerburg, P. Daniel, Melin, Jean-Baptiste, Menanteau, Felipe, Meyers, Joel, Millea, Marius, Mohr, Joseph, Moncelsi, Lorenzo, Monzani, Maria, Mroczkowski, Tony, Mukherjee, Suvodip, Nagy, Johanna, Namikawa, Toshiya, Nati, Federico, Natoli, Tyler, Newburgh, Laura, Niemack, Michael D., Nishino, Haruki, Nord, Brian, Novosad, Valentine, O'Brient, Roger, Padin, Stephen, Palladino, Steven, Partridge, Bruce, Petravick, Don, Pierpaoli, Elena, Pogosian, Levon, Prabhu, Karthik, Pryke, Clement, Puglisi, Giuseppe, Racine, Benjamin, Rahlin, Alexandra, Rao, Mayuri Sathyanarayana, Raveri, Marco, Reichardt, Christian L., Remazeilles, Mathieu, Rocha, Graca, Roe, Natalie A., Roy, Anirban, Ruhl, John E., Salatino, Maria, Saliwanchik, Benjamin, Schaan, Emmanuel, Schillaci, Alessandro, Schmitt, Benjamin, Schmittfull, Marcel M., Scott, Douglas, Sehgal, Neelima, Shandera, Sarah, Sherwin, Blake D., Shirokoff, Erik, Simon, Sara M., Slosar, Anze, Spergel, David, Germaine, Tyler St., Staggs, Suzanne T., Stark, Antony, Starkman, Glenn D., Stompor, Radek, Stoughton, Chris, Suzuki, Aritoki, Tajima, Osamu, Teply, Grant P., Thompson, Keith, Thorne, Ben, Timbie, Peter, Tomasi, Maurizio, Tristram, Matthieu, Tucker, Gregory, Umiltà, Caterina, van Engelen, Alexander, Vavagiakis, Eve M., Vieira, Joaquin D., Vieregg, Abigail G., Wagoner, Kasey, Wallisch, Benjamin, Wang, Gensheng, Watson, Scott, Westbrook, Ben, Whitehorn, Nathan, Wollack, Edward J., Wu, W. L. Kimmy, Xu, Zhilei, Yang, H. Y. Eric, Yasini, Siavash, Yefremenko, Volodymyr G., Yoon, Ki Won, Young, Edward, Yu, Cyndia, Zonca, Andrea, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Théorique - UMR CNRS 3681 (IPHT), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), CMB-S4, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université Paris-Sud - Paris 11 (UP11), Apollo - University of Cambridge Repository, Van Swinderen Institute for Particle Physics and G, Cosmic Frontier, Abazajian, K, Addison, G, Adshead, P, Ahmed, Z, Akerib, D, Ali, A, Allen, S, Alonso, D, Alvarez, M, Amin, M, Anderson, A, Arnold, K, Ashton, P, Baccigalupi, C, Bard, D, Barkats, D, Barron, D, Barry, P, Bartlett, J, Basu Thakur, R, Battaglia, N, Bean, R, Bebek, C, Bender, A, Benson, B, Bianchini, F, Bischoff, C, Bleem, L, Bock, J, Bocquet, S, Boddy, K, Richard Bond, J, Borrill, J, Bouchet, F, Brinckmann, T, Brown, M, Bryan, S, Buza, V, Byrum, K, Hervias Caimapo, C, Calabrese, E, Calafut, V, Caldwell, R, Carlstrom, J, Carron, J, Cecil, T, Challinor, A, Chang, C, Chinone, Y, Sherry Cho, H, Cooray, A, Coulton, W, Crawford, T, Crites, A, Cukierman, A, Cyr-Racine, F, De Haan, T, Delabrouille, J, Devlin, M, Di Valentino, E, Dierickx, M, Dobbs, M, Duff, S, Dvorkin, C, Eimer, J, Elleflot, T, Errard, J, Essinger-Hileman, T, Fabbian, G, Feng, C, Ferraro, S, Filippini, J, Flauger, R, Flaugher, B, Fraisse, A, Frolov, A, Galitzki, N, Gallardo, P, Galli, S, Ganga, K, Gerbino, M, Gluscevic, V, Goeckner-Wald, N, Green, D, Grin, D, Grohs, E, Gualtieri, R, Gudmundsson, J, Gullett, I, Gupta, N, Habib, S, Halpern, M, Halverson, N, Hanany, S, Harrington, K, Hasegawa, M, Hasselfield, M, Hazumi, M, Heitmann, K, Henderson, S, Hensley, B, Hill, C, Colin Hill, J, Hlozek, R, Patty Ho, S, Hoang, T, Holder, G, Holzapfel, W, Hood, J, Hubmayr, J, Huffenberger, K, Hui, H, Irwin, K, Jeong, O, Johnson, B, Jones, W, Hwan Kang, J, Karkare, K, Katayama, N, Keskitalo, R, Kisner, T, Knox, L, Koopman, B, Kosowsky, A, Kovac, J, Kovetz, E, Kuhlmann, S, Kuo, C, Kusaka, A, Lahteenmaki, A, Lawrence, C, Lee, A, Lewis, A, Li, D, Linder, E, Loverde, M, Lowitz, A, Lubin, P, Madhavacheril, M, Mantz, A, Marques, G, Matsuda, F, Mauskopf, P, Mccarrick, H, Mcmahon, J, Daniel Meerburg, P, Melin, J, Menanteau, F, Meyers, J, Millea, M, Mohr, J, Moncelsi, L, Monzani, M, Mroczkowski, T, Mukherjee, S, Nagy, J, Namikawa, T, Nati, F, Natoli, T, Newburgh, L, Niemack, M, Nishino, H, Nord, B, Novosad, V, O'Brient, R, Padin, S, Palladino, S, Partridge, B, Petravick, D, Pierpaoli, E, Pogosian, L, Prabhu, K, Pryke, C, Puglisi, G, Racine, B, Rahlin, A, Sathyanarayana Rao, M, Raveri, M, Reichardt, C, Remazeilles, M, Rocha, G, Roe, N, Roy, A, Ruhl, J, Salatino, M, Saliwanchik, B, Schaan, E, Schillaci, A, Schmitt, B, Schmittfull, M, Scott, D, Sehgal, N, Shandera, S, Sherwin, B, Shirokoff, E, Simon, S, Slosar, A, Spergel, D, S, T, Staggs, S, Stark, A, Starkman, G, Stompor, R, Stoughton, C, Suzuki, A, Tajima, O, Teply, G, Thompson, K, Thorne, B, Timbie, P, Tomasi, M, Tristram, M, Tucker, G, Umilta, C, Van Engelen, A, Vavagiakis, E, Vieira, J, Vieregg, A, Wagoner, K, Wallisch, B, Wang, G, Watson, S, Westbrook, B, Whitehorn, N, Wollack, E, Kimmy Wu, W, Xu, Z, Eric Yang, H, Yasini, S, Yefremenko, V, Won Yoon, K, Young, E, Yu, C, Zonca, A, University of California Irvine, Johns Hopkins University, University of Illinois at Urbana-Champaign, SLAC National Accelerator Laboratory, University of California Berkeley, Stanford University, University of Oxford, Rice University, Fermi National Accelerator Laboratory, University of California San Diego, International School for Advanced Studies, Lawrence Berkeley National Laboratory, Harvard University, University of New Mexico, Argonne National Laboratory, Université Paris-Diderot, California Institute of Technology, Cornell University, University of Melbourne, University of Cincinnati, Ludwig Maximilian University of Munich, University of Toronto, UMR7095, Stony Brook University, University of Manchester, Arizona State University, Florida State University, Cardiff University, Dartmouth College, University of Geneva, University of Cambridge, The University of Tokyo, University of Groningen, University of Chicago, University of Pennsylvania, McGill University, National Institute of Standards and Technology, NASA Goddard Space Flight Center, University of Sussex, Princeton University, Simon Fraser University, National Institute for Nuclear Physics, Haverford College, Stockholm University, Case Western Reserve University, University of British Columbia, University of Colorado Boulder, University of Minnesota Twin Cities, University of Michigan, Ann Arbor, Simons Foundation, Columbia University, University of Virginia, University of California Davis, Yale University, University of Pittsburgh, Ben-Gurion University of the Negev, Department of Electronics and Nanoengineering, Jet Propulsion Laboratory, University of California Santa Barbara, Perimeter Institute for Theoretical Physics, Service d'Astrophysique CEA, European Southern Observatory, Washington University St. Louis, University of Milan - Bicocca, University of Southern California, Institute for Advanced Studies, Pennsylvania State University, Brookhaven National Laboratory, Kyoto University, University of Wisconsin-Madison, University of Milano, Université Paris-Saclay, Brown University, Syracuse University, University of California Los Angeles, Aalto-yliopisto, and Aalto University

Subjects
Astrophysics and Astronomy, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cosmology, CMB, Settore FIS/05, Space and Planetary Science, astro-ph.CO, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Galaxies and Cosmology, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

CMB-S4---the next-generation ground-based cosmic microwave background (CMB) experiment---is set to significantly advance the sensitivity of CMB measurements and enhance our understanding of the origin and evolution of the Universe, from the highest energies at the dawn of time through the growth of structure to the present day. Among the science cases pursued with CMB-S4, the quest for detecting primordial gravitational waves is a central driver of the experimental design. This work details the development of a forecasting framework that includes a power-spectrum-based semi-analytic projection tool, targeted explicitly towards optimizing constraints on the tensor-to-scalar ratio, $r$, in the presence of Galactic foregrounds and gravitational lensing of the CMB. This framework is unique in its direct use of information from the achieved performance of current Stage 2--3 CMB experiments to robustly forecast the science reach of upcoming CMB-polarization endeavors. The methodology allows for rapid iteration over experimental configurations and offers a flexible way to optimize the design of future experiments given a desired scientific goal. To form a closed-loop process, we couple this semi-analytic tool with map-based validation studies, which allow for the injection of additional complexity and verification of our forecasts with several independent analysis methods. We document multiple rounds of forecasts for CMB-S4 using this process and the resulting establishment of the current reference design of the primordial gravitational-wave component of the Stage-4 experiment, optimized to achieve our science goals of detecting primordial gravitational waves for $r > 0.003$ at greater than $5��$, or, in the absence of a detection, of reaching an upper limit of $r < 0.001$ at $95\%$ CL., 24 pages, 8 figures, 9 tables, submitted to ApJ. arXiv admin note: text overlap with arXiv:1907.04473

Published
2022

33. Performance and characterization of the SPT-3G digital frequency-domain multiplexed readout system using an improved noise and crosstalk model

Author

Montgomery, Joshua, primary, Ade, Peter A. R., additional, Ahmed, Zeeshan, additional, Anderes, Ethan, additional, Anderson, Adam J., additional, Archipley, Melanie, additional, Avva, Jessica S., additional, Aylor, Kevin, additional, Balkenhol, Lennart, additional, Barry, Peter S., additional, Thakur, Ritoban B., additional, Benabed, Karim, additional, Bender, Amy N., additional, Benson, Bradford A., additional, Bianchini, Federico, additional, Bleem, Lindsey E., additional, Bouchet, Francois R., additional, Bryant, Lincoln, additional, Byrum, Karen, additional, Carlstrom, John E., additional, Carter, Faustin W., additional, Cecil, Thomas W., additional, Chang, Clarence L., additional, Chaubal, Prakrut, additional, Chen, Geoffrey, additional, Cho, Hsiaomei, additional, Chou, Ti-Lin, additional, Cliche, Jean-Francois, additional, Crawford, Tom M., additional, Cukierman, Ari, additional, Daley, Cail, additional, de Haan, Tijmen, additional, Denison, Edward V., additional, Dibert, Karia, additional, Ding, Junjia, additional, Dobbs, Matt A., additional, Dutcher, Daniel, additional, Elleflot, Tucker, additional, Everett, Wendeline, additional, Feng, Cahng, additional, Ferguson, Kyle R., additional, Foster, Allen, additional, Fu, Jianyang, additional, Galli, Silvia, additional, Gambrel, Anne E., additional, Gardner, Robert W., additional, Goeckner-Wald, Neil, additional, Groh, John C., additional, Gualtieri, Riccardo, additional, Guns, Sam, additional, Gupta, Nikhel, additional, Guyser, Robert, additional, Halverson, Nils W., additional, Harke-Hosemann, Angelina H., additional, Harrington, Nicholas L., additional, Henning, Jason W., additional, Hilton, Gene C., additional, Hivon, Eric, additional, Holzapfel, William L., additional, Hood, John C., additional, Howe, Doug, additional, Huang, Nicholas, additional, Irwin, Kent D., additional, Jeong, Oliver B., additional, Jonas, Michelle, additional, Jones, Adam, additional, Khaire, Trupti S., additional, Knox, Lloyd, additional, Kofman, Anna M., additional, Korman, Milo, additional, Kubik, Donna L., additional, Kuhlmann, Stephen, additional, Kuo, Chao-Lin, additional, Lee, Adrian T., additional, Leitch, Erik M., additional, Lowitz, Amy E., additional, Lu, Chunyu, additional, Meyer, Stephan S., additional, Michalik, Daniel, additional, Millea, Marius, additional, Nadolski, Andrew, additional, Natoli, Tyler, additional, Nguyen, Hogan, additional, Noble, Gavin I., additional, Novosad, Valentine, additional, Omori, Yuuki, additional, Padin, Steve, additional, Pan, Zhaodi, additional, Paschos, Pascal, additional, Pearson, John, additional, Posada, Chrystian M., additional, Prabhu, Karthik, additional, Quan, Wei, additional, Rahlin, Alexandra, additional, Reichardt, Christian L., additional, Riebel, David, additional, Riedel, Benedikt, additional, Rouble, Maclean, additional, Ruhl, John E., additional, Sayre, James T., additional, Schiappucci, Eduardo, additional, Shirokoff, Erik, additional, Smecher, Graeme, additional, Sobrin, Joshua A., additional, Stark, Antony A., additional, Stephen, Judith, additional, Story, Kyle T., additional, Suzuki, Aritoki, additional, Thompson, Keith L., additional, Thorne, Ben, additional, Tucker, Carole, additional, Umilta, Caterina, additional, Vale, Leila R., additional, Vanderlinde, Keith, additional, Vieira, Joaquin D., additional, Wang, Gensheng, additional, Whitehorn, Nathan, additional, Wu, Wai L. K., additional, Yefremenko, Volodymyr, additional, Yoon, Ki W., additional, and Young, Matt R., additional

Published
2022
Full Text
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34. Event Horizon Telescope imaging of the archetypal blazar 3C 279 at an extreme 20 microarcsecond resolution

Author

Kim, Jae-Young, Krichbaum, Thomas P., Broderick, Avery E., Wielgus, Maciek, Blackburn, Lindy, Gomez, Jose L., Johnson, Michael D., Bouman, Katherine L., Chael, Andrew, Akiyama, Kazunori, Jorstad, Svetlana, Marscher, Alan P., Issaoun, Sara, Janssen, Michael, Chan, Chi-kwan, Savolainen, Tuomas, Pesce, Dominic W., Ozel, Feryal, Alberdi, Antxon, Alef, Walter, Asada, Keiichi, Azulay, Rebecca, Baczko, Anne-Kathrin, Ball, David, Balokovic, Mislav, Barrett, John, Bintley, Dan, Boland, Wilfred, Bower, Geoffrey C., Bremer, Michael, Brinkerink, Christiaan D., Brissenden, Roger, Britzen, Silke, Broguiere, Dominique, Bronzwaer, Thomas, Byun, Do-Young, Carlstrom, John E., Chatterjee, Shami, Chatterjee, Koushik, Chen, Ming-Tang, Chen, Yongjun, Cho, Ilje, Christian, Pierre, Conway, John E., Cordes, James M., Crew, Geoffrey B., Cui, Yuzhu, Davelaar, Jordy, De Laurentis, Mariafelicia, Deane, Roger, Dempsey, Jessica, Desvignes, Gregory, Dexter, Jason, Doeleman, Sheperd S., Eatough, Ralph P., Falcke, Heino, Fish, Vincent L., Fomalont, Ed, Fraga-Encinas, Raquel, Friberg, Per, Fromm, Christian M., Galison, Peter, Gammie, Charles F., Garcia, Roberto, Gentaz, Olivier, Georgiev, Boris, Goddi, Ciriaco, Gold, Roman, Gu, Minfeng, Gurwell, Mark, Hada, Kazuhiro, Hecht, Michael H., Hesper, Ronald, Ho, Luis C., Ho, Paul, Honma, Mareki, Huang, Chih-Wei L., Huang, Lei, Hughes, David H., Ikeda, Shiro, Inoue, Makoto, James, David J., Jannuzi, Buell T., Jeter, Britton, Jiang, Wu, Jimenez-Rosales, Alejandra, Jung, Taehyun, Karami, Mansour, Karuppusamy, Ramesh, Kawashima, Tomohisa, Keating, Garrett K., Kettenis, Mark, Kim, Junhan, Kim, Jongsoo, Kino, Motoki, Koay, Jun Yi, Koch, Patrick M., Koyama, Shoko, Kramer, Michael, Kramer, Carsten, Kuo, Cheng-Yu, Lauer, Tod R., Lee, Sang-Sung, Li, Yan-Rong, Li, Zhiyuan, Lindqvist, Michael, Lico, Rocco, Liu, Kuo, Liuzzo, Elisabetta, Lo, Wen-Ping, Lobanov, Andrei P., Loinard, Laurent, Lonsdale, Colin, Lu, Ru-Sen, MacDonald, Nicholas R., Mao, Jirong, Markoff, Sera, Marrone, Daniel P., Marti-Vidal, Ivan, Matsushita, Satoki, Matthews, Lynn D., Medeiros, Lia, Menten, Karl M., Mizuno, Yosuke, Mizuno, Izumi, Moran, James M., Moriyama, Kotaro, Moscibrodzka, Monika, Mueller, Cornelia, Nagai, Hiroshi, Nagar, Neil M., Nakamura, Masanori, Narayan, Ramesh, Narayanan, Gopal, Natarajan, Iniyan, Neri, Roberto, Ni, Chunchong, Noutsos, Aristeidis, Okino, Hiroki, Olivares, Hector, Ortiz-Leon, Gisela N., Oyama, Tomoaki, Palumbo, Daniel C. M., Park, Jongho, Patel, Nimesh, Pen, Ue-Li, Pietu, Vincent, Plambeck, Richard, PopStefanija, Aleksandar, Porth, Oliver, Prather, Ben, Preciado-Lopez, Jorge A., Psaltis, Dimitrios, Pu, Hung-Yi, Ramakrishnan, Venkatessh, Rao, Ramprasad, Rawlings, Mark G., Raymond, Alexander W., Rezzolla, Luciano, Ripperda, Bart, Roelofs, Freek, Rogers, Alan, Ros, Eduardo, Rose, Mel, Roshanineshat, Arash, Rottmann, Helge, Roy, Alan L., Ruszczyk, Chet, Ryan, Benjamin R., Rygl, Kazi L. J., Sanchez, Salvador, Sanchez-Arguelles, David, Sasada, Mahito, Schloerb, F. Peter, Schuster, Karl-Friedrich, Shao, Lijing, Shen, Zhiqiang, Small, Des, Sohn, Bong Won, SooHoo, Jason, Tazaki, Fumie, Tiede, Paul, Tilanus, Remo P. J., Titus, Michael, Toma, Kenji, Torne, Pablo, Trent, Tyler, Traianou, Efthalia, Trippe, Sascha, Tsuda, Shuichiro, van Bemmel, Ilse, van Langevelde, Huib Jan, van Rossum, Daniel R., Wagner, Jan, Wardle, John, Ward-Thompson, Derek, Weintroub, Jonathan, Wex, Norbert, Wharton, Robert, Wong, George N., Wu, Qingwen, Yoon, Doosoo, Young, Andre, Young, Ken, Younsi, Ziri, Yuan, Feng, Yuan, Ye-Fei, Zensus, J. Anton, Zhao, Guangyao, Zhao, Shan-Shan, Zhu, Ziyan, Algaba, Juan-Carlos, Allardi, Alexander, Amestica, Rodrigo, Anczarski, Jadyn, Bach, Uwe, Baganoff, Frederick K., Beaudoin, Christopher, Benson, Bradford A., Berthold, Ryan, Blanchard, Jay M., Blundell, Ray, Bustamente, Sandra, Cappallo, Roger, Castillo-Dominguez, Edgar, Chang, Chih-Cheng, Chang, Shu-Hao, Chang, Song-Chu, Chen, Chung-Chen, Chilson, Ryan, Chuter, Tim C., Rosado, Rodrigo Cordova, Coulson, Iain M., Crowley, Joseph, Derome, Mark, Dexter, Matthew, Dornbusch, Sven, Dudevoir, Kevin A., Dzib, Sergio A., Eckart, Andreas, Eckert, Chris, Erickson, Neal R., Everett, Wendeline B., Faber, Aaron, Farah, Joseph R., Fath, Vernon, Folkers, Thomas W., Forbes, David C., Freund, Robert, Gomez-Ruiz, Arturo, I, Gale, David M., Gao, Feng, Geertsema, Gertie, Graham, David A., Greer, Christopher H., Grosslein, Ronald, Gueth, Frederic, Haggard, Daryl, Halverson, Nils W., Han, Chih-Chiang, Han, Kuo-Chang, Hao, Jinchi, Hasegawa, Yutaka, Henning, Jason W., Hernandez-Gomez, Antonio, Herrero-Illana, Ruben, Heyminck, Stefan, Hirota, Akihiko, Hoge, James, Huang, Yau-De, Impellizzeri, C. M. Violette, Jiang, Homin, John, David, Kamble, Atish, Keisler, Ryan, Kimura, Kimihiro, Kono, Yusuke, Kubo, Derek, Kuroda, John, Lacasse, Richard, Laing, Robert A., Leitch, Erik M., Li, Chao-Te, Lin, Lupin C-C, Liu, Ching-Tang, Liu, Kuan-Yu, Lu, Li-Ming, Marson, Ralph G., Martin-Cocher, Pierre L., Massingill, Kyle D., Matulonis, Callie, McColl, Martin P., McWhirter, Stephen R., Messias, Hugo, Meyer-Zhao, Zheng, Michalik, Daniel, Montana, Alfredo, Montgomerie, William, Mora-Klein, Matias, Muders, Dirk, Nadolski, Andrew, Navarro, Santiago, Neilsen, Joseph, Nguyen, Chi H., Nishioka, Hiroaki, Norton, Timothy, Nowak, Michael A., Nystrom, George, Ogawa, Hideo, Oshiro, Peter, Parsons, Harriet, Penalver, Juan, Phillips, Neil M., Poirier, Michael, Pradel, Nicolas, Primiani, Rurik A., Raffin, Philippe A., Rahlin, Alexandra S., Reiland, George, Risacher, Christopher, Ruiz, Ignacio, Saez-Madain, Alejandro F., Sassella, Remi, Schellart, Pim, Shaw, Paul, Silva, Kevin M., Shiokawa, Hotaka, Smith, David R., Snow, William, Souccar, Kamal, Sousa, Don, Sridharan, T. K., Srinivasan, Ranjani, Stahm, William, Stark, Antony A., Story, Kyle, Timmer, Sjoerd T., Vertatschitsch, Laura, Walther, Craig, Wei, Ta-Shun, Whitehorn, Nathan, Whitney, Alan R., Woody, David P., Wouterloot, Jan G. A., Wright, Melvin, Yamaguchi, Paul, Yu, Chen-Yu, Zeballos, Milagros, Zhang, Shuo, Ziurys, Lucy, Kim, Jae-Young, Krichbaum, Thomas P., Broderick, Avery E., Wielgus, Maciek, Blackburn, Lindy, Gomez, Jose L., Johnson, Michael D., Bouman, Katherine L., Chael, Andrew, Akiyama, Kazunori, Jorstad, Svetlana, Marscher, Alan P., Issaoun, Sara, Janssen, Michael, Chan, Chi-kwan, Savolainen, Tuomas, Pesce, Dominic W., Ozel, Feryal, Alberdi, Antxon, Alef, Walter, Asada, Keiichi, Azulay, Rebecca, Baczko, Anne-Kathrin, Ball, David, Balokovic, Mislav, Barrett, John, Bintley, Dan, Boland, Wilfred, Bower, Geoffrey C., Bremer, Michael, Brinkerink, Christiaan D., Brissenden, Roger, Britzen, Silke, Broguiere, Dominique, Bronzwaer, Thomas, Byun, Do-Young, Carlstrom, John E., Chatterjee, Shami, Chatterjee, Koushik, Chen, Ming-Tang, Chen, Yongjun, Cho, Ilje, Christian, Pierre, Conway, John E., Cordes, James M., Crew, Geoffrey B., Cui, Yuzhu, Davelaar, Jordy, De Laurentis, Mariafelicia, Deane, Roger, Dempsey, Jessica, Desvignes, Gregory, Dexter, Jason, Doeleman, Sheperd S., Eatough, Ralph P., Falcke, Heino, Fish, Vincent L., Fomalont, Ed, Fraga-Encinas, Raquel, Friberg, Per, Fromm, Christian M., Galison, Peter, Gammie, Charles F., Garcia, Roberto, Gentaz, Olivier, Georgiev, Boris, Goddi, Ciriaco, Gold, Roman, Gu, Minfeng, Gurwell, Mark, Hada, Kazuhiro, Hecht, Michael H., Hesper, Ronald, Ho, Luis C., Ho, Paul, Honma, Mareki, Huang, Chih-Wei L., Huang, Lei, Hughes, David H., Ikeda, Shiro, Inoue, Makoto, James, David J., Jannuzi, Buell T., Jeter, Britton, Jiang, Wu, Jimenez-Rosales, Alejandra, Jung, Taehyun, Karami, Mansour, Karuppusamy, Ramesh, Kawashima, Tomohisa, Keating, Garrett K., Kettenis, Mark, Kim, Junhan, Kim, Jongsoo, Kino, Motoki, Koay, Jun Yi, Koch, Patrick M., Koyama, Shoko, Kramer, Michael, Kramer, Carsten, Kuo, Cheng-Yu, Lauer, Tod R., Lee, Sang-Sung, Li, Yan-Rong, Li, Zhiyuan, Lindqvist, Michael, Lico, Rocco, Liu, Kuo, Liuzzo, Elisabetta, Lo, Wen-Ping, Lobanov, Andrei P., Loinard, Laurent, Lonsdale, Colin, Lu, Ru-Sen, MacDonald, Nicholas R., Mao, Jirong, Markoff, Sera, Marrone, Daniel P., Marti-Vidal, Ivan, Matsushita, Satoki, Matthews, Lynn D., Medeiros, Lia, Menten, Karl M., Mizuno, Yosuke, Mizuno, Izumi, Moran, James M., Moriyama, Kotaro, Moscibrodzka, Monika, Mueller, Cornelia, Nagai, Hiroshi, Nagar, Neil M., Nakamura, Masanori, Narayan, Ramesh, Narayanan, Gopal, Natarajan, Iniyan, Neri, Roberto, Ni, Chunchong, Noutsos, Aristeidis, Okino, Hiroki, Olivares, Hector, Ortiz-Leon, Gisela N., Oyama, Tomoaki, Palumbo, Daniel C. M., Park, Jongho, Patel, Nimesh, Pen, Ue-Li, Pietu, Vincent, Plambeck, Richard, PopStefanija, Aleksandar, Porth, Oliver, Prather, Ben, Preciado-Lopez, Jorge A., Psaltis, Dimitrios, Pu, Hung-Yi, Ramakrishnan, Venkatessh, Rao, Ramprasad, Rawlings, Mark G., Raymond, Alexander W., Rezzolla, Luciano, Ripperda, Bart, Roelofs, Freek, Rogers, Alan, Ros, Eduardo, Rose, Mel, Roshanineshat, Arash, Rottmann, Helge, Roy, Alan L., Ruszczyk, Chet, Ryan, Benjamin R., Rygl, Kazi L. J., Sanchez, Salvador, Sanchez-Arguelles, David, Sasada, Mahito, Schloerb, F. Peter, Schuster, Karl-Friedrich, Shao, Lijing, Shen, Zhiqiang, Small, Des, Sohn, Bong Won, SooHoo, Jason, Tazaki, Fumie, Tiede, Paul, Tilanus, Remo P. J., Titus, Michael, Toma, Kenji, Torne, Pablo, Trent, Tyler, Traianou, Efthalia, Trippe, Sascha, Tsuda, Shuichiro, van Bemmel, Ilse, van Langevelde, Huib Jan, van Rossum, Daniel R., Wagner, Jan, Wardle, John, Ward-Thompson, Derek, Weintroub, Jonathan, Wex, Norbert, Wharton, Robert, Wong, George N., Wu, Qingwen, Yoon, Doosoo, Young, Andre, Young, Ken, Younsi, Ziri, Yuan, Feng, Yuan, Ye-Fei, Zensus, J. Anton, Zhao, Guangyao, Zhao, Shan-Shan, Zhu, Ziyan, Algaba, Juan-Carlos, Allardi, Alexander, Amestica, Rodrigo, Anczarski, Jadyn, Bach, Uwe, Baganoff, Frederick K., Beaudoin, Christopher, Benson, Bradford A., Berthold, Ryan, Blanchard, Jay M., Blundell, Ray, Bustamente, Sandra, Cappallo, Roger, Castillo-Dominguez, Edgar, Chang, Chih-Cheng, Chang, Shu-Hao, Chang, Song-Chu, Chen, Chung-Chen, Chilson, Ryan, Chuter, Tim C., Rosado, Rodrigo Cordova, Coulson, Iain M., Crowley, Joseph, Derome, Mark, Dexter, Matthew, Dornbusch, Sven, Dudevoir, Kevin A., Dzib, Sergio A., Eckart, Andreas, Eckert, Chris, Erickson, Neal R., Everett, Wendeline B., Faber, Aaron, Farah, Joseph R., Fath, Vernon, Folkers, Thomas W., Forbes, David C., Freund, Robert, Gomez-Ruiz, Arturo, I, Gale, David M., Gao, Feng, Geertsema, Gertie, Graham, David A., Greer, Christopher H., Grosslein, Ronald, Gueth, Frederic, Haggard, Daryl, Halverson, Nils W., Han, Chih-Chiang, Han, Kuo-Chang, Hao, Jinchi, Hasegawa, Yutaka, Henning, Jason W., Hernandez-Gomez, Antonio, Herrero-Illana, Ruben, Heyminck, Stefan, Hirota, Akihiko, Hoge, James, Huang, Yau-De, Impellizzeri, C. M. Violette, Jiang, Homin, John, David, Kamble, Atish, Keisler, Ryan, Kimura, Kimihiro, Kono, Yusuke, Kubo, Derek, Kuroda, John, Lacasse, Richard, Laing, Robert A., Leitch, Erik M., Li, Chao-Te, Lin, Lupin C-C, Liu, Ching-Tang, Liu, Kuan-Yu, Lu, Li-Ming, Marson, Ralph G., Martin-Cocher, Pierre L., Massingill, Kyle D., Matulonis, Callie, McColl, Martin P., McWhirter, Stephen R., Messias, Hugo, Meyer-Zhao, Zheng, Michalik, Daniel, Montana, Alfredo, Montgomerie, William, Mora-Klein, Matias, Muders, Dirk, Nadolski, Andrew, Navarro, Santiago, Neilsen, Joseph, Nguyen, Chi H., Nishioka, Hiroaki, Norton, Timothy, Nowak, Michael A., Nystrom, George, Ogawa, Hideo, Oshiro, Peter, Parsons, Harriet, Penalver, Juan, Phillips, Neil M., Poirier, Michael, Pradel, Nicolas, Primiani, Rurik A., Raffin, Philippe A., Rahlin, Alexandra S., Reiland, George, Risacher, Christopher, Ruiz, Ignacio, Saez-Madain, Alejandro F., Sassella, Remi, Schellart, Pim, Shaw, Paul, Silva, Kevin M., Shiokawa, Hotaka, Smith, David R., Snow, William, Souccar, Kamal, Sousa, Don, Sridharan, T. K., Srinivasan, Ranjani, Stahm, William, Stark, Antony A., Story, Kyle, Timmer, Sjoerd T., Vertatschitsch, Laura, Walther, Craig, Wei, Ta-Shun, Whitehorn, Nathan, Whitney, Alan R., Woody, David P., Wouterloot, Jan G. A., Wright, Melvin, Yamaguchi, Paul, Yu, Chen-Yu, Zeballos, Milagros, Zhang, Shuo, and Ziurys, Lucy

Abstract

3C 279 is an archetypal blazar with a prominent radio jet that show broadband flux density variability across the entire electromagnetic spectrum. We use an ultra-high angular resolution technique - global Very Long Baseline Interferometry (VLBI) at 1.3 mm (230 GHz) - to resolve the innermost jet of 3C 279 in order to study its fine-scale morphology close to the jet base where highly variable gamma -ray emission is thought to originate, according to various models. The source was observed during four days in April 2017 with the Event Horizon Telescope at 230 GHz, including the phased Atacama Large Millimeter/submillimeter Array (ALMA), at an angular resolution of similar to 20 mu as (at a redshift of z=0.536 this corresponds to similar to 0.13 pc similar to 1700 Schwarzschild radii with a black hole mass M-BH=8x10(8) M-circle dot). Imaging and model-fitting techniques were applied to the data to parameterize the fine-scale source structure and its variation. We find a multicomponent inner jet morphology with the northernmost component elongated perpendicular to the direction of the jet, as imaged at longer wavelengths. The elongated nuclear structure is consistent on all four observing days and across different imaging methods and model-fitting techniques, and therefore appears robust. Owing to its compactness and brightness, we associate the northern nuclear structure as the VLBI core. This morphology can be interpreted as either a broad resolved jet base or a spatially bent jet. We also find significant day-to-day variations in the closure phases, which appear most pronounced on the triangles with the longest baselines. Our analysis shows that this variation is related to a systematic change of the source structure. Two inner jet components move non-radially at apparent speeds of similar to 15 c and similar to 20 c (similar to 1.3 and similar to 1.7 mu as day(-1), respectively), which more strongly supports the scenario of traveling shocks or instabilities in a be

Published
2020

35. Overview of the medium and high frequency telescopes of the LiteBIRD space mission

Author

Lystrup, Makenzie, Montier, L, Mot, B, de Bernardis, P, Maffei, B, Pisano, G, Columbro, F, Gudmundsson, J, Henrot-Versillé, S, Lamagna, L, Montgomery, J, Prouvé, T, Russell, M, Savini, G, Stever, S, Thompson, K, Tsujimoto, M, Tucker, C, Westbrook, B, Ade, P, Adler, A, Allys, E, Arnold, K, Auguste, D, Aumont, J, Aurlien, R, Austermann, J, Baccigalupi, C, Banday, A, Banerji, R, Barreiro, R, Basak, S, Beall, J, Beck, D, Beckman, S, Bermejo, J, Bersanelli, M, Bonis, J, Borrill, J, Boulanger, F, Bounissou, S, Brilenkov, M, Brown, M, Bucher, M, Calabrese, E, Campeti, P, Carones, A, Casas, F, Challinor, A, Chan, V, Cheung, K, Chinone, Y, Cliche, J, Colombo, L, Cubas, J, Cukierman, A, Curtis, D, D'Alessandro, G, Dachlythra, N, De Petris, M, Dickinson, C, Diego-Palazuelos, P, Dobbs, M, Dotani, T, Duband, L, Duff, S, Duval, J, Ebisawa, K, Elleflot, T, Eriksen, H, Errard, J, Essinger-Hileman, T, Finelli, F, Flauger, R, Franceschet, C, Fuskeland, U, Galloway, M, Ganga, K, Gao, J, Genova-Santos, R, Gerbino, M, Gervasi, M, Ghigna, T, Gjerløw, E, Gradziel, M, Grain, J, Grupp, F, Gruppuso, A, de Haan, T, Halverson, N, Hargrave, P, Hasebe, T, Hasegawa, M, Hattori, M, Hazumi, M, Herman, D, Herranz, D, Hill, C, Hilton, G, Hirota, Y, Hivon, E, Hlozek, R, Hoshino, Y, de la Hoz, E, Hubmayr, J, Ichiki, K, Iida, T, Imada, H, Ishimura, K, Ishino, H, Jaehnig, G, Kaga, T, Kashima, S, Katayama, N, Kato, A, Kawasaki, T, Keskitalo, R, Kisner, T, Kobayashi, Y, Kogiso, N, Kogut, A, Kohri, K, Komatsu, E, Komatsu, K, Konishi, K, Krachmalnicoff, N, Kreykenbohm, I, Kuo, C, Kushino, A, Lanen, J, Lattanzi, M, Lee, A, Leloup, C, Levrier, F, Linder, E, Louis, T, Luzzi, G, Maciaszek, T, Maino, D, Maki, M, Mandelli, S, Martinez-Gonzalez, E, Masi, S, Matsumura, T, Mennella, A, Migliaccio, M, Minami, Y, Mitsuda, K, Morgante, G, Murata, Y, Murphy, J, Nagai, M, Nagano, Y, Nagasaki, T, Nagata, R, Nakamura, S, Namikawa, T, Natoli, P, Nerval, S, Nishibori, T, Nishino, H, O'Sullivan, C, Ogawa, H, Oguri, S, Ohsaki, H, Ohta, I, Okada, N, Pagano, L, Paiella, A, Paoletti, D, Patanchon, G, Peloton, J, Piacentini, F, Polenta, G, Poletti, D, Puglisi, G, Rambaud, D, Raum, C, Realini, S, Reinecke, M, Remazeilles, M, Ritacco, A, Roudil, G, Rubino-Martin, J, Sakurai, H, Sakurai, Y, Sandri, M, Sasaki, M, Scott, D, Seibert, J, Sekimoto, Y, Sherwin, B, Shinozaki, K, Shiraishi, M, Shirron, P, Signorelli, G, Smecher, G, Stompor, R, Sugai, H, Sugiyama, S, Suzuki, A, Suzuki, J, Svalheim, T, Switzer, E, Takaku, R, Takakura, H, Takakura, S, Takase, Y, Takeda, Y, Tartari, A, Taylor, E, Terao, Y, Thommesen, H, Thorne, B, Toda, T, Tomasi, M, Tominaga, M, Trappe, N, Tristram, M, Tsuji, M, Ullom, J, Vermeulen, G, Vielva, P, Villa, F, Vissers, M, Vittorio, N, Wehus, I, Weller, J, Wilms, J, Winter, B, Wollack, E, Yamasaki, N, Yoshida, T, Yumoto, J, Zannoni, M, Zonca, A, Montier, Ludovic, Mot, Baptiste, de Bernardis, Paolo, Maffei, Bruno, Pisano, Giampaolo, Columbro, Fabio, Gudmundsson, Jon E., Henrot-Versillé, Sophie, Lamagna, Luca, Montgomery, Joshua, Prouvé, Thomas, Russell, Megan, Savini, Giorgio, Stever, Samantha, Thompson, Keith L., Tsujimoto, Masahiro, Tucker, Carole, Westbrook, Benjamin, Ade, Peter A., Adler, Alexandre, Allys, Erwan, Arnold, Kam, Auguste, Didier, Aumont, Jonathan, Aurlien, Ragnhild, Austermann, Jason, Baccigalupi, Carlo, Banday, Anthony J., Banerji, Ranajoy, Barreiro, Rita B., Basak, Soumen, Beall, Jim, Beck, Dominic, Beckman, Shawn, Bermejo, Juan, Bersanelli, Marco, Bonis, Julien, Borrill, Julian, Boulanger, Francois, Bounissou, Sophie, Brilenkov, Maksym, Brown, Michael, Bucher, Martin, Calabrese, Erminia, Campeti, Paolo, Carones, Alessandro, Casas, Francisco J., Challinor, Anthony, Chan, Victor, Cheung, Kolen, Chinone, Yuji, Cliche, Jean F., Colombo, Loris, Cubas, Javier, Cukierman, Ari, Curtis, David, D'Alessandro, Giuseppe, Dachlythra, Nadia, De Petris, Marco, Dickinson, Clive, Diego-Palazuelos, Patricia, Dobbs, Matt, Dotani, Tadayasu, Duband, Lionel, Duff, Shannon, Duval, Jean M., Ebisawa, Ken, Elleflot, Tucker, Eriksen, Hans K., Errard, Josquin, Essinger-Hileman, Thomas, Finelli, Fabio, Flauger, Raphael, Franceschet, Cristian, Fuskeland, Unni, Galloway, Mathew, Ganga, Ken, Gao, Jian R., Genova-Santos, Ricardo, Gerbino, Martina, Gervasi, Massimo, Ghigna, Tommaso, Gjerløw, Eirik, Gradziel, Marcin L., Grain, Julien, Grupp, Frank, Gruppuso, Alessandro, de Haan, Tijmen, Halverson, Nils W., Hargrave, Peter, Hasebe, Takashi, Hasegawa, Masaya, Hattori, Makoto, Hazumi, Masashi, Herman, Daniel, Herranz, Diego, Hill, Charles A., Hilton, Gene, Hirota, Yukimasa, Hivon, Eric, Hlozek, Renee A., Hoshino, Yurika, de la Hoz, Elena, Hubmayr, Johannes, Ichiki, Kiyotomo, Iida, Teruhito, Imada, Hiroaki, Ishimura, Kosei, Ishino, Hirokazu, Jaehnig, Greg, Kaga, Tooru, Kashima, Shingo, Katayama, Nobuhiko, Kato, Akihiro, Kawasaki, Takeo, Keskitalo, Reijo, Kisner, Theodore, Kobayashi, Yohei, Kogiso, Nozomu, Kogut, Alan, Kohri, Kazunori, Komatsu, Eiichiro, Komatsu, Kunimoto, Konishi, Kuniaki, Krachmalnicoff, Nicoletta, Kreykenbohm, Ingo, Kuo, Chao-Lin L., Kushino, Akihiro, Lanen, Jeff V., Lattanzi, Massimiliano, Lee, Adrian T., Leloup, Clément, Levrier, François, Linder, Eric, Louis, Thibaut, Luzzi, Gemma, Maciaszek, Thierry, Maino, Davide, Maki, Muneyoshi, Mandelli, Stefano, Martinez-Gonzalez, Enrique, Masi, Silvia, Matsumura, Tomotake, Mennella, Aniello, Migliaccio, Marina, Minami, Yuto, Mitsuda, Kazuhisa, Morgante, Gianluca, Murata, Yasuhiro, Murphy, John A., Nagai, Makoto, Nagano, Yuya, Nagasaki, Taketo, Nagata, Ryo, Nakamura, Shogo, Namikawa, Toshiya, Natoli, Paolo, Nerval, Simran, Nishibori, Toshiyuki, Nishino, Haruki, O'Sullivan, Créidhe, Ogawa, Hideo, Ogawa, Hiroyuki, Oguri, Shugo, Ohsaki, Hiroyuki, Ohta, Izumi S., Okada, Norio, Okada, Nozomi, Pagano, Luca, Paiella, Alessandro, Paoletti, Daniela, Patanchon, Guillaume, Peloton, Julien, Piacentini, Francesco, Polenta, Gianluca, Poletti, Davide, Puglisi, Giuseppe, Rambaud, Damien, Raum, Christopher, Realini, Sabrina, Reinecke, Martin, Remazeilles, Mathieu, Ritacco, Alessia, Roudil, Gilles, Rubino-Martin, Jose A., Sakurai, Haruyuki, Sakurai, Yuki, Sandri, Maura, Sasaki, Manami, Scott, Douglas, Seibert, Joseph, Sekimoto, Yutaro, Sherwin, Blake, Shinozaki, Keisuke, Shiraishi, Maresuke, Shirron, Peter, Signorelli, Giovanni, Smecher, Graeme, Stompor, Radek, Sugai, Hajime, Sugiyama, Shinya, Suzuki, Aritoki, Suzuki, Junichi, Svalheim, Trygve L., Switzer, Eric, Takaku, Ryota, Takakura, Hayato, Takakura, Satoru, Takase, Yusuke, Takeda, Youichi, Tartari, Andrea, Taylor, Ellen, Terao, Yutaka, Thommesen, Harald, Thorne, Ben, Toda, Takayuki, Tomasi, Maurizio, Tominaga, Mayu, Trappe, Neil, Tristram, Matthieu, Tsuji, Masatoshi, Ullom, Joe, Vermeulen, Gerard, Vielva, Patricio, Villa, Fabrizio, Vissers, Michael, Vittorio, Nicola, Wehus, Ingunn, Weller, Jochen, Wilms, Joern, Winter, Berend, Wollack, Edward J., Yamasaki, Noriko Y., Yoshida, Tetsuya, Yumoto, Junji, Zannoni, Mario, Zonca, Andrea, Lystrup, Makenzie, Montier, L, Mot, B, de Bernardis, P, Maffei, B, Pisano, G, Columbro, F, Gudmundsson, J, Henrot-Versillé, S, Lamagna, L, Montgomery, J, Prouvé, T, Russell, M, Savini, G, Stever, S, Thompson, K, Tsujimoto, M, Tucker, C, Westbrook, B, Ade, P, Adler, A, Allys, E, Arnold, K, Auguste, D, Aumont, J, Aurlien, R, Austermann, J, Baccigalupi, C, Banday, A, Banerji, R, Barreiro, R, Basak, S, Beall, J, Beck, D, Beckman, S, Bermejo, J, Bersanelli, M, Bonis, J, Borrill, J, Boulanger, F, Bounissou, S, Brilenkov, M, Brown, M, Bucher, M, Calabrese, E, Campeti, P, Carones, A, Casas, F, Challinor, A, Chan, V, Cheung, K, Chinone, Y, Cliche, J, Colombo, L, Cubas, J, Cukierman, A, Curtis, D, D'Alessandro, G, Dachlythra, N, De Petris, M, Dickinson, C, Diego-Palazuelos, P, Dobbs, M, Dotani, T, Duband, L, Duff, S, Duval, J, Ebisawa, K, Elleflot, T, Eriksen, H, Errard, J, Essinger-Hileman, T, Finelli, F, Flauger, R, Franceschet, C, Fuskeland, U, Galloway, M, Ganga, K, Gao, J, Genova-Santos, R, Gerbino, M, Gervasi, M, Ghigna, T, Gjerløw, E, Gradziel, M, Grain, J, Grupp, F, Gruppuso, A, de Haan, T, Halverson, N, Hargrave, P, Hasebe, T, Hasegawa, M, Hattori, M, Hazumi, M, Herman, D, Herranz, D, Hill, C, Hilton, G, Hirota, Y, Hivon, E, Hlozek, R, Hoshino, Y, de la Hoz, E, Hubmayr, J, Ichiki, K, Iida, T, Imada, H, Ishimura, K, Ishino, H, Jaehnig, G, Kaga, T, Kashima, S, Katayama, N, Kato, A, Kawasaki, T, Keskitalo, R, Kisner, T, Kobayashi, Y, Kogiso, N, Kogut, A, Kohri, K, Komatsu, E, Komatsu, K, Konishi, K, Krachmalnicoff, N, Kreykenbohm, I, Kuo, C, Kushino, A, Lanen, J, Lattanzi, M, Lee, A, Leloup, C, Levrier, F, Linder, E, Louis, T, Luzzi, G, Maciaszek, T, Maino, D, Maki, M, Mandelli, S, Martinez-Gonzalez, E, Masi, S, Matsumura, T, Mennella, A, Migliaccio, M, Minami, Y, Mitsuda, K, Morgante, G, Murata, Y, Murphy, J, Nagai, M, Nagano, Y, Nagasaki, T, Nagata, R, Nakamura, S, Namikawa, T, Natoli, P, Nerval, S, Nishibori, T, Nishino, H, O'Sullivan, C, Ogawa, H, Oguri, S, Ohsaki, H, Ohta, I, Okada, N, Pagano, L, Paiella, A, Paoletti, D, Patanchon, G, Peloton, J, Piacentini, F, Polenta, G, Poletti, D, Puglisi, G, Rambaud, D, Raum, C, Realini, S, Reinecke, M, Remazeilles, M, Ritacco, A, Roudil, G, Rubino-Martin, J, Sakurai, H, Sakurai, Y, Sandri, M, Sasaki, M, Scott, D, Seibert, J, Sekimoto, Y, Sherwin, B, Shinozaki, K, Shiraishi, M, Shirron, P, Signorelli, G, Smecher, G, Stompor, R, Sugai, H, Sugiyama, S, Suzuki, A, Suzuki, J, Svalheim, T, Switzer, E, Takaku, R, Takakura, H, Takakura, S, Takase, Y, Takeda, Y, Tartari, A, Taylor, E, Terao, Y, Thommesen, H, Thorne, B, Toda, T, Tomasi, M, Tominaga, M, Trappe, N, Tristram, M, Tsuji, M, Ullom, J, Vermeulen, G, Vielva, P, Villa, F, Vissers, M, Vittorio, N, Wehus, I, Weller, J, Wilms, J, Winter, B, Wollack, E, Yamasaki, N, Yoshida, T, Yumoto, J, Zannoni, M, Zonca, A, Montier, Ludovic, Mot, Baptiste, de Bernardis, Paolo, Maffei, Bruno, Pisano, Giampaolo, Columbro, Fabio, Gudmundsson, Jon E., Henrot-Versillé, Sophie, Lamagna, Luca, Montgomery, Joshua, Prouvé, Thomas, Russell, Megan, Savini, Giorgio, Stever, Samantha, Thompson, Keith L., Tsujimoto, Masahiro, Tucker, Carole, Westbrook, Benjamin, Ade, Peter A., Adler, Alexandre, Allys, Erwan, Arnold, Kam, Auguste, Didier, Aumont, Jonathan, Aurlien, Ragnhild, Austermann, Jason, Baccigalupi, Carlo, Banday, Anthony J., Banerji, Ranajoy, Barreiro, Rita B., Basak, Soumen, Beall, Jim, Beck, Dominic, Beckman, Shawn, Bermejo, Juan, Bersanelli, Marco, Bonis, Julien, Borrill, Julian, Boulanger, Francois, Bounissou, Sophie, Brilenkov, Maksym, Brown, Michael, Bucher, Martin, Calabrese, Erminia, Campeti, Paolo, Carones, Alessandro, Casas, Francisco J., Challinor, Anthony, Chan, Victor, Cheung, Kolen, Chinone, Yuji, Cliche, Jean F., Colombo, Loris, Cubas, Javier, Cukierman, Ari, Curtis, David, D'Alessandro, Giuseppe, Dachlythra, Nadia, De Petris, Marco, Dickinson, Clive, Diego-Palazuelos, Patricia, Dobbs, Matt, Dotani, Tadayasu, Duband, Lionel, Duff, Shannon, Duval, Jean M., Ebisawa, Ken, Elleflot, Tucker, Eriksen, Hans K., Errard, Josquin, Essinger-Hileman, Thomas, Finelli, Fabio, Flauger, Raphael, Franceschet, Cristian, Fuskeland, Unni, Galloway, Mathew, Ganga, Ken, Gao, Jian R., Genova-Santos, Ricardo, Gerbino, Martina, Gervasi, Massimo, Ghigna, Tommaso, Gjerløw, Eirik, Gradziel, Marcin L., Grain, Julien, Grupp, Frank, Gruppuso, Alessandro, de Haan, Tijmen, Halverson, Nils W., Hargrave, Peter, Hasebe, Takashi, Hasegawa, Masaya, Hattori, Makoto, Hazumi, Masashi, Herman, Daniel, Herranz, Diego, Hill, Charles A., Hilton, Gene, Hirota, Yukimasa, Hivon, Eric, Hlozek, Renee A., Hoshino, Yurika, de la Hoz, Elena, Hubmayr, Johannes, Ichiki, Kiyotomo, Iida, Teruhito, Imada, Hiroaki, Ishimura, Kosei, Ishino, Hirokazu, Jaehnig, Greg, Kaga, Tooru, Kashima, Shingo, Katayama, Nobuhiko, Kato, Akihiro, Kawasaki, Takeo, Keskitalo, Reijo, Kisner, Theodore, Kobayashi, Yohei, Kogiso, Nozomu, Kogut, Alan, Kohri, Kazunori, Komatsu, Eiichiro, Komatsu, Kunimoto, Konishi, Kuniaki, Krachmalnicoff, Nicoletta, Kreykenbohm, Ingo, Kuo, Chao-Lin L., Kushino, Akihiro, Lanen, Jeff V., Lattanzi, Massimiliano, Lee, Adrian T., Leloup, Clément, Levrier, François, Linder, Eric, Louis, Thibaut, Luzzi, Gemma, Maciaszek, Thierry, Maino, Davide, Maki, Muneyoshi, Mandelli, Stefano, Martinez-Gonzalez, Enrique, Masi, Silvia, Matsumura, Tomotake, Mennella, Aniello, Migliaccio, Marina, Minami, Yuto, Mitsuda, Kazuhisa, Morgante, Gianluca, Murata, Yasuhiro, Murphy, John A., Nagai, Makoto, Nagano, Yuya, Nagasaki, Taketo, Nagata, Ryo, Nakamura, Shogo, Namikawa, Toshiya, Natoli, Paolo, Nerval, Simran, Nishibori, Toshiyuki, Nishino, Haruki, O'Sullivan, Créidhe, Ogawa, Hideo, Ogawa, Hiroyuki, Oguri, Shugo, Ohsaki, Hiroyuki, Ohta, Izumi S., Okada, Norio, Okada, Nozomi, Pagano, Luca, Paiella, Alessandro, Paoletti, Daniela, Patanchon, Guillaume, Peloton, Julien, Piacentini, Francesco, Polenta, Gianluca, Poletti, Davide, Puglisi, Giuseppe, Rambaud, Damien, Raum, Christopher, Realini, Sabrina, Reinecke, Martin, Remazeilles, Mathieu, Ritacco, Alessia, Roudil, Gilles, Rubino-Martin, Jose A., Sakurai, Haruyuki, Sakurai, Yuki, Sandri, Maura, Sasaki, Manami, Scott, Douglas, Seibert, Joseph, Sekimoto, Yutaro, Sherwin, Blake, Shinozaki, Keisuke, Shiraishi, Maresuke, Shirron, Peter, Signorelli, Giovanni, Smecher, Graeme, Stompor, Radek, Sugai, Hajime, Sugiyama, Shinya, Suzuki, Aritoki, Suzuki, Junichi, Svalheim, Trygve L., Switzer, Eric, Takaku, Ryota, Takakura, Hayato, Takakura, Satoru, Takase, Yusuke, Takeda, Youichi, Tartari, Andrea, Taylor, Ellen, Terao, Yutaka, Thommesen, Harald, Thorne, Ben, Toda, Takayuki, Tomasi, Maurizio, Tominaga, Mayu, Trappe, Neil, Tristram, Matthieu, Tsuji, Masatoshi, Ullom, Joe, Vermeulen, Gerard, Vielva, Patricio, Villa, Fabrizio, Vissers, Michael, Vittorio, Nicola, Wehus, Ingunn, Weller, Jochen, Wilms, Joern, Winter, Berend, Wollack, Edward J., Yamasaki, Noriko Y., Yoshida, Tetsuya, Yumoto, Junji, Zannoni, Mario, and Zonca, Andrea

Abstract

LiteBIRD is a JAXA-led Strategic Large-Class mission designed to search for the existence of the primordial gravitational waves produced during the inflationary phase of the Universe, through the measurements of their imprint onto the polarization of the cosmic microwave background (CMB). These measurements, requiring unprecedented sensitivity, will be performed over the full sky, at large angular scales, and over 15 frequency bands from 34 GHz to 448 GHz. The LiteBIRD instruments consist of three telescopes, namely the Low-, Medium-and High-Frequency Telescope (respectively LFT, MFT and HFT). We present in this paper an overview of the design of the Medium-Frequency Telescope (89{224 GHz) and the High-Frequency Telescope (166{448 GHz), the so-called MHFT, under European responsibility, which are two cryogenic refractive telescopes cooled down to 5 K. They include a continuous rotating half-wave plate as the first optical element, two high-density polyethylene (HDPE) lenses and more than three thousand transition-edge sensor (TES) detectors cooled to 100 mK. We provide an overview of the concept design and the remaining specific challenges that we have to face in order to achieve the scientific goals of LiteBIRD.

Published
2020

36. CMB-S4 Technology Book, First Edition

Author

Abitbol, Maximilian H., Ahmed, Zeeshan, Barron, Darcy, Thakur, Ritoban Basu, Bender, Amy N., Benson, Bradford A., Bischoff, Colin A., Bryan, Sean A., Carlstrom, John E., Chang, Clarence L., Chuss, David T., Crowley, Kevin T., Cukierman, Ari, de Haan, Tijmen, Dobbs, Matt, Essinger-Hileman, Tom, Filippini, Jeffrey P., Ganga, Ken, Gudmundsson, Jon E., Halverson, Nils W., Hanany, Shaul, Henderson, Shawn W., Hill, Charles A., Ho, Shuay-Pwu P., Hubmayr, Johannes, Irwin, Kent, Jeong, Oliver, Johnson, Bradley R., Kernasovskiy, Sarah A., Kovac, John M., Kusaka, Akito, Lee, Adrian T., Maria, Salatino, Mauskopf, Philip, McMahon, Jeff J., Moncelsi, Lorenzo, Nadolski, Andrew W., Nagy, Johanna M., Niemack, Michael D., O'Brient, Roger C., Padin, Stephen, Parshley, Stephen C., Pryke, Clement, Roe, Natalie A., Rostem, Karwan, Ruhl, John, Simon, Sara M., Staggs, Suzanne T., Suzuki, Aritoki, Switzer, Eric R., Tajima, Osamu, Thompson, Keith L., Timbie, Peter, Tucker, Gregory S., Vieira, Joaquin D., Vieregg, Abigail G., Westbrook, Benjamin, Wollack, Edward J., Yoon, Ki Won, Young, Karl S., Young, Edward Y., AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), CMB-S4, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
detector: technology, Astrophysics::Instrumentation and Methods for Astrophysics, electronics: readout, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), optics, detector: design, activity report
Abstract

CMB-S4 is a proposed experiment to map the polarization of the Cosmic Microwave Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible from the ground. The science goals and capabilities of CMB-S4 in illuminating cosmic inflation, measuring the sum of neutrino masses, searching for relativistic relics in the early universe, characterizing dark energy and dark matter, and mapping the matter distribution in the universe have been described in the CMB-S4 Science Book. This Technology Book is a companion volume to the Science Book. The ambitious science goals of CMB-S4, a "Stage-4" experiment, require a step forward in experimental capability from the current Stage=II experiments. To guide this process, we summarize the current state of CMB instrumentation technology, and identify R&D efforts necessary to advance it for use in CMB-S4. The book focuses on technical challenges in four broad areas: Telescope Design; Receiver Optics; Focal-Plane Optical Coupling; and Focal-Plane Sensor and Readout., 191 pages

Published
2019

37. 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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38. LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization

Author

Hazumi, Masashi, primary, Ade, Peter A., additional, Adler, Alexandre, additional, Allys, Erwan, additional, Arnold, Kam, additional, Auguste, Didier, additional, Aumont, Jonathan, additional, Aurlien, Ragnhild, additional, Austermann, Jason, additional, Baccigalupi, Carlo, additional, Banday, Anthony J., additional, Banjeri, R., additional, Barreiro, Rita B., additional, Basak, Soumen, additional, Beall, Jim, additional, Beck, Dominic, additional, Beckman, Shawn, additional, Bermejo, Juan, additional, de Bernardis, Paolo, additional, Bersanelli, Marco, additional, Bonis, Julien, additional, Borrill, Julian, additional, Boulanger, Francois, additional, Bounissou, Sophie, additional, Brilenkov, Maksym, additional, Brown, Michael, additional, Bucher, Martin, additional, Calabrese, Erminia, additional, Campeti, Paolo, additional, Carones, Alessandro, additional, Casas, Francisco J., additional, Challinor, Anthony, additional, Chan, Victor, additional, Cheung, Kolen, additional, Chinone, Yuji, additional, Cliche, Jean F., additional, Colombo, Loris, additional, Columbro, Fabio, additional, Cubas, Javier, additional, Cukierman, Ari, additional, Curtis, David, additional, D'Alessandro, Giuseppe, additional, Dachlythra, Nadia, additional, De Petris, Marco, additional, Dickinson, Clive, additional, Diego-Palazuelos, Patricia, additional, Dobbs, Matt, additional, Dotani, Tadayasu, additional, Duband, Lionel, additional, Duff, Shannon, additional, Duval, Jean M., additional, Ebisawa, Ken, additional, Elleflot, Tucker, additional, Eriksen, Hans K., additional, Errard, Josquin, additional, Essinger-Hileman, Thomas, additional, Finelli, Fabio, additional, Flauger, Raphael, additional, Franceschet, Cristian, additional, Fuskeland, Unni, additional, Galloway, Mathew, additional, Ganga, Ken, additional, Gao, Jian R., additional, Genova-Santos, Ricardo, additional, Gerbino, Martina, additional, Gervasi, Massimo, additional, Ghigna, Tommaso, additional, Gjerløw, Eirik, additional, Gradziel, Marcin L., additional, Grain, Julien, additional, Grupp, Frank, additional, Gruppuso, Alessandro, additional, Gudmundsson, Jon E., additional, de Haan, Tijmen, additional, Halverson, Nils W., additional, Hargrave, Peter, additional, Hasebe, Takashi, additional, Hasegawa, Masaya, additional, Hattori, Makoto, additional, Henrot-Versillé, Sophie, additional, Herman, Daniel, additional, Herranz, Diego, additional, Hill, Charles A., additional, Hilton, Gene, additional, Hirota, Yukimasa, additional, Hivon, Eric, additional, Hlozek, Renee A., additional, Hoshino, Yurika, additional, de la Hoz, Elena, additional, Hubmayr, Johannes, additional, Ichiki, Kiyotomo, additional, Iida, Teruhito, additional, Imada, Hiroaki, additional, Ishimura, Kosei, additional, Ishino, Hirokazu, additional, Jaehnig, Greg, additional, Kaga, Tooru, additional, Kashima, Shingo, additional, Katayama, Nobuhiko, additional, Kato, Akihiro, additional, Kawasaki, Takeo, additional, Keskitalo, Reijo, additional, Kisner, Theodore, additional, Kobayashi, Yohei, additional, Kogiso, Nozomu, additional, Kogut, Alan, additional, Kohri, Kazunori, additional, Komatsu, Eiichiro, additional, Komatsu, Kunimoto, additional, Konishi, Kuniaki, additional, Krachmalnicoff, Nicoletta, additional, Kreykenbohm, Ingo, additional, Kuo, Chao-Lin L., additional, Kushino, Akihiro, additional, Lamagna, Luca, additional, Lanen, Jeff V., additional, Lattanzi, Massimiliano, additional, Lee, Adrian T., additional, Leloup, Clément, additional, Levrier, François, additional, Linder, Eric, additional, Louis, Thibaut, additional, Luzzi, Gemma, additional, Maciaszek, Thierry, additional, Maffei, Bruno, additional, Maino, Davide, additional, Maki, Muneyoshi, additional, Mandelli, Stefano, additional, Martinez-Gonzalez, Enrique, additional, Masi, Silvia, additional, Matsumura, Tomotake, additional, Mennella, Aniello, additional, Migliaccio, Marina, additional, Minami, Yuto, additional, Mitsuda, Kazuhisa, additional, Montgomery, Joshua, additional, Montier, Ludovic, additional, Morgante, Gianluca, additional, Mot, Baptiste, additional, Murata, Yasuhiro, additional, Murphy, John A., additional, Nagai, Makoto, additional, Nagano, Yuya, additional, Nagasaki, Taketo, additional, Nagata, Ryo, additional, Nakamura, Shogo, additional, Namikawa, Toshiya, additional, Natoli, Paolo, additional, Nerval, Simran, additional, Nishibori, Toshiyuki, additional, Nishino, Haruki, additional, Noviello, Fabio, additional, O'Sullivan, Créidhe, additional, Ogawa, Hideo, additional, Ogawa, Hiroyuki, additional, Oguri, Shugo, additional, Ohsaki, Hiroyuki, additional, Ohta, Izumi S., additional, Okada, Norio, additional, Okada, Nozomi, additional, Pagano, Luca, additional, Paiella, Alessandro, additional, Paoletti, Daniela, additional, Patanchon, Guillaume, additional, Peloton, Julien, additional, Piacentini, Francesco, additional, Pisano, Giampaolo, additional, Polenta, Gianluca, additional, Poletti, Davide, additional, Prouvé, Thomas, additional, Puglisi, Giuseppe, additional, Rambaud, Damien, additional, Raum, Christopher, additional, Realini, Sabrina, additional, Reinecke, Martin, additional, Remazeilles, Mathieu, additional, Ritacco, Alessia, additional, Roudil, Gilles, additional, Rubino-Martin, Jose A., additional, Russell, Megan, additional, Sakurai, Haruyuki, additional, Sakurai, Yuki, additional, Sandri, Maura, additional, Sasaki, Manami, additional, Savini, Giorgio, additional, Scott, Douglas, additional, Seibert, Joseph, additional, Sekimoto, Yutaro, additional, Sherwin, Blake, additional, Shinozaki, Keisuke, additional, Shiraishi, Maresuke, additional, Shirron, Peter, additional, Signorelli, Giovanni, additional, Smecher, Graeme, additional, Stever, Samantha, additional, Stompor, Radek, additional, Sugai, Hajime, additional, Sugiyama, Shinya, additional, Suzuki, Aritoki, additional, Suzuki, Junichi, additional, Svalheim, Trygve L., additional, Switzer, Eric, additional, Takaku, Ryota, additional, Takakura, Hayato, additional, Takakura, Satoru, additional, Takase, Yusuke, additional, Takeda, Youichi, additional, Tartari, Andrea, additional, Taylor, Ellen, additional, Terao, Yutaka, additional, Thommesen, Harald, additional, Thompson, Keith L., additional, Thorne, Ben, additional, Toda, Takayuki, additional, Tomasi, Maurizio, additional, Tominaga, Mayu, additional, Trappe, Neil, additional, Tristram, Matthieu, additional, Tsuji, Masatoshi, additional, Tsujimoto, Masahiro, additional, Tucker, Carole, additional, Ullom, Joe, additional, Vermeulen, Gerard, additional, Vielva, Patricio, additional, Villa, Fabrizio, additional, Vissers, Michael, additional, Vittorio, Nicola, additional, Wehus, Ingunn, additional, Weller, Jochen, additional, Westbrook, Benjamin, additional, Wilms, Joern, additional, Winter, Berend, additional, Wollack, Edward J., additional, Yamasaki, Noriko Y., additional, Yoshida, Tetsuya, additional, Yumoto, Junji, additional, Zannoni, Mario, additional, and Zonca, Andrea, additional

Published
2020
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39. Concept design of low frequency telescope for CMB B-mode polarization satellite LiteBIRD

Author

Sekimoto, Yutaro, primary, Ade, Peter, additional, Adler, Alexandre, additional, Allys, Erwan, additional, Arnold, Kam, additional, Auguste, Didier, additional, Aumont, Jonathan, additional, Aurlien, Ragnhild, additional, Austermann, Jason, additional, Baccigalupi, Carlo, additional, Banday, Anthony, additional, Banerji, Ranajoy, additional, Barreiro, Rita, additional, Basak, Soumen, additional, Beall, Jim, additional, Beck, Dominic, additional, Beckman, Shawn, additional, Bermejo, Juan, additional, de Bernardis, Paolo, additional, Bersanelli, Marco, additional, Bonis, Julien, additional, Borrill, Julian, additional, Boulanger, Francois, additional, Bounissou, Sophie, additional, Brilenkov, Maksym, additional, Brown, Michael, additional, Bucher, Martin, additional, Calabrese, Erminia, additional, Campeti, Paolo, additional, Carones, Alessandro, additional, Casas, Francisco, additional, Challinor, Anthony, additional, Chan, Victor, additional, Cheung, Kolen, additional, Chinone, Yuji, additional, Cliche, Jean, additional, Colombo, Loris, additional, Columbro, Fabio, additional, Cubas, Javier, additional, Cukierman, Ari, additional, Curtis, David, additional, D'Alessandro, Giuseppe, additional, Dachlythra, Nadia, additional, De Petris, Marco, additional, Dickinson, Clive, additional, Diego-Palazuelos, Patricia, additional, Dobbs, Matt, additional, Dotani, Tadayasu, additional, Duband, Lionel, additional, Duff, Shannon, additional, Duval, Jean, additional, Ebisawa, Ken, additional, Elleflot, Tucker, additional, Eriksen, Hans, additional, Errard, Josquin, additional, Essinger-Hileman, Thomas, additional, Finelli, Fabio, additional, Flauger, Raphael, additional, Franceschet, Cristian, additional, Fuskeland, Unni, additional, Galloway, Mathew, additional, Ganga, Ken, additional, Gao, Jian, additional, Genova-Santos, Ricardo, additional, Gerbino, Martina, additional, Gervasi, Massimo, additional, Ghigna, Tommaso, additional, Gjerløw, Eirik, additional, Gradziel, Marcin, additional, Grain, Julien, additional, Grupp, Frank, additional, Gruppuso, Alessandro, additional, Gudmundsson, Jon, additional, de Haan, Tijmen, additional, Halverson, Nils, additional, Hargrave, Peter, additional, Hasebe, Takashi, additional, Hasegawa, Masaya, additional, Hattori, Makoto, additional, Hazumi, Masashi, additional, Henrot-Versillé, Sophie, additional, Herman, Daniel, additional, Herranz, Diego, additional, Hill, Charles, additional, Hilton, Gene, additional, Hirota, Yukimasa, additional, hivon, Eric, additional, Hlozek, Renee, additional, Hoshino, Yurika, additional, de la Hoz, Elena, additional, Hubmayr, Johannes, additional, Ichiki, Kiyotomo, additional, iida, Teruhito, additional, Imada, Hiroaki, additional, Ishimura, Kosei, additional, Ishino, Hirokazu, additional, Jaehnig, Greg, additional, Kaga, Tooru, additional, Kashima, Shingo, additional, Katayama, Nobuhiko, additional, Kato, Akihiro, additional, Kawasaki, Takeo, additional, Keskitalo, Reijo, additional, Kisner, Theodore, additional, Kobayashi, Yohei, additional, Kogiso, Nozomu, additional, Kogut, Alan, additional, Kohri, Kazunori, additional, Komatsu, Eiichiro, additional, Komatsu, Kunimoto, additional, Konishi, Kuniaki, additional, Krachmalnicoff, Nicoletta, additional, Kreykenbohm, Ingo, additional, Kuo, Chao-Lin, additional, Kushino, Akihiro, additional, Lamagna, Luca, additional, Lanen, Jeff, additional, Lattanzi, Massimiliano, additional, Lee, Adrien, additional, Leloup, Clément, additional, Levrier, François, additional, Linder, Eric, additional, Louis, Thibaut, additional, Luzzi, Gemma, additional, Maciaszek, Thierry, additional, Maffei, Bruno, additional, Maino, Davide, additional, Maki, Muneyoshi, additional, Mandelli, Stefano, additional, Martinez-Gonzalez, Enrique, additional, Masi, Silvia, additional, Matsumura, Tomotake, additional, Mennella, Aniello, additional, Migliaccio, Marina, additional, Minanmi, Yuto, additional, Mitsuda, Kazuhisa, additional, Montgomery, Josua, additional, Montier, Ludovic, additional, Morgante, Gianluca, additional, Mot, Baptise, additional, Murata, Yasuhiro, additional, Murphy, John, additional, Nagai, Makoto, additional, Nagano, Yuya, additional, Nagasaki, Takeo, additional, Nagata, Ryo, additional, Nakamura, Shogo, additional, Namikawa, Toshiya, additional, Natoli, Paolo, additional, Nerval, Simran, additional, Nishibori, Toshiyuki, additional, Nishino, Haruki, additional, O'Sullivan, Créidhe, additional, Ogawa, Hideo, additional, Ogawa, Hiroyuki, additional, Oguri, Shogo, additional, Osaki, Hiroyuki, additional, Ohta, Izumi, additional, Okada, Norio, additional, Okada, Nozomi, additional, Pagano, Luca, additional, Paiella, Alessandro, additional, Paoletti, Daniela, additional, Patanchon, Guillaume, additional, Peloton, Julien, additional, Piacentini, Francesco, additional, Pisano, Giampaolo, additional, Polenta, Gianluca, additional, Poletti, Davide, additional, Prouvé, Thomas, additional, Puglisi, Giuseppe, additional, Tambaud, Damien, additional, Raum, Christopher, additional, Realini, Sabrina, additional, Reinecke, Martin, additional, Remazeilles, Mathieu, additional, Ritacco, Alessa, additional, Roudil, Gilles, additional, Rubino-Martin, Jose, additional, Russell, Megan, additional, Sakurai, Haruyuki, additional, Sakurai, Yuki, additional, Sandri, Maura, additional, Sasaki, Manami, additional, Savini, Giorgio, additional, Scott, Douglas, additional, Seibert, Joseph, additional, Sherwin, Blake, additional, Shinozaki, Keisuke, additional, Shiraishi, Maresuke, additional, Shirron, Peter, additional, Signorelli, Giovanni, additional, Smecher, Graeme, additional, Stever, Samantha, additional, Stompor, Radek, additional, Sugai, Hajime, additional, Sugiyama, Shinya, additional, Suzuki, aritoki, additional, Suzuki, Junichi, additional, Svalheim, Trygve, additional, Switzer, Eric, additional, Takaku, Ryota, additional, Takakura, hayato, additional, Takakura, satoru, additional, Takase, Yusuke, additional, Takeda, Youichi, additional, Tartari, Andrea, additional, Taylor, Ellen, additional, Terao, Yutaka, additional, Thommesen, Harald, additional, Thompson, Keith L., additional, Thorne, Ben, additional, Toda, Takayuki, additional, Tomasi, Maurizio, additional, Tominaga, Mayu, additional, Trappe, Neil, additional, Tristram, Matthieu, additional, Tsuji, Masatoshi, additional, Tsujimoto, Masahiro, additional, Tucker, Carole, additional, Ullom, Joe, additional, Vermeulen, Gerard, additional, Vielva, Patricio, additional, Villa, Fabrizio, additional, Vissers, Michael, additional, Vittorio, Nicola, additional, Wehus, Ingunn, additional, Weller, Jochen, additional, Westbrook, Benjamin, additional, Wilms, Joern, additional, Winter, Berend, additional, Wollack, Edward, additional, Yamasaki, Noriko Y., additional, Yoshida, Tetsuya, additional, Yumoto, Junji, additional, Zannoni, Mario, additional, and Zonca, Andrea, additional

Published
2020
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40. Detector fabrication development for the LiteBIRD satellite mission

Author

Westbrook, Benjamin, primary, Raum, Christopher, additional, Beckman, Shawn, additional, Lee, Adrian, additional, Farias, Nicole, additional, Sasse, Trevor, additional, Suzuki, Aritoki, additional, Kane, Elijah, additional, Austermann, Jay E., additional, Beall, James A., additional, Duff, Shannon, additional, Hubmayr, Johannes, additional, Hilton, Gene, additional, Van Lanen, Jeff, additional, Vissers, Michael, additional, Link, Michael, additional, Halverson, Nils, additional, Jaehnig, Gregory, additional, Ghinga, Tommasso, additional, Stever, Samantha, additional, Minami, Yuto, additional, Thompson, Keith L., additional, Russell, Megan, additional, Arnold, Kam, additional, Seibert, Joseph, additional, and Silva-Feaver, Maximiliano, additional

Published
2020
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41. Overview of the medium and high frequency telescopes of the LiteBIRD space mission

Author

Montier, Ludovic, primary, Mot, Baptiste, additional, de Bernardis, Paolo, additional, Maffei, Bruno, additional, Pisano, Giampaolo, additional, Columbro, Fabio, additional, Gudmundsson, Jon E., additional, Henrot-Versillé, Sophie, additional, Lamagna, Luca, additional, Montgomery, Joshua, additional, Prouvé, Thomas, additional, Russell, Megan, additional, Savini, Giorgio, additional, Stever, Samantha, additional, Thompson, Keith L., additional, Tsujimoto, Masahiro, additional, Tucker, Carole, additional, Westbrook, Benjamin, additional, Ade, Peter A., additional, Adler, Alexandre, additional, Allys, Erwan, additional, Arnold, Kam, additional, Auguste, Didier, additional, Aumont, Jonathan, additional, Aurlien, Ragnhild, additional, Austermann, Jason, additional, Baccigalupi, Carlo, additional, Banday, Anthony J., additional, Banerji, Ranajoy, additional, Barreiro, Rita B., additional, Basak, Soumen, additional, Beall, Jim, additional, Beck, Dominic, additional, Beckman, Shawn, additional, Bermejo, Juan, additional, Bersanelli, Marco, additional, Bonis, Julien, additional, Borrill, Julian, additional, Boulanger, Francois, additional, Bounissou, Sophie, additional, Brilenkov, Maksym, additional, Brown, Michael, additional, Bucher, Martin, additional, Calabrese, Erminia, additional, Campeti, Paolo, additional, Carones, Alessandro, additional, Casas, Francisco J., additional, Challinor, Anthony, additional, Chan, Victor, additional, Cheung, Kolen, additional, Chinone, Yuji, additional, Cliche, Jean F., additional, Colombo, Loris, additional, Cubas, Javier, additional, Cukierman, Ari, additional, Curtis, David, additional, D'Alessandro, Giuseppe, additional, Dachlythra, Nadia, additional, De Petris, Marco, additional, Dickinson, Clive, additional, Diego-Palazuelos, Patricia, additional, Dobbs, Matt, additional, Dotani, Tadayasu, additional, Duband, Lionel, additional, Duff, Shannon, additional, Duval, Jean M., additional, Ebisawa, Ken, additional, Elleflot, Tucker, additional, Eriksen, Hans K., additional, Errard, Josquin, additional, Essinger-Hileman, Thomas, additional, Finelli, Fabio, additional, Flauger, Raphael, additional, Franceschet, Cristian, additional, Fuskeland, Unni, additional, Galloway, Mathew, additional, Ganga, Ken, additional, Gao, Jian R., additional, Genova-Santos, Ricardo, additional, Gerbino, Martina, additional, Gervasi, Massimo, additional, Ghigna, Tommaso, additional, Gjerløw, Eirik, additional, Gradziel, Marcin L., additional, Grain, Julien, additional, Grupp, Frank, additional, Gruppuso, Alessandro, additional, de Haan, Tijmen, additional, Halverson, Nils W., additional, Hargrave, Peter, additional, Hasebe, Takashi, additional, Hasegawa, Masaya, additional, Hattori, Makoto, additional, Hazumi, Masashi, additional, Herman, Daniel, additional, Herranz, Diego, additional, Hill, Charles A., additional, Hilton, Gene, additional, Hirota, Yukimasa, additional, Hivon, Eric, additional, Hlozek, Renee A., additional, Hoshino, Yurika, additional, de la Hoz, Elena, additional, Hubmayr, Johannes, additional, Ichiki, Kiyotomo, additional, Iida, Teruhito, additional, Imada, Hiroaki, additional, Ishimura, Kosei, additional, Ishino, Hirokazu, additional, Jaehnig, Greg, additional, Kaga, Tooru, additional, Kashima, Shingo, additional, Katayama, Nobuhiko, additional, Kato, Akihiro, additional, Kawasaki, Takeo, additional, Keskitalo, Reijo, additional, Kisner, Theodore, additional, Kobayashi, Yohei, additional, Kogiso, Nozomu, additional, Kogut, Alan, additional, Kohri, Kazunori, additional, Komatsu, Eiichiro, additional, Komatsu, Kunimoto, additional, Konishi, Kuniaki, additional, Krachmalnicoff, Nicoletta, additional, Kreykenbohm, Ingo, additional, Kuo, Chao-Lin L., additional, Kushino, Akihiro, additional, Lanen, Jeff V., additional, Lattanzi, Massimiliano, additional, Lee, Adrian T., additional, Leloup, Clément, additional, Levrier, François, additional, Linder, Eric, additional, Louis, Thibaut, additional, Luzzi, Gemma, additional, Maciaszek, Thierry, additional, Maino, Davide, additional, Maki, Muneyoshi, additional, Mandelli, Stefano, additional, Martinez-Gonzalez, Enrique, additional, Masi, Silvia, additional, Matsumura, Tomotake, additional, Mennella, Aniello, additional, Migliaccio, Marina, additional, Minami, Yuto, additional, Mitsuda, Kazuhisa, additional, Morgante, Gianluca, additional, Murata, Yasuhiro, additional, Murphy, John A., additional, Nagai, Makoto, additional, Nagano, Yuya, additional, Nagasaki, Taketo, additional, Nagata, Ryo, additional, Nakamura, Shogo, additional, Namikawa, Toshiya, additional, Natoli, Paolo, additional, Nerval, Simran, additional, Nishibori, Toshiyuki, additional, Nishino, Haruki, additional, O'Sullivan, Créidhe, additional, Ogawa, Hideo, additional, Ogawa, Hiroyuki, additional, Oguri, Shugo, additional, Ohsaki, Hiroyuki, additional, Ohta, Izumi S., additional, Okada, Norio, additional, Okada, Nozomi, additional, Pagano, Luca, additional, Paiella, Alessandro, additional, Paoletti, Daniela, additional, Patanchon, Guillaume, additional, Peloton, Julien, additional, Piacentini, Francesco, additional, Polenta, Gianluca, additional, Poletti, Davide, additional, Puglisi, Giuseppe, additional, Rambaud, Damien, additional, Raum, Christopher, additional, Realini, Sabrina, additional, Reinecke, Martin, additional, Remazeilles, Mathieu, additional, Ritacco, Alessia, additional, Roudil, Gilles, additional, Rubino-Martin, Jose A., additional, Sakurai, Haruyuki, additional, Sakurai, Yuki, additional, Sandri, Maura, additional, Sasaki, Manami, additional, Scott, Douglas, additional, Seibert, Joseph, additional, Sekimoto, Yutaro, additional, Sherwin, Blake, additional, Shinozaki, Keisuke, additional, Shiraishi, Maresuke, additional, Shirron, Peter, additional, Signorelli, Giovanni, additional, Smecher, Graeme, additional, Stompor, Radek, additional, Sugai, Hajime, additional, Sugiyama, Shinya, additional, Suzuki, Aritoki, additional, Suzuki, Junichi, additional, Svalheim, Trygve L., additional, Switzer, Eric, additional, Takaku, Ryota, additional, Takakura, Hayato, additional, Takakura, Satoru, additional, Takase, Yusuke, additional, Takeda, Youichi, additional, Tartari, Andrea, additional, Taylor, Ellen, additional, Terao, Yutaka, additional, Thommesen, Harald, additional, Thorne, Ben, additional, Toda, Takayuki, additional, Tomasi, Maurizio, additional, Tominaga, Mayu, additional, Trappe, Neil, additional, Tristram, Matthieu, additional, Tsuji, Masatoshi, additional, Ullom, Joe, additional, Vermeulen, Gerard, additional, Vielva, Patricio, additional, Villa, Fabrizio, additional, Vissers, Michael, additional, Vittorio, Nicola, additional, Wehus, Ingunn, additional, Weller, Jochen, additional, Wilms, Joern, additional, Winter, Berend, additional, Wollack, Edward J., additional, Yamasaki, Noriko Y., additional, Yoshida, Tetsuya, additional, Yumoto, Junji, additional, Zannoni, Mario, additional, and Zonca, Andrea, additional

Published
2020
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42. Design and experimental investigation of a planar metamaterial silicon based lenslet

Author

Gascard, Thomas, primary, Pisano, Giampaolo, additional, Doyle, Simon, additional, Shitvov, Alexey, additional, Austermann, Jason, additional, Beall, James A., additional, Hubmayr, Johannes, additional, Raymond, Benjamin, additional, Halverson, Nils, additional, Jaehnig, Gregory, additional, McKenney, Christopher M., additional, and Suzuki, Aritoki, additional

Published
2020
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44. CMB-S4

Author

Carlstrom, John, Abazajian, Kevork, Addison, Graeme, Adshead, Peter, Ahmed, Zeeshan, Allen, Steven W., Alonso, David, Alvarez, Marcelo, Anderson, Adam, Arnold, Kam S., Baccigalupi, Carlo, Schaan, Emmanuel, Schillaci, Alessandro, Schmittfull, Marcel M., Scott, Douglas, Sehgal, Neelima, Shandera, Sarah, Sheehy, Christopher, Sherwin, Blake D., Shirokoff, Erik, Bean, Rachel, Hložek, Renee, Simon, Sara M., Slosar, Anze, Somerville, Rachel, Staggs, Suzanne T., Stark, Antony, Stompor, Radek, Story, Kyle T., Stoughton, Chris, Suzuki, Aritoki, Tajima, Osamu, Holder, Gil, Bebek, Chris, Teply, Grant P., Thompson, Keith, Timbie, Peter, Tomasi, Maurizio, Treu, Jesse I., Tristram, Matthieu, Tucker, Gregory, Umilta, Caterina, van Engelen, Alexander, Holzapfel, William, Vieira, Joaquin D., Bender, Amy N., Vieregg, Abigail G., Vogelsberger, Mark, Wang, Gensheng, Watson, Scott, White, Martin, Whitehorn, Nathan, Wollack, Edward J., Wu, W. L. Kimmy, Hubmayr, Johannes, Xu, Zhilei, Yasini, Siavash, Benson, Bradford A., Yeck, James, Yoon, Ki Won, Young, Edward, Zonca, Andrea, Berger, Edo, Bhimani, Sanah, Bischoff, Colin A., Huffenberger, Kevin M., Bleem, Lindsey, Bocquet, Sebastian, Boddy, Kimberly, BONATO, MATTEO, Bond, J. Richard, Borrill, Julian, Bouchet, François R., Brown, Michael L., Bryan, Sean, Burkhart, Blakesley, Huffer, Michael, Buza, Victor, Byrum, Karen, Calabrese, Erminia, Calafut, Victoria, Caldwell, Robert, Carlstrom, John E., Carron, Julien, Cecil, Thomas, Challinor, Anthony, Chang, Clarence L., Hui, Howard, Chinone, Yuji, Cho, Hsiao-Mei Sherry, Cooray, Asantha, Crawford, Thomas M., Crites, Abigail, Cukierman, Ari, Cyr-Racine, Francis-Yan, de Haan, Tijmen, DE ZOTTI, Gianfranco, Delabrouille, Jacques, Irwin, Kent, Demarteau, Marcel, Devlin, Mark, Di Valentino, Eleonora, Dobbs, Matt, Duff, Shannon, Duivenvoorden, Adriaan, Dvorkin, Cora, Edwards, William, Eimer, Joseph, Errard, Josquin, Johnson, Bradley R., Essinger-Hileman, Thomas, Fabbian, Giulio, Feng, Chang, Ferraro, Simone, Filippini, Jeffrey P., Flauger, Raphael, Flaugher, Brenna, Fraisse, Aurelien A., Frolov, Andrei, Galitzki, Nicholas, Johnstone, Doug, Galli, Silvia, Ganga, Ken, Gerbino, Martina, Gilchriese, Murdock, Gluscevic, Vera, Green, Daniel, Grin, Daniel, Grohs, Evan, Gualtieri, Riccardo, Guarino, Victor, Bailey, Kathy, Gudmundsson, Jon E., Habib, Salman, Haller, Gunther, Halpern, Mark, Halverson, Nils W., Hanany, Shaul, Harrington, Kathleen, Hasegawa, Masaya, Hasselfield, Matthew, Hazumi, Masashi, Jones, William C., Heitmann, Katrin, Henderson, Shawn, Henning, Jason W., Hill, J. Colin, Karkare, Kirit, Katayama, Nobuhiko, Kerby, James, Kernovsky, Sarah, Keskitalo, Reijo, Kisner, Theodore, Knox, Lloyd, Kosowsky, Arthur, Kovac, John, Barkats, Denis, Kovetz, Ely D., Kuhlmann, Steve, Kuo, Chao-lin, Kurita, Nadine, Kusaka, Akito, Lahteenmaki, Anne, Lawrence, Charles R., Lee, Adrian T., Lewis, Antony, Li, Dale, Barron, Darcy, Linder, Eric, Loverde, Marilena, Lowitz, Amy, Madhavacheril, Mathew S., Mantz, Adam, Matsuda, Frederick, Mauskopf, Philip, McMahon, Jeff, Meerburg, P. Daniel, Melin, JeanBaptiste, Barry, Peter S., Meyers, Joel, Millea, Marius, Mohr, Joseph, Moncelsi, Lorenzo, Mroczkowski, Tony, Mukherjee, Suvodip, Munchmeyer, Moritz, Nagai, Daisuke, Nagy, Johanna, Namikawa, Toshiya, Bartlett, James G., Nati, Federico, Natoli, Tyler, Negrello, Mattia, Newburgh, Laura, Niemack, Michael D., Nishino, Haruki, Nordby, Martin, Novosad, Valentine, O'Connor, Paul, Obied, Georges, Basu Thakur, Ritoban, Padin, Stephen, Pandey, Shivam, Partridge, Bruce, Pierpaoli, Elena, Pogosian, Levon, Pryke, Clement, Puglisi, Giuseppe, Racine, Benjamin, Raghunathan, Srinivasan, Rahlin, Alexandra, Battaglia, Nicholas, Rajagopalan, Srini, Raveri, Marco, Reichanadter, Mark, Reichardt, Christian L., Remazeilles, Mathieu, Rocha, Graca, Roe, Natalie A., Roy, Anirban, Ruhl, John, Salatino, Maria, Baxter, Eric, and Saliwanchik, Benjamin

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics
Abstract

We describe the stage 4 cosmic microwave background ground-based experiment CMB-S4.

Published
2019

45. First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole

Author

Akiyama, Kazunori, Alberdi, Antxon, Alef, Walter, Asada, Keiichi, Azulay, Rebecca, Baczko, Anne-Kathrin, Ball, David, Balokovic, Mislav, Barrett, John, Bintley, Dan, Blackburn, Lindy, Boland, Wilfred, Bouman, Katherine L., Bower, Geoffrey C., Bremer, Michael, Brinkerink, Christiaan D., Brissenden, Roger, Britzen, Silke, Broderick, Avery E., Broguiere, Dominique, Bronzwaer, Thomas, Byun, Do-Young, Carlstrom, John E., Chael, Andrew, Chan, Chi-kwan, Chatterjee, Shami, Chatterjee, Koushik, Chen, Ming-Tang, Chen, Yongjun, Cho, Ilje, Christian, Pierre, Conway, John E., Cordes, James M., Crew, Geoffrey B., Cui, Yuzhu, Davelaar, Jordy, De Laurentis, Mariafelicia, Deane, Roger, Dempsey, Jessica, Desvignes, Gregory, Dexter, Jason, Doeleman, Sheperd S., Eatough, Ralph P., Falcke, Heino, Fish, Vincent L., Fomalont, Ed, Fraga-Encinas, Raquel, Freeman, William T., Friberg, Per, Fromm, Christian M., Gomez, Jose L., Galison, Peter, Gammie, Charles F., Garcia, Roberto, Gentaz, Olivier, Georgiev, Boris, Goddi, Ciriaco, Gold, Roman, Gu, Minfeng, Gurwell, Mark, Hada, Kazuhiro, Hecht, Michael H., Hesper, Ronald, Ho, Luis C., Ho, Paul, Honma, Mareki, Huang, Chih-Wei L., Huang, Lei, Hughes, David H., Ikeda, Shiro, Inoue, Makoto, Issaoun, Sara, James, David J., Jannuzi, Buell T., Janssen, Michael, Jeter, Britton, Jiang, Wu, Johnson, Michael D., Jorstad, Svetlana, Jung, Taehyun, Karami, Mansour, Karuppusamy, Ramesh, Kawashima, Tomohisa, Keating, Garrett K., Kettenis, Mark, Kim, Jae-Young, Kim, Junhan, Kim, Jongsoo, Kino, Motoki, Koay, Jun Yi, Koch, Patrick M., Koyama, Shoko, Kramer, Michael, Kramer, Carsten, Krichbaum, Thomas P., Kuo, Cheng-Yu, Lauer, Tod R., Lee, Sang-Sung, Li, Yan-Rong, Li, Zhiyuan, Lindqvist, Michael, Liu, Kuo, Liuzzo, Elisabetta, Lo, Wen-Ping, Lobanov, Andrei P., Loinard, Laurent, Lonsdale, Colin, Lu, Ru-Sen, MacDonald, Nicholas R., Mao, Jirong, Markoff, Sera, Marrone, Daniel P., Marscher, Alan P., Marti-Vidal, Ivan, Matsushita, Satoki, Matthews, Lynn D., Medeiros, Lia, Menten, Karl M., Mizuno, Yosuke, Mizuno, Izumi, Moran, James M., Moriyama, Kotaro, Moscibrodzka, Monika, Mueller, Cornelia, Nagai, Hiroshi, Nagar, Neil M., Nakamura, Masanori, Narayan, Ramesh, Narayanan, Gopal, Natarajan, Iniyan, Neri, Roberto, Ni, Chunchong, Noutsos, Aristeidis, Okino, Hiroki, Olivares, Hector, Ortiz-Leon, Gisela N., Oyama, Tomoaki, Ozel, Feryal, Palumbo, Daniel C. M., Patel, Nimesh, Pen, Ue-Li, Pesce, Dominic W., Pietu, Vincent, Plambeck, Richard, PopStefanija, Aleksandar, Porth, Oliver, Prather, Ben, Preciado-Lopez, Jorge A., Psaltis, Dimitrios, Pu, Hung-Yi, Ramakrishnan, Venkatessh, Rao, Ramprasad, Rawlings, Mark G., Raymond, Alexander W., Rezzolla, Luciano, Ripperda, Bart, Roelofs, Freek, Rogers, Alan, Ros, Eduardo, Rose, Mel, Roshanineshat, Arash, Rottmann, Helge, Roy, Alan L., Ruszczyk, Chet, Ryan, Benjamin R., Rygl, Kazi L. J., Sanchez, Salvador, Sanchez-Arguelles, David, Sasada, Mahito, Savolainen, Tuomas, Schloerb, F. Peter, Schuster, Karl-Friedrich, Shao, Lijing, Shen, Zhiqiang, Small, Des, Sohn, Bong Won, SooHoo, Jason, Tazaki, Fumie, Tiede, Paul, Tilanus, Remo P. J., Titus, Michael, Toma, Kenji, Torne, Pablo, Trent, Tyler, Trippe, Sascha, Tsuda, Shuichiro, van Bemmel, Ilse, van Langevelde, Huib Jan, van Rossum, Daniel R., Wagner, Jan, Wardle, John, Weintroub, Jonathan, Wex, Norbert, Wharton, Robert, Wielgus, Maciek, Wong, George N., Wu, Qingwen, Young, Ken, Young, Andre, Younsi, Ziri, Yuan, Feng, Yuan, Ye-Fei, Zensus, J. Anton, Zhao, Guangyao, Zhao, Shan-Shan, Zhu, Ziyan, Algaba, Juan-Carlos, Allardi, Alexander, Amestica, Rodrigo, Anczarski, Jadyn, Bach, Uwe, Baganoff, Frederick K., Beaudoin, Christopher, Benson, Bradford A., Berthold, Ryan, Blanchard, Jay M., Blundell, Ray, Bustamente, Sandra, Cappallo, Roger, Castillo-Dominguez, Edgar, Chang, Chih-Cheng, Chang, Shu-Hao, Chang, Song-Chu, Chen, Chung-Chen, Chilson, Ryan, Chuter, Tim C., Rosado, Rodrigo Cordova, Coulson, Iain M., Crawford, Thomas M., Crowley, Joseph, David, John, Derome, Mark, Dexter, Matthew, Dornbusch, Sven, Dudevoir, Kevin A., Dzib, Sergio A., Eckart, Andreas, Eckert, Chris, Erickson, Neal R., Everett, Wendeline B., Faber, Aaron, Farah, Joseph R., Fath, Vernon, Folkers, Thomas W., Forbes, David C., Freund, Robert, Gomez-Ruiz, Arturo I., Gale, David M., Gao, Feng, Geertsema, Gertie, Graham, David A., Greer, Christopher H., Grosslein, Ronald, Gueth, Frederic, Haggard, Daryl, Halverson, Nils W., Han, Chih-Chiang, Han, Kuo-Chang, Hao, Jinchi, Hasegawa, Yutaka, Henning, Jason W., Hernandez-Gomez, Antonio, Herrero-Illana, Ruben, Heyminck, Stefan, Hirota, Akihiko, Hoge, James, Huang, Yau-De, Impellizzeri, C. M. Violette, Jiang, Homin, Kamble, Atish, Keisler, Ryan, Kimura, Kimihiro, Kono, Yusuke, Kubo, Derek, Kuroda, John, Lacasse, Richard, Laing, Robert A., Leitch, Erik M., Li, Chao-Te, Lin, Lupin C. -C., Liu, Ching-Tang, Liu, Kuan-Yu, Lu, Li-Ming, Marson, Ralph G., Martin-Cocher, Pierre L., Massingill, Kyle D., Matulonis, Callie, McColl, Martin P., McWhirter, Stephen R., Messias, Hugo, Meyer-Zhao, Zheng, Michalik, Daniel, Montana, Alfredo, Montgomerie, William, Mora-Klein, Matias, Muders, Dirk, Nadolski, Andrew, Navarro, Santiago, Neilsen, Joseph, Nguyen, Chi H., Nishioka, Hiroaki, Norton, Timothy, Nowak, Michael A., Nystrom, George, Ogawa, Hideo, Oshiro, Peter, Parsons, Harriet, Paine, Scott N., Penalver, Juan, Phillips, Neil M., Poirier, Michael, Pradel, Nicolas, Primiani, Rurik A., Raffin, Philippe A., Rahlin, Alexandra S., Reiland, George, Risacher, Christopher, Ruiz, Ignacio, Saez-Madain, Alejandro F., Sassella, Remi, Schellart, Pim, Shaw, Paul, Silva, Kevin M., Shiokawa, Hotaka, Smith, David R., Snow, William, Souccar, Kamal, Sousa, Don, Sridharan, T. K., Srinivasan, Ranjani, Stahm, William, Stark, Anthony A., Story, Kyle, Timmer, Sjoerd T., Vertatschitsch, Laura, Walther, Craig, Wei, Ta-Shun, Whitehorn, Nathan, Whitney, Alan R., Woody, David P., Wouterloot, Jan G. A., Wright, Melvin, Yamaguchi, Paul, Yu, Chen-Yu, Zeballos, Milagros, Zhang, Shuo, Ziurys, Lucy, Akiyama, Kazunori, Alberdi, Antxon, Alef, Walter, Asada, Keiichi, Azulay, Rebecca, Baczko, Anne-Kathrin, Ball, David, Balokovic, Mislav, Barrett, John, Bintley, Dan, Blackburn, Lindy, Boland, Wilfred, Bouman, Katherine L., Bower, Geoffrey C., Bremer, Michael, Brinkerink, Christiaan D., Brissenden, Roger, Britzen, Silke, Broderick, Avery E., Broguiere, Dominique, Bronzwaer, Thomas, Byun, Do-Young, Carlstrom, John E., Chael, Andrew, Chan, Chi-kwan, Chatterjee, Shami, Chatterjee, Koushik, Chen, Ming-Tang, Chen, Yongjun, Cho, Ilje, Christian, Pierre, Conway, John E., Cordes, James M., Crew, Geoffrey B., Cui, Yuzhu, Davelaar, Jordy, De Laurentis, Mariafelicia, Deane, Roger, Dempsey, Jessica, Desvignes, Gregory, Dexter, Jason, Doeleman, Sheperd S., Eatough, Ralph P., Falcke, Heino, Fish, Vincent L., Fomalont, Ed, Fraga-Encinas, Raquel, Freeman, William T., Friberg, Per, Fromm, Christian M., Gomez, Jose L., Galison, Peter, Gammie, Charles F., Garcia, Roberto, Gentaz, Olivier, Georgiev, Boris, Goddi, Ciriaco, Gold, Roman, Gu, Minfeng, Gurwell, Mark, Hada, Kazuhiro, Hecht, Michael H., Hesper, Ronald, Ho, Luis C., Ho, Paul, Honma, Mareki, Huang, Chih-Wei L., Huang, Lei, Hughes, David H., Ikeda, Shiro, Inoue, Makoto, Issaoun, Sara, James, David J., Jannuzi, Buell T., Janssen, Michael, Jeter, Britton, Jiang, Wu, Johnson, Michael D., Jorstad, Svetlana, Jung, Taehyun, Karami, Mansour, Karuppusamy, Ramesh, Kawashima, Tomohisa, Keating, Garrett K., Kettenis, Mark, Kim, Jae-Young, Kim, Junhan, Kim, Jongsoo, Kino, Motoki, Koay, Jun Yi, Koch, Patrick M., Koyama, Shoko, Kramer, Michael, Kramer, Carsten, Krichbaum, Thomas P., Kuo, Cheng-Yu, Lauer, Tod R., Lee, Sang-Sung, Li, Yan-Rong, Li, Zhiyuan, Lindqvist, Michael, Liu, Kuo, Liuzzo, Elisabetta, Lo, Wen-Ping, Lobanov, Andrei P., Loinard, Laurent, Lonsdale, Colin, Lu, Ru-Sen, MacDonald, Nicholas R., Mao, Jirong, Markoff, Sera, Marrone, Daniel P., Marscher, Alan P., Marti-Vidal, Ivan, Matsushita, Satoki, Matthews, Lynn D., Medeiros, Lia, Menten, Karl M., Mizuno, Yosuke, Mizuno, Izumi, Moran, James M., Moriyama, Kotaro, Moscibrodzka, Monika, Mueller, Cornelia, Nagai, Hiroshi, Nagar, Neil M., Nakamura, Masanori, Narayan, Ramesh, Narayanan, Gopal, Natarajan, Iniyan, Neri, Roberto, Ni, Chunchong, Noutsos, Aristeidis, Okino, Hiroki, Olivares, Hector, Ortiz-Leon, Gisela N., Oyama, Tomoaki, Ozel, Feryal, Palumbo, Daniel C. M., Patel, Nimesh, Pen, Ue-Li, Pesce, Dominic W., Pietu, Vincent, Plambeck, Richard, PopStefanija, Aleksandar, Porth, Oliver, Prather, Ben, Preciado-Lopez, Jorge A., Psaltis, Dimitrios, Pu, Hung-Yi, Ramakrishnan, Venkatessh, Rao, Ramprasad, Rawlings, Mark G., Raymond, Alexander W., Rezzolla, Luciano, Ripperda, Bart, Roelofs, Freek, Rogers, Alan, Ros, Eduardo, Rose, Mel, Roshanineshat, Arash, Rottmann, Helge, Roy, Alan L., Ruszczyk, Chet, Ryan, Benjamin R., Rygl, Kazi L. J., Sanchez, Salvador, Sanchez-Arguelles, David, Sasada, Mahito, Savolainen, Tuomas, Schloerb, F. Peter, Schuster, Karl-Friedrich, Shao, Lijing, Shen, Zhiqiang, Small, Des, Sohn, Bong Won, SooHoo, Jason, Tazaki, Fumie, Tiede, Paul, Tilanus, Remo P. J., Titus, Michael, Toma, Kenji, Torne, Pablo, Trent, Tyler, Trippe, Sascha, Tsuda, Shuichiro, van Bemmel, Ilse, van Langevelde, Huib Jan, van Rossum, Daniel R., Wagner, Jan, Wardle, John, Weintroub, Jonathan, Wex, Norbert, Wharton, Robert, Wielgus, Maciek, Wong, George N., Wu, Qingwen, Young, Ken, Young, Andre, Younsi, Ziri, Yuan, Feng, Yuan, Ye-Fei, Zensus, J. Anton, Zhao, Guangyao, Zhao, Shan-Shan, Zhu, Ziyan, Algaba, Juan-Carlos, Allardi, Alexander, Amestica, Rodrigo, Anczarski, Jadyn, Bach, Uwe, Baganoff, Frederick K., Beaudoin, Christopher, Benson, Bradford A., Berthold, Ryan, Blanchard, Jay M., Blundell, Ray, Bustamente, Sandra, Cappallo, Roger, Castillo-Dominguez, Edgar, Chang, Chih-Cheng, Chang, Shu-Hao, Chang, Song-Chu, Chen, Chung-Chen, Chilson, Ryan, Chuter, Tim C., Rosado, Rodrigo Cordova, Coulson, Iain M., Crawford, Thomas M., Crowley, Joseph, David, John, Derome, Mark, Dexter, Matthew, Dornbusch, Sven, Dudevoir, Kevin A., Dzib, Sergio A., Eckart, Andreas, Eckert, Chris, Erickson, Neal R., Everett, Wendeline B., Faber, Aaron, Farah, Joseph R., Fath, Vernon, Folkers, Thomas W., Forbes, David C., Freund, Robert, Gomez-Ruiz, Arturo I., Gale, David M., Gao, Feng, Geertsema, Gertie, Graham, David A., Greer, Christopher H., Grosslein, Ronald, Gueth, Frederic, Haggard, Daryl, Halverson, Nils W., Han, Chih-Chiang, Han, Kuo-Chang, Hao, Jinchi, Hasegawa, Yutaka, Henning, Jason W., Hernandez-Gomez, Antonio, Herrero-Illana, Ruben, Heyminck, Stefan, Hirota, Akihiko, Hoge, James, Huang, Yau-De, Impellizzeri, C. M. Violette, Jiang, Homin, Kamble, Atish, Keisler, Ryan, Kimura, Kimihiro, Kono, Yusuke, Kubo, Derek, Kuroda, John, Lacasse, Richard, Laing, Robert A., Leitch, Erik M., Li, Chao-Te, Lin, Lupin C. -C., Liu, Ching-Tang, Liu, Kuan-Yu, Lu, Li-Ming, Marson, Ralph G., Martin-Cocher, Pierre L., Massingill, Kyle D., Matulonis, Callie, McColl, Martin P., McWhirter, Stephen R., Messias, Hugo, Meyer-Zhao, Zheng, Michalik, Daniel, Montana, Alfredo, Montgomerie, William, Mora-Klein, Matias, Muders, Dirk, Nadolski, Andrew, Navarro, Santiago, Neilsen, Joseph, Nguyen, Chi H., Nishioka, Hiroaki, Norton, Timothy, Nowak, Michael A., Nystrom, George, Ogawa, Hideo, Oshiro, Peter, Parsons, Harriet, Paine, Scott N., Penalver, Juan, Phillips, Neil M., Poirier, Michael, Pradel, Nicolas, Primiani, Rurik A., Raffin, Philippe A., Rahlin, Alexandra S., Reiland, George, Risacher, Christopher, Ruiz, Ignacio, Saez-Madain, Alejandro F., Sassella, Remi, Schellart, Pim, Shaw, Paul, Silva, Kevin M., Shiokawa, Hotaka, Smith, David R., Snow, William, Souccar, Kamal, Sousa, Don, Sridharan, T. K., Srinivasan, Ranjani, Stahm, William, Stark, Anthony A., Story, Kyle, Timmer, Sjoerd T., Vertatschitsch, Laura, Walther, Craig, Wei, Ta-Shun, Whitehorn, Nathan, Whitney, Alan R., Woody, David P., Wouterloot, Jan G. A., Wright, Melvin, Yamaguchi, Paul, Yu, Chen-Yu, Zeballos, Milagros, Zhang, Shuo, and Ziurys, Lucy

Abstract

When surrounded by a transparent emission region, black holes are expected to reveal a dark shadow caused by gravitational light bending and photon capture at the event horizon. To image and study this phenomenon, we have assembled the Event Horizon Telescope, a global very long baseline interferometry array observing at a wavelength of 1.3 mm. This allows us to reconstruct event-horizon-scale images of the supermassive black hole candidate in the center of the giant elliptical galaxy M87. We have resolved the central compact radio source as an asymmetric bright emission ring with a diameter of 42 +/- 3 mu as, which is circular and encompasses a central depression in brightness with a flux ratio greater than or similar to 10: 1. The emission ring is recovered using different calibration and imaging schemes, with its diameter and width remaining stable over four different observations carried out in different days. Overall, the observed image is consistent with expectations for the shadow of a Kerr black hole as predicted by general relativity. The asymmetry in brightness in the ring can be explained in terms of relativistic beaming of the emission from a plasma rotating close to the speed of light around a black hole. We compare our images to an extensive library of ray-traced general-relativistic magnetohydrodynamic simulations of black holes and derive a central mass of M = (6.5 +/- 0.7) x 10(9) M-circle dot. Our radio-wave observations thus provide powerful evidence for the presence of supermassive black holes in centers of galaxies and as the central engines of active galactic nuclei. They also present a new tool to explore gravity in its most extreme limit and on a mass scale that was so far not accessible.

Published
2019

46. A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of POLARBEAR Data

Author

The POLARBEAR Collaboration: Ade, P. A. R., Aguilar, Mario, Akiba, Yoshiki, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beck, D., Bianchini, F., Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Crowley, K., Cukierman, Ari, Dunner, R., Dobbs, M., Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Feeney, S. M., Feng, C., Fujino, Takuro, Galitzki, Nicholas, Gilbert, A., Goeckner-Wald, Neil, Groh, J. C., Hall, G., Halverson, Nils W., Hamada, T., Hasegawa, Masaya, Hazumi, Masashi, Hill, Charles, Howe, Logan, Inoue, Yuki, Jaehnig, G., Jaffe, Andrew H., Jeong, Oliver, Kaneko, Daisuke, Katayama, Nobuhiko, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Krachmalnicoff, Nicoletta, Kusaka, Akito, Le Jeune, M., Lee, Adrian T., Leitch, E. M., Leon, David, Linder, E., Lowry, Lindsay, Matsuda, Frederick, Matsumura, Tomotake, Minami, Y., Montgomery, J., Navaroli, Martin, Nishino, Haruki, Paar, Hans, Peloton, Julien, Pham, A. T. P., Poletti, Davide, Puglisi, Giuseppe, Reichardt, Christian L., Richards, P. L., Ross, Colin, Segawa, Y., Sherwin, B. D., Silva-Feaver, M., Siritanasak, Praween, Stebor, N., Stompor, R., Suzuki, Aritoki, Tajima, Osamu, Takakura, S., Takatori, Sayuri, Tanabe, D., Teply, Grant P., Tomaru, T., Tucker, C., Whitehorn, N., Zahn, A., 秋葉, 祥希, 茅根, 裕司, 長谷川, 雅也, 羽澄, 昌史, 井上, 優貴, 片山, 伸彦, 松村, 知岳, 西野, 玄記, 鈴木, 有春, 田島, 治, The POLARBEAR Collaboration: Ade, P. A. R., Aguilar, Mario, Akiba, Yoshiki, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beck, D., Bianchini, F., Boettger, David, Borrill, Julian, Chapman, Scott, Chinone, Yuji, Crowley, K., Cukierman, Ari, Dunner, R., Dobbs, M., Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Feeney, S. M., Feng, C., Fujino, Takuro, Galitzki, Nicholas, Gilbert, A., Goeckner-Wald, Neil, Groh, J. C., Hall, G., Halverson, Nils W., Hamada, T., Hasegawa, Masaya, Hazumi, Masashi, Hill, Charles, Howe, Logan, Inoue, Yuki, Jaehnig, G., Jaffe, Andrew H., Jeong, Oliver, Kaneko, Daisuke, Katayama, Nobuhiko, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Krachmalnicoff, Nicoletta, Kusaka, Akito, Le Jeune, M., Lee, Adrian T., Leitch, E. M., Leon, David, Linder, E., Lowry, Lindsay, Matsuda, Frederick, Matsumura, Tomotake, Minami, Y., Montgomery, J., Navaroli, Martin, Nishino, Haruki, Paar, Hans, Peloton, Julien, Pham, A. T. P., Poletti, Davide, Puglisi, Giuseppe, Reichardt, Christian L., Richards, P. L., Ross, Colin, Segawa, Y., Sherwin, B. D., Silva-Feaver, M., Siritanasak, Praween, Stebor, N., Stompor, R., Suzuki, Aritoki, Tajima, Osamu, Takakura, S., Takatori, Sayuri, Tanabe, D., Teply, Grant P., Tomaru, T., Tucker, C., Whitehorn, N., Zahn, A., 秋葉, 祥希, 茅根, 裕司, 長谷川, 雅也, 羽澄, 昌史, 井上, 優貴, 片山, 伸彦, 松村, 知岳, 西野, 玄記, 鈴木, 有春, and 田島, 治

Abstract

著者人数: 81名, Accepted: 2017-09-20

Published
2018

47. Performance of a continuously rotating half-wave plate on the POLARBEAR telescope

Author

Aguilar, Mario, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Beckman, Shawn, Boettger, David, Borrill, Julian, Chapman, Scott, Cukierman, Ari, Ducout, Anne, Elleflot, Tucker, Errard, Josquin, Fabbian, Giulio, Fujino, Takuro, Galitzki, Nicholas, Goeckner-Wald, Neil, Halverson, Nils W., Hill, Charles, Howe, Logan, Jaffe, Andrew H., Jeong, Oliver, Kaneko, Daisuke, Keating, Brian, Keskitalo, Reijo, Kisner, Theodore, Krachmalnicoff, Nicoletta, Kusaka, Akito, Lee, Adrian T., Leon, David, Lowry, Lindsay, Matsuda, Frederick, Navaroli, Martin, Paar, Hans, Peloton, Julien, Poletti, Davide, Puglisi, Giuseppe, Reichardt, Christian L., Ross, Colin, Siritanasak, Praween, Takatori, Sayuri, Teply, Grant, Takakura, Satoru, Akiba, Yoshiki, Chinone, Yuji, Hasegawa, Masaya, Hattori, Kaori, Hazumi, Masashi, Inoue, Yuki, Katayama, Nobuhiko, Matsumura, Tomotake, Nishino, Haruki, Suzuki, Aritoki, Tajima, Osamu, Institut Lagrange de Paris, Sorbonne Universités, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Takakura, S, Aguilar, M, Akiba, Y, Arnold, K, Baccigalupi, C, Barron, D, Beckman, S, Boettger, D, Borrill, J, Chapman, S, Chinone, Y, Cukierman, A, Ducout, A, Elleflot, T, Errard, J, Fabbian, G, Fujino, T, Galitzki, N, Goeckner-Wald, N, Halverson, N, Hasegawa, M, Hattori, K, Hazumi, M, Hill, C, Howe, L, Inoue, Y, Jaffe, A, Jeong, O, Kaneko, D, Katayama, N, Keating, B, Keskitalo, R, Kisner, T, Krachmalnicoff, N, Kusaka, A, Lee, A, Leon, D, Lowry, L, Matsuda, F, Matsumura, T, Navaroli, M, Nishino, H, Paar, H, Peloton, J, Poletti, D, Puglisi, G, Reichardt, C, Ross, C, Siritanasak, P, Suzuki, A, Tajima, O, Takatori, S, Teply, G, Sorbonne Université (SU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Institut d'astrophysique spatiale ( IAS ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES)

Subjects
Physics - Instrumentation and Detectors, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Cosmic microwave background, measurement methods, cosmic background radiation, 01 natural sciences, Waveplate, Atomic, law.invention, Particle and Plasma Physics, law, CMBR experiments, Stokes parameters, 010303 astronomy & astrophysics, [ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], physics.ins-det, Leakage (electronics), Physics, Settore FIS/05, Detector, Instrumentation and Detectors (physics.ins-det), Nuclear & Particles Physics, Cardinal point, symbols, astro-ph.CO, CMBR experiment, Astrophysics - Instrumentation and Methods for Astrophysics, Astronomical and Space Sciences, performance, Astrophysics - Cosmology and Nongalactic Astrophysics, noise, Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, temperature: fluctuation, 010309 optics, Primary mirror, Telescope, symbols.namesake, Optics, Settore FIS/05 - Astronomia e Astrofisica, 0103 physical sciences, Nuclear, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation and Methods for Astrophysics (astro-ph.IM), detector: design, polarization, business.industry, Molecular, Astronomy and Astrophysics, sensitivity, optics, gravitational waves and CMBR polarization, astro-ph.IM, business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

著者人数: 53名, Accepted: 2017-04-15, 資料番号: SA1170067000

Published
2017

48. Design and characterization of the SPT-3G receiver

Author

Sobrin, Joshua A., primary, Ade, Peter, primary, Ahmed, Zeeshan, primary, Anderson, Adam, primary, Avva, Jessica, primary, Basu Thakur, Ritoban, primary, Cliche, Jean-Francois, primary, Cukierman, Ari, primary, de Haan, Tijmen, primary, Ding, Junjia, primary, Dobbs, Matt, primary, Dutcher, Daniel, primary, Everett, Wendeline, primary, Foster, Allen, primary, Gallichio, Jason, primary, Gilbert, Adam, primary, Groh, John, primary, Guns, Sam, primary, Halverson, Nils, primary, Harke-Hosemann, Angelina, primary, Harrington, Nicholas, primary, Henning, Jason, primary, Holzapfel, William, primary, Huang, Nicholas, primary, Irwin, Kent, primary, Jeong, Oliver, primary, Jonas, Michelle, primary, Khaire, Trupti, primary, Kofman, Anna, primary, Korman, Milo, primary, Kubik, Donna, primary, Kuhlmann, Steve, primary, Kuo, Chao-Lin, primary, Lee, Adrian, primary, Lowitz, Amy, primary, Meyer, Stephan, primary, Michalik, Daniel, primary, Montgomery, Joshua, primary, Nadolski, Andrew, primary, Natoli, Tyler, primary, Nguyen, Hogan, primary, Noble, Gavin, primary, Novosad, Valentine, primary, Padin, Stephen, primary, Pan, Zhaodi, primary, Pearson, John, primary, Posada, Chrystian, primary, Quan, Wei, primary, Rahlin, Alexandra, primary, Ruhl, John, primary, Sayre, James, primary, Shirokoff, Erik, primary, Smecher, Graeme, primary, Stark, Antony, primary, Story, Kyle, primary, Bender, Amy, primary, Benson, Bradford, primary, Carlstrom, John, primary, Carter, Faustin, primary, Cecil, Tom, primary, Chang, Clarence, primary, Suzuki, Aritoki, primary, Thompson, Keith, primary, Tucker, Carole, primary, Vanderlinde, Keith, primary, Vieira, Joaquin, primary, Wang, Genshen, primary, Whitehorn, Nathan, primary, Yefremenko, Volodymyr, primary, Yoon, Ki Won, primary, and Young, Matt, primary

Published
2018
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49. Concept design of the LiteBIRD satellite for CMB B-mode polarization

Author

Sekimoto, Yutaro, primary, Noviello, Fabio, primary, Ota, Izumi, primary, Winter, B., primary, Ade, Peter, primary, Mangilli, Anna, primary, Aumont, Jonathan, primary, Austermann, Jason, primary, Baccigalupi, Carlo, primary, Banday, Anthony, primary, Banerji, Ranajoy, primary, Basak, Soumen, primary, Beckman, Shawn, primary, Bersanelli, Marco, primary, Borill, Julian, primary, Boulanger, Francois, primary, Brown, Michael, primary, Bucher, Martin, primary, Calabrese, Erminia, primary, Challinor, Anthony, primary, Chinone, Yuji, primary, Columbro, Fabio, primary, Cukierman, Ari, primary, Curtis, David, primary, de Bernardis, Paolo, primary, de Petris, Marco, primary, Dobbs, Matthieu, primary, Dotani, Tadayasu, primary, Duband, Lionel, primary, Ducout, Anne, primary, Ebisawa, Ken, primary, Elleflot, Tucker, primary, Eriksen, Hans Kristian, primary, Errand, Josquin, primary, Flauger, Raphael, primary, Franceschet, Cristian, primary, Fuskeland, Unni, primary, Ganga, Ken, primary, Gao, Jian-Rong, primary, Ghigna, Tommaso, primary, Grain, Julien, primary, Gruppuso, Alessandro, primary, Halverson, Nils, primary, Hargrave, Peter, primary, Hasebe, Takashi, primary, Hasegawa, Masaya, primary, Hattori, Makoto, primary, Hazumi, Masashi, primary, Henrot-Versille, Sophie, primary, Hill, Charles, primary, Hirota, Yukimasa, primary, Hivon, Eric, primary, Hoang, Duc Thuong, primary, Hubmayr, Johannes, primary, Ichiki, Kiyotomo, primary, Imada, Hiroaki, primary, Ishino, Hirokazu, primary, Jaehnig, Greg, primary, Arnold, Kam, primary, Kanai, Hiroaki, primary, Kashima, Shingo, primary, Katayama, Nobu, primary, Kawasaki, Takeo, primary, Keskitalo, Rijo, primary, Kibayashi, Atsuko, primary, Kikuchi, Takahiro, primary, Kimura, Kimihiro, primary, Kisner, Theodore, primary, Kobayashi, Yohei, primary, Kogiso, Nozomu, primary, Kohri, Kazunori, primary, Komatsu, Eiichiro, primary, Komatsu, Kunimoto, primary, Konishi, Kuniaki, primary, Krachmalnicoff, Nicoletta, primary, Kuo, Chao Lin, primary, Kurinsky, Noah, primary, Kushino, Akihiro, primary, Lamagna, Luca, primary, Lee, Adrian, primary, Linder, Eric, primary, Maffei, Buruno, primary, Maki, Muneyoshi, primary, Martinez-Gonzalez, Enrique, primary, Masi, Silvia, primary, Matsumura, Tomotakake, primary, Mennella, Aniello, primary, Minami, Yuto, primary, Mitsuda, Kazuhisa, primary, Molinari, Diego, primary, Montier, Ludovic, primary, Morgante, Gianluca, primary, Mot, Baptiste, primary, Murata, Yasuhiro, primary, Murphy, Anthony, primary, Nagai, Makoto, primary, Nagata, Ryo, primary, Nakamura, Shogo, primary, Namikawa, Toshiya, primary, Natoli, Paolo, primary, Nishibori, Toshiyuki, primary, Nishino, Haruki, primary, O'Sullivan, Creidhe, primary, Ochi, Hiroki, primary, Ogawa, Hideo, primary, Ogawa, Hiroyuki, primary, Ohsaki, Hiroyuki, primary, Okada, Nozomi, primary, Piacentini, Francesco, primary, Pisano, Giampaolo, primary, Polenta, Gianluca, primary, Poletti, Davide, primary, Puglisi, Giuseppe, primary, Raum, Christopher, primary, Remazeilles, Mathieu, primary, Sakurai, Haruyuki, primary, Sakurai, Yuki, primary, Savini, Giorgio, primary, Sherwin, Blake, primary, Shinozaki, Keisuke, primary, Shiraishi, Maresuke, primary, Signorelli, Giovanni, primary, Smecher, Graeme, primary, Stompor, Radek, primary, Sugai, Hajime, primary, Sugiyama, Shinya, primary, Suzuki, Aritoki, primary, Suzuki, Junichi, primary, Takaku, Ryota, primary, Takakura, Hayato, primary, Takakura, Satoru, primary, Taylor, Ellen, primary, Terao, Yutaka, primary, Thompson, Keith L., primary, Thorne, Ben, primary, Tomasi, Maurizio, primary, Tomida, Hiroshi, primary, Trappe, Neil, primary, Tristram, Matthieu, primary, Tsuji, Masatoshi, primary, Tsujimoto, Masahiro, primary, Uozumi, Satoru, primary, Utsunomiya, Shin, primary, Vittorio, Nicola, primary, Watanabe, Naoki, primary, Wehus, Ingunn, primary, Westbrook, Benjamin, primary, Yamamoto, Ryo, primary, Yamasaki, Noriko, primary, Yanagisawa, Masato, primary, Yoshida, Tetsuya, primary, Yumoto, Junji, primary, Zannoni, Mario, primary, Zonca, Andrea, primary, Kataoka, Yuichiro, primary, Patanchon, Guillaume, primary, and Realini, S., primary

Published
2018
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50. Year two instrument status of the SPT-3G cosmic microwave background receiver

Author

Carter, Faustin W., primary, Cecil, Thomas W., primary, Chang, Clarence L., primary, Cho, Hsaio-Mei, primary, Cliche, Jean-François, primary, Crawford, Thomas M., primary, Cukierman, Ari, primary, Denison, Edward V., primary, de Haan, Tijmen, primary, Ding, Junjia, primary, Dobbs, Matthew A., primary, Dutcher, Daniel, primary, Everett, Wendeline, primary, Foster, Allen, primary, Groh, John C., primary, Gilbert, Adam, primary, Halverson, Nils W., primary, Harke-Hosemann, Angelina H., primary, Harrington, Nicholas L., primary, Henning, Jason W., primary, Hilton, Gene C., primary, Holder, Gil P., primary, Holzapfel, William L., primary, Huang, Nicholas, primary, Irwin, Kent D., primary, Jeong, Oliver B., primary, Jonas, Michelle, primary, Khaire, Trupti S., primary, Knox, Lloyd, primary, Kofman, Anna M., primary, Korman, Milo, primary, Kubik, Donna L., primary, Kuhlmann, Steve, primary, Kuo, Chao-Lin, primary, Lee, Adrian T., primary, Leitch, Erik M., primary, Lowitz, Amy E., primary, Meyer, Stephan S., primary, Michalik, Daniel, primary, Montgomery, Joshua, primary, Nadolski, Andrew, primary, Natoli, Tyler, primary, Ngyuen, Hogan, primary, Noble, Gavin I., primary, Novosad, Valentine, primary, Padin, Stephen, primary, Pan, Zhaodi, primary, Pearson, John, primary, Posada, Chrystian M., primary, Rahlin, Alexandra, primary, Reichardt, Christian L., primary, Ruhl, John E., primary, Sayre, James T., primary, Shirokoff, Erik, primary, Smecher, Graeme, primary, Sobrin, Joshua A., primary, Stark, Antony A., primary, Story, Kyle T., primary, Suzuki, Aritoki, primary, Thompson, Keith L., primary, Tucker, Carole, primary, Vale, Leila R., primary, Vanderlinde, Keith, primary, Vieira, Joaquin, primary, Wang, Gensheng, primary, Whitehorn, Nathan, primary, Yefremenko, Vladimir, primary, Yoon, Ki Won, primary, Young, Matthew, primary, Bender, Amy N., primary, Ade, Peter A. R., primary, Ahmed, Zeeshan, primary, Anderson, Adam J., primary, Avva, Jessica S., primary, Barry, Peter S., primary, Thakur, Ritoban B., primary, Benson, Bradford A., primary, Bleem, Lindsey S., primary, Byrum, Karen, primary, Carlstrom, John E., primary, Aylor, Kevin, primary, Bocquet, Sebastian, primary, Dodelson, Scott, primary, Gallicchio, Jason, primary, Guns, Sam, primary, Quan, Wei, primary, Raghunathan, Srinivasan, primary, Wu, Wai Ling, primary, and Jones, Adam, primary

Published
2018
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