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1. A low noise CMOS camera system for 2D resonant inelastic soft X-ray scattering

Author

Nord Andresen, Christos Bakalis, Peter Denes, Azriel Goldschmidt, Ian Johnson, John M. Joseph, Armin Karcher, Amanda Krieger, and Craig Tindall

Subjects
RIXS, x-ray, CMOS sensor, spectrometer, back-illumination, low noise, Physics, QC1-999
Abstract

Resonant Inelastic X-ray Scattering (RIXS) is a powerful spectroscopic technique to study quantum properties of materials in the bulk. A novel variant of RIXS, called 2D RIXS, enables concurrent measurement of the scattered X-ray spectrum for a wide range of input energies, improving on the typically low throughput of 1D RIXS. In the soft X-ray domain, 2D RIXS demands an X-ray camera system with small pixels, large area, high quantum efficiency and low noise to limit the false detection rate in long duration exposures. We designed and implemented a 7.5 Megapixel back-illuminated CMOS detector with 5 μm pixels and high quantum efficiency in the 200–1,000 eV X-ray energy range for the QERLIN 2D RIXS spectrometer at the Advanced Light Source. The QERLIN beamline and detector are currently in commissioning. The camera noise from in-situ 3 s long dark exposures is 7e− or less and the leakage current is 6.5 × 10−3 e−/(pixel ∙ s). For individual 500 eV X-rays, the expected efficiency is greater than 75% and the false detection rate is ∼1 × 10−5 per pixel.

Published
2023
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2. The Robotic Multiobject Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI)

Author

Joseph Harry Silber, Parker Fagrelius, Kevin Fanning, Michael Schubnell, Jessica Nicole Aguilar, Steven Ahlen, Jon Ameel, Otger Ballester, Charles Baltay, Chris Bebek, Dominic Benton Beard, Robert Besuner, Laia Cardiel-Sas, Ricard Casas, Francisco Javier Castander, Todd Claybaugh, Carl Dobson, Yutong Duan, Patrick Dunlop, Jerry Edelstein, William T. Emmet, Ann Elliott, Matthew Evatt, Irena Gershkovich, Julien Guy, Stu Harris, Henry Heetderks, Ian Heetderks, Klaus Honscheid, Jose Maria Illa, Patrick Jelinsky, Sharon R. Jelinsky, Jorge Jimenez, Armin Karcher, Stephen Kent, David Kirkby, Jean-Paul Kneib, Andrew Lambert, Mike Lampton, Daniela Leitner, Michael Levi, Jeremy McCauley, Aaron Meisner, Timothy N. Miller, Ramon Miquel, Juliá Mundet, Claire Poppett, David Rabinowitz, Kevin Reil, David Roman, David Schlegel, Santiago Serrano, William Van Shourt, David Sprayberry, Gregory Tarlé, Suk Sien Tie, Curtis Weaverdyck, Kai Zhang, Marco Azzaro, Stephen Bailey, Santiago Becerril, Tami Blackwell, Mohamed Bouri, David Brooks, Elizabeth Buckley-Geer, Jose Peñate Castro, Mark Derwent, Arjun Dey, Govinda Dhungana, Peter Doel, Daniel J. Eisenstein, Nasib Fahim, Juan Garcia-Bellido, Enrique Gaztañaga, Satya Gontcho A Gontcho, Gaston Gutierrez, Philipp Hörler, Robert Kehoe, Theodore Kisner, Anthony Kremin, Luzius Kronig, Martin Landriau, Laurent Le Guillou, Paul Martini, John Moustakas, Nathalie Palanque-Delabrouille, Xiyan Peng, Will Percival, Francisco Prada, Carlos Allende Prieto, Guillermo Gonzalez de Rivera, Eusebio Sanchez, Justo Sanchez, Ray Sharples, Marcelle Soares-Santos, Edward Schlafly, Benjamin Alan Weaver, Zhimin Zhou, Yaling Zhu, Hu Zou, and (DESI Collaboration)

Subjects
Dark energy, Astronomical instrumentation, Spectrometers, Galaxy spectroscopy, Astronomy, QB1-991
Abstract

A system of 5020 robotic fiber positioners was installed in 2019 on the Mayall Telescope, at Kitt Peak National Observatory. The robots automatically retarget their optical fibers every 10–20 minutes, each to a precision of several microns, with a reconfiguration time of fewer than 2 minutes. Over the next 5 yr, they will enable the newly constructed Dark Energy Spectroscopic Instrument (DESI) to measure the spectra of 35 million galaxies and quasars. DESI will produce the largest 3D map of the universe to date and measure the expansion history of the cosmos. In addition to the 5020 robotic positioners and optical fibers, DESI’s Focal Plane System includes six guide cameras, four wave front cameras, 123 fiducial point sources, and a metrology camera mounted at the primary mirror. The system also includes associated structural, thermal, and electrical systems. In all, it contains over 675,000 individual parts. We discuss the design, construction, quality control, and integration of all these components. We include a summary of the key requirements, the review and acceptance process, on-sky validations of requirements, and lessons learned for future multiobject, fiber-fed spectrographs.

Published
2022
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3. The Robotic Multiobject Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI)

Author

Joseph Harry Silber, Parker Fagrelius, Kevin Fanning, Michael Schubnell, Jessica Nicole Aguilar, Steven Ahlen, Jon Ameel, Otger Ballester, Charles Baltay, Chris Bebek, Dominic Benton Beard, Robert Besuner, Laia Cardiel-Sas, Ricard Casas, Francisco Javier Castander, Todd Claybaugh, Carl Dobson, Yutong Duan, Patrick Dunlop, Jerry Edelstein, William T. Emmet, Ann Elliott, Matthew Evatt, Irena Gershkovich, Julien Guy, Stu Harris, Henry Heetderks, Ian Heetderks, Klaus Honscheid, Jose Maria Illa, Patrick Jelinsky, Sharon R. Jelinsky, Jorge Jimenez, Armin Karcher, Stephen Kent, David Kirkby, Jean-Paul Kneib, Andrew Lambert, Mike Lampton, Daniela Leitner, Michael Levi, Jeremy McCauley, Aaron Meisner, Timothy N. Miller, Ramon Miquel, Juliá Mundet, Claire Poppett, David Rabinowitz, Kevin Reil, David Roman, David Schlegel, Santiago Serrano, William Van Shourt, David Sprayberry, Gregory Tarlé, Suk Sien Tie, Curtis Weaverdyck, Kai Zhang, Marco Azzaro, Stephen Bailey, Santiago Becerril, Tami Blackwell, Mohamed Bouri, David Brooks, Elizabeth Buckley-Geer, Jose Peñate Castro, Mark Derwent, Arjun Dey, Govinda Dhungana, Peter Doel, Daniel J. Eisenstein, Nasib Fahim, Juan Garcia-Bellido, Enrique Gaztañaga, Satya Gontcho A Gontcho, Gaston Gutierrez, Philipp Hörler, Robert Kehoe, Theodore Kisner, Anthony Kremin, Luzius Kronig, Martin Landriau, Laurent Le Guillou, Paul Martini, John Moustakas, Nathalie Palanque-Delabrouille, Xiyan Peng, Will Percival, Francisco Prada, Carlos Allende Prieto, Guillermo Gonzalez de Rivera, Eusebio Sanchez, Justo Sanchez, Ray Sharples, Marcelle Soares-Santos, Edward Schlafly, Benjamin Alan Weaver, Zhimin Zhou, Yaling Zhu, Hu Zou, Ministerio de Ciencia e Innovación (España), European Commission, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, DESI, and UAM. Departamento de Física Teórica

Subjects
Spectrometers (1554), Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astronomical Instrumentation (799), FOS: Physical sciences, Física, Astronomy and Astrophysics, Dark Energy (351), Space and Planetary Science, astro-ph.CO, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Galaxy Spectroscopy (2171), Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Instrumentation and Methods for Astrophysics (astro-ph.IM), astro-ph.IM, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Full list of authors: Silber, Joseph Harry; Fagrelius, Parker; Fanning, Kevin; Schubnell, Michael; Aguilar, Jessica Nicole; Ahlen, Steven; Ameel, Jon; Ballester, Otger; Baltay, Charles; Bebek, Chris; Beard, Dominic Benton; Besuner, Robert; Cardiel-Sas, Laia; Casas, Ricard; Castander, Francisco Javier; Claybaugh, Todd; Dobson, Carl; Duan, Yutong; Dunlop, Patrick; Edelstein, Jerry; Emmet, William T.; Elliott, Ann; Evatt, Matthew; Gershkovich, Irena; Guy, Julien; Harris, Stu; Heetderks, Henry; Heetderks, Ian; Honscheid, Klaus; Maria Illa, Jose; Jelinsky, Patrick; Jelinsky, Sharon R.; Jimenez, Jorge; Karcher, Armin; Kent, Stephen; Kirkby, David; Kneib, Jean-Paul; Lambert, Andrew; Lampton, Mike; Leitner, Daniela; Levi, Michael; McCauley, Jeremy; Meisner, Aaron; Miller, Timothy N.; Miquel, Ramon; Mundet, Julia; Poppett, Claire; Rabinowitz, David; Reil, Kevin; Roman, David; Schlegel, David; Serrano, Santiago; Van Shourt, William; Sprayberry, David; Tarle, Gregory; Tie, Suk Sien; Weaverdyck, Curtis; Zhang, Kai; Azzaro, Marco; Bailey, Stephen; Becerril, Santiago; Blackwell, Tami; Bouri, Mohamed; Brooks, David; Buckley-Geer, Elizabeth; Penate Castro, Jose; Derwent, Mark; Dey, Arjun; Dhungana, Govinda; Doel, Peter; Eisenstein, Daniel J.; Fahim, Nasib; Garcia-Bellido, Juan; Gaztanaga, Enrique; Gontcho, Satya Gontcho A.; Gutierrez, Gaston; Horler, Philipp; Kehoe, Robert; Kisner, Theodore; Kremin, Anthony; Kronig, Luzius; Landriau, Martin; Le Guillou, Laurent; Martini, Paul; Moustakas, John; Palanque-Delabrouille, Nathalie; Peng, Xiyan; Percival, Will; Prada, Francisco; Allende Prieto, Carlos; Gonzalez de Rivera, Guillermo; Sanchez, Eusebio; Sanchez, Justo; Sharples, Ray; Soares-Santos, Marcelle; Schlafly, Edward; Weaver, Benjamin Alan; Zhou, Zhimin; Zhu, Yaling; Zou, Hu; DESI Collaboration.--This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited., A system of 5020 robotic fiber positioners was installed in 2019 on the Mayall Telescope, at Kitt Peak National Observatory. The robots automatically retarget their optical fibers every 10–20 minutes, each to a precision of several microns, with a reconfiguration time of fewer than 2 minutes. Over the next 5 yr, they will enable the newly constructed Dark Energy Spectroscopic Instrument (DESI) to measure the spectra of 35 million galaxies and quasars. DESI will produce the largest 3D map of the universe to date and measure the expansion history of the cosmos. In addition to the 5020 robotic positioners and optical fibers, DESI's Focal Plane System includes six guide cameras, four wave front cameras, 123 fiducial point sources, and a metrology camera mounted at the primary mirror. The system also includes associated structural, thermal, and electrical systems. In all, it contains over 675,000 individual parts. We discuss the design, construction, quality control, and integration of all these components. We include a summary of the key requirements, the review and acceptance process, on-sky validations of requirements, and lessons learned for future multiobject, fiber-fed spectrographs. © 2022. The Author(s). Published by the American Astronomical Society., The authors in the Barcelona-Madrid Regional Participation Group (BCN-MAD RPG) wish to acknowledge support by MICIN under grants PID2019-111317 GB, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, MDM-2015-0509, and CEX2020-001058-M, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. M.A., S.B., N.F., F.P., G.G.R., and J.S. acknowledge support from the Spanish MICINN grants MultiDark CSD2009-00064, IFT-UAM/CSIC Severo Ochoa Award SEV-2012-0249 and AYA2014-60641-C2-1-P, CSIC-AVS contract through MICINN grant AYA2010-21231-C02-01 and CDTI grant IDC-20101033, and support from the Campus of International Excellence UAM+CSIC. This research is supported by the Director, Office of Science, Office of High Energy Physics of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231, and by the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility under the same contract; additional support for DESI is provided by the U.S. National Science Foundation, Division of Astronomical Sciences under Contract No. AST-0950945 to the NSF's National Optical-Infrared Astronomy Research Laboratory; the Science and Technologies Facilities Council of the United Kingdom; the Gordon and Betty Moore Foundation; the Heising-Simons Foundation; the French Alternative Energies and Atomic Energy Commission (CEA); the National Council of Science and Technology of Mexico (CONACYT); the Ministry of Science and Innovation of Spain (MICINN), and by the DESI Member Institutions: https://www.desi.lbl.gov/collaborating-institutions., With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2021-001131-S).

Published
2023

4. Installation of the Dark Energy Spectroscopic Instrument at the Mayall 4-meter telescope

Author

Michael Schubnell, John B. Donaldson, Gregory Tarle, Pat Jelinsky, Michael Hawes, David J. Brooks, Francisco Prada, Daniel Pappalardo, Bob Stupak, Michael Levi, Derek Guenther, Parker Fagrelius, Armin Karcher, G. Gutierrez, Ashley J. Ross, C. Baltay, Patrick Dunlop, K. Honscheid, David Sprayberry, Enrique Gaztanaga, William V. Shourt, Robert Besuner, Kai Zhang, Yutong Duan, Ray M. Sharples, Christophe Magneville, Andrew Peter Doel, Matt Evatt, Lori Allen, Joseph H. Silber, P. H. Carton, Paul Martini, Jerry Edelstein, Robert Marshall, Claire Poppett, Richard R. Joyce, Martin Landriau, and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)

Subjects
Optical fiber, multi-object spectrograph, Physics::Instrumentation and Detectors, FOS: Physical sciences, 01 natural sciences, Baryon, Mayall, law.invention, 010309 optics, Telescope, Primary mirror, DESI, Optics, law, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], dark energy, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Serrurier truss, Physics, Instrument control, BAO, business.industry, Astrophysics::Instrumentation and Methods for Astrophysics, Hour angle, laser tracker, Cardinal point, Laser tracker, Physics::Accelerator Physics, business, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

International audience; The Dark Energy Spectroscopic Instrument (DESI) is a Stage IV ground-based dark energy experiment that will measure the expansion history of the Universe using the Baryon Acoustic Oscillation technique. The spectra of 35 million galaxies and quasars over 14000 square degrees will be measured during the life of the experiment. We describe the installation of the major elements of the instrument at the Mayall 4m telescope, completed in late 2019. The previous prime focus corrector, spider vanes, and upper rings were removed from the Mayall’s Serrurier truss and replaced with the newlyconstructed DESI ring, vanes, cage, hexapod, and optical corrector. The new corrector was optically aligned with the primary mirror using a laser tracker system. The DESI focal plane system was integrated to the corrector, with each of its ten 500-fiber-positioner petal segments installed using custom installation hardware and the laser tracker. Ten DESI spectrographs with 30 cryostats were installed in a newly assembled clean room in the Large Coude Room. The ten cables carrying 5000 optical fibers from the positioners in the focal plane were routed down the telescope through cable wraps at the declination and hour angle axes, and their integral slitheads were integrated with the ten spectrographs. The fiber view camera assembly was installed to the Mayall’s primary mirror cell. Servers for the instrument control system replaced existing computer equipment. The fully integrated instrument has been commissioned and is ready to start its operations phase.

Published
2021

5. Supernova neutrino burst detection with the deep underground neutrino experiment: DUNE Collaboration

Author

M. A. Hernandez Morquecho, Jonas Rademacker, P. De Lurgio, C. A. Ternes, E. T. Worcester, H. Schellman, G. P. Zeller, C. J. Solano Salinas, Mingshui Chen, Andrew White, S. Berkman, André Rubbia, C. Barnes, Joshua Barrow, B. Bhuyan, O. V. Mineev, M. Bishai, Sandip Pakvasa, M. Chalifour, N. Poonthottathil, H. Berns, A. S. Hesam, S. H. Kettell, John Marshall, G. Sirri, Evgueni Goudzovski, M. A. Arroyave, J. Hugon, M. Kirby, D. Brailsford, Laura Paulucci, A. Hourlier, E. Hazen, L. Pasqualini, Christian Farnese, Armin Karcher, D. Smargianaki, Christopher L. Marshall, M. Karolak, H. Mendez, Y.-J. Jwa, Y. Karyotakis, Artur M. Ankowski, B. Morgan, L. Patrizii, Stefan Antusch, Paola Sala, N. Moggi, Claire Shepherd-Themistocleous, G. Mandrioli, M. R. While, A. M. Gago, R. Diurba, J. Berger, Alessandro Menegolli, B. Carlus, D. Boyden, T. Le, G. Christodoulou, L. Hertel, J. S. Díaz, B. Ramson, R. Gandrajula, Akitaka Ariga, Marvin L Marshak, R. Zaki, Ina Sarcevic, Eric W. Hoppe, Manuel Alejandro Segura Delgado, Kam-Biu Luk, M. Tzanov, K. Qi, J. A. B. Coelho, C. Vignoli, C. E. Lane, Giuseppe Benedetto Cerati, N. Bostan, David Delepine, Dave M Newbold, F. Krennrich, C. Mauger, J. Yu, D. Edmunds, P. Novella, K. Zeug, Z. Parsa, L. O. Arnold, Janice L. Thompson, F. Kamiya, K. Kothekar, S. Calvez, A. Chiriacescu, T. Rehak, M. V. Diwan, V. Savinov, P. Melas, T. Safford, E. Tatar, Hui Wang, V. Bellini, C. Alt, B. Abi, W. Flanagan, V. Papadimitriou, G. Zhu, S. Centro, J. J. Russell, W. C. Griffith, H. R. Gallagher, M. A. Uchida, N. Martinez, L. Greenler, Bo Yu, A. V. Waldron, D. J. Payne, C. Gotti, T. Miedema, S. Magill, Deywis Moreno, Utku Kose, Julián Félix, D. MacFarland, K. Gollwitzer, F. Varanini, S. Henry, K. Grzelak, B. Guo, Frank Filthaut, J. Reichenbacher, F. Muheim, Ralf Lehnert, T. A. Bolton, J. Greer, Y. T. Tsai, L. Camilleri, S. Nagu, J. A. Maloney, Z. Vallari, F. Bay, H.E. Rogers, Andrea Dell'Acqua, Y. Cui, P. A. Rodrigues, C. Wret, J. Zuklin, Paul Keener, D. A. Harris, Andrea Zani, Mario Campanelli, M. Newcomer, H. W. Sobel, C. Distefano, Ornella Palamara, M. A. Ramirez Delgado, J. D. Eisch, Riccardo Papaleo, D. Cherdack, Paolo Carniti, Leigh H. Whitehead, Karol Hennessy, S. Söldner-Rembold, P. Fernandez Menendez, J. Han, C. Y. Chi, M. Groh, Jeremy Wolcott, R. LaZur, Yu. Onishchuk, T. Hamernik, L. Pickering, John Evans, A. Weinstein, A. Sitraka, L. Bagby, S. J. Brice, Nicolas Lurkin, E. Raguzin, L. C. J. Rice, H. Carranza, Milos Lokajicek, K. Nishimura, H. S. Budd, C. S. Lin, A. A. Machado, Kevin J. Kelly, D. Sgalaberna, J. M. LoSecco, R. Petti, Y. Xiao, Ionel Lazanu, E. Zhivun, C. McGrew, Marzio Nessi, Chia-Chan Chang, M. Nebot-Guinot, C. Grant, Jaroslaw Pasternak, Z. Djurcic, W. Gu, D. Duchesneau, N. Kazaryan, Kendall Mahn, Jorge Molina, M. Oberling, H. O. Back, S. Sacerdoti, J. Sensenig, C. Montanari, E. Conley, B. Howard, D. M. DeMuth, A. Chatterjee, S. Kohn, F. Drielsma, J. L. Bazo Alba, Jane Nachtman, Y. A. Ramachers, D. A. Martinez Caicedo, R. M. de Almeida, Yasar Onel, V. Zutshi, Sandeep Miryala, Enrique Calvo, V. Radeka, C. Touramanis, S. Manly, P. Hamilton, R. G. Van de Water, J. Hoff, K. V. Tsang, J. Maneira, C. Rubbia, J. Calcutt, K. Warburton, M. Nalbandyan, T. Loew, P. Ding, F. Diaz, R. Hatcher, M. Zhao, A. Olivares Del Campo, F. Cavalier, Joshua R. Klein, Vasundhara Singh, Christopher Brew, Pavel Snopok, Y. Rigaut, Dave Sankey, J. Asaadi, E. Valencia, E. James, Roberto Gutiérrez, J. Pinzino, Rakesh Kumar, Ranjan Dharmapalan, Lynn Wood, S. Narita, R.A. Rameika, R. Illingworth, D. Vargas, Patrick Dunne, A. Bitadze, Yichen Li, A. G. Cocco, C. Andreopoulos, T. Kosc, R. J. Wilson, S. Fuess, E. Cristaldo, H. Razafinime, Alessandro Montanari, B. Zamorano, Warner A. Miller, M. C. Sanchez, Marc Weber, Wladyslaw Henryk Trzaska, A. Izmaylov, C. Morris, Dong Jo Kim, H. Muramatsu, K. Spurgeon, Z. Pavlovic, R. Gran, Claudia Brizzolari, D. Vanegas Forero, S. Biagi, M. Tenti, Alberto Cervelli, M. Roda, F. Terranova, C. Cuesta, J. Marteau, Irakli Lomidze, W. Metcalf, X. Luo, A. Booth, G. Petrillo, N.V. Mokhov, J. Barranco Monarca, Jianbei Liu, Zviad Tsamalaidze, H. da Motta, L. M. Cremaldi, Carl Grace, M. Bonesini, M. Muether, O. G. Miranda, A. N. Khotjantsev, N. Tsverava, R. B. Patterson, T. Young, A. Stuart, M. J. Wilking, D. Redondo, S. R. Mishra, F. Bento Neves, A. Gendotti, A. Himmel, M. Rajaoalisoa, P. Bour, C. Wilkinson, M. Greenwood, F. F. Wilson, Nektarios Benekos, Marco Adinolfi, D. Pugnere, T. Wongjirad, M. A. Vermeulen, Andrew Brandt, E. Bechetoille, S. Roy, A. Delbart, N. J. C. Spooner, J. M. Paley, C. Patrick, Antonio Ereditato, José W. F. Valle, N. Yershov, Renato Potenza, D. Lorca, M. Toups, R. Guenette, E. Pantic, L. Di Giulio, J. Martin-Albo, L. Molina Bueno, M. P. Decowski, Gustaaf Brooijmans, K. Moffat, V. Galymov, Dario Gnani, L. Mualem, S. Tufanli, J. Mills, Irina Mocioiu, D. Mladenov, A. L. Renshaw, C. N. Booth, L. Zambelli, Orlando L. G. Peres, S. Menary, P. C. de Holanda, D. A. Dwyer, S. Prince, J. Haiston, Marco Pallavicini, T. J. Langford, E. Niner, Nikolaos Simos, L. V. Gomez Bermeo, E. Gamberini, Haleh Khani Hadavand, E. Chardonnet, A. Mastbaum, G. Prior, Filippo Resnati, J. Stock, M. Kordosky, F. Andrianala, B. Tapia Oregui, N. Nayak, James Stewart, W. Ketchum, C. A. Moura, J. Spitz, L. Stanco, E. McCluskey, Ihn Sik Seong, L. W. Koerner, J. Franc, B. R. Littlejohn, R. M. Berner, K. Vaziri, A. Marchionni, K. Mason, A. Rafique, Randall P. Johnson, E. Motuk, J. A. Nowak, T. Patzak, M. D. Messier, G. Savage, A. M. Iliescu, Yasaman Farzan, David Cussans, J. Soto-Oton, Alex Reynolds, K. Biery, Yanchu Wang, Konstantinos Manolopoulos, S. Bordoni, James Mueller, William J. Marciano, V. Aushev, W. Fox, G. Pessina, C. M. Sutera, E. Smith, A. D. Marino, J. J. De Vries, S. Shafaq, Olga Mena, S. Ravat, W. Mu, D. Marfatia, C. Hohl, R. Haenni, R. K. Plunkett, P. Cotte, C. Jesús-Valls, J.V. Dawson, F. Azfar, T. Wachala, A. P. Furmanski, Barry King, P.T. Smith, Juraj Bracinik, Andrew Blake, L. Jiang, Kristian Harder, J. Hewes, D. Newhart, A. J. Roeth, R. Acciarri, A. Borkum, N. McConkey, R. Mazza, Keith Rielage, J. G. Boissevain, J. Smolik, A. McNab, Stephen P. Gent, C. Castromonte, G. Vasseur, G. Lehmann Miotto, N. Dokania, Paolo Calafiura, Q. David, C. S. Mishra, Vlastimil Kus, Seodong Shin, M. Santos-Maldonado, S. Li, Sukalyan Chattopadhyay, Laura Dominé, Silvia Pascoli, Kim Siyeon, J. Zalesak, Gabriella Carini, Thorsten Lux, M. Dabrowski, Pedro A. N. Machado, T. Alion, A. Scarff, L. Corwin, L. Simard, S. L. Mufson, L. Pagani, J. Rodriguez Rondon, Alec Habig, Sandro Palestini, P. N. Ratoff, Timothy M. Shaw, D. Braga, S. Di Domizio, G. Meng, C. Petta, T. Kutter, Matheus Hostert, S. Murphy, R. Bajou, R. Northrop, V. J. Guarino, A. Joglekar, Marco Verzocchi, L. S. Gomez Fajardo, K. S. McFarland, C. T. Macias, Jürgen Pozimski, R. Raboanary, F. Sergiampietri, P. Schlabach, Z. Ahmad, Rex Tayloe, F. Marinho, F. Barao, Jianming Bian, D. Autiero, Poonam Mehta, C. Backhouse, Stephen J. Parke, J. Perry, T. Schaffer, B. Russell, K. Herner, R. Van Berg, J. Chaves, Francesco Gonnella, B. Paulos, N. Solomey, Laura Manenti, R. Sipos, S. Matsuno, Z. Ghorbani-Moghaddam, J. K. Nelson, Hem Raj Sharma, Karol Lang, S. Bertolucci, Piera Sapienza, M. Shamma, A. Lambert, N. P. Samios, Andrew Smith, M. Manrique Plata, J. Bremer, C. K. Jung, G. Yang, I. Kreslo, Kyung-Suk Cho, A. Sousa, J. Urheim, D. Montanari, Giorgio Riccobene, A. Heavey, Grzegorz Deptuch, Stephen Hillier, M. Gold, Sergei Striganov, G. Brunetti, M. Vagins, T. Yang, A. Rappoldi, S. Ventura, S. Dennis, J. Ahmed, Narendra Sahu, Yi Chen, S. P. Kasetti, M. Betancourt, E. Pennacchio, Y. Penichot, K. Francis, F. Cavanna, Chao Zhang, A. Muir, A. Mazzacane, P. P. Koller, D. Whittington, N. Gallice, Wei Wu, G. Karagiorgi, F. W. Sippach, T. Li, F. Bonini, S. J. Patton, E. Church, M. Parvu, James A. Anderson, V. A. 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A., Adamov, G., Adams, D., Adinolfi, M., Ahmad, Z., Ahmed, J., Alion, T., Alonso Monsalve, S., Alt, C., Anderson, J., Andreopoulos, C., Andrews, M. P., Andrianala, F., Andringa, S., Ankowski, A., Antonova, M., Antusch, S., Aranda-Fernandez, A., Ariga, A., Arnold, L. O., Arroyave, M. A., Asaadi, J., Aurisano, A., Aushev, V., Autiero, D., Azfar, F., Back, H., Back, J. J., Backhouse, C., Baesso, P., Bagby, L., Bajou, R., Balasubramanian, S., Baldi, P., Bambah, B., Barao, F., Barenboim, G., Barker, G. J., Barkhouse, W., Barnes, C., Barr, G., Barranco Monarca, J., Barros, N., Barrow, J. L., Bashyal, A., Basque, V., Bay, F., Alba, J. L. B., Beacom, J. F., Bechetoille, E., Behera, B., Bellantoni, L., Bellettini, G., Bellini, V., Beltramello, O., Belver, D., Benekos, N., Bento Neves, F., Berger, J., Berkman, S., Bernardini, P., Berner, R. M., Berns, H., Bertolucci, S., Betancourt, M., Bezawada, Y., Bhattacharjee, M., Bhuyan, B., Biagi, S., Bian, J., Biassoni, M., Biery, K., Bilki, B., Bishai, M., Bitadze, A., Blake, A., Blanco Siffert, B., Blaszczyk, F. D. M., Blazey, G. C., Blucher, E., Boissevain, J., Bolognesi, S., Bolton, T., Bonesini, M., Bongrand, M., Bonini, F., Booth, A., Booth, C., Bordoni, S., Borkum, A., Boschi, T., Bostan, N., Bour, P., Boyd, S. B., Boyden, D., Bracinik, J., Braga, D., Brailsford, D., Brandt, A., Bremer, J., Brew, C., Brianne, E., Brice, S. J., Brizzolari, C., Bromberg, C., Brooijmans, G., Brooke, J., Bross, A., Brunetti, G., Buchanan, N., Budd, H., Caiulo, D., Calafiura, P., Calcutt, J., Calin, M., Calvez, S., Calvo, E., Camilleri, L., Caminata, A., Campanelli, M., Caratelli, D., Carini, G., Carlus, B., Carniti, P., Caro Terrazas, I., Carranza, H., Castillo, A., Castromonte, C., Cattadori, C., Cavalier, F., Cavanna, F., Centro, S., Cerati, G., Cervelli, A., Cervera Villanueva, A., Chalifour, M., Chang, C., Chardonnet, E., Chatterjee, A., Chattopadhyay, S., Chaves, J., Chen, H., Chen, M., Chen, Y., Cherdack, D., Chi, C., Childress, S., Chiriacescu, A., Cho, K., Choubey, S., Christensen, A., Christian, D., Christodoulou, G., Church, E., Clarke, P., Coan, T. E., Cocco, A. G., Coelho, J. A. B., Conley, E., Conrad, J. M., Convery, M., Corwin, L., Cotte, P., Cremaldi, L., Cremonesi, L., Crespo-Anadon, J. 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Subjects
Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics, Computer Science::Digital Libraries, 01 natural sciences, Physics::Geophysics, Neutrino experiment, 0103 physical sciences, Deep Underground Neutrino Experiment, 010303 astronomy & astrophysics, Engineering (miscellaneous), Supernova, Neutrino, Physics, Time projection chamber, Neutrino, LAr TPC, Accretion (meteorology), 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Galaxy, Supernova, Neutrino detector, Computer Science::Mathematical Software, Liquid argon, High Energy Physics::Experiment, Neutrino
Abstract

This document was prepared by the DUNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada;CERN;MŠMT,Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundación “La Caixa” and MICINN, Spain; SERI and SNSF, Switzerland; TÜB˙ITAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231., Data Availability Statement This manuscript has no associated data or the data will not be deposited. [Authors’ comment: This manuscript describes sensitivity studies for the DUNE experiment using simulation only, and as such there are no experimental data to report.], The deep underground neutrino experiment (DUNE), a 40-kton underground liquid argon time projection chamber experiment, will be sensitive to the electron-neutrino flavor component of the burst of neutrinos expected from the next Galactic core-collapse supernova. Such an observation will bring unique insight into the astrophysics of core collapse as well as into the properties of neutrinos. The general capabilities of DUNE for neutrino detection in the relevant few- to few-tens-of-MeV neutrino energy range will be described. As an example, DUNE’s ability to constrain the νe spectral parameters of the neutrino burst will be considered., Commissariat à l'Énergie Atomique et aux Énergies Alternatives CEA, Fundação de Amparo à Pesquisa do Estado de São Paulo FAPESP, U.S. Department of Energy DE-AC02-05CH11231 USDOE, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro FAPERJ, Ministerstvo Školství, Mládeže a Tělovýchovy MŠMT, Fundação para a Ciência e a Tecnologia FCT, Royal Society, Ministerio de Ciencia e Innovación MICINN, Natural Sciences and Engineering Research Council of Canada NSERC, UK Research and Innovation UKRI, Instituto Nazionale di Fisica Nucleare INFN, Centre National de la Recherche Scientifique CNRS, Conselho Nacional de Desenvolvimento Científico e Tecnológico CNPq, National Research Foundation of Korea NRF, Institut National de Physique Nucléaire et de Physique des Particules IN2P3, H2020-EU, European Commission EC, European Regional Development Fund ERDF, TÜBİTAK, CERN, U.S. Department of Energy USDOE, Fundação de Amparo à Pesquisa do Estado de Goiás FAPEG, Multiple Sclerosis Center of Atlanta MSCA, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung SNF, Singapore Eye Research Institute SERI, Fermi Research Alliance, LLC DE-AC02-07CH11359, National Science Foundation NSF, Science and Technology Facilities Council STFC

Published
2021
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6. Volume IV The DUNE far detector single-phase technology

Author

L. Di Giulio, J. Martin-Albo, S. Ravat, W. Mu, D. Marfatia, T. Kosc, D. Autiero, Poonam Mehta, A. Borkum, N. McConkey, G. Karagiorgi, Robert Wilson, L. M. Cremaldi, Stephen P. Gent, T. Young, Julián Félix, D. MacFarland, Andrew Smith, M. Manrique Plata, J. Freestone, D. Rivera, B. Stillwell, Marco Verzocchi, A. Lambert, Orlando L. G. Peres, K. Gollwitzer, E. Kemp, G. Yang, I. Kreslo, F. Varanini, M. Chalifour, A. Holin, S. J. Patton, R. J. Nichol, Giovanni Bellettini, V. A. Kudryavtsev, M. Sorel, E. Church, S. Kasai, H. O. Back, A. Lister, S. Santana, C. Mariani, Carlos Escobar, J. C. Freeman, Kaushik De, M. J. Rodriguez Alonso, M. A. Acero, A. Christensen, G. S. Varner, S. Sacerdoti, D. Shooltz, Seodong Shin, M. Santos-Maldonado, T. Schaffer, Jeremy Wolcott, J. Vasel, J. A. Gonzalez-Cuevas, J. Franc, C. Mossey, Jonas Rademacker, G. P. Zeller, Joshua Barrow, John Marshall, Alessandro Thea, H. A. Tanaka, W. C. Louis, E. Hazen, Armin Karcher, D. Smargianaki, Christopher L. Marshall, M. Soderberg, A. C. Weber, Christopher J. Milne, E. Brianne, A. Aranda-Fernandez, J. Calcutt, K. Warburton, M. Nalbandyan, Dave Sankey, J. Asaadi, F. Diaz, E. Valencia, B. Kirby, A. Bross, K. Koehler, M. A. Uchida, Y. Bezawada, D. Warner, C. E. Thorn, Srubabati Goswami, Z. Williams, Gregory Iles, A. Friedland, K. M. Heeger, V. P. Luzio, G. C. Blazey, J. Barranco Monarca, Carl Grace, A. M. Gago, E. James, M. Newcomer, H. W. Sobel, Roberto Gutiérrez, C. Vignoli, R. Hatcher, M. Zhao, F. Cavalier, M. A. Hernandez Morquecho, N. Poonthottathil, Ara Ioannisian, W. Metcalf, T. Wongjirad, H. T. Rakotondramanana, D. Cherdack, M. A. Ramirez Delgado, R. Diurba, G. Christodoulou, S. Calvez, T. Durkin, H. Y. Wei, M. Muether, S. Roy, A. Caminata, A. Scarpelli, Christopher Brew, Pavel Snopok, Y. Rigaut, L. Escudero Sanchez, K. Kothekar, W. Flanagan, V. Papadimitriou, S. J. Brice, Nicolas Lurkin, M. V. Diwan, Andrew White, S. Berkman, H. Muramatsu, Z. Pavlovic, A. A. Machado, Christian Farnese, A. Mastbaum, Alfredo G. Cocco, G. Zhu, S. Centro, S. Henry, J. Rout, P. de Jong, H. Carranza, Milos Lokajicek, K. Nishimura, A. Delbart, N. J. C. Spooner, C. McGrew, E. Pantic, Mario Campanelli, David Cussans, B. T. Fleming, K. Negishi, F. Spagliardi, J. Nesbit, André Rubbia, Akitaka Ariga, Marvin L Marshak, F. Pietropaolo, F. D. M. Blaszczyk, T. Hasegawa, Kate Scholberg, O. Gogota, R. Poling, Simon Jones, A. Tonazzo, M. P. Andrews, R. Petti, S. Bertolucci, M. Bonesini, A. F. Moor, C. Barnes, A. S. Hesam, S. H. Kettell, M. Bongrand, M. R. While, D. J. Payne, C. Gotti, A. Chiriacescu, Paul Keener, Leigh H. Whitehead, James Stewart, A. Mazzacane, L. W. Koerner, T. Rehak, C. Andreopoulos, F. Terranova, Jaroslaw Pasternak, E. Raguzin, L. C. J. Rice, J. L. Bazo Alba, S. Li, J. Hartnell, M. Potekhin, N. Moggi, D. J. Summers, J. Berger, L. Cremonesi, Katsuya Yonehara, T. E. Coan, Claire Shepherd-Themistocleous, B. Radics, Karol Hennessy, S. Söldner-Rembold, C. S. Lin, L. Greenler, B. 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Subjects
Technology, 530 Physics, media_common.quotation_subject, Neutrino oscillations, liquid Argon TPC, DUNE technical design report, single phase LArTPC, Electrons, FREE-ELECTRONS, 01 natural sciences, 7. Clean energy, 09 Engineering, 030218 nuclear medicine & medical imaging, Standard Model, 03 medical and health sciences, neutrino, 0302 clinical medicine, LIQUID ARGON, 0103 physical sciences, Grand Unified Theory, High Energy Physics, Aerospace engineering, Instrumentation, Instruments & Instrumentation, Mathematical Physics, media_common, Physics, Science & Technology, 02 Physical Sciences, 010308 nuclear & particles physics, business.industry, Detector, Lıquıd Argonfree, Nuclear & Particles Physics, Symmetry (physics), Universe, Long baseline neutrino experiment, CP violation, Antimatter, Neutrino, business, Event (particle physics)
Abstract

This document was prepared by the DUNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. The DUNE collaboration also acknowledges the international, national, and regional funding agencies supporting the institutions who have contributed to completing this Technical Design Report., The preponderance of matter over antimatter in the early universe, the dynamics of the supernovae that produced the heavy elements necessary for life, and whether protons eventually decay—these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our universe, its current state, and its eventual fate. DUNE is an international world-class experiment dedicated to addressing these questions as it searches for leptonic charge-parity symmetry violation, stands ready to capture supernova neutrino bursts, and seeks to observe nucleon decay as a signature of a grand unified theory underlying the standard model. Central to achieving DUNE's physics program is a far detector that combines the many tens-of-kiloton fiducial mass necessary for rare event searches with sub-centimeter spatial resolution in its ability to image those events, allowing identification of the physics signatures among the numerous backgrounds. In the single-phase liquid argon time-projection chamber (LArTPC) technology, ionization charges drift horizontally in the liquid argon under the influence of an electric field towards a vertical anode, where they are read out with fine granularity. A photon detection system supplements the TPC, directly enhancing physics capabilities for all three DUNE physics drivers and opening up prospects for further physics explorations. The DUNE far detector technical design report (TDR) describes the DUNE physics program and the technical designs of the single- and dual-phase DUNE liquid argon TPC far detector modules. Volume IV presents an overview of the basic operating principles of a single-phase LArTPC, followed by a description of the DUNE implementation. Each of the subsystems is described in detail, connecting the high-level design requirements and decisions to the overriding physics goals of DUNE., Fermi Research Alliance, LLC (FRA) DE-AC02-07CH11359

Published
2020

7. Volume I. Introduction to DUNE

Author

E. Hazen, Armin Karcher, D. Smargianaki, Christopher L. Marshall, K. Spurgeon, M. Gold, C. Vignoli, C. J. Solano Salinas, M. J. Wilking, K. Kothekar, G. Sirri, Evgueni Goudzovski, H. Mendez, W. Flanagan, V. Papadimitriou, D. Redondo, S. R. Mishra, Y.-J. Jwa, G. Petrillo, M. Spanu, Xiaolu Ji, O. V. Mineev, M. Bishai, S. Menary, L. Molina Bueno, P. C. de Holanda, H. Berns, A. Gendotti, A. M. Szelc, R. Gandhi, A. Himmel, M. Rajaoalisoa, P. Bour, N. Kazaryan, L. Mualem, Gareth J. Barker, C. Cattadori, S. Ravat, W. Mu, D. Marfatia, T. Miedema, Kendall Mahn, Jorge Molina, Filippo Resnati, S. Magill, E. Niner, D. Autiero, Poonam Mehta, John Evans, J. S. Díaz, P. Novella, J. Fowler, G. Karagiorgi, S. J. M. Peeters, William J. Marciano, S. Bordoni, James Mueller, J. Martín-Albo, W. Fox, K. Grzelak, C. Hohl, R. Haenni, S. Alonso Monsalve, B. Howard, G. Ge, Alexander Tapper, Thomas Strauss, Silvia Pascoli, B. Stillwell, A. Lambert, A. Holin, K. V. Tsang, J. Maneira, R.A. Rameika, Juraj Bracinik, C. Wret, M. Tenti, Alberto Cervelli, Sukalyan Chattopadhyay, Laura Dominé, K. Herner, Hem Raj Sharma, S. Kasai, A. Higuera Pichardo, M. Betancourt, A. Scarff, R. Northrop, M. V. Diwan, D. J. Payne, C. Gotti, M. A. Vermeulen, R. M. Berner, J. J. De Vries, S. Shafaq, Yu. G. Kudenko, L. Pickering, B. Bhuyan, C. Kuruppu, Janet Conrad, D. Brailsford, R. Van Berg, J. Chaves, B. Paulos, R. Sipos, E. Pennacchio, F. W. Sippach, T. Li, S. Striganov, Laura Paulucci, S. Manly, P. Hamilton, R. G. Van de Water, R. Nandakumar, B. Szczerbinska, D. Cherdack, H. Carranza, Milos Lokajicek, K. Nishimura, E. Kearns, A. C. Ezeribe, J. Hoff, A. McNab, A. Stuart, G. Vasseur, C. Petta, M. Wetstein, M. M. Khabibullin, A. Bitadze, Yichen Li, G. Brunetti, L. Suter, L. Pasqualini, S. Martynenko, Ph. Lebrun, B. Morgan, L. Patrizii, A. Guglielmi, D. Wenman, S. C. Timm, R. Sharma, R. Saakyan, R. Gran, C. McGrew, C. Andreopoulos, A. Mann, F. Terranova, C. Cuesta, O. G. Miranda, C. 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Subjects
detector: technology, deep underground detector [neutrino], 530 Physics, Physics::Instrumentation and Detectors, Data management, media_common.quotation_subject, far detector, Long baseline neutrino experiment CP violation, 01 natural sciences, 030218 nuclear medicine & medical imaging, Neutrino oscillations. Neutrino Detectors. CP violation. Matter stability, design [detector], 03 medical and health sciences, neutrino, neutrino: deep underground detector, 0302 clinical medicine, near detector, 0103 physical sciences, Deep Underground Neutrino Experiment, ddc:610, Neutrino oscillation, Instrumentation, detector: design, Mathematical Physics, activity report, media_common, 010308 nuclear & particles physics, business.industry, Detector, Volume (computing), Modular design, time projection chamber: liquid argon, Universe, technology [detector], liquid argon [time projection chamber], Systems engineering, High Energy Physics::Experiment, Neutrino oscillations, DUNE technical design report, executive summary, detector technologies, data management, Neutrino, business
Abstract

Journal of Instrumentation 15(08), T08008 (1-228) (2020). doi:10.1088/1748-0221/15/08/T08008, The preponderance of matter over antimatter in the early universe, the dynamics of the supernovae that produced the heavy elements necessary for life, and whether protons eventually decay—these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our universe, its current state, and its eventual fate. The Deep Underground Neutrino Experiment (DUNE) is an international world-class experiment dedicated to addressing these questions as it searches for leptonic charge-parity symmetry violation, stands ready to capture supernova neutrino bursts, and seeks to observe nucleon decay as a signature of a grand unified theory underlying the standard model. The DUNE far detector technical design report (TDR) describes the DUNE physics program and the technical designs of the single- and dual-phase DUNE liquid argon TPC far detector modules. This TDR is intended to justify the technical choices for the far detector that flow down from the high-level physics goals through requirements at all levels of the Project. Volume I contains an executive summary that introduces the DUNE science program, the far detector and the strategy for its modular designs, and the organization and management of the Project. The remainder of Volume I provides more detail on the science program that drives the choice of detector technologies and on the technologies themselves. It also introduces the designs for the DUNE near detector and the DUNE computing model, for which DUNE is planning design reports. Volume II of this TDR describes DUNE's physics program in detail. Volume III describes the technical coordination required for the far detector design, construction, installation, and integration, and its organizational structure. Volume IV describes the single-phase far detector technology. A planned Volume V will describe the dual-phase technology., Published by Inst. of Physics, London

Published
2020

8. First results on ProtoDUNE-SP liquid argon time projection chamber performance from a beam test at the CERN Neutrino Platform

Author

Francesco Tortorici, Andrea Zani, J. Moon, P. E. L. Clarke, C. Palomares, M. B. Smy, M. Oberling, J. Migenda, F. Pietropaolo, T. Hasegawa, A. de Gouvea, N.V. Mokhov, S. Rescia, Andrés Castillo, F. Marinho, Mario Campanelli, Jürgen Pozimski, R. Raboanary, F. Sergiampietri, D. A. Sanders, John F. Beacom, Steven Gardiner, P. Madigan, R. Sulej, M. V. Diwan, D. J. Payne, L. Pickering, S. Manly, P. Hamilton, R. G. Van de Water, Chao Zhang, J. Wang, J. Hoff, Burak Bilki, Rex Tayloe, M. A. Uchida, A. Stuart, O. Dvornikov, P. De Lurgio, C. A. Ternes, J. A. Nowak, R. Bajou, P. Schlabach, E. Seltskaya, C. Lastoria, D. Naples, Kazuhiro Terao, A. Paudel, E. T. Worcester, C. Gotti, Michael Mulhearn, S. B. Boyd, T. Hill, D. Douglas, Daniel Gastler, G. A. Valdiviesso, S. Emery, M. C. Goodman, D. C. Christian, M. Newcomer, H. W. Sobel, N. Poonthottathil, Mingshui Chen, J. Urheim, B. Viren, D. Montanari, Giorgio Riccobene, I. Rakhno, M. A. Ramirez Delgado, J. Mousseau, Ara Ioannisian, H. T. Rakotondramanana, L. Molina Bueno, A. Rappoldi, Matthaeus Leitner, K. Fahey, S. J. Brice, M. E. Convery, Nicolas Lurkin, Bindu A. Bambah, S. Ravat, W. Mu, M. A. Arroyave, A. A. Machado, R. Petti, Rukmani Mohanta, Andrew Norman, V. N. Solovov, X. Pons, J. Marteau, Irakli Lomidze, Zviad Tsamalaidze, H. da Motta, M. Mellinato, M. Karolak, D. Autiero, Poonam Mehta, G. Karagiorgi, Sudarshan Paramesvaran, S. Davini, R. L. Talaga, V. Paolone, V. Pec, J. Pillow, S. Vergani, Simon Lin, K. Wood, Jaroslaw Pasternak, G. C. Blazey, Katsuya Yonehara, T. E. Coan, B. Radics, W. Gu, A. M. Teklu, E. Blucher, S. Childress, S. Matsuno, Christian Farnese, Akitaka Ariga, Marvin L Marshak, A. Chiriacescu, F. Terranova, E. Raguzin, L. C. J. Rice, L. Domine, M. Pozzato, T. Miao, L. Da Silva Peres, D. Mladenov, T. Durkin, H. Y. Wei, L. Escudero Sanchez, T. Usher, A. Rafique, A. Verdugo, B. Stillwell, A. Lambert, K. Negishi, A. Falcone, A. Holin, J. L. Bazo Alba, J. Rout, E. D. Zimmerman, M. A. Leigui de Oliveira, A. Olivier, J. Nesbit, Aldo Penzo, Kate Scholberg, Giovanni Bellettini, S. Kasai, O. Gogota, B. Ramson, P. de Jong, R. Zaki, A. Tonazzo, H. Schellman, E. Kemp, T. Rehak, I. De Bonis, Pedro A. N. Machado, B. T. Fleming, M. P. Andrews, M. Bishai, T. Alion, N. Martinez, L. Greenler, Deywis Moreno, T. Loew, H. Berns, P. Ding, M. J. Dolinski, R. J. Nichol, B. Guo, Frank Filthaut, Stefan Antusch, Nikolaos Charitonidis, Patrick Green, R. Howell, Z. Parsa, M. Sorel, J. C. Freeman, J. A. Musser, D. Gratieri, J. Reichenbacher, S. Ventura, Kaushik De, M. J. Rodriguez Alonso, Patrick Dunne, A. Scaramelli, M. Tenti, J. R. T. de Mello Neto, Raj Gandhi, Riccardo Papaleo, M. C. Sanchez, V. Zutshi, Sandeep Miryala, Enrique Calvo, N. Tsverava, V. Radeka, C. Touramanis, J. M. Paley, Antonio Ereditato, J. S. Díaz, Marco Pallavicini, D. MacFarland, G. Savage, J. Soto-Oton, P. Fernandez Menendez, J. Han, C. Y. Chi, M. Groh, N. Yershov, M. Chalifour, E. Hazen, M. A. Acero, C. Mossey, L. 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A., Martynenko, S., Mason, K., Mastbaum, A., Masud, M., Matsuno, S., Matthews, J., Mauger, C., Mauri, N., Mavrokoridis, K., Mazza, R., Mazzacane, A., Mazzucato, E., Mccluskey, E., Mcconkey, N., Mcfarland, K. S., Mcgrew, C., Mcnab, A., Mefodiev, A., Mehta, P., Melas, P., Mellinato, M., Mena, O., Menary, S., Mendez, H., Menegolli, A., Meng, G., Messier, M. D., Metcalf, W., Mewes, M., Meyer, H., Miao, T., Michna, G., Miedema, T., Migenda, J., Milincic, R., Miller, W., Mills, J., Milne, C., Mineev, O., Miranda, O. G., Miryala, S., Mishra, C. S., Mishra, S. R., Mislivec, A., Mladenov, D., Mocioiu, I., Moffat, K., Moggi, N., Mohanta, R., Mohayai, T. A., Mokhov, N., Molina, J., Bueno, L. M., Montanari, A., Montanari, C., Montanari, D., Zetina, L. M. M., Moon, J., Mooney, M., Moor, A., Moreno, D., Morgan, B., Morris, C., Mossey, C., Motuk, E., Moura, C. A., Mousseau, J., Mu, W., Mualem, L., Mueller, J., Muether, M., Mufson, S., Muheim, F., Muir, A., Mulhearn, M., Muramatsu, H., Murphy, S., Musser, J., Nachtman, J., Nagu, S., Nalbandyan, M., Nandakumar, R., Naples, D., Narita, S., Navas-Nicolas, D., Nayak, N., Nebot-Guinot, M., Necib, L., Negishi, K., Nelson, J. K., Nesbit, J., Nessi, M., Newbold, D., Newcomer, M., Newhart, D., Nichol, R., Niner, E., Nishimura, K., Norman, A., Norrick, A., Northrop, R., Novella, P., Nowak, J. A., Oberling, M., Campo, A. O. D., Olivier, A., Onel, Y., Onishchuk, Y., Ott, J., Pagani, L., Pakvasa, S., Palamara, O., Palestini, S., Paley, J. M., Pallavicini, M., Palomares, C., Pantic, E., Paolone, V., Papadimitriou, V., Papaleo, R., Papanestis, A., Paramesvaran, S., Parke, S., Parsa, Z., Parvu, M., Pascoli, S., Pasqualini, L., Pasternak, J., Pater, J., Patrick, C., Patrizii, L., Patterson, R. B., Patton, S. J., Patzak, T., Paudel, A., Paulos, B., Paulucci, L., Pavlovic, Z., Pawloski, G., Payne, D., Pec, V., Peeters, S. J. M., Penichot, Y., Pennacchio, E., Penzo, A., Peres, O. L. G., Perry, J., Pershey, D., Pessina, G., Petrillo, G., Petta, C., Petti, R., Piastra, F., Pickering, L., Pietropaolo, F., Pillow, J., Pinzino, J., Plunkett, R., Poling, R., Pons, X., Poonthottathil, N., Pordes, S., Potekhin, M., Potenza, R., Potukuchi, B. V. K. S., Pozimski, J., Pozzato, M., Prakash, S., Prakash, T., Prince, S., Prior, G., Pugnere, D., Qi, K., Qian, X., Raaf, J. L., Raboanary, R., Radeka, V., Rademacker, J., Radics, B., Rafique, A., Raguzin, E., Rai, M., Rajaoalisoa, M., Rakhno, I., Rakotondramanana, H. T., Rakotondravohitra, L., Ramachers, Y. A., Rameika, R., Delgado, M. A. R., Ramson, B., Rappoldi, A., Raselli, G., Ratoff, P., Ravat, S., Razafinime, H., Real, J. S., Rebel, B., Redondo, D., Reggiani-Guzzo, M., Rehak, T., Reichenbacher, J., Reitzner, S. D., Renshaw, A., Rescia, S., Resnati, F., Reynolds, A., Riccobene, G., Rice, L. C. J., Rielage, K., Rigamonti, A., Rigaut, Y., Rivera, D., Rochester, L., Roda, M., Rodrigues, P., Alonso, M. J. R., Rondon, J. R., Roeth, A. J., Rogers, H., Rosauro-Alcaraz, S., Rosenthal, M., Rossella, M., Rout, J., Roy, S., Rubbia, A., Rubbia, C., Russell, B., Russell, J., Ruterbories, D., Saakyan, R., Sacerdoti, S., Safford, T., Sahu, N., Sala, P., Salukvadze, G., Samios, N., Sanchez, M. C., Sanders, D. A., Sankey, D., Santana, S., Santos-Maldonado, M., Saoulidou, N., Sapienza, P., Sarasty, C., Sarcevic, I., Savage, G., Savinov, V., Scaramelli, A., Scarff, A., Scarpelli, A., Schellman, H., Schlabach, P., Schmitz, D., Scholberg, K., Schukraft, A., Segreto, E., Seltskaya, E., Sensenig, J., Seong, I., Sergi, A., Sergiampietri, F., Sgalaberna, D., Shaevitz, M. H., Shafaq, S., Shamma, M., Sharma, H. R., Sharma, R., Shaw, T., Shepherd-Themistocleous, C., Shin, S., Shooltz, D., Shrock, R., Simard, L., Simos, N., Sinclair, J., Sinev, G., Singh, J., Singh, V., Sipos, R., Sippach, F. W., Sirri, G., Sitraka, A., Siyeon, K., Smargianaki, D., Smith, A., Smith, E., Smith, P., Smolik, J., Smy, M., Snopok, P., Nunes, M. S., Sobel, H., Soderberg, M., Salinas, C. J. S., Soldner-Rembold, S., Solomey, N., Solovov, V., Sondheim, W. E., Sorel, M., Soto-Oton, J., Sousa, A., Soustruznik, K., Spagliardi, F., Spanu, M., Spitz, J., Spooner, N. J. C., Spurgeon, K., Staley, R., Stancari, M., Stanco, L., Stefan, D., Steiner, H. M., Stewart, J., Stillwell, B., Stock, J., Stocker, F., Stokes, T., Strait, M., Strauss, T., Striganov, S., Stuart, A., Sulej, R., Summers, D., Surdo, A., Susic, V., Suter, L., Sutera, C. M., Svoboda, R., Szczerbinska, B., Szelc, A. M., Talaga, R., Tanaka, H. A., Oregui, B. T., Tapper, A., Tariq, S., Tatar, E., Tayloe, R., Teklu, A. M., Tenti, M., Terao, K., Ternes, C. A., Terranova, F., Testera, G., Thea, A., Thompson, J. L., Thorn, C., Timm, S. C., Tonazzo, A., Torti, M., Tortola, M., Tortorici, F., Totani, D., Toups, M., Touramanis, C., Trevor, J., Trzaska, W. H., Tsai, Y. T., Tsamalaidze, Z., Tsang, K. V., Tsverava, N., Tufanli, S., Tull, C., Tyley, E., Tzanov, M., Uchida, M. A., Urheim, J., Usher, T., Vagins, M. R., Vahle, P., Valdiviesso, G. A., Valencia, E., Vallari, Z., Valle, J. W. F., Vallecorsa, S., Berg, R. V., De Water, R. G. V., Forero, D. V., Varanini, F., Vargas, D., Varner, G., Vasel, J., Vasseur, G., Vaziri, K., Ventura, S., Verdugo, A., Vergani, S., Vermeulen, M. A., Verzocchi, M., De Souza, H. V., Vignoli, C., Vilela, C., Viren, B., Vrba, T., Wachala, T., Waldron, A. V., Wallbank, M., Wang, H., Wang, J., Wang, Y., Warburton, K., Warner, D., Wascko, M., Waters, D., Watson, A., Weatherly, P., Weber, A., Weber, M., Wei, H., Weinstein, A., Wenman, D., Wetstein, M., While, M. R., White, A., Whitehead, L. H., Whittington, D., Wilking, M. J., Wilkinson, C., Williams, Z., Wilson, F., Wilson, R. J., Wolcott, J., Wongjirad, T., Wood, K., Wood, L., Worcester, E., Worcester, M., Wret, C., Wu, W., Xiao, Y., Yang, G., Yang, T., Yershov, N., Yonehara, K., Young, T., Yu, B., Yu, H. W., Yu, H. Z., Yu, J., Yu, Z. Y., Zaki, R., Zalesak, J., Zambelli, L., Zamorano, B., Zani, A., Zazueta, L., Zeller, G. P., Zennamo, J., Zeug, K., Zhang, C., Zhao, M., Zhivun, E., Zhu, G., Zimmerman, E. D., Zito, M., Zucchelli, S., Zuklin, J., Zutshi, V., Zwaska, R., Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), 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 de Paris (UP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), DUNE, Abi, B, Abud, A, Acciarri, R, Acero, M, Adamov, G, Adamowski, M, Adams, D, Adrien, P, Adinolfi, M, Ahmad, Z, Ahmed, J, Alion, T, Monsalve, S, Alt, C, Anderson, J, Andreopoulos, C, Andrews, M, Andrianala, F, Andringa, S, Ankowski, A, Antonova, M, Antusch, S, Aranda-Fernandez, A, Ariga, A, Arnold, L, Arroyave, M, Asaadi, J, Aurisano, A, Aushev, V, Autiero, D, Azfar, F, Back, H, Back, J, Backhouse, C, Baesso, P, Bagby, L, Bajou, R, Balasubramanian, S, Baldi, P, Bambah, B, Barao, F, Barenboim, G, Barker, G, Barkhouse, W, Barnes, C, Barr, G, Monarca, J, Barros, N, Barrow, J, Bashyal, A, Basque, V, Bay, F, Alba, J, Beacom, J, Bechetoille, E, Behera, B, Bellantoni, L, Bellettini, G, Bellini, V, Beltramello, O, Belver, D, Benekos, N, Neves, F, Berger, J, Berkman, S, Bernardini, P, Berner, R, Berns, H, Bertolucci, S, Betancourt, M, Bezawada, Y, Bhattacharjee, M, Bhuyan, B, Biagi, S, Bian, J, Biassoni, M, Biery, K, Bilki, B, Bishai, M, Bitadze, A, Blake, A, Siffert, B, Blaszczyk, F, Blazey, G, Blucher, E, Boissevain, J, Bolognesi, S, Bolton, T, Bonesini, M, Bongrand, M, Bonini, F, Booth, A, Booth, C, Bordoni, S, Borkum, A, Boschi, T, Bostan, N, Bour, P, Boyd, S, Boyden, D, Bracinik, J, Braga, D, Brailsford, D, Brandt, A, Bremer, J, Brew, C, Brianne, E, Brice, S, Brizzolari, C, Bromberg, C, Brooijmans, G, Brooke, J, Bross, A, Brunetti, G, Buchanan, N, Budd, H, Caiulo, D, Calafiura, P, Calcutt, J, Calin, M, Calvez, S, Calvo, E, Camilleri, L, Caminata, A, Campanelli, M, Caratelli, D, Carini, G, Carlus, B, Carniti, P, Terrazas, I, Carranza, H, Castillo, A, Castromonte, C, Cattadori, C, Cavalier, F, Cavanna, F, Centro, S, Cerati, G, Cervelli, A, Villanueva, A, Chalifour, M, Chang, C, Chardonnet, E, Charitonidis, N, Chatterjee, A, Chattopadhyay, S, Chatzidaki, P, Chaves, J, Chen, H, Chen, M, Chen, Y, Cherdack, D, Chi, C, Childress, S, Chiriacescu, A, Cho, K, Choubey, S, Christensen, A, Christian, D, Christodoulou, G, Church, E, Clarke, P, Coan, T, Cocco, A, Coelho, J, Conley, E, Conrad, J, Convery, M, Corwin, L, Cotte, P, Cremaldi, L, Cremonesi, L, Crespo-Anadon, J, Cristaldo, E, Cross, R, Cuesta, C, Cui, Y, Cussans, D, Dabrowski, M, Motta, H, Peres, L, David, C, David, Q, Davies, G, Davini, S, Dawson, J, De, K, Almeida, R, Debbins, P, Bonis, I, Decowski, M, De Gouv a, A, Holanda, P, Astiz, I, Deisting, A, Jong, P, Delbart, A, Delepine, D, Delgado, M, Dell'Acqua, A, Lurgio, P, Neto, J, Demuth, D, Dennis, S, Densham, C, Deptuch, G, Roeck, A, Romeri, V, Vries, J, Dharmapalan, R, Dias, M, Diaz, F, Diaz, J, Domizio, S, Giulio, L, Ding, P, Noto, L, Distefano, C, Diurba, R, Diwan, M, Djurcic, Z, Dokania, N, Dolinski, M, Domine, L, Douglas, D, Drielsma, F, Duchesneau, D, Duffy, K, Dunne, P, Durkin, T, Duyang, H, Dvornikov, O, Dwyer, D, Dyshkant, A, Eads, M, Edmunds, D, Eisch, J, Emery, S, Ereditato, A, Escobar, C, Sanchez, L, Evans, J, Ewart, E, Ezeribe, A, Fabre, C, Fahey, K, Falcone, A, Farnese, C, Farzan, Y, Felix, J, Fernandez-Martinez, E, Menendez, P, Ferraro, F, Fields, L, Filkins, A, Filthaut, F, Fitzpatrick, R, Flanagan, W, Fleming, B, Flight, R, Fowler, J, Fox, W, Franc, J, Francis, K, Franco, D, Freeman, J, Freestone, J, Fried, J, Friedland, A, Fuess, S, Furic, I, Furmanski, A, Gago, A, Gallagher, H, Gallego-Ros, A, Gallice, N, Galymov, V, Gamberini, E, Gamble, T, Gandhi, R, Gandrajula, R, Gao, S, Garcia-Gamez, D, Garcia-Peris, M, Gardiner, S, Gastler, D, Ge, G, Gelli, B, Gendotti, A, Gent, S, Ghorbani-Moghaddam, Z, Gibin, D, Gil-Botella, I, Girerd, C, Giri, A, Gnani, D, Gogota, O, Gold, M, Gollapinni, S, Gollwitzer, K, Gomes, R, Bermeo, L, Fajardo, L, Gonnella, F, Gonzalez-Cuevas, J, Goodman, M, Goodwin, O, Goswami, S, Gotti, C, Goudzovski, E, Grace, C, Graham, M, Gramellini, E, Gran, R, Granados, E, Grant, A, Grant, C, Gratieri, D, Green, P, Green, S, Greenler, L, Greenwood, M, Greer, J, Griffith, W, Groh, M, Grudzinski, J, Grzelak, K, Gu, W, Guarino, V, Guenette, R, Guglielmi, A, Guo, B, Guthikonda, K, Gutierrez, R, Guzowski, P, Guzzo, M, Gwon, S, Haaf, K, Habig, A, Hackenburg, A, Hadavand, H, Haenni, R, Hahn, A, Haigh, J, Haiston, J, Hamernik, T, Hamilton, P, Han, J, Harder, K, Harris, D, Hartnell, J, Hasegawa, T, Hatcher, R, Hazen, E, Heavey, A, Heeger, K, Heise, J, Hennessy, K, Henry, S, Morquecho, M, Herner, K, Hertel, L, Hesam, A, Hewes, J, Higuera, A, Hill, T, Hillier, S, Himmel, A, Hoff, J, Hohl, C, Holin, A, Hoppe, E, Horton-Smith, G, Hostert, M, Hourlier, A, Howard, B, Howell, R, Hrivnak, J, Huang, J, Hugon, J, Iles, G, Ilic, N, Iliescu, A, Illingworth, R, Ioannisian, A, Itay, R, Izmaylov, A, James, E, Jargowsky, B, Jediny, F, Jes s-Valls, C, Ji, X, Jiang, L, Jimenez, S, Jipa, A, Joglekar, A, Johnson, C, Johnson, R, Jones, B, Jones, S, Jung, C, Junk, T, Jwa, Y, Kabirnezhad, M, Kaboth, A, Kadenko, I, Kamiya, F, Karagiorgi, G, Karcher, A, Karolak, M, Karyotakis, Y, Kasai, S, Kasetti, S, Kashur, L, Kazaryan, N, Kearns, E, Keener, P, Kelly, K, Kemp, E, Kendziora, C, Ketchum, W, Kettell, S, Khabibullin, M, Khotjantsev, A, Khvedelidze, A, Kim, D, King, B, Kirby, B, Kirby, M, Klein, J, Koehler, K, Koerner, L, Kohn, S, Koller, P, Kordosky, M, Kosc, T, Kose, U, Kostelecky, V, Kothekar, K, Krennrich, F, Kreslo, I, Kudenko, Y, Kudryavtsev, V, Kulagin, S, Kumar, J, Kumar, R, Kuruppu, C, Kus, V, Kutter, T, Lacarelle, B, Lambert, A, Lande, K, Lane, C, Lang, K, Langford, T, Lasorak, P, Last, D, Lastoria, C, Laundrie, A, Lawrence, A, Lazanu, I, Lazur, R, Le, T, Learned, J, Lebrun, P, Miotto, G, Lehnert, R, De Oliveira, M, Leitner, M, Leyton, M, Li, L, Li, S, Li, T, Li, Y, Liao, H, Lin, C, Lin, S, Lister, A, Littlejohn, B, Liu, J, Liu, T, Lockwitz, S, Loew, T, Lokajicek, M, Lomidze, I, Long, K, Loo, K, Lorca, D, Lord, T, Losecco, J, Louis, W, Luk, K, Luo, X, Lurkin, N, Lux, T, Luzio, V, Macfarland, D, Machado, A, Machado, P, Macias, C, Macier, J, Maddalena, A, Madigan, P, Magill, S, Mahn, K, Maio, A, Maloney, J, Mandrioli, G, Maneira, J, Manenti, L, Manly, S, Mann, A, Manolopoulos, K, Plata, M, Marchionni, A, Marciano, W, Marfatia, D, Mariani, C, Maricic, J, Marinho, F, Marino, A, Marshak, M, Marshall, C, Marshall, J, Marteau, J, Martin-Albo, J, Martinez, N, Martinez Caicedo, D, Martynenko, S, Mason, K, Mastbaum, A, Masud, M, Matsuno, S, Matthews, J, Mauger, C, Mauri, N, Mavrokoridis, K, Mazza, R, Mazzacane, A, Mazzucato, E, Mccluskey, E, Mcconkey, N, Mcfarland, K, Mcgrew, C, Mcnab, A, Mefodiev, A, Mehta, P, Melas, P, Mellinato, M, Mena, O, Menary, S, Mendez, H, Menegolli, A, Meng, G, Messier, M, Metcalf, W, Mewes, M, Meyer, H, Miao, T, Michna, G, Miedema, T, Migenda, J, Milincic, R, Miller, W, Mills, J, Milne, C, Mineev, O, Miranda, O, Miryala, S, Mishra, C, Mishra, S, Mislivec, A, Mladenov, D, Mocioiu, I, Moffat, K, Moggi, N, Mohanta, R, Mohayai, T, Mokhov, N, Molina, J, Bueno, L, Montanari, A, Montanari, C, Montanari, D, Zetina, L, Moon, J, Mooney, M, Moor, A, Moreno, D, Morgan, B, Morris, C, Mossey, C, Motuk, E, Moura, C, Mousseau, J, Mu, W, Mualem, L, Mueller, J, Muether, M, Mufson, S, Muheim, F, Muir, A, Mulhearn, M, Muramatsu, H, Murphy, S, Musser, J, Nachtman, J, Nagu, S, Nalbandyan, M, Nandakumar, R, Naples, D, Narita, S, Navas-Nicolas, D, Nayak, N, Nebot-Guinot, M, Necib, L, Negishi, K, Nelson, J, Nesbit, J, Nessi, M, Newbold, D, Newcomer, M, Newhart, D, Nichol, R, Niner, E, Nishimura, K, Norman, A, Norrick, A, Northrop, R, Novella, P, Nowak, J, Oberling, M, Campo, A, Olivier, A, Onel, Y, Onishchuk, Y, Ott, J, Pagani, L, Pakvasa, S, Palamara, O, Palestini, S, Paley, J, Pallavicini, M, Palomares, C, Pantic, E, Paolone, V, Papadimitriou, V, Papaleo, R, Papanestis, A, Paramesvaran, S, Parke, S, Parsa, Z, Parvu, M, Pascoli, S, Pasqualini, L, Pasternak, J, Pater, J, Patrick, C, Patrizii, L, Patterson, R, Patton, S, Patzak, T, Paudel, A, Paulos, B, Paulucci, L, Pavlovic, Z, Pawloski, G, Payne, D, Pec, V, Peeters, S, Penichot, Y, Pennacchio, E, Penzo, A, Peres, O, Perry, J, Pershey, D, Pessina, G, Petrillo, G, Petta, C, Petti, R, Piastra, F, Pickering, L, Pietropaolo, F, Pillow, J, Pinzino, J, Plunkett, R, Poling, R, Pons, X, Poonthottathil, N, Pordes, S, Potekhin, M, Potenza, R, Potukuchi, B, Pozimski, J, Pozzato, M, Prakash, S, Prakash, T, Prince, S, Prior, G, Pugnere, D, Qi, K, Qian, X, Raaf, J, Raboanary, R, Radeka, V, Rademacker, J, Radics, B, Rafique, A, Raguzin, E, Rai, M, Rajaoalisoa, M, Rakhno, I, Rakotondramanana, H, Rakotondravohitra, L, Ramachers, Y, Rameika, R, Ramson, B, Rappoldi, A, Raselli, G, Ratoff, P, Ravat, S, Razafinime, H, Real, J, Rebel, B, Redondo, D, Reggiani-Guzzo, M, Rehak, T, Reichenbacher, J, Reitzner, S, Renshaw, A, Rescia, S, Resnati, F, Reynolds, A, Riccobene, G, Rice, L, Rielage, K, Rigamonti, A, Rigaut, Y, Rivera, D, Rochester, L, Roda, M, Rodrigues, P, Alonso, M, Rondon, J, Roeth, A, Rogers, H, Rosauro-Alcaraz, S, Rosenthal, M, Rossella, M, Rout, J, Roy, S, Rubbia, A, Rubbia, C, Russell, B, Russell, J, Ruterbories, D, Saakyan, R, Sacerdoti, S, Safford, T, Sahu, N, Sala, P, Salukvadze, G, Samios, N, Sanchez, M, Sanders, D, Sankey, D, Santana, S, Santos-Maldonado, M, Saoulidou, N, Sapienza, P, Sarasty, C, Sarcevic, I, Savage, G, Savinov, V, Scaramelli, A, Scarff, A, Scarpelli, A, Schellman, H, Schlabach, P, Schmitz, D, Scholberg, K, Schukraft, A, Segreto, E, Seltskaya, E, Sensenig, J, Seong, I, Sergi, A, Sergiampietri, F, Sgalaberna, D, Shaevitz, M, Shafaq, S, Shamma, M, Sharma, H, Sharma, R, Shaw, T, Shepherd-Themistocleous, C, Shin, S, Shooltz, D, Shrock, R, Simard, L, Simos, N, Sinclair, J, Sinev, G, Singh, J, Singh, V, Sipos, R, Sippach, F, Sirri, G, Sitraka, A, Siyeon, K, Smargianaki, D, Smith, A, Smith, E, Smith, P, Smolik, J, Smy, M, Snopok, P, Nunes, M, Sobel, H, Soderberg, M, Salinas, C, Soldner-Rembold, S, Solomey, N, Solovov, V, Sondheim, W, Sorel, M, Soto-Oton, J, Sousa, A, Soustruznik, K, Spagliardi, F, Spanu, M, Spitz, J, Spooner, N, Spurgeon, K, Staley, R, Stancari, M, Stanco, L, Stefan, D, Steiner, H, Stewart, J, Stillwell, B, Stock, J, Stocker, F, Stokes, T, Strait, M, Strauss, T, Striganov, S, Stuart, A, Sulej, R, Summers, D, Surdo, A, Susic, V, Suter, L, Sutera, C, Svoboda, R, Szczerbinska, B, Szelc, A, Talaga, R, Tanaka, H, Oregui, B, Tapper, A, Tariq, S, Tatar, E, Tayloe, R, Teklu, A, Tenti, M, Terao, K, Ternes, C, Terranova, F, Testera, G, Thea, A, Thompson, J, Thorn, C, Timm, S, Tonazzo, A, Torti, M, Tortola, M, Tortorici, F, Totani, D, Toups, M, Touramanis, C, Trevor, J, Trzaska, W, Tsai, Y, Tsamalaidze, Z, Tsang, K, Tsverava, N, Tufanli, S, Tull, C, Tyley, E, Tzanov, M, Uchida, M, Urheim, J, Usher, T, Vagins, M, Vahle, P, Valdiviesso, G, Valencia, E, Vallari, Z, Valle, J, Vallecorsa, S, Berg, R, De Water, R, Forero, D, Varanini, F, Vargas, D, Varner, G, Vasel, J, Vasseur, G, Vaziri, K, Ventura, S, Verdugo, A, Vergani, S, Vermeulen, M, Verzocchi, M, De Souza, H, Vignoli, C, Vilela, C, Viren, B, Vrba, T, Wachala, T, Waldron, A, Wallbank, M, Wang, H, Wang, J, Wang, Y, Warburton, K, Warner, D, Wascko, M, Waters, D, Watson, A, Weatherly, P, Weber, A, Weber, M, Wei, H, Weinstein, A, Wenman, D, Wetstein, M, While, M, White, A, Whitehead, L, Whittington, D, Wilking, M, Wilkinson, C, Williams, Z, Wilson, F, Wilson, R, Wolcott, J, Wongjirad, T, Wood, K, Wood, L, Worcester, E, Worcester, M, Wret, C, Wu, W, Xiao, Y, Yang, G, Yang, T, Yershov, N, Yonehara, K, Young, T, Yu, B, Yu, H, Yu, J, Yu, Z, Zaki, R, Zalesak, J, Zambelli, L, Zamorano, B, Zani, A, Zazueta, L, Zeller, G, Zennamo, J, Zeug, K, Zhang, C, Zhao, M, Zhivun, E, Zhu, G, Zimmerman, E, Zito, M, Zucchelli, S, Zuklin, J, Zutshi, V, Zwaska, R, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-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), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), XENON (IHEF, IoP, FNWI), ATLAS (IHEF, IoP, FNWI), Abi B., Abud A.A., Acciarri R., Acero M.A., Adamov G., Adamowski M., Adams D., Adrien P., Adinolfi M., Ahmad Z., Ahmed J., Alion T., Monsalve S.A., Alt C., Anderson J., Andreopoulos C., Andrews M.P., Andrianala F., Andringa S., Ankowski A., Antonova M., Antusch S., Aranda-Fernandez A., Ariga A., Arnold L.O., Arroyave M.A., Asaadi J., Aurisano A., Aushev V., Autiero D., Azfar F., Back H., Back J.J., Backhouse C., Baesso P., Bagby L., Bajou R., Balasubramanian S., Baldi P., Bambah B., Barao F., Barenboim G., Barker G.J., Barkhouse W., Barnes C., Barr G., Monarca J.B., Barros N., Barrow J.L., Bashyal A., Basque V., Bay F., Alba J.L.B., Beacom J.F., Bechetoille E., Behera B., Bellantoni L., Bellettini G., Bellini V., Beltramello O., Belver D., Benekos N., Neves F.B., Berger J., Berkman S., Bernardini P., Berner R.M., Berns H., Bertolucci S., Betancourt M., Bezawada Y., Bhattacharjee M., Bhuyan B., Biagi S., Bian J., Biassoni M., Biery K., Bilki B., Bishai M., Bitadze A., Blake A., Siffert B.B., Blaszczyk F.D.M., Blazey G.C., Blucher E., Boissevain J., Bolognesi S., Bolton T., Bonesini M., Bongrand M., Bonini F., Booth A., Booth C., Bordoni S., Borkum A., Boschi T., Bostan N., Bour P., Boyd S.B., Boyden D., Bracinik J., Braga D., Brailsford D., Brandt A., Bremer J., Brew C., Brianne E., Brice S.J., Brizzolari C., Bromberg C., Brooijmans G., Brooke J., Bross A., Brunetti G., Buchanan N., Budd H., Caiulo D., Calafiura P., Calcutt J., Calin M., Calvez S., Calvo E., Camilleri L., Caminata A., Campanelli M., Caratelli D., Carini G., Carlus B., Carniti P., Terrazas I.C., Carranza H., Castillo A., Castromonte C., Cattadori C., Cavalier F., Cavanna F., Centro S., Cerati G., Cervelli A., Villanueva A.C., Chalifour M., Chang C., Chardonnet E., Charitonidis N., Chatterjee A., Chattopadhyay S., Chatzidaki P., Chaves J., Chen H., Chen M., Chen Y., Cherdack D., Chi C., Childress S., Chiriacescu A., Cho K., Choubey S., Christensen A., Christian D., Christodoulou G., Church E., Clarke P., Coan T.E., Cocco A.G., Coelho J.A.B., Conley E., Conrad J.M., Convery M., Corwin L., Cotte P., Cremaldi L., Cremonesi L., Crespo-Anadon J.I., Cristaldo E., Cross R., Cuesta C., Cui Y., Cussans D., Dabrowski M., Motta H.D., Peres L.D.S., David C., David Q., Davies G.S., Davini S., Dawson J., De K., Almeida R.M.D., Debbins P., Bonis I.D., Decowski M.P., De Gouv a A., Holanda P.C.D., Astiz I.L.D.I., Deisting A., Jong P.D., Delbart A., Delepine D., Delgado M., Dell'Acqua A., Lurgio P.D., Neto J.R.T.D.M., Demuth D.M., Dennis S., Densham C., Deptuch G., Roeck A.D., Romeri V.D., Vries J.J.D., Dharmapalan R., DIas M., DIaz F., DIaz J.S., Domizio S.D., Giulio L.D., DIng P., Noto L.D., DIstefano C., DIurba R., DIwan M., Djurcic Z., Dokania N., Dolinski M.J., Domine L., Douglas D., Drielsma F., Duchesneau D., Duffy K., Dunne P., Durkin T., Duyang H., Dvornikov O., Dwyer D.A., Dyshkant A.S., Eads M., Edmunds D., Eisch J., Emery S., Ereditato A., Escobar C.O., Sanchez L.E., Evans J.J., Ewart E., Ezeribe A.C., Fabre C., Fahey K., Falcone A., Farnese C., Farzan Y., Felix J., Fernandez-Martinez E., Menendez P.F., Ferraro F., Fields L., Filkins A., Filthaut F., Fitzpatrick R.S., Flanagan W., Fleming B., Flight R., Fowler J., Fox W., Franc J., Francis K., Franco D., Freeman J., Freestone J., Fried J., Friedland A., Fuess S., Furic I., Furmanski A.P., Gago A., Gallagher H., Gallego-Ros A., Gallice N., Galymov V., Gamberini E., Gamble T., Gandhi R., Gandrajula R., Gao S., Garcia-Gamez D., Garcia-Peris M., Gardiner S., Gastler D., Ge G., Gelli B., Gendotti A., Gent S., Ghorbani-Moghaddam Z., Gibin D., Gil-Botella I., Girerd C., Giri A.K., Gnani D., Gogota O., Gold M., Gollapinni S., Gollwitzer K., Gomes R.A., Bermeo L.V.G., Fajardo L.S.G., Gonnella F., Gonzalez-Cuevas J.A., Goodman M.C., Goodwin O., Goswami S., Gotti C., Goudzovski E., Grace C., Graham M., Gramellini E., Gran R., Granados E., Grant A., Grant C., Gratieri D., Green P., Green S., Greenler L., Greenwood M., Greer J., Griffith W.C., Groh M., Grudzinski J., Grzelak K., Gu W., Guarino V., Guenette R., Guglielmi A., Guo B., Guthikonda K.K., Gutierrez R., Guzowski P., Guzzo M.M., Gwon S., Haaf K., Habig A., Hackenburg A., Hadavand H., Haenni R., Hahn A., Haigh J., Haiston J., Hamernik T., Hamilton P., Han J., Harder K., Harris D.A., Hartnell J., Hasegawa T., Hatcher R., Hazen E., Heavey A., Heeger K.M., Heise J., Hennessy K., Henry S., Morquecho M.A.H., Herner K., Hertel L., Hesam A.S., Hewes J., Higuera A., Hill T., Hillier S.J., Himmel A., Hoff J., Hohl C., Holin A., Hoppe E., Horton-Smith G.A., Hostert M., Hourlier A., Howard B., Howell R., Hrivnak J., Huang J., Hugon J., Iles G., Ilic N., Iliescu A.M., Illingworth R., Ioannisian A., Itay R., Izmaylov A., James E., Jargowsky B., Jediny F., Jes s-Valls C., Ji X., Jiang L., Jimenez S., Jipa A., Joglekar A., Johnson C., Johnson R., Jones B., Jones S., Jung C.K., Junk T., Jwa Y., Kabirnezhad M., Kaboth A., Kadenko I., Kamiya F., Karagiorgi G., Karcher A., Karolak M., Karyotakis Y., Kasai S., Kasetti S.P., Kashur L., Kazaryan N., Kearns E., Keener P., Kelly K.J., Kemp E., Kendziora C., Ketchum W., Kettell S.H., Khabibullin M., Khotjantsev A., Khvedelidze A., Kim D., King B., Kirby B., Kirby M., Klein J., Koehler K., Koerner L.W., Kohn S., Koller P.P., Kordosky M., Kosc T., Kose U., Kostelecky V.A., Kothekar K., Krennrich F., Kreslo I., Kudenko Y., Kudryavtsev V.A., Kulagin S., Kumar J., Kumar R., Kuruppu C., Kus V., Kutter T., Lacarelle B., Lambert A., Lande K., Lane C.E., Lang K., Langford T., Lasorak P., Last D., Lastoria C., Laundrie A., Lawrence A., Lazanu I., Lazur R., Le T., Learned J., Lebrun P., Miotto G.L., Lehnert R., De Oliveira M.A.L., Leitner M., Leyton M., Li L., Li S., Li S.W., Li T., Li Y., Liao H., Lin C.S., Lin S., Lister A., Littlejohn B.R., Liu J., Liu T., Lockwitz S., Loew T., Lokajicek M., Lomidze I., Long K., Loo K., Lorca D., Lord T., Losecco J.M., Louis W.C., Luk K.B., Luo X., Lurkin N., Lux T., Luzio V.P., MacFarland D., MacHado A.A., MacHado P., MacIas C.T., MacIer J.R., Maddalena A., Madigan P., Magill S., Mahn K., Maio A., Maloney J.A., Mandrioli G., Maneira J., Manenti L., Manly S., Mann A., Manolopoulos K., Plata M.M., Marchionni A., Marciano W., Marfatia D., Mariani C., Maricic J., Marinho F., Marino A.D., Marshak M., Marshall C., Marshall J., Marteau J., Martin-Albo J., Martinez N., Martinez Caicedo D.A., Martynenko S., Mason K., Mastbaum A., Masud M., Matsuno S., Matthews J., Mauger C., Mauri N., Mavrokoridis K., Mazza R., Mazzacane A., Mazzucato E., McCluskey E., McConkey N., McFarland K.S., McGrew C., McNab A., Mefodiev A., Mehta P., Melas P., Mellinato M., Mena O., Menary S., Mendez H., Menegolli A., Meng G., Messier M.D., Metcalf W., Mewes M., Meyer H., Miao T., Michna G., Miedema T., Migenda J., Milincic R., Miller W., Mills J., Milne C., Mineev O., Miranda O.G., Miryala S., Mishra C.S., Mishra S.R., Mislivec A., Mladenov D., Mocioiu I., Moffat K., Moggi N., Mohanta R., Mohayai T.A., Mokhov N., Molina J., Bueno L.M., Montanari A., Montanari C., Montanari D., Zetina L.M.M., Moon J., Mooney M., Moor A., Moreno D., Morgan B., Morris C., Mossey C., Motuk E., Moura C.A., Mousseau J., Mu W., Mualem L., Mueller J., Muether M., Mufson S., Muheim F., Muir A., Mulhearn M., Muramatsu H., Murphy S., Musser J., Nachtman J., Nagu S., Nalbandyan M., Nandakumar R., Naples D., Narita S., Navas-Nicolas D., Nayak N., Nebot-Guinot M., Necib L., Negishi K., Nelson J.K., Nesbit J., Nessi M., Newbold D., Newcomer M., Newhart D., Nichol R., Niner E., Nishimura K., Norman A., Norrick A., Northrop R., Novella P., Nowak J.A., Oberling M., Campo A.O.D., Olivier A., Onel Y., Onishchuk Y., Ott J., Pagani L., Pakvasa S., Palamara O., Palestini S., Paley J.M., Pallavicini M., Palomares C., Pantic E., Paolone V., Papadimitriou V., Papaleo R., Papanestis A., Paramesvaran S., Parke S., Parsa Z., Parvu M., Pascoli S., Pasqualini L., Pasternak J., Pater J., Patrick C., Patrizii L., Patterson R.B., Patton S.J., Patzak T., Paudel A., Paulos B., Paulucci L., Pavlovic Z., Pawloski G., Payne D., Pec V., Peeters S.J.M., Penichot Y., Pennacchio E., Penzo A., Peres O.L.G., Perry J., Pershey D., Pessina G., Petrillo G., Petta C., Petti R., Piastra F., Pickering L., Pietropaolo F., Pillow J., Pinzino J., Plunkett R., Poling R., Pons X., Poonthottathil N., Pordes S., Potekhin M., Potenza R., Potukuchi B.V.K.S., Pozimski J., Pozzato M., Prakash S., Prakash T., Prince S., Prior G., Pugnere D., Qi K., Qian X., Raaf J.L., Raboanary R., Radeka V., Rademacker J., Radics B., Rafique A., Raguzin E., Rai M., Rajaoalisoa M., Rakhno I., Rakotondramanana H.T., Rakotondravohitra L., Ramachers Y.A., Rameika R., Delgado M.A.R., Ramson B., Rappoldi A., Raselli G., Ratoff P., Ravat S., Razafinime H., Real J.S., Rebel B., Redondo D., Reggiani-Guzzo M., Rehak T., Reichenbacher J., Reitzner S.D., Renshaw A., Rescia S., Resnati F., Reynolds A., Riccobene G., Rice L.C.J., Rielage K., Rigamonti A., Rigaut Y., Rivera D., Rochester L., Roda M., Rodrigues P., Alonso M.J.R., Rondon J.R., Roeth A.J., Rogers H., Rosauro-Alcaraz S., Rosenthal M., Rossella M., Rout J., Roy S., Rubbia A., Rubbia C., Russell B., Russell J., Ruterbories D., Saakyan R., Sacerdoti S., Safford T., Sahu N., Sala P., Salukvadze G., Samios N., Sanchez M.C., Sanders D.A., Sankey D., Santana S., Santos-Maldonado M., Saoulidou N., Sapienza P., Sarasty C., Sarcevic I., Savage G., Savinov V., Scaramelli A., Scarff A., Scarpelli A., Schellman H., Schlabach P., Schmitz D., Scholberg K., Schukraft A., Segreto E., Seltskaya E., Sensenig J., Seong I., Sergi A., Sergiampietri F., Sgalaberna D., Shaevitz M.H., Shafaq S., Shamma M., Sharma H.R., Sharma R., Shaw T., Shepherd-Themistocleous C., Shin S., Shooltz D., Shrock R., Simard L., Simos N., Sinclair J., Sinev G., Singh J., Singh V., Sipos R., Sippach F.W., Sirri G., Sitraka A., Siyeon K., Smargianaki D., Smith A., Smith E., Smith P., Smolik J., Smy M., Snopok P., Nunes M.S., Sobel H., Soderberg M., Salinas C.J.S., Soldner-Rembold S., Solomey N., Solovov V., Sondheim W.E., Sorel M., Soto-Oton J., Sousa A., Soustruznik K., Spagliardi F., Spanu M., Spitz J., Spooner N.J.C., Spurgeon K., Staley R., Stancari M., Stanco L., Stefan D., Steiner H.M., Stewart J., Stillwell B., Stock J., Stocker F., Stokes T., Strait M., Strauss T., Striganov S., Stuart A., Sulej R., Summers D., Surdo A., Susic V., Suter L., Sutera C.M., Svoboda R., Szczerbinska B., Szelc A.M., Talaga R., Tanaka H.A., Oregui B.T., Tapper A., Tariq S., Tatar E., Tayloe R., Teklu A.M., Tenti M., Terao K., Ternes C.A., Terranova F., Testera G., Thea A., Thompson J.L., Thorn C., Timm S.C., Tonazzo A., Torti M., Tortola M., Tortorici F., Totani D., Toups M., Touramanis C., Trevor J., Trzaska W.H., Tsai Y.T., Tsamalaidze Z., Tsang K.V., Tsverava N., Tufanli S., Tull C., Tyley E., Tzanov M., Uchida M.A., Urheim J., Usher T., Vagins M.R., Vahle P., Valdiviesso G.A., Valencia E., Vallari Z., Valle J.W.F., Vallecorsa S., Berg R.V., De Water R.G.V., Forero D.V., Varanini F., Vargas D., Varner G., Vasel J., Vasseur G., Vaziri K., Ventura S., Verdugo A., Vergani S., Vermeulen M.A., Verzocchi M., De Souza H.V., Vignoli C., Vilela C., Viren B., Vrba T., Wachala T., Waldron A.V., Wallbank M., Wang H., Wang J., Wang Y., Warburton K., Warner D., Wascko M., Waters D., Watson A., Weatherly P., Weber A., Weber M., Wei H., Weinstein A., Wenman D., Wetstein M., While M.R., White A., Whitehead L.H., Whittington D., Wilking M.J., Wilkinson C., Williams Z., Wilson F., Wilson R.J., Wolcott J., Wongjirad T., Wood K., Wood L., Worcester E., Worcester M., Wret C., Wu W., Xiao Y., Yang G., Yang T., Yershov N., Yonehara K., Young T., Yu B., Yu H.W., Yu H.Z., Yu J., Yu Z.Y., Zaki R., Zalesak J., Zambelli L., Zamorano B., Zani A., Zazueta L., Zeller G.P., Zennamo J., Zeug K., Zhang C., Zhao M., Zhivun E., Zhu G., Zimmerman E.D., Zito M., Zucchelli S., Zuklin J., Zutshi V., Zwaska R., and Science and Technology Facilities Council (STFC)

Subjects
Technology, HIGH-ENERGY, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, far detector, beam transport, Noble liquid detectors (scintillation, ionization, double-phase), Cms Experıment, 01 natural sciences, 7. Clean energy, 09 Engineering, Particle identification, High Energy Physics - Experiment, 030218 nuclear medicine & medical imaging, High Energy Physics - Experiment (hep-ex), 0302 clinical medicine, Noble liquid detectors (scintillation, Detectors and Experimental Techniques, Instrumentation, Instruments & Instrumentation, physics.ins-det, time resolution, Mathematical Physics, Physics, 02 Physical Sciences, Time projection chamber, Large Hadron Collider, Detector, Instrumentation and Detectors (physics.ins-det), double-phase), Nuclear & Particles Physics, LIGHT, Neutrino, Particle Physics - Experiment, performance, Noble liquid detectors,(scintillation, ionization, double-phase), noise, CERN Lab, Large detector systems for particle and astroparticle physics, Noble liquid detectors (scintillation, ionization, double-phase), Time projection Chambers (TPC), 530 Physics, energy loss, Time projection chambers, FOS: Physical sciences, Particle detector, Nuclear physics, 03 medical and health sciences, neutrino: deep underground detector, 0103 physical sciences, ionization, Deep Underground Neutrino Experiment, High Energy Physics, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], signal processing, activity report, Science & Technology, 010308 nuclear & particles physics, hep-ex, Large detector systems for particle and astroparticle physics, Time projection Chambers (TPC), 530 Physik, sensitivity, calibration, time projection chamber: liquid argon, Experimental High Energy Physics, Large detector systems for particle and astroparticle physic, single-phase), High Energy Physics::Experiment, photon: detector, particle identification, charged particle: irradiation, Beam (structure)
Abstract

The ProtoDUNE-SP detector was constructed and operated on the CERN Neutrino Platform. We thank the CERN management for providing the infrastructure for this experiment and gratefully acknowledge the support of the CERN EP, BE, TE, EN, IT and IPT Departments for NP04/ProtoDUNE-SP. This documentwas prepared by theDUNEcollaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MSMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundacion "La Caixa" and MICINN, Spain; SERI and SNSF, Switzerland; TUBITAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231., The ProtoDUNE-SP detector is a single-phase liquid argon time projection chamber with an active volume of 7.2× 6.1× 7.0 m3. It is installed at the CERN Neutrino Platform in a specially-constructed beam that delivers charged pions, kaons, protons, muons and electrons with momenta in the range 0.3 GeV/c to 7 GeV/c. Beam line instrumentation provides accurate momentum measurements and particle identification. The ProtoDUNE-SP detector is a prototype for the first far detector module of the Deep Underground Neutrino Experiment, and it incorporates full-size components as designed for that module. This paper describes the beam line, the time projection chamber, the photon detectors, the cosmic-ray tagger, the signal processing and particle reconstruction. It presents the first results on ProtoDUNE-SP's performance, including noise and gain measurements, dE/dx calibration for muons, protons, pions and electrons, drift electron lifetime measurements, and photon detector noise, signal sensitivity and time resolution measurements. The measured values meet or exceed the specifications for the DUNE far detector, in several cases by large margins. ProtoDUNE-SP's successful operation starting in 2018 and its production of large samples of high-quality data demonstrate the effectiveness of the single-phase far detector design., National Council for Scientific and Technological Development (CNPq), Carlos Chagas Filho Foundation for Research Support of the State of Rio de Janeiro (FAPERJ), FAPEG, Brazil, Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Canada Foundation for Innovation, Natural Sciences and Engineering Research Council of Canada (NSERC), Ministry of Education, Youth & Sports - Czech Republic Czech Republic Government, European Union (EU), H2020-EU, French Atomic Energy Commission, Istituto Nazionale di Fisica Nucleare (INFN), NRF, South Korea, La Caixa Foundation, Spanish Government, Swiss National Science Foundation (SNSF), Turkiye Bilimsel ve Teknolojik Arastirma Kurumu (TUBITAK), Royal Society of London, United States Department of Energy (DOE), National Science Foundation (NSF) DE-AC02-05CH11231, IPP, Canada, CERN, MSCA, Centre National de la Recherche Scientifique (CNRS), Portuguese Foundation for Science and Technology, CAM, Spain, SERI, Switzerland, UKRI/STFC, United Kingdom, DE-AC02-07CH11359

Published
2020

9. Long-baseline neutrino oscillation physics potential of the DUNE experiment: DUNE Collaboration

Author

M. Spanu, Xiaolu Ji, A. M. Szelc, Gareth J. Barker, C. Cattadori, J. Fried, J. Fowler, S. J. M. Peeters, S. Alonso Monsalve, G. Ge, Alexander Tapper, Thomas Strauss, B. Bhuyan, D. Vanegas Forero, A. L. Renshaw, A. P. Furmanski, P.T. Smith, D. Newhart, E. Raguzin, A. J. Roeth, R. Acciarri, Karol Lang, V. Savinov, P. Melas, A. Heavey, Grzegorz Deptuch, Kevin J. Kelly, D. Sgalaberna, R. LaZur, E. Pennacchio, F. W. Sippach, Kristian Harder, M. A. Uchida, J. Hewes, Sandro Palestini, K. Spurgeon, Sandip Pakvasa, F. Stocker, H. W. Sobel, A. Gallego-Ros, N. Buchanan, C. Grant, T. Li, T. Gamble, J. J. Grudzinski, N. Mauri, L. Molina Bueno, Jeremy Wolcott, Andrea Zani, M. J. Wilking, A. Olivares Del Campo, Joshua R. Klein, A. Hourlier, Jonas Rademacker, G. P. Zeller, A. Lawrence, D. Brailsford, M. Chalifour, I. Gil-Botella, R. Flight, H. Vieira de Souza, D. Redondo, S. R. Mishra, Paola Sala, Joshua Barrow, John Marshall, K. Francis, S. Ravat, W. Mu, D. 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Shaevitz M.H., Shafaq S., Shamma M., Sharma H.R., Sharma R., Shaw T., Shepherd-Themistocleous C., Shin S., Shooltz D., Shrock R., Simard L., Simos N., Sinclair J., Sinev G., Singh J., Singh V., Sipos R., Sippach F.W., Sirri G., Sitraka A., Siyeon K., Smargianaki D., Smith A., Smith E., Smith P., Smolik J., Smy M., Snopok P., Nunes M.S., Sobel H., Soderberg M., Salinas C.J.S., Soldner-Rembold S., Solomey N., Solovov V., Sondheim W.E., Sorel M., Soto-Oton J., Sousa A., Soustruznik K., Spagliardi F., Spanu M., Spitz J., Spooner N.J.C., Spurgeon K., Staley R., Stancari M., Stanco L., Steiner H.M., Stewart J., Stillwell B., Stock J., Stocker F., Stokes T., Strait M., Strauss T., Striganov S., Stuart A., Summers D., Surdo A., Susic V., Suter L., Sutera C.M., Svoboda R., Szczerbinska B., Szelc A.M., Talaga R., Tanaka H.A., Oregui B.T., Tapper A., Tariq S., Tatar E., Tayloe R., Teklu A.M., Tenti M., Terao K., Ternes C.A., Terranova F., Testera G., Thea A., Thompson J.L., Thorn C., Timm S.C., Tonazzo A., Torti M., Tortola M., Tortorici F., Totani D., Toups M., Touramanis C., Trevor J., Trzaska W.H., Tsai Y.T., Tsamalaidze Z., Tsang K.V., Tsverava N., Tufanli S., Tull C., Tyley E., Tzanov M., Uchida M.A., Urheim J., Usher T., Vagins M.R., Vahle P., Valdiviesso G.A., Valencia E., Vallari Z., Valle J.W.F., Vallecorsa S., Van Berg R., Van de Water R.G., Forero D.V., Varanini F., Vargas D., Varner G., Vasel J., Vasseur G., Vaziri K., Ventura S., Verdugo A., Vergani S., Vermeulen M.A., Verzocchi M., de Souza H.V., Vignoli C., Vilela C., Viren B., Vrba T., Wachala T., Waldron A.V., Wallbank M., Wang H., Wang J., Wang Y., Warburton K., Warner D., Wascko M., Waters D., Watson A., Weatherly P., Weber A., Weber M., Wei H., Weinstein A., Wenman D., Wetstein M., While M.R., White A., Whitehead L.H., Whittington D., Wilking M.J., Wilkinson C., Williams Z., Wilson F., Wilson R.J., Wolcott J., Wongjirad T., Wood K., Wood L., Worcester E., Worcester M., Wret C., Wu W., Xiao Y., Yang G., 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D., Renshaw, A., Rescia, S., Resnati, F., Reynolds, A., Riccobene, G., Rice, L. C. J., Rielage, K., Rigaut, Y., Rivera, D., Rochester, L., Roda, M., Rodrigues, P., Alonso, M. J. R., Rondon, J. R., Roeth, A. J., Rogers, H., Rosauro-Alcaraz, S., Rossella, M., Rout, J., Roy, S., Rubbia, A., Rubbia, C., Russell, B., Russell, J., Ruterbories, D., Saakyan, R., Sacerdoti, S., Safford, T., Sahu, N., Sala, P., Samios, N., Sanchez, M. C., Sanders, D. A., Sankey, D., Santana, S., Santos-Maldonado, M., Saoulidou, N., Sapienza, P., Sarasty, C., Sarcevic, I., Savage, G., Savinov, V., Scaramelli, A., Scarff, A., Scarpelli, A., Schaffer, T., Schellman, H., Schlabach, P., Schmitz, D., Scholberg, K., Schukraft, A., Segreto, E., Sensenig, J., Seong, I., Sergi, A., Sergiampietri, F., Sgalaberna, D., Shaevitz, M. H., Shafaq, S., Shamma, M., Sharma, H. R., Sharma, R., Shaw, T., Shepherd-Themistocleous, C., Shin, S., Shooltz, D., Shrock, R., Simard, L., Simos, N., Sinclair, J., Sinev, G., Singh, J., Singh, V., Sipos, R., Sippach, F. W., Sirri, G., Sitraka, A., Siyeon, K., Smargianaki, D., Smith, A., Smith, E., Smith, P., Smolik, J., Smy, M., Snopok, P., Nunes, M. S., Sobel, H., Soderberg, M., Salinas, C. J. S., Soldner-Rembold, S., Solomey, N., Solovov, V., Sondheim, W. E., Sorel, M., Soto-Oton, J., Sousa, A., Soustruznik, K., Spagliardi, F., Spanu, M., Spitz, J., Spooner, N. J. C., Spurgeon, K., Staley, R., Stancari, M., Stanco, L., Steiner, H. M., Stewart, J., Stillwell, B., Stock, J., Stocker, F., Stokes, T., Strait, M., Strauss, T., Striganov, S., Stuart, A., Summers, D., Surdo, A., Susic, V., Suter, L., Sutera, C. M., Svoboda, R., Szczerbinska, B., Szelc, A. M., Talaga, R., Tanaka, H. A., Oregui, B. T., Tapper, A., Tariq, S., Tatar, E., Tayloe, R., Teklu, A. M., Tenti, M., Terao, K., Ternes, C. A., Terranova, F., Testera, G., Thea, A., Thompson, J. L., Thorn, C., Timm, S. C., Tonazzo, A., Torti, M., Tortola, M., Tortorici, F., Totani, D., Toups, M., Touramanis, C., Trevor, J., Trzaska, W. H., Tsai, Y. T., Tsamalaidze, Z., Tsang, K. V., Tsverava, N., Tufanli, S., Tull, C., Tyley, E., Tzanov, M., Uchida, M. A., Urheim, J., Usher, T., Vagins, M. R., Vahle, P., Valdiviesso, G. A., Valencia, E., Vallari, Z., Valle, J. W. F., Vallecorsa, S., Van Berg, R., Van de Water, R. G., Forero, D. V., Varanini, F., Vargas, D., Varner, G., Vasel, J., Vasseur, G., Vaziri, K., Ventura, S., Verdugo, A., Vergani, S., Vermeulen, M. A., Verzocchi, M., de Souza, H. V., Vignoli, C., Vilela, C., Viren, B., Vrba, T., Wachala, T., Waldron, A. V., Wallbank, M., Wang, H., Wang, J., Wang, Y., Warburton, K., Warner, D., Wascko, M., Waters, D., Watson, A., Weatherly, P., Weber, A., Weber, M., Wei, H., Weinstein, A., Wenman, D., Wetstein, M., While, M. R., White, A., Whitehead, L. H., Whittington, D., Wilking, M. J., Wilkinson, C., Williams, Z., Wilson, F., Wilson, R. J., Wolcott, J., Wongjirad, T., Wood, K., Wood, L., Worcester, E., Worcester, M., Wret, C., Wu, W., Xiao, Y., Yang, G., Yang, T., Yershov, N., Yonehara, K., Young, T., Yu, B., Yu, J., Zaki, R., Zalesak, J., Zambelli, L., Zamorano, B., Zani, A., Zazueta, L., Zeller, G. P., Zennamo, J., Zeug, K., Zhang, C., Zhao, M., Zhivun, E., Zhu, G., Zimmerman, E. D., Zito, M., Zucchelli, S., Zuklin, J., Zutshi, V., and Zwaska, R.

Subjects
Physics and Astronomy (miscellaneous), Physics::Instrumentation and Detectors, 01 natural sciences, Particle detector, Physics, Particles & Fields, Nuclear physics, neutrino, 0103 physical sciences, Neutrino oscillations, neutrino physiscs, Deep Underground Neutrino Experiment, Deep Underground Neutrino Experiment, Neutrino oscillation experiment, DISTRIBUTIONS, Fermilab, High Energy Physics, LEPTON SCATTERING, 010306 general physics, Neutrino oscillation, Engineering (miscellaneous), Physics, Science & Technology, 010308 nuclear & particles physics, Detector, High Energy Physics::Phenomenology, Neutrino detector, Physical Sciences, High Energy Physics::Experiment, Neutrino, Lepton
Abstract

The sensitivity of the Deep Underground Neutrino Experiment (DUNE) to neutrino oscillation is determined, based on a full simulation, reconstruction, and event selection of the far detector and a full simulation and parameterized analysis of the near detector. Detailed uncertainties due to the flux prediction, neutrino interaction model, and detector effects are included. DUNE will resolve the neutrino mass ordering to a precision of 5$$\sigma $$ σ , for all $$\delta _{\mathrm{CP}}$$ δ CP values, after 2 years of running with the nominal detector design and beam configuration. It has the potential to observe charge-parity violation in the neutrino sector to a precision of 3$$\sigma $$ σ (5$$\sigma $$ σ ) after an exposure of 5 (10) years, for 50% of all $$\delta _{\mathrm{CP}}$$ δ CP values. It will also make precise measurements of other parameters governing long-baseline neutrino oscillation, and after an exposure of 15 years will achieve a similar sensitivity to $$\sin ^{2} 2\theta _{13}$$ sin 2 2 θ 13 to current reactor experiments.

Published
2020

10. A 40mW/channel Image Sensor Line Driver IC with Independently Tunable Gain and Settling Time

Author

Armin Karcher, Carl Grace, Aikaterini Papadopoulou, and Peter Denes

Subjects
Transimpedance amplifier, CMOS, Computer science, Settling time, Operational transconductance amplifier, Hardware_INTEGRATEDCIRCUITS, Line driver, Electronic engineering, Instrumentation amplifier, Image sensor, Chip
Abstract

A 16-channel analog front-end integrated circuit (IC) for interfacing an image sensor with single-ended analog output to a differential-input digitizer is presented. The IC is designed for image sensors used in single-electron counting direct detection cameras with applications in cryogenic electron microscopy (cryo-EM), but it’s high flexibility allows usage with a variety of sensors. An operational transconductance amplifier (OTA) and a transimpedance amplifier (TIA) replace the traditional instrumentation amplifier, to allow power reduction and decoupling of the gain and bandwidth stages. This allows for a tunable gain in order to exploit the digitizer full-scale range, and an independent bandwidth tuning capability to accommodate a variety of sensors. Additionally, the front-end supports a very wide input common-mode range, and provides offset correction capability as well as frame marker operation. The chip is fabricated in a commercially available 180nm CMOS technology using dual 3.3V/1.8V supply. It achieves more than ±10% gain tunability at 0-1.2V sensor dark-level range, and up to 142MHz operation. Power consumption is measured at 37mW/channel with 155µV input-referred noise, at nominal conditions. The chip is a low-power, low-noise, highly optimized solution allowing area and power reduction in camera assemblies.

Published
2019

11. Testing the 10 spectrograph units for DESI: approach and results

Author

Perruchot, Sandrine, primary, Blanc, Pierre-Éric, additional, Guy, Julien, additional, Le Guillou, Laurent, additional, Ronayette, Samuel, additional, Régal, Xavier, additional, Castagnoli, Gérard, additional, Le Van Suu, Auguste, additional, Sepulveda, Eduardo, additional, Jullo, Eric, additional, Cuby, Jean-Gabriel, additional, Karkar, Sonia, additional, Ghislain, Patrick, additional, Repain, Philippe, additional, Carton, P.-H., additional, Magneville, C., additional, Ealet, Anne, additional, Escoffier, Stéphanie, additional, Secroun, Aurélia, additional, Honscheid, Klaus, additional, Elliott, Ann, additional, Jelinsky, Patrick N., additional, David, Brooks, additional, Peter, Doel, additional, Yutong, Duan, additional, Jerry, Edelstein, additional, Juan Cruz, Estrada, additional, Enrique, Gastañaga, additional, Armin, Karcher, additional, Martin, Landriau, additional, Michael, Levi, additional, Paul, Martini, additional, Nathalie, Palanque-Delabrouille, additional, Francisco, Prada, additional, Gragory, Tarle, additional, and Kai, Zhang, additional

Published
2020
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12. ProtoDESI: First On-Sky Technology Demonstration for the Dark Energy Spectroscopic Instrument

Author

Ann Elliott, Anthony Paat, José M. Illa, David J. Schlegel, Laia Cardiel, A. N. Robertson, W. Emmet, Michael Levi, Arjun Dey, Richard R. Joyce, David Rabinowitz, A. Lambert, Parker Fagrelius, Ronald G. Probst, Armin Karcher, Christian Soto, G. Tarle, D. Summers, Christopher J. Manser, Yutong Duan, Jorge Jiménez, Lori Allen, Joseph H. Silber, Behzad Abareshi, O. Ballester, Paul Martini, Michael Schubnell, David Sprayberry, Michael Lampton, C. Baltay, Stephen J. Kent, K. Honscheid, E. Buckley-Geer, C. M. Rockosi, Karen Butler, Robert Besuner, Benjamin A. Weaver, Kevin Reil, Irena Gershkovich, Santiago Serrano, and Robert Marshall

Subjects
Physics, media_common.quotation_subject, observational [methods], Astronomy, FOS: Physical sciences, Astronomy and Astrophysics, telescopes, Astronomy & Astrophysics, 01 natural sciences, 010309 optics, ) dark energy [(cosmology], Space and Planetary Science, Sky, 0103 physical sciences, Dark energy, Astrophysics - Instrumentation and Methods for Astrophysics, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), miscellaneous [instrumentation], Astronomical and Space Sciences, media_common, astro-ph.IM
Abstract

The Dark Energy Spectroscopic Instrument (DESI) is under construction to measure the expansion history of the universe using the baryon acoustic oscillations technique. The spectra of 35 million galaxies and quasars over 14,000 square degrees will be measured during a 5-year survey. A new prime focus corrector for the Mayall telescope at Kitt Peak National Observatory will deliver light to 5,000 individually targeted fiber-fed robotic positioners. The fibers in turn feed ten broadband multi-object spectrographs. We describe the ProtoDESI experiment, that was installed and commissioned on the 4-m Mayall telescope from August 14 to September 30, 2016. ProtoDESI was an on-sky technology demonstration with the goal to reduce technical risks associated with aligning optical fibers with targets using robotic fiber positioners and maintaining the stability required to operate DESI. The ProtoDESI prime focus instrument, consisting of three fiber positioners, illuminated fiducials, and a guide camera, was installed behind the existing Mosaic corrector on the Mayall telescope. A Fiber View Camera was mounted in the Cassegrain cage of the telescope and provided feedback metrology for positioning the fibers. ProtoDESI also provided a platform for early integration of hardware with the DESI Instrument Control System that controls the subsystems, provides communication with the Telescope Control System, and collects instrument telemetry data. Lacking a spectrograph, ProtoDESI monitored the output of the fibers using a Fiber Photometry Camera mounted on the prime focus instrument. ProtoDESI was successful in acquiring targets with the robotically positioned fibers and demonstrated that the DESI guiding requirements can be met., Comment: Accepted version

Published
2018

13. Status of the CCD development for the Dark Energy Spectroscopic Instrument

Author

N. Palaio, J.S. Lee, G. Wang, S. Haque, M. Bonati, P. Jelinsky, William F. Kolbe, Donald E. Groom, J. Emes, S.E. Holland, R. Frost, R. Groulx, Chris Bebek, Juan Estrada, David J. Schlegel, and Armin Karcher

Subjects
010302 applied physics, Physics, visible and IR photons, Oscillation, business.industry, 01 natural sciences, Noise (electronics), Nuclear & Particles Physics, Baryon, Other Physical Sciences, Optics, Engineering, Affordable and Clean Energy, 0103 physical sciences, Physical Sciences, Dark energy, Quantum efficiency, Solid state detectors, business, 010303 astronomy & astrophysics, Instrumentation, Photon detectors for UV, visible and IR photons (solid-state), Mathematical Physics
Abstract

© 2017 IOP Publishing Ltd and Sissa Medialab srl. We describe improvements in CCD performance that have been achieved on 4k×4k, (15 μm)2-pixel, fully depleted CCDs for the Dark Energy Spectroscopic Instrument (DESI) [1]. With respect to our previous work on CCDs for the Dark Energy Camera and the Baryon Oscillation Spectroscopic Survey, our goals for the DESI CCD development were to improve read noise and quantum efficiency, improve the astrometric precision, and decrease pixel-size variations. We report experimental results on recently fabricated CCDs to be used in DESI.

Published
2017

14. Mosaic3: a red-sensitive upgrade for the prime focus camera at the Mayall 4m telescope

Author

David J. Schlegel, Bob Stupak, Armin Karcher, Chris Bebek, John B. Donaldson, Dick Joyce, David Rabinowitz, Dustin Lang, Philip N. Daly, Michael Levi, Bob Marshall, F. Valdes, Lori Allen, Bob Blum, David Sprayberry, Arjun Dey, C. Baltay, Will Emmet, M. Fitzpatrick, Heidi Schweiker, Behzad Abareshi, and Tom Hurteau

Subjects
Physics, Galactic astronomy, 010308 nuclear & particles physics, media_common.quotation_subject, Astronomy, Astrophysics, Astronomical survey, 01 natural sciences, Galaxy, law.invention, Telescope, Upgrade, Sky, Observatory, law, 0103 physical sciences, Baryon acoustic oscillations, 010303 astronomy & astrophysics, media_common
Abstract

The Dark Energy Spectroscopic Instrument (DESI) is under construction and will be used to measure the expansion history of the Universe using the Baryon Acoustic Oscillation (BAO) technique and the growth of structure using redshift-space distortions (RSD). The spectra of 30 million galaxies over 14000 sq deg will be measured over the course of the experiment. In order to provide spectroscopic targets for the DESI survey, we are carrying out a three-band (g,r,z ) imaging survey of the sky using the NOAO 4-m telescopes at Kitt Peak National Observatory (KPNO) and the Cerro Tololo Interamerican Observatory (CTIO). At KPNO, we will use an upgraded version of the Mayall 4m telescope prime focus camera, Mosaic3, to carry out a z-band survey of the Northern Galactic Cap at declinations δ≥+30 degrees. By equipping an existing Dewar with four 4kx4k fully depleted CCDs manufactured by the Lawrence Berkeley National Laboratory (LBNL), we increased the z-band throughput of the system by a factor of 1.6. These devices have the thickest active area fielded at a telescope. The Mosaic3 z-band survey will be complemented by g-band and r-band observations using the Bok telescope and 90 Prime imager on Kitt Peak. We describe the upgrade and performance of the Mosaic3 instrument and the scope of the northern survey.

Published
2016

15. The dark energy camera

Author

P. Doel, A. A. Plazas, Kevin Reil, R. H. Schindler, J.-P. Rheault, Douglas L. Tucker, A. Roodman, Armin Karcher, Ricardo L. C. Ogando, L. Beaufore, B. Yanny, G. Gutierrez, R. Schmitt, H. Cease, Marco Bonati, G. Derylo, Katherine Schultz, K. Honscheid, Rebecca A. Bernstein, Curtis Weaverdyck, Robert J. Woods, Eric H. Neilsen, Josh Frieman, Jennifer L. Marshall, R. Flores, M. Jonas, J. Lee, Darren L. DePoy, S.E. Holland, O. Alvarez, Richard G. Kron, Jiangang Hao, John Peoples, H. T. Diehl, Terri Shaw, J. Emes, A. Sypniewski, D. Boprie, Donna Kubik, B. Flaugher, S. E. Kuhlmann, B. Bigelow, Juan Estrada, V. Scarpine, J. M. Cela-Ruiz, Michael Schubnell, R. Angstadt, Cheryl Jackson, David J. James, W. C. Wester, D. A. Finley, J. Rauch, K. Patton, K. Kuehn, Ann Elliott, Alex Drlica-Wagner, N. Palio, A. Lathrop, O. Ballester, F. Munoz, M. Antonik, K. Kuk, D. Huffman, T. M. C. Abbott, J. De Vicente, Ricardo Schmidt, O. Lahav, J. Campa, Michael D. Gladders, Steve Kent, Robert C. Nichol, J. Annis, Mark Kozlovsky, E. J. Sanchez, B. Gregory, G. Wang, Tianjun Li, Steve Chappa, E. Dede, M. G. Watson, C. Cooper, Robert Connon Smith, H. Rogers, Gary Bernstein, Jon J Thaler, Brian Nord, Jamieson Olsen, Natalie A. Roe, C. Tran, Javier Castilla, K. W. Merritt, W. Stuermer, Ramon Miquel, I. Karliner, Francisco J. Castander, G. Martinez, R. Tighe, David J. Brooks, Peter Lewis, G. Tarle, L. N. da Costa, A. Fausti Neto, L. Scott, Laia Cardiel-Sas, S. Serrano, Edward C. Chi, Richard Kessler, Michael Levi, A. Stefanik, E. Suchyta, J. Eiting, Alistair R. Walker, Marcelle Soares-Santos, Scott Holm, P. Schurter, I. Mandrichenko, E. Buckley-Geer, and D. W. Gerdes

Subjects
Cosmology and Gravitation, Aperture, FOS: Physical sciences, Field of view, Noise (electronics), law.invention, Telescope, WNU, Optics, surveys, law, Shutter, photometers [instrumentation], Instrumentation and Methods for Astrophysics (astro-ph.IM), STFC, Physics, detectors [instrumentation], Pixel, business.industry, RCUK, Astronomy and Astrophysics, observations [cosmology], atlases, Cardinal point, Space and Planetary Science, Astrophysics - Instrumentation and Methods for Astrophysics, business, Focus (optics), catalogs, astro-ph.IM
Abstract

The Dark Energy Camera is a new imager with a 2.2-degree diameter field of view mounted at the prime focus of the Victor M. Blanco 4-meter telescope on Cerro Tololo near La Serena, Chile. The camera was designed and constructed by the Dark Energy Survey Collaboration, and meets or exceeds the stringent requirements designed for the wide-field and supernova surveys for which the collaboration uses it. The camera consists of a five element optical corrector, seven filters, a shutter with a 60 cm aperture, and a CCD focal plane of 250 micron thick fully-depleted CCDs cooled inside a vacuum Dewar. The 570 Mpixel focal plane comprises 62 2kx4k CCDs for imaging and 12 2kx2k CCDs for guiding and focus. The CCDs have 15 microns x15 microns pixels with a plate scale of 0.263 arc sec per pixel. A hexapod system provides state-of-the-art focus and alignment capability. The camera is read out in 20 seconds with 6-9 electrons readout noise. This paper provides a technical description of the camera's engineering, construction, installation, and current status., Comment: submitted to AJ Corresponding Authors H. T. Diehl (diehl@fnal.gov)

Published
2015

16. Radiation Tolerance of Fully-Depleted P-Channel CCDs Designed for the SNAP Satellite

Author

Steven E. Holland, William F. Kolbe, J. Saha, Chris Bebek, Kyle S. Dawson, N. A. Roe, J. Emes, Armin Karcher, K. Takasaki, Nicholas P. Palaio, Guobin Wang, and Sharon R. Jelinsky

Subjects
Physics, Nuclear and High Energy Physics, business.industry, Astrophysics (astro-ph), Cyclotron, FOS: Physical sciences, Astrophysics, Electron, law.invention, Wavelength, Optics, P channel, Nuclear Energy and Engineering, Radiation tolerance, law, Quantum efficiency, Irradiation, Electrical and Electronic Engineering, business, Dark current
Abstract

Thick, fully depleted p-channel charge-coupled devices (CCDs) have been developed at the Lawrence Berkeley National Laboratory (LBNL). These CCDs have several advantages over conventional thin, n-channel CCDs, including enhanced quantum efficiency and reduced fringing at near-infrared wavelengths and improved radiation tolerance. Here we report results from the irradiation of CCDs with 12.5 and 55 MeV protons at the LBNL 88-Inch Cyclotron and with 0.1-1 MeV electrons at the LBNL Co60 source. These studies indicate that the LBNL CCDs perform well after irradiation, even in the parameters in which significant degradation is observed in other CCDs: charge transfer efficiency, dark current, and isolated hot pixels. Modeling the radiation exposure over a six-year mission lifetime with no annealing, we expect an increase in dark current of 20 e/pixel/hr, and a degradation of charge transfer efficiency in the parallel direction of 3e-6 and 1e-6 in the serial direction. The dark current is observed to improve with an annealing cycle, while the parallel CTE is relatively unaffected and the serial CTE is somewhat degraded. As expected, the radiation tolerance of the p-channel LBNL CCDs is significantly improved over the conventional n-channel CCDs that are currently employed in space-based telescopes such as the Hubble Space Telescope., 11 pages, 10 figures, submitted to IEEE Transactions

Published
2008

17. Reduced Charge Diffusion in Thick, Fully Depleted CCDs With Enhanced Red Sensitivity

Author

Jessamyn A. Fairfield, Armin Karcher, Donald E. Groom, Chris Bebek, W.F. Koble, S.E. Holland, Wolfgang Lorenzon, Stephen Bailey, and Natalie A. Roe

Subjects
Point spread function, Physics, Nuclear and High Energy Physics, business.industry, Biasing, Substrate (electronics), symbols.namesake, Acceleration, Optics, Nuclear Energy and Engineering, Gaussian function, symbols, Electrical and Electronic Engineering, Diffusion (business), business, Image resolution, Voltage
Abstract

Lateral charge diffusion in charge-coupled devices (CCDs) dominates the device point-spread function (PSF), which can affect both image quality and spectroscopic resolution. We present new data and theoretical interpretations for lateral charge diffusion in thick, fully depleted CCDs developed at Lawrence Berkeley National Laboratory (LBNL). Because they can be overdepleted, the LBNL devices have no field-free region and diffusion is controlled through the application of an external bias voltage. Recent improvements in CCD design at LBNL allow the application of bias voltages exceeding 200 V. We give results for a 3512times3512 format, 10.5 mum pixel back-illuminated p-channel CCD developed for the SuperNova/Acceleration Probe (SNAP), a proposed satellite-based experiment designed to study dark energy. Lateral charge diffusion, which is well described by a symmetric two-dimensional (2-D) Gaussian function, was measured at substrate bias voltages between 3 and 115 V. At a bias voltage of 115 V, we measure a root-mean square (rms) diffusion of 3.7plusmn0.2mum. Lateral charge diffusion in LBNL CCDs will meet the SNAP requirements

Published
2006

18. A binary link tracker for the BABAR level 1 trigger system

Author

T.H. Liu, M. S. Gill, Krista M. Marks, Carl Grace, M. E. Levi, Alexander H. Montgomery, H.K. Chen, D. Kasen, C. LeClerc, F.A. Kirsten, S.F. Dow, J. F. Kral, J.K. Johnson, R.C. Jared, A. Berenyi, Armin Karcher, A. Romosan, A.B. Meyer, R. Minor, Stefan Gehrig, K. Dao, and H. von der Lippe

Subjects
Physics, Nuclear and High Energy Physics, business.industry, Hardware description language, Detector, Electrical engineering, Programmable logic device, Nuclear Energy and Engineering, Logic gate, Nuclear electronics, VHDL, Electrical and Electronic Engineering, Control logic, Field-programmable gate array, business, computer, Computer hardware, computer.programming_language
Abstract

The BABAR detector at PEP-II will operate in a high-luminosity e/sup +/e/sup -/ collider environment near the /spl Upsi/(4S) resonance with the primary goal of studying CP violation in the B meson system. In this environment, typical physics events of interest involve multiple charged particles. These events are identified by counting these tracks in a fast first level (Level 1) trigger system, by reconstructing the tracks in "real time". For this purpose, a Binary Link Tracker Module (BLTM) was designed and fabricated for the BABAR Level 1 Drift Chamber trigger system. The BLTM is responsible for linking track segments, constructed by the Track Segment Finder Modules (TSFM), into complete tracks. A single BLTM module processes a 360 MBytes/s stream of segment hit data, corresponding to information from the entire Drift Chamber, and implements a fast and robust algorithm that tolerates high hit occupancies as well as local inefficiencies of the Drift Chamber. The algorithms and the necessary control logic of the BLTM were implemented in Field Programmable Gate Arrays (FPGAs), using the VHDL hardware description language. The finished 9U/spl times/400 mm Euro-format board contains roughly 75,000 gates of programmable logic or about 10,000 lines of VHDL code synthesized into five FPGAs.

Published
1999

19. Design and performance of the Elefant digitizer IC for the BaBar drift chamber

Author

H. von der Lippe, S.F. Dow, M. Momayezi, Armin Karcher, David Ando, and M. E. Levi

Subjects
Nuclear and High Energy Physics, Engineering, business.industry, Detector, Transistor, Electrical engineering, Hardware_PERFORMANCEANDRELIABILITY, Integrated circuit, Flash ADC, law.invention, Nuclear Energy and Engineering, CMOS, law, Nuclear electronics, Hardware_INTEGRATEDCIRCUITS, Electronic engineering, Electrical and Electronic Engineering, Full custom, business, Electronic circuit
Abstract

A 250,000 transistor full custom integrated circuit for the readout of drift chamber signals has been developed, produced and characterized. The "Elefant" (ELEctronics For Amplitude 'N Timing) Digitizer IC is designed to measure both the charge and the single electron time of arrival of sense wire signals from the BaBar drift chamber. By combining a FADC (flash analog-to-digital converter) and a TDC (time-to-digital converter) for each channel, the digitizer IC can be optimized and simplified, to achieve the physics goals required of the drift chamber while reducing the per channel costs of the electronics. The Elefant IC also implements portions of the BaBar trigger protocols to simplify the connection of the chip to the rest of the BaBar detector. Each IC contains eight complete independent channels. The circuit has been implemented in a 0.8 /spl mu/m triple metal CMOS process and fabricated in production quantity to fully instrument the BaBar drift chamber and are now in operation. Performance results of the IC will be presented.

Published
1999

20. Continuously live image processor for drift chamber track segment triggering

Author

R. Minor, Stefan Gehrig, Carl Grace, Krista M. Marks, A.B. Meyer, K. Dao, A. Berenyi, D. Kasen, H. von der Lippe, J.E. Kral, J.K. Johnson, S.F. Dow, R.C. Jared, M. S. Gill, H.K. Chen, C. LeClerc, T.H. Liu, Alexander H. Montgomery, F.A. Kirsten, A. Romosan, Armin Karcher, and M. E. Levi

Subjects
Nuclear and High Energy Physics, Engineering, business.industry, Image processor, Interface (computing), Pipeline (computing), BaBar experiment, Printed circuit board, Nuclear Energy and Engineering, Nuclear electronics, VHDL, Electronic engineering, Electrical and Electronic Engineering, Field-programmable gate array, business, computer, Computer hardware, computer.programming_language
Abstract

The first portion of the BABAR experiment Level 1 Drift Chamber Trigger pipeline is the Track Segment Finder (TSF). Using a novel method incorporating both occupancy and drift-time information, the TSF system continually searches for segments in the supercells of the full 7104-wire Drift Chamber hit image at 3.7 MHz. The TSF was constructed to operate in a potentially high beam-background environment while achieving high segment-finding efficiency, deadtime-free operation, a spatial resolution of

Published
1999

21. CCD research and development at Lawrence Berkeley National Laboratory

Author

S.E. Holland, Natalie A. Roe, Peter Denes, F. Dion, J. Emes, J.S. Lee, S. Haque, William F. Kolbe, Rebecca Coles, Chris Bebek, R. Groulx, G. Wang, Donald E. Groom, N. Palaio, C. H. Tran, R. Frost, and Armin Karcher

Subjects
Physics, Fabrication, Optics, business.industry, Amplifier, Noise reduction, Near-infrared spectroscopy, Optoelectronics, Quantum efficiency, Charge-coupled device, business, Noise (electronics), Capacitance
Abstract

We describe work at Lawrence Berkeley National Laboratory (LBNL) to develop enhanced performance, fully depleted, back-illuminated charge-coupled devices for astronomy and astrophysics. The CCDs are fabricated on high-resistivity substrates and are typically 200–300 μm thick for improved near-infrared response. The primary research and development areas include methods to reduce read noise, increase quantum efficiency and readout speed, and the development of fabrication methods for the efficient production of CCDs for large focal planes. In terms of noise reduction, we will describe technology developments with our industrial partner Teledyne DALSA Semiconductor to develop a buried-contact technology for reduced floating-diffusion capacitance, as well as efforts to develop ”skipper” CCDs with sub-electron noise utilizing non-destructive readout amplifiers allowing for multiple sampling of the charge packets. Improvements in quantum efficiency in the near-infrared utilizing ultra-high resistivity substrates that allow full depletion of 500 μm and thicker substrates will be described, as well as studies to improve the blue and UV sensitivity by investigating the limits on the thickness of the back-side ohmic contact layer used in the LBNL technology. Improvements in readout speed by increasing the number of readout ports will be described, including work on high frame-rate CCDs for x-ray synchrotrons with as many as 192 amplifiers per CCD. Finally, we will describe improvements in fabrication methods, developed in the course of producing over 100 science-grade 2k × 4k CCDs for the Dark Energy Survey Camera.

Published
2012

22. Design and performance of an R-θ fiber positioner for the BigBOSS instrument

Author

Armin Karcher, Paul Perry, K. Wilson, P. Jelinsky, C. Schenk, Mario Cepeda, H. Heetderks, Rodney Post, Michael Sholl, Frederic Becker, Thomas Johnson, Robert Besuner, Jerry Edelstein, Zengxaing Zhou, Chris Bebek, E. Anderssen, and Joseph H. Silber

Subjects
Optical fiber, Computer science, business.industry, Kinematics, Redshift, law.invention, Power (physics), Telescope, Optics, law, Eccentric, Polar, business, Spectrograph, Envelope (motion)
Abstract

The BigBOSS instrument is a proposed multi-object spectrograph for the Mayall 4m telescope at Kitt Peak, which will measure the redshift of 20 million galaxies and map the expansion history of the universe over the past 8 billion years, surveying 10-20 times the volume of existing studies. For each 20 minute observation, 5000 optical fibers are individually positioned by a close-packed array of 5000 robotic positioner mechanisms. Key mechanical constraints on the positioners are: o12mm hardware envelope, o14mm overlapping patrol zones, open-loop targeting accuracy ≤ 40μm, and step resolution ≤ 5μm, among other requirements on envelope, power, stability, and speed. This paper describes the design and performance of a newly-developed fiber positioner with R-θ polar kinematics, in which a flexure-based linear R-axis is stacked on a rotational θ-axis. Benefits over the usual eccentric parallel axis θ-φ kinematic approach include faster repositioning, simplified anti-collision schemes, and inherent anti-backlash preload. Performance results are given for complete positioner assemblies as well as sub-component hardware characterization.

Published
2012

23. Design of low-noise output amplifiers for P-channel charge-coupled devices fabricated on high-resistivity silicon

Author

Armin Karcher, S.E. Holland, Y. Yu, R. Frost, G. Wang, F. Dion, Natalie A. Roe, S. Haque, R. Groulx, and William F. Kolbe

Subjects
Materials science, FET amplifier, business.industry, Amplifier, Transistor, Low-noise amplifier, law.invention, law, Current sense amplifier, Hardware_INTEGRATEDCIRCUITS, Linear amplifier, Optoelectronics, Instrumentation amplifier, business, Direct-coupled amplifier
Abstract

We describe the design and optimization of low-noise, single-stage output amplifiers for p-channel charge-coupled devices (CCDs) used for scientific applications in astronomy and other fields. The CCDs are fabricated on highresistivity, 4000-5000 Ω-cm, n-type silicon substrates. Single-stage amplifiers with different output structure designs and technologies have been characterized. The standard output amplifier is designed with an n+ polysilicon gate that has a metal connection to the sense node. In an effort to lower the output amplifier readout noise by minimizing the capacitance seen at the sense node, buried-contact technology has been investigated. In this case, the output transistor has a p+ polysilicon gate that connects directly to the p+ sense node. Output structures with buried-contact areas as small as 2 μm × 2 μm are characterized. In addition, the geometry of the source-follower transistor was varied, and we report test results on the conversion gain and noise of the various amplifier structures. By use of buried-contact technology, better amplifier geometry, optimization of the amplifier biases and improvements in the test electronics design, we obtain a 45% reduction in noise, corresponding to 1.7 e- rms at 70 kpixels/sec.

Published
2012

24. The BABAR Physics Book: Physics at an Asymmetric B Factory

Author

B.F.L. Ward, D.A. Roberts, Stefan Kluth, David Atwood, P. N. Y. David, V. Suraiya, E. I. Rosenberg, C. T. Day, A. A. Salnikov, F. Anulli, S. Dittongo, Armin Karcher, Jonathan M. Flynn, M. Benkebil, Kalelkar, Stephen F. Schaffner, G. Carlino, M.E. Levi, V. Savinov, C. P. Jessop, M. K. Sullivan, Fabio Morsani, M. Rotondo, N. Regnault, R. Aleksan, G. De Nardo, S. S. Hertzbach, J. Va’vra, A. I. McNab, Ralph Müller-Pfefferkorn, Herbert Koch, C. Lu, D. Judd, M. Turri, G. Lynch, Gerhard Buchalla, M. L. Kocian, A. DeSilva, Tom Rizzo, A. M. Eisner, Janice Button-Shafer, G. R. Bonneaud, Y. u. G. Kolomensky, K.C. Moffeit, R. H. Schindler, J. Dorfan, J. M. Bauer, L. M. Cremaldi, L. Piemontese, A. M. Boyarski, R. Bartoldus, Zongfu Yu, Alyssa Garcia, G. Hamel de Monchenault, R. S. Panvini, D.H. Coward, G. Zioulas, H. Yu, A. Asmone, D. Falciai, D. J. B. Smith, F. Zhang, P.P. Xie, J. A. Nash, M. Lo Vetere, Stefano Mazzoni, J. M. Bishop, D. Fujino, Ikaros I.Y. Bigi, A. Mass, Zoltan Ligeti, Paola Grosso, G. Finocchiaro, V. Luth, D. G. Hitlin, P. Rankin, G. Castelli, Krisztian Peters, J. Pavlovich, R.D. Peccei, M. V. Purohit, D. Renner, T. Dignan, Francesco Lanni, P. Strother, F. Forti, M. Verderi, Ph Leruste, A. Khan, E. Tetteh-Lartey, J. Albert, E. Chen, B. Stugu, E. Gabathuler, T. Schalk, R. M. Bionta, A. Stahl, G. Wormser, A.K. McKemey, R. Kroeger, W. R. Innes, C. Evangelista, W.A. Wenzel, C. Gatto, B. Mayer, F. C. Porter, D. B. MacFarlane, C.T. Sachrajda, P.L. Anthony, J. Brose, A. B. Meyer, A. Snyder, T.J. Champion, A. Calcaterra, C. Roat, X. C. Lou, F. Costantini, D. P. Stoker, O. Hamon, Laurent Lellouch, R.G. Alsmiller, D. Wyler, H. Lan, Willem G. J. Langeveld, U. Nauenberg, J. O. Nielsen, P.A. Hart, O. Pene, D. Su, M. C. Gonzalez-Garcia, M. Carpinelli, Valerio Re, G. Triggiani, B.B. Naranjo, W. Dunwoodie, T. A. Gabriel, A. Samuel, M. Piccolo, Tiehui Liu, A. Valassi, S. Chuniv, N. A. Roe, G. P. Dubois-Felsmann, A. Trunov, G. Batignani, Ren-Yuan Zhu, G. Blaylock, A.S. Dighe, Reinhold Rückl, R. Faccini, F. Ferrarotto, A. J. Lankford, C. Dallapiccola, H. Marsiske, Randall P. Johnson, R. N. Cahn, H. Krieg, R. M. Martin, Maria Roberta Monge, D. R. Johnson, C.G. Boyd, F. Le Diberder, G. Vasileiadis, T. Himel, C. A. Heusch, J. Allison, S. F. Ganzhur, C. LeClerc, Marcel Kunze, D.E. Dorfan, M. Mandelkern, L. Martin, A. Bajic, J. D. Richman, W. S. Lockman, W. J. Wisniewski, L.S. Rochester, Luca Silvestrini, V. E. Blinov, B. Camanzi, F. Dal Corso, Giorgi, G. Michelon, N. Dyce, S. J. Yellin, A. Hasan, M. T. Ronan, J. M. Roney, David London, Luca Lista, E. Lamanna, G. Dahlinger, Q. Fan, Andreas Hoecker, D. A. Sanders, M. R. Convery, J. G. Smith, Crisostomo Sciacca, D. Aston, E.P. Potter, G. Rizzo, L. Lanceri, Guido Martinelli, R. Pitthan, W. Yang, N. De Groot, P. J. Oddone, D. W. G. S. Leith, D.P. Coupal, Michael Doser, R. Zaliznyak, A. Walkden, D. Fong, E. Mandelli, I. M. Peruzzi, Peter Elmer, C. Hast, G. Piredda, N. Copty, M. Morii, E. Charles, Yuval Grossman, G. Calderini, K. T. McDonald, Pierluigi Paolucci, N. Savvas, R. W. Kadel, Benjamin Grinstein, C. Hearty, R. Kerth, J. L. Wittlin, V.V. Serbo, Marco Pallavicini, F. Galeazzi, M. Turcotte, M. Mugge, A. Firestone, Sridhara Dasu, Alexey A. Petrov, D. J. Summers, J.H. Cooke, Mark B. Wise, I. Adam, M. Munson, B. N. Ratcliff, S. I. Serednyakov, F. Bianchi, Laura Reina, A. de Lesquen, Sh. Rahatlou, Alessandra Forti, T. J. Brandt, M. Pripstein, A. Perazzo, V. I. Telnov, M. Milek, Enrico Robutti, R. Prepost, N. D. Qi, R. Schwierz, K. van Bibber, Lodovico Ratti, Jeremy A. Johnson, M. Folegani, A. Palano, W. D. Shephard, A. Romosan, P.F. Jacques, J.H. Weatherall, Russell S. Hamilton, R. R. Kofler, D. Zanin, P. C. Kim, A. Eppich, B. Foster, F. Palombo, Vivek Sharma, Ingrid U. Scott, D. E. Wagoner, W. Orejudos, G. Cavoto, C. C. Buchanan, Brad Abbott, David Nathan Brown, B. DiGirolamo, H. L. Lynch, P. J. Clark, Michael C. Carroll, R. G. Jacobsen, Y. Guo, G. Vuagnin, M. Lusignoli, A. Romero, W. T. Meyer, M. Prest, C. L. Davis, Johann Cohen-Tanugi, R. Vitale, F.E. Close, R. Gamet, Stephen J. McMahon, Francesca Borzumati, T. S. Mattison, Helen R. Quinn, E. A. Kravchenko, M. Weaver, Thomas Mannel, P. D. Dauncey, R. Baldini-Ferroli, M. Haire, Jayashree Roy, K. Paick, Robert Wilson, A. Pugliese, Hartmut Sadrozinski, D. Kirkby, G. Vasseur, Roland Bernet, G.C. Branco, Daniel A. Bauer, M. M. Macri, A. Leona, J.L. Hewett, A. Jawahery, V.G. Shelkov, A. Gaidot, Andrew J. Martin, Michael S. Witherell, T.L. Geld, C. H. Cheng, J.F. Kral, P.D. Barnes, F. F. Wilson, A. R. Clark, G. P. Gopal, S. Emery, S. Playfer, N. M. Cason, J. R. Fry, C. P. O'Grady, S. J. Patton, G. Manzin, T.I. Meyer, A. P. Onuchin, C. Patrignani, U. Mallik, R. Contri, G.P. Chen, V. Tisserand, A. V. Telnov, P. Kunz, W.G. Yan, Matthias Neubert, A. R. Buzykaev, R. de Sangro, V. Lepeltier, H.A. Tanaka, Giovanni Crosetti, J. A. Kadyk, M. Benayoun, D. Boutigny, D. H. Wright, S. Ren, C. Voci, M.P. Worah, V. M. Braun, S. Bettarini, Franco Buccella, S. Fahey, W. H. Toki, C. C. Young, B. Spaan, Jérôme Charles, M. Falbo-Kenkel, J.D. McFall, Patricia Ball, T. Glanzman, H. Briand, H. Mao, D.L. Wagner, A. D. Bukin, A. Zallo, G.L. Godfrey, N. Cavallo, Donghui Li, R. Seitz, Stéphane Plaszczynski, H. Zobernig, Alexander L. Kagan, James D. Wells, A. A. Grillo, C. Touramanis, T. Pulliam, G. W. London, A. B. Breon, A. Masiero, A. W. Borgland, M.G. Pia, A. Woch, V. Zacek, F. Ferroni, O. Wen, Gabriella Sciolla, G. Grosdidier, J. Beringer, J. Schwiening, Frank Gaede, T.L. Hall, N. Kuznetsova, M. Rama, Andris Skuja, J. J. Walsh, J. A. McKenna, A. Tumanov, Fernando Dutra, Valery Pozdnyakov, P. Poropat, G. S. Abrams, I. Dunietz, Anders Ryd, Michael Steinke, S. Morganti, Z. W. Yin, A. J.R. Weinstein, Giulia Ricciardi, G. D. Lafferty, P. M. Patel, A. M. Lutz, S. J. Gowdy, J. Lory, Stephen Robert Wagner, C. Cretsinger, M. Bondioli, A. J. S. Smith, Sau Lan Wu, M. George, N. Paver, I. De Bonis, K. R. Schubert, D. Guetta, J. W. Lamsa, J. Chauveau, G. Simi, H. B. Crawley, Y. S. Zhu, H. Schmücker, E. Vallazza, Alexander Khodjamirian, G. Della Ricca, Sokoloff, E.D. Frank, A. Frey, David Norvil Brown, P. C. Bloom, M.N. Kreisler, Y. B. Pan, Richard Mount, R. Kowalewski, Enrico Nardi, G. Musolino, Y. Nir, K. Lingel, M. Marino, Jane S. Tinslay, C. C. Zhang, J.J. Reidy, Craig R. Wuest, T.J. Pavel, B. Franek, L. Keller, G. De Domenico, M. H. Kelsey, Robert Fleischer, D. R. Quarrie, M. Morandin, C. Yeche, R. Waldi, E. Roussot, Lydia Roos, A. Vitelli, M. Morganti, J. Secrest, D. R. Muller, J. Ohnemus, J.C. Andress, M. H. Schune, G. Burdman, M. Zito, P. Sanders, Owen Rosser Long, A. Seiden, R. Stroili, A. A. Korol, R. K. Yamamoto, J. J. Back, Remi Lafaye, S. Versille, C. Thiebaux, C. Campagnari, M. G. Green, M. Zhao, S. Mettarini, L. Gladney, Amarjit Soni, B. T. Meadows, J. M. LoSecco, L. Behr, G. Raven, P. R. Burchat, L. Oliver, Y. Zheng, R. Parodi, Adam F. Falk, K. T. Flood, V. Miftakov, D. Silverman, N. I. Geddes, C.S. Sutton, J. L. Narjoux, G. Eigen, R. Kapur, E. W. Varnes, J. G. Branson, D. Gamba, W. Zhao, S. Devmal, Y. Karyotakis, C. De La Vaissiere, R. L. Malchow, V. N. Ivanchenko, V. Speziali, Mossadek Talby, P. F. Harrison, P.F. Manfredi, W. T. Ford, X. Shi, Tim Adye, Philip Colangelo, A. Le Yaouanc, G. Mancinelli, J. L. Harton, Yu. I. Skovpen, B. Lewandowski, Davide Piccolo, F. Bulos, Ulrich Nierste, A. Soffer, E. Mirkes, R.J. Plano, A. Mokhtarani, A. Santroni, A. Lusiani, K.G. Baird, Fabian Zomer, Antonio Pich, J. M. Izen, H. Nicholson, E. Nehrlich, L. Del Buono, K. Hall, D. S. Yan, Jens H. Kuhn, S. Yang, Francesco Fabozzi, J. Trischuk, R. Messner, M. Ciuchini, C.S. Lin, V. Eschenburg, P. Taras, A. Lu, Elliott D. Bloom, Scott D. Metzler, L. Bosisio, R. C. W. Henderson, Ulrik Egede, R. Cowan, Y.Y. Keum, Corrado Angelini, A. Smol, J. Martin, B. A. Schumm, Gino Isidori, A. Buzzo, R. J. Barlow, Sercan Sen, M. Posocco, and F. De Fazio

Subjects
Physics, Nuclear physics, Particle physics, law, Form factor (quantum field theory), CP violation, BaBar experiment, Particle accelerator, Linear particle accelerator, law.invention, B-factory
Abstract

Results of a year-long workshop devoted to a review of the physics opportunities of the BABAR experiment at the PEP-II B Factory, at the Stanford Linear Accelerator Center laboratory are presented.

Published
2010

25. A low noise, radiation tolerant CCD readout processor for the proposed SNAP satellite

Author

R. Abiad, Armin Karcher, Chris Bebek, J.-P. Walder, Dario Gnani, H. von der Lippe, B. Krieger, G. Chao, and J. Reith

Subjects
Physics, Preamplifier, business.industry, Dynamic range, Electrical engineering, Hardware_PERFORMANCEANDRELIABILITY, Chip, Noise (electronics), CMOS, Operating temperature, Nuclear electronics, Hardware_INTEGRATEDCIRCUITS, business, Voltage reference
Abstract

To simplify the system integration, thermal design and wiring of the SNAP satellite focal plane a custom IC has been developed that can digitize the four output channels of a CCD. This CCD readout IC is designed to operate at room temperature for test purposes and at 140 K, the operating temperature of the focal plane. The chip consists of four-channels of pre-amplifier, double correlated sampler and 14-bit pipeline AD converter. The chip incorporates an innovative circuitry that selects one of three gain levels on a per-pixel basis to achieve greater than 16-bit dynamic range. It has an on-chip voltage reference and programmable configuration registers. We have tested the performance both at room temperature and at 140 K, as well as the radiation tolerance. The ASIC, implemented in a standard 0.25 mum CMOS technology, has a measured readout noise of 6.2 muV rms at 100 kHz readout speed, a measured non-linearity of plusmn5 LSB and a power consumption of 121 mW.

Published
2007

26. A CCD clock controller ASIC using novel design techniques integrated in a CMOS 0.8μm SOI high voltage process

Author

H. von der Lippe, Dario Gnani, B. Krieger, G. Chao, J.-P. Walder, Chris Bebek, R. Abiad, and Armin Karcher

Subjects
Computer science, business.industry, Electrical engineering, High voltage, Hardware_PERFORMANCEANDRELIABILITY, Integrated circuit design, Current source, Application-specific integrated circuit, CMOS, Hardware_INTEGRATEDCIRCUITS, Charge pump, CPU core voltage, business, Voltage
Abstract

An ASIC designed to provide the clock signals to the focal plane CCDs for the SNAP satellite project is presented. A prototype has been implemented in a CMOS 0.8 mum SOI high voltage process in order to accommodate a 20 V output swing. The circuit consists of a main charge pump multiplying the 4 V power supply voltage +/-16 V followed by a controlled current source setting the clock voltage plateaus. A bridge of switches provides the clock voltage transitions at the output. This circuit is designed to operate at room temperature for test purpose and at 140 K, which will be the operating temperature. Novel design techniques used in this chip will be presented in detail along with measurement results obtained on the prototypes.

Published
2007

27. Technology development for 4k × 4k, back- illuminated, fully depleted scientific CCD imagers

Author

S.R. Jelinksy, J.H. Ernes, S.E. Holland, Kyle S. Dawson, William F. Kolbe, G. Wang, Donald E. Groom, Armin Karcher, Chris Bebek, N. Palaio, Natalie A. Roe, C. H. Tran, and P.J. Daniels

Subjects
Physics, Fabrication, Pixel, business.industry, Nuclear electronics, Optoelectronics, Large format, Cryogenics, business, Noise (electronics), Die (integrated circuit), Dark current
Abstract

We have developed scientific charge-coupled devices (CCDs) that are fabricated on high-resistivity, n-type silicon substrates, and have demonstrated fully depleted operation for substrate thicknesses of 200-675 mum with formats as large as 2048 times 4096 (15 mum pixels) and 3512 times 3512 (10.5 mum pixels). The main application area for these devices is space and ground-based astronomy, and the CCDs are operated at cryogenic temperatures with slow-scan readout for good performance in terms of dark current and noise. In this work we describe the technology development efforts needed to realize a 4k times 4k (15 mum pixel) CCD with a die area of (64 mm)2. In particular, we describe improved gettering techniques for low dark current and high charge transfer efficiency that have been developed in order to improve fabrication yields for these very large format CCDs.

Published
2007

28. A precision voltage and current reference for the SNAP CCD readout IC

Author

B. Krieger, I. Grosshans, Armin Karcher, S. Kurz, J.-P. Walder, and G. Chao

Subjects
Power supply rejection ratio, Materials science, Bandgap voltage reference, business.industry, Electrical engineering, Diode-or circuit, Hardware_PERFORMANCEANDRELIABILITY, Integrated circuit layout, CMOS, Hardware_INTEGRATEDCIRCUITS, Optoelectronics, Silicon bandgap temperature sensor, business, Voltage reference, Diode
Abstract

A bandgap reference circuit capable of generating precision voltages below the Vg0 of silicon has been fabricated in a 0.25um, 2.5 V CMOS process. The circuit described is based on an existing topology that intrinsically generates a temperature compensated reference current, which can then be mirrored to provide both current and voltage references. With regard to bandgap reference design, a major deficiency of most modern sub-micron CMOS processes is the lack of any well-characterized forward-biased junction device. A method of device measurement and parameter extraction is presented that allows for the precise simulation of a fixed diode layout for the temperature range -150 to +70 C. The extracted diode model was used to optimize the bandgap design. Measurements of the prototype IC indicate an initial accuracy of 35 mV, a PSRR >60 dB, 12-bit noise performance, and a 10 mV voltage deviation over a range of more than 150 C degrees.

Published
2007

29. CCD development for the Dark Energy Spectroscopic Instrument

Author

N. Palaio, William F. Kolbe, J.S. Lee, Donald E. Groom, Chris Bebek, J. Emes, S. Haque, G. Wang, Armin Karcher, and S.E. Holland

Subjects
Physics, Physics::Instrumentation and Detectors, business.industry, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Semiconductor device, Noise (electronics), Galaxy, Redshift, Wavelength, Optics, Dark energy, Quantum efficiency, Photomask, business, Instrumentation, Mathematical Physics
Abstract

We describe research and development efforts directed towards the production of 4 k × 4 k, 15 μm-pixel, fully depleted CCDs for the Dark Energy Spectroscopic Instrument (DESI). The requirements for DESI include the spectroscopic characterization of large numbers of faint galaxies at high redshift. The identification of the type and the determination of the redshift of the targeted galaxies require the use of thick, fully depleted CCDs with high quantum efficiency at near-infrared wavelengths. We describe our work to improve the CCD performance in terms of quantum efficiency and read noise. We also discuss efforts to reduce the level of image-distortion effects that have been observed on previous CCDs that are due to resistivity striations in the starting silicon and periodic errors in the photomasks used to produce the CCDs.

Published
2015

30. Radiation Tolerance of High-Resistivity LBNL CCDs

Author

K. Takasaki, Kyle S. Dawson, N. Palaio, William F. Kolbe, Armin Karcher, Guobin Wang, Chris Bebek, Natalie A. Roe, J.H. Ernes, S.E. Holland, and Sharon R. Jelinsky

Subjects
Physics, Point spread function, Physics::Instrumentation and Detectors, business.industry, Cyclotron, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, law.invention, Wavelength, Optics, Radiation tolerance, law, Physics::Accelerator Physics, Optoelectronics, Quantum efficiency, Astrophysics::Earth and Planetary Astrophysics, Irradiation, business, Charge transfer efficiency, Dark current
Abstract

Thick, fully-depleted p-channel charge-coupled devices (CCDs) have been developed at the Lawrence Berkeley National Laboratory (LBNL). These CCDs have several advantages over conventional n-channel CCDs, including enhanced quantum efficiency and reduced fringing at near-infrared wavelengths, a small point spread function, and improved radiation tolerance. Here we report results from the irradiation of CCDs with 12.5 and 55 MeV protons at the LBNL 88-Inch Cyclotron. These studies indicate that the CCDs still perform well after irradiation, even in the parameters in which significant degradation is expected: charge transfer efficiency, dark current, and isolated hot pixels. As expected, the radiation tolerance of the LBNL CCDs is significantly improved over conventional n-channel CCDs currently employed in space-based telescopes such as the Hubble Space Telescope (HST).

Published
2006

31. High-voltage-compatable, fully depleted CCDs

Author

Stephen Holland, Max H. Fabricius, Armin Karcher, Natalie A. Roe, Kyle S. Dawson, Chris Bebek, Jessaym A. Fairfield, Guobin Wang, N. Palaio, John E. Emes, Donald E. Groom, and William F. Kolbe

Subjects
Physics, Substrate bias voltage, Optics, Silicon, chemistry, business.industry, Optoelectronics, chemistry.chemical_element, High voltage, Substrate (electronics), business, National laboratory, Static induction transistor
Abstract

We describe charge-coupled device (CCD) developmentactivities at the Lawrence Berkeley National Laboratory (LBNL).Back-illuminated CCDs fabricated on 200-300 mu m thick, fully depleted,high-resistivity silicon substrates are produced in partnership with acommercial CCD foundry.The CCDs are fully depleted by the application ofa substrate bias voltage. Spatial resolution considerations requireoperation of thick, fully depleted CCDs at high substrate bias voltages.We have developed CCDs that are compatible with substrate bias voltagesof at least 200V. This improves spatial resolution for a given thickness,and allows for full depletion of thicker CCDs than previously considered.We have demonstrated full depletion of 650-675 mu m thick CCDs, withpotential applications in direct x-ray detection. In this work we discussthe issues related to high-voltage operation of fully depleted CCDs, aswell as experimental results on high-voltage-compatible CCDs.

Published
2006

32. Quantum efficiency characterization of back-illuminated CCDs: Part II. Reflectivity measurements

Author

Donald E. Groom, Armin Karcher, Chris Bebek, Natalie A. Roe, and Maximilian Fabricius

Subjects
Physics, Optical fiber, business.industry, law.invention, Photodiode, Optical path, Signal-to-noise ratio, Optics, law, Optoelectronics, Quantum efficiency, Charge-coupled device, business, Optical path length, Monochromator
Abstract

The usual quantum efficiency (QE) measurement heavily relies on a calibrated photodiode (PD) and the knowledge of the CCDs gain. Either can introduce significant systematic errors. But reflectivity can also be used to verify QE measurements. 1 - R > QE, where R is the reflectivity, and over a significant wavelength range, 1 - R = QE. An unconventional reflectometer has been developed to make this measurement. R is measured in two steps, using light from the lateral monochromator port via an optical fiber. The beam intensity is measured directly with aPD, then both the PD and CCD are moved so that the optical path length is unchanged and the light reflects once from the CCD; the PD current ratio gives R. Unlike traditional schemes this approach makes only one reflection from the CCD surface. Since the reflectivity of the LBNL CCDs might be as low as 2 percent this increases the signal to noise ratio dramatically. The goal is a 1 percent accuracy. We obtain good agreement between 1 - R and the direct QE results.

Published
2006

33. Quantum efficiency characterization of LBNL CCD's: Part I. The quantum efficiency machine

Author

Armin Karcher, Donald E. Groom, Jens Steckert, William F. Kolbe, Chris Bebek, Natalie A. Roe, and Maximilian Fabricius

Subjects
Physics, business.industry, Instrumentation, Light scattering, Photodiode, law.invention, Wavelength, Optics, Integrating sphere, law, Shutter, Optoelectronics, Quantum efficiency, business, Monochromator
Abstract

Instrumentation was developed in 2004 and 2005 to measure the quantum efficiency of the Lawrence Berkeley National Lab (LBNL) total-depletion CCD's, intended for astronomy and space applications. This paper describes the basic instrument. Although it is conventional even to the parts list, there are important innovations. A xenon arc light source was chosen for its high blue/UV and low red/IR output as compared with a tungsten light. Intensity stabilization has been difficult, but since only flux ratios matter this is not critical. Between the light source and an Oriel MS257 monochromator are a shutter and two filter wheels. High-bandpass and low-bandpass filter pairs isolate the 150-nm wide bands appropriate to the wavelength, thus minimizing scattered light and providing order blocking. Light from the auxiliary port enters a 20-inch optical sphere, and the 4-inch output port is at right angles to the input port. An 80 cm drift space produces near-uniform illumination on the CCD. Next to the cold CCD inside the horizontal dewar is a calibrated reference photodiode which is regulated to the PD calibration temperature, 25° C. The ratio of the CCD and in-dewar reference PD signals provides the QE measurement. Additional cross-calibration to a PD on the integrating sphere permits lower-intensity exposures.

Published
2006

34. Integrating Signal Processing and A/D CONVERSION in One Focal Plane Mounted ASIC

Author

Markus Redelstab, Brad Krieger, Armin Karcher, Hendrik von der Lippe, Jean Pierre Walder, Chris Bebek, and Maximilian Fabricius

Subjects
Physics, Signal processing, business.industry, Pipeline (computing), Electrical engineering, Astrophysics, Chip, Photodiode, law.invention, Cardinal point, Application-specific integrated circuit, law, Electronic engineering, Signal integrity, business, Voltage reference
Abstract

Author(s): Karcher, Armin; Bebek, Chris J.; Fabricius, Maximilian; Krieger, Brad; Lippe, Henrik vd; Redelstab, Marcus; Walder, Jean-Peirre | Abstract: The CRIC (CCD Readout IC) ASIC has been designed to meet the power, space and radiation requirements of the SNAP satellite. It incorporates four channels consisting of a pre-amplifier, double correlated sampler and pipeline A/D converter with integrated voltage reference. The CRIC chip has been specifically designed to operate both at room temperature and at typical focal plane temperatures down to 130K. This minimizes wiring complexity while maintaining signal integrity on complex focal planes. CRIC is half of a two ASIC CCD readout system; the other ASIC in development is a bias and clock voltage generator. Also in development, are 16 and 32 channel versions of CRIC for use with hybrid photodiode and near infrared pixel arrays.

Published
2006

35. Supernova / Acceleration Probe: a Satellite Experiment to Study the Nature of the Dark Energy

Author

William W. Craig, Eric Prieto, A. L. Spadafora, A. S. Fruchter, T. Diehl, Gregory Tarle, M. E. Levi, N. Palaio, Susana E. Deustua, Josh Frieman, G. Samdja, Alain Mazure, M. L. Lampton, L. Gladney, Armin Karcher, H. Heetderks, N. Kuznetsova, Eric V. Linder, Edvard Mörtsell, D. W. Gerdes, Douglas L. Tucker, Christopher Stoughton, O. Le Fevre, Saul Perlmutter, Michael L. Brown, Steven E. Kahn, J. I. Lamoureux, Guofeng Wang, Scott Dodelson, Roger F. Malina, D. Rusin, Natalie A. Roe, C. Baltay, Nick Mostek, Dragan Huterer, G. Goldhaber, S. C. Loken, J. P. Marriner, R. Lafever, Hakeem M. Oluseyi, Ralph C. Bohlin, S. T. Holland, A. D. Tomasch, H. von der Lippe, Bhuvnesh Jain, Patrick N. Jelinsky, G. Kushner, E. Basa, John Peoples, Peter Nugent, Jason Rhodes, J. Annis, Greg Aldering, R. Pain, B. Krieger, Alain Bonissent, Keith Taylor, C. R. Bower, F. DeJongh, S. L. Mufson, V. Scarpine, E. Barrelet, D. E. Groom, J.-P. Walder, W. Emmet, Michael Sholl, L. Hui, Lars Bergström, Gary Bernstein, J. A. Musser, W. C. Wester, D. Rabinowitz, M. Hoff, Shawn McKee, J. Snyder, Andrew Szymkowiak, Eugene D. Commins, David H. Pankow, Philip J. Marshall, Timothy A. McKay, N. Morgan, Manfred Bester, Wolfgang Lorenzon, C. T. Day, Andre Tilquin, M.E. Huffer, Roger Smith, Dominique Fouchez, D. Vincent, M. Campbell, A. Goobar, Steve Kent, A. Stebbine, Richard Ellis, Ramon Miquel, William Carithers, Richard Massey, Roger Blandford, Alex G. Kim, P. Limon, H. Lin, A. Refregier, Chris Bebek, Anne Ealet, Pierre Astier, W. Althouse, William F. Kolbe, Michael Schubnell, Rahman Amanullah, George F. Smoot, and C. Bigelow

Subjects
Physics, 010308 nuclear & particles physics, Astronomy, Shape of the universe, Astrophysics::Cosmology and Extragalactic Astrophysics, Cosmological constant, Astrophysics, 7. Clean energy, 01 natural sciences, Galaxy, Redshift, Gravitational lens, Vacuum energy, 13. Climate action, 0103 physical sciences, Dark energy, 010303 astronomy & astrophysics, Weak gravitational lensing
Abstract

The Supernova/Acceleration Probe (SNAP) is a proposed space-based experiment designed to study the dark energy and alternative explanations of the acceleration of the Universe's expansion by performing a series of complementary systematics-controlled astrophysical measurements. We here describe a self-consistent reference mission design that can accomplish this goal with the two leading measurement approaches being the Type Ia supernova Hubble diagram and a wide-area weak gravitational lensing survey. This design has been optimized to first order and is now under study for further modification and optimization. A 2-m three-mirror anastigmat wide-field telescope feeds a focal plane consisting of a 0.7 square-degree imager tiled with equal areas of optical CCDs and near infrared sensors, and a high-efficiency low-resolution integral field spectrograph. The instrumentation suite provides simultaneous discovery and light-curve measurements of supernovae and then can target individual objects for detailed spectral characterization. The SNAP mission will discover thousands of Type Ia supernovae out to z = 3 and will obtain high-signal-to-noise calibrated light-curves and spectra for a subset of > 2000 supernovae at redshifts between z = 0.1 and 1.7 in a northern field and in a southern field. A wide-field survey covering one thousand square degrees in both northern and southern fields resolves {approx} 100 galaxies per square arcminute, or a total of more than 300 million galaxies. With the PSF stability afforded by a space observatory, SNAP will provide precise and accurate measurements of gravitational lensing. The high-quality data available in space, combined with the large sample of supernovae, will enable stringent control of systematic uncertainties. The resulting data set will be used to determine the energy density of dark energy and parameters that describe its dynamical behavior. The data also provide a direct test of theoretical models for the dark energy, including discrimination of vacuum energy due to the cosmological constant and various classes of dynamical scalar fields. If we assume we live in a cosmological-constant-dominated Universe, the matter density, dark energy density, and flatness of space can all be measured with SNAP supernova and weak-lensing measurements to a systematics-limited accuracy of 1%. For a flat universe, the density-to-pressure ratio of dark energy or equation of state w(z) can be similarly measured to 5% for the present value w{sub 0} and {approx} 0.1 for the time variation w' {triple_bond} dw/d ln a|{sub z=1}. For a fiducial SUGRA-inspired universe, w{sub 0} and w' can be measured to an even tighter uncertainty of 0.03 and 0.06 respectively. Note that no external priors are needed. As more accurate theoretical predictions for the small-scale weak-lensing shear develop, the conservative estimates adopted here for space-based systematics should improve, allowing even tighter constraints. While the survey strategy is tailored for supernova and weak gravitational lensing observations, the large survey area, depth, spatial resolution, time-sampling, and nine-band optical to NIR photometry will support additional independent and/or complementary dark-energy measurement approaches as well as a broad range of auxiliary science programs.

Published
2005

36. Supernova Acceleration Probe: Studying Dark Energy with Type Ia Supernovae

Author

P. Limon, Albert Stebbins, Ralph C. Bohlin, Douglas L. Tucker, Armin Karcher, H. Heetderks, Edvard Mörtsell, H. Lin, G. Smadja, J. Musser, C. T. Day, T. Davies, Andre Tilquin, H. von der Lippe, B. Besuner, Martin White, Justin Albert, M. L. Lampton, N. Kuznetsova, A. Refregier, N. Palaio, Susana E. Deustua, L. Gladney, G. Goldhaber, Alex G. Kim, Roger F. Malina, Nick Mostek, Chris Bebek, V. Scarpine, D. Cole, William Carithers, A. D. Tomasch, Richard Massey, Bhuvnesh Jain, Keith Taylor, Roger Blandford, J. P. Marriner, Greg Aldering, David H. Pankow, Michael Seiffert, Eric Prieto, C. R. Bower, Alain Bonissent, Peter Nugent, D. Figer, R. Lafever, John Peoples, D. Vincent, M. Campbell, Stephen Bailey, Michael Sholl, B. Krieger, Alain Mazure, J. I. Lamoureux, M.E. Huffer, Anne Ealet, N. Morgan, S. C. Loken, Dominique Fouchez, A. S. Fruchter, M. Deharveng, V. Lebrun, O. Le Fevre, F. DeJongh, Guofeng Wang, Andrew Szymkowiak, J. Snyder, L. Marian, D. Rusin, Natalie A. Roe, Wolfgang Lorenzon, M. E. Levi, P. Jelinsky, Ramon Miquel, E. Barrelet, L. Hui, W. Emmet, R. Nakajima, Roger Smith, G. Tarle, C. Baltay, Stéphane Basa, Michael L. Brown, Hakeem M. Oluseyi, Christopher Stoughton, S. Allam, S. L. Mufson, M. Frerking, Steven E. Kahn, C. Juramy, W. C. Wester, D. Rabinowitz, D. Peterson, Scott Dodelson, Lars Bergström, H. Shuka, F. Stabenau, B. Bigelow, A. Goobar, Michael Schubnell, B. Mcginnis, M. Hoff, D. E. Groom, Steve Kent, Rahman Amanullah, J.-P. Walder, Saul Perlmutter, Richard Ellis, G. Kushner, Eugene D. Commins, Manfred Bester, Gary Bernstein, Shawn McKee, M. Aumeunier, Philip J. Marshall, A. L. Spadafora, T. Dobson, T. Diehl, B. Mobqsher, D. W. Gerdes, Pierre Astier, W. Althouse, William F. Kolbe, Josh Frieman, Eric V. Linder, Timothy A. McKay, George F. Smoot, William W. Craig, Dragan Huterer, S. T. Holland, A. Weinstein, Jason Rhodes, J. Annis, R. Pain, 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), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), SNAP, Flores, Sylvie, Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Type (model theory), [SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph], 01 natural sciences, 7. Clean energy, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Acceleration, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, 010306 general physics, Computer Science::Distributed, Parallel, and Cluster Computing, media_common, Physics, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, Astrophysics (astro-ph), Astronomy, Universe, Supernova, [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Dark energy
Abstract

The Supernova Acceleration Probe (SNAP) will use Type Ia supernovae (SNe Ia) as distance indicators to measure the effect of dark energy on the expansion history of the Universe. (SNAP's weak-lensing program is described in a companion White Paper.) The experiment exploits supernova distance measurements up to their fundamental systematic limit; strict requirements on the monitoring of each supernova's properties lead to the need for a space-based mission. Results from pre-SNAP experiments, which characterize fundamental SN Ia properties, will be used to optimize the SNAP observing strategy to yield data, which minimize both systematic and statistical uncertainties. SNAP has achieved technological readiness and the collaboration is poised to begin construction., Comment: 12 pages, 4 figures; White paper to the Dark Energy Task Force

Published
2005

37. Seeing the Nature of the Accelerating Physics: It's a SNAP

Author

D. Figer, D. Vincent, M. Campbell, Christopher Stoughton, Peter Nugent, George F. Smoot, A. L. Spadafora, M.E. Huffer, M. Frerking, Armin Karcher, Laura Marian, Andrew Szymkowiak, B. Besuner, Martin White, Saul Perlmutter, Alex G. Kim, Kyle Dawson, T. Dobson, R. Nakajima, Stéphane Basa, Michael L. Brown, Keith Taylor, Eric Prieto, Wolfgang Lorenzon, Steven E. Kahn, C. Juramy, P. Limon, C. R. Bower, C. Baltay, Nick Mostek, Roger Smith, S. C. Loken, G. Kushner, Hakeem M. Oluseyi, M. Deharveng, N. Palaio, Eric V. Linder, Susana E. Deustua, H. Lin, G. Smadja, J.-P. Walder, Gerson Goldhaber, M. Aumeunier, Gary Bernstein, H. von der Lippe, Timothy A. McKay, Philip J. Marshall, Pierre Astier, A. Refregier, Chris Bebek, Bahram Mobasher, E. Barrelet, Shawn McKee, J. Albert, Dominique Fouchez, W. Althouse, L. Gladney, R. Lafever, V. Scarpine, D. Cole, John Peoples, William F. Kolbe, B. Krieger, B. Bigelow, M. L. Lampton, N. Kuznetsova, L. Hui, Eugene D. Commins, Guofeng Wang, Tamara M. Davis, H. T. Diehl, Manfred Bester, Reynald Pain, Don Frederic DeJongh, W. Emmet, J. P. Marriner, D. Rabinowitz, Hemant Shukla, O. Le Fevre, S. Allam, Alain Mazure, S. Mufson, Edvard Mörtsell, Michael Levi, David H. Pankow, N. Morgan, H. Heetderks, Ariel Goobar, Albert Stebbins, B. Mcginnis, Richard Ellis, Andre Tilquin, William Wester, Douglas L. Tucker, Joshua A. Frieman, Ramon Miquel, C. T. Day, Bhuvnesh Jain, Steve Kent, D. Peterson, P. Jelinsky, Michael Schubnell, William Carithers, Rahman Amanullah, Richard Massey, Donald E. Groom, Roger Blandford, Roger F. Malina, A. D. Tomasch, G. Tarle, Greg Aldering, Alain Bonissent, Michael Sholl, V. Lebrun, Ralph C. Bohlin, Michael Seiffert, Stephen Bailey, J. I. Lamoureux, J. Snyder, William W. Craig, M. Hoff, Dragan Huterer, S. T. Holland, A. Weinstein, Jason Rhodes, J. Annis, D. W. Gerdes, D. Rusin, Natalie A. Roe, L. Bergstom, Scott Dodelson, F. Stabenau, A. S. Fruchter, and J. Musser

Subjects
Physics, Acceleration, Supernova, Dark energy, Astrophysics::Cosmology and Extragalactic Astrophysics, Cosmological constant, Astrophysics, Computer Science::Distributed, Parallel, and Cluster Computing, True insight
Abstract

For true insight into the nature of dark energy, measurements of the precision and accuracy of the Supernova/Acceleration Probe (SNAP) are required. Precursor or scaled-down experiments are unavoidably limited, even for distinguishing the cosmological constant. They can pave the way for, but should not delay, SNAP by developing calibration, refinement, and systematics control (and they will also provide important, exciting astrophysics).

Published
2005

38. Probing Dark Energy via Weak Gravitational Lensing with the SuperNova Acceleration Probe (SNAP)

Author

Greg Aldering, M. Hoff, Ralph C. Bohlin, S. L. Mufson, Andrew Szymkowiak, L. Gladney, O. Le Fevre, D. Cole, Nick Mostek, N. Palaio, Susana E. Deustua, Wolfgang Lorenzon, P. Limon, M. L. Lampton, Dragan Huterer, Scott Dodelson, N. Kuznetsova, Alain Mazure, H. Shuka, S. T. Holland, F. Stabenau, Josh Frieman, Roger Smith, Guofeng Wang, T. Davies, B. Besuner, Martin White, A. Weinstein, Roger F. Malina, Jason Rhodes, J. Annis, R. Lafever, G. Kushner, J. Albert, H. Lin, Saul Perlmutter, Lars Bergström, G. Smadja, R. Pain, Eric V. Linder, B. Krieger, John Peoples, A. D. Tomasch, B. Bigelow, J. Musser, Peter Nugent, A. Refregier, William W. Craig, L. Marian, H. von der Lippe, Michael Seiffert, D. E. Groom, Keith Taylor, Timothy A. McKay, Eric Prieto, Chris Bebek, C. R. Bower, D. Peterson, Albert Stebbins, G. Tarle, Stephen Bailey, J. I. Lamoureux, Christopher Stoughton, J.-P. Walder, F. DeJongh, Alex G. Kim, W. Emmet, Eugene D. Commins, V. Scarpine, M. Frerking, Gary Bernstein, A. Goobar, Douglas L. Tucker, Michael Schubnell, C. T. Day, Andre Tilquin, D. Figer, Shawn McKee, Edvard Mörtsell, Rahman Amanullah, M. Deharveng, Dominique Fouchez, W. C. Wester, D. Rabinowitz, M.E. Huffer, R. Nakajima, J. Snyder, T. Dobson, Armin Karcher, Stéphane Basa, Michael L. Brown, David H. Pankow, Steven E. Kahn, Anne Ealet, C. Juramy, Steve Kent, A. S. Fruchter, S. C. Loken, G. Goldhaber, Bhuvnesh Jain, Alain Bonissent, M. Aumeunier, Philip J. Marshall, J. P. Marriner, M. E. Levi, E. Barrelet, P. Jelinsky, Michael Sholl, A. L. Spadafora, L. Hui, T. Diehl, B. Mcginnis, Richard Ellis, B. Mobqsher, V. Lebrun, S. Allam, William Carithers, George F. Smoot, Richard Massey, Roger Blandford, Pierre Astier, W. Althouse, William F. Kolbe, D. W. Gerdes, D. Rusin, Natalie A. Roe, Ramon Miquel, N. Morgan, H. Heetderks, Manfred Bester, D. Vincent, M. Campbell, C. Baltay, Hakeem M. Oluseyi, Flores, Sylvie, 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), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), SNAP, Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Point spread function, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, [SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph], 01 natural sciences, law.invention, Telescope, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], law, 0103 physical sciences, 010306 general physics, Weak gravitational lensing, Physics, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, Astrophysics (astro-ph), Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Redshift, Galaxy, Supernova, [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Dark energy, Joint Dark Energy Mission
Abstract

SNAP is a candidate for the Joint Dark Energy Mission (JDEM) that seeks to place constraints on the dark energy using two distinct methods. The first, Type Ia SN, is discussed in a companion white paper. The second method is weak gravitational lensing, which relies on the coherent distortions in the shapes of background galaxies by foreground mass structures. The excellent spatial resolution and photometric accuracy afforded by a 2-meter space-based observatory are crucial for achieving the high surface density of resolved galaxies, the tight control of systematic errors in the telescope's Point Spread Function (PSF), and the exquisite redshift accuracy and depth required by this project. These are achieved by the elimination of atmospheric distortion and much of the thermal and gravity loads on the telescope. The SN and WL methods for probing dark energy are highly complementary and the error contours from the two methods are largely orthogonal., 17 pages, 6 figures; White paper to the Dark Energy Task Force

Published
2005

39. Characterization and deployment of large-format fully depleted back-illuminated p-channel CCDs for precision astronomy

Author

Greg Aldering, Stephen Holland, Armin Karcher, Bojan T. Turko, Marcus Jackson, Michael Levi, Hakeem M. Oluseyi, Chris Bebek, Samiyah Farid, William F. Kolbe, and Natalie A. Roe

Subjects
Physics, Silicon, business.industry, chemistry.chemical_element, Linearity, Large format, Noise (electronics), Dot pitch, Characterization (materials science), Optics, chemistry, Optoelectronics, business, Energy (signal processing), Dark current
Abstract

We present new characterization results for a large format, 15 um pixel pitch, 2kx4k format, p-channel CCD fabricated on high resistivity silicon at Lawrence Berkeley National Laboratory. The fully-depleted device is 300 um thick and backside illuminated utilizing 4-side buttable packaging. We report on measurements of standard operating characteristics including charge transfer efficiency, readout noise, cosmetics performance, dark current, and well depth. We have also made preliminary measurements of the device's X-Ray energy resolution and tests of device linearity.

Published
2004

40. An integral field spectrograph for SNAP

Author

Anne Ealet, Eric Prieto, Alain Bonissent, Roger Malina, G‰rard Smadja, A. Tilquin, Gary Bernstein, Stephane Basa, D. Fouchez, Olivier Le Fevre, Alain Mazure, Greg Aldering, R. Amanullah, Pierre Astier, E. Barrelet, Christopher J. Bebek, Lars Bergstrom, Manfred Bester, Roger Blandford, Ralph C. Bohlin, Charles R. Bower, Mark L. Brown, Myron Campbell, William C. Carithers, Jr., Eugene D. Commins, W. Craig, C. Day, F. DeJongh, Susana E. Deustua, H. T. Diehl, S. Dodelson, Richard S. Ellis, M. Emmet, Josh Frieman, Andrew Fruchter, D. Gerdes, L. Gladney, Gerson Goldhaber, Ariel Goobar, Donald E. Groom, Henry D. Heetderks, M. Hoff, Stephen E. Holland, M. Huffer, L. Hui, Dragan Huterer, B. Jain, Patrick N. Jelinsky, Armin Karcher, Steven M. Kent, Steven M. Kahn, Alex G. Kim, William F. Kolbe, B. Krieger, G. Kushner, N. Kuznetsova, Robin E. Lafever, J. I. Lamoureux, Michael L. Lampton, Michael E. Levi, P. Limon, Huan Lin, Eric V. Linder, Stewart C. Loken, W. Lorenzon, J. Marriner, P. Marshall, R. Massey, Timothy A. McKay, Shawn P. McKee, Ramon Miquel, Nicholas Morgan, E. M÷rtsell, Nick Mostek, Stuart Mufson, J. A. Musser, Peter E. Nugent, Hakeem M. Oluseyi, Reynald Pain, Nick P. Palaio, David H. Pankow, John Peoples, Jr., Saul Perlmutter, David Rabinowitz, Alexandre Refregier, Jason Rhodes, Natalie A. Roe, D. Rusin, V. Scarpine, Michael S. Schubnell, Michael J. Sholl, Roger M. Smith, George F. Smoot, Jeffrey A. Snyder, Anthony Spadafora, A. Stebbins, Christopher Stoughton, Andrew Szymkowiak, Gregory Tarl‰, Keith Taylor, Andrew D. Tomasch, Douglas Tucker, Henrik von der Lippe, D. Vincent, Jean-Pierre Walder, Guobin Wang, W. Wester, and Mather, John C.

Subjects
Physics, business.industry, Measure (physics), Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Redshift, Acceleration, Optics, Integral field spectrograph, Calibration, Joint Dark Energy Mission, Astrophysics::Earth and Planetary Astrophysics, Spectral resolution, business, Spectrograph, Astrophysics::Galaxy Astrophysics
Abstract

A well-adapted visible and infrared spectrograph has been developed for the SNAP (SuperNova/Acceleration Probe) experiment proposed for JDEM. The primary goal of this instrument is to ensure the control of Type Ia supernovae. The spectrograph is also a key element for calibration and is able to measure redshift of some thousands of galaxy spectra both in visible and IR. An instrument based on an integral field method with the powerful concept of imager slicing has been designed and is presented. We present the current design and expected performances. We show that with the current optimization and the proposed technology, we expect the most sensitive instrument proposed on this kind of mission. We recall the readiness of the concept and of the slicer technology thanks to large prototyping efforts performed in France which validate the proposition

Published
2004

41. SNAP Telescope

Author

Michael J. Sholl, Michael L. Lampton, Greg Aldering, W. Althouse, R. Amanullah, James T. Annis, Pierre Astier, Charles Baltay, E. Barrelet, Stephane Basa, Christopher J. Bebek, Lars Bergstrom, Gary Bernstein, Manfred Bester, Bruce C. Bigelow, Roger Blandford, Ralph C. Bohlin, Alain Bonissent, Charles R. Bower, Mark L. Brown, Myron Campbell, William C. Carithers, Jr., Eugene D. Commins, W. Craig, C. Day, F. DeJongh, Susana E. Deustua, T. Diehl, S. Dodelson, Anne Ealet, Richard S. Ellis, W. Emmet, D. Fouchez, Josh Frieman, Andrew Fruchter, D. Gerdes, L. Gladney, Gerson Goldhaber, Ariel Goobar, Donald E. Groom, Henry D. Heetderks, M. Hoff, Stephen E. Holland, M. Huffer, L. Hui, Dragan Huterer, B. Jain, Patrick N. Jelinsky, Armin Karcher, Steven M. Kahn, Steven M. Kent, Alex G. Kim, William F. Kolbe, B. Krieger, G. Kushner, N. Kuznetsova, Robin E. Lafever, J. I. Lamoureux, Olivier Le Fevre, Michael E. Levi, P. Limon, Huan Lin, Eric V. Linder, Stewart C. Loken, W. Lorenzon, Roger Malina, J. Marriner, P. Marshall, R. Massey, Alain Mazure, Timothy A. McKay, Shawn P. McKee, Ramon Miquel, Nicholas Morgan, E. M÷rtsell, Nick Mostek, Stuart Mufson, J. A. Musser, Peter E. Nugent, Hakeem M. Oluseyi, Reynald Pain, Nick P. Palaio, David H. Pankow, John Peoples, Jr., Saul Perlmutter, Eric Prieto, David Rabinowitz, Alexandre Refregier, Jason Rhodes, Natalie A. Roe, D. Rusin, V. Scarpine, Michael S. Schubnell, G‰rard Smadja, Roger M. Smith, George F. Smoot, Jeffrey A. Snyder, Anthony Spadafora, A. Stebbins, Christopher Stoughton, Andrew Szymkowiak, Gregory Tarl‰, Keith Taylor, A. Tilquin, Andrew D. Tomasch, Douglas Tucker, D. Vincent, Henrik von der Lippe, Jean-Pierre Walder, Guobin Wang, W. Wester, and Mather, John C.

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

Mission requirements, the baseline design, and optical systems budgets for the SuperNova/Acceleration Probe (SNAP) telescope are presented. SNAP is a proposed space-based experiment designed to study dark energy and alternate explanations of the acceleration of the universe’s expansion by performing a series of complementary systematics-controlled astrophysical measurements. The goals of the mission are a Type Ia supernova Hubble diagram and a wide-field weak gravitational lensing survey. A 2m widefield three-mirror telescope feeds a focal plane consisting of 36 CCDs and 36 HgCdTe detectors and a high-efficiency, low resolution integral field spectrograph. Details of the maturing optical system, with emphasis on structural stability during terrestrial testing as well as expected environments during operations at L2 are discussed. The overall stray light mitigation system, including illuminated surfaces and visible objects are also presented.

Published
2004

42. Development of fully depleted back-illuminated charge-coupled devices

Author

Armin Karcher, Natalie A. Roe, Chris Bebek, Donald E. Groom, Guobin Wang, N. Palaio, William F. Kolbe, Bojan T. Turko, and Stephen Holland

Subjects
Acceleration, Materials science, Fabrication, Pixel, business.industry, Optoelectronics, Wafer, business, National laboratory, Performance results
Abstract

The status of CCD development efforts at Lawrence Berkeley National Laboratory is reviewed. Fabrication technologies for the production of back-illuminated, fully depleted CCD’s on 150 mm diameter wafers are described. In addition, preliminary performance results for high-voltage compatible CCD’s, including a 3512 × 3512, 10.5 µm pixel CCD for the proposed SuperNova Acceleration Probe project, are presented.

Published
2004

43. LBNL four-side buttable CCD package development

Author

Tom Miller, Natalie A. Roe, Stephen Holland, Chris Bebek, Michela Uslenghi, Christopher Hernikl, Hakeem M. Oluseyi, Michael Levi, Armin Karcher, and J. Bercovitz

Subjects
Measurement method, Assurance qualite, Computer science, business.industry, Flatness (systems theory), Package design, Electrical engineering, Electronic packaging, Mechanical engineering, Charge-coupled device, business, Quality assurance, Astronomical imaging
Abstract

We have developed a precision, 4-side buttable CCD package for 2kx2k and 2kx4k format devices with minimal mechanical stress on the CCD, excellent thermal properties, reliable electrical connectivity, and shim-free mounting. We report on the package design, assembly and quality assurance procedures, measurements of packaged device flatness and flatness excursions when cooled from room temperature to 140 K, package performance and plans for future development.

Published
2004

44. SNAP telescope: an update

Author

Ralph C. Bohlin, D. Fouchez, Edvard Mörtsell, Robert Besuner, Alex G. Kim, J. Bercovitz, Nick Mostek, Michael H. Krim, Armin Karcher, Michael Schubnell, Myron Campbell, Keith Taylor, William Carithers, Alain Mazure, S. Mufson, William Emmett, Charles R. Bower, Eric V. Linder, Michael Levi, Rahman Amanullah, N. Morgan, J. A. Musser, Carl W. Akerlof, R. Lafever, Stéphane Basa, Timothy A. McKay, Guobin Wang, George F. Smoot, Henrik von der Lippe, Ariel Goobar, Peter Nugent, D. Vincent, Donald E. Groom, Pierre Astier, Daniel Levin, Jean-Pierre Walder, William E. Johnston, N. Palaio, Susana E. Deustua, William F. Kolbe, J. I. Lamoureux, Gary Berstein, J.F. Genat, Ramon Miquel, Stephen Holland, David H. Pankow, J. Snyder, H. Heetderks, Saul Perlmutter, Andre Tilquin, M. Eriksson, S. C. Loken, E. Barrelet, Greg Aldering, G. Smadja, R. W. Kadel, C. Baltay, Richard S. Ellis, Chris Bebek, Hakeem M. Oluseyi, David Rabinowitz, Dragan Huterer, Jason Rhodes, Andrew Szymkowiak, Manfred Bester, Lars Bergström, C. T. Day, Roger Smith, Eugene D. Commins, Reynald Pain, A. L. Spadafora, G. Goldhaber, Shawn McKee, Roger F. Malina, Andrew S. Fruchter, A. D. Tomasch, Anne Ealet, Gregory Tarle, R. DiGennaro, Alain Bonissent, Alexandre Refregier, Michael Sholl, Eric Prieto, Natalie A. Roe, Oliver LeFevre, Michael Lampton, and MacEwen, Howard A.

Subjects
Physics, Wavefront, business.industry, Stray light, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Anastigmat, Astronomy, Three-mirror anastigmat, Astrophysics::Cosmology and Extragalactic Astrophysics, Orbital mechanics, Redshift, law.invention, Telescope, Optics, law, Astrophysics::Solar and Stellar Astrophysics, Adaptive optics, business, Astrophysics::Galaxy Astrophysics
Abstract

We present the baseline telescope design for the telescope for the SuperNova/Acceleration Probe (SNAP) space mission. SNAP’s purpose is to determine expansion history of the Universe by measuring the redshifts, magnitudes, and spectral classifications of thousands of supernovae with unprecedented accuracy. Discovering and measuring these supernovae demand both a wide optical field and a high sensitivity throughout the visible and near IR wavebands. We have adopted the annular-field three-mirror anastigmat (TMA) telescope configuration, whose classical aberrations (including chromatic) are zero. We show a preliminary optmechanical design that includes important features for stray light control and on-orbit adjustment and alignment of the optics. We briefly discuss stray light and tolerance issues, and present a preliminary wavefront error budget for the SNAP Telescope. We conclude by describing some of the design tasks being carried out during the current SNAP research and development phase.

Published
2004

45. Weak lensing from space I: instrumentation and survey strategy

Author

S. Harris, H. von der Lippe, Dominique Fouchez, Lars Bergström, C. T. Day, Alex G. Kim, B. Bigelow, Chris Bebek, Myron Campbell, A. L. Spadafora, Saul Perlmutter, Eric Prieto, R. Pratt, M. L. Lampton, S.E. Holland, G. Smadja, A. S. Fruchter, Armin Karcher, B. Krieger, J.-P. Walder, N. Morgan, Gary Bernstein, Peter Nugent, C. Baltay, Eric V. Linder, Shawn McKee, Ariel Goobar, Justin Albert, William E. Johnston, Timothy A. McKay, Hakeem M. Oluseyi, N. Palaio, Susana E. Deustua, Greg Aldering, J. Bercovitz, Nick Mostek, George F. Smoot, David Rabinowitz, Roger F. Malina, Pierre Astier, David Bacon, Keith Taylor, C. R. Bower, William F. Kolbe, R. Lafever, Andrew Szymkowiak, H. Heetderks, David H. Pankow, A. D. Tomasch, G. Kushner, J. A. Musser, Wolfgang Lorenzon, Peter Harvey, D. Rusin, Natalie A. Roe, W. Emmet, Anne Ealet, Roger Smith, S. C. Loken, Ramon Miquel, Edvard Mörtsell, Gerson Goldhaber, E. Barrelet, R. DiGennaro, Alain Bonissent, M. E. Levi, Andre Tilquin, S. L. Mufson, Alexandre Refregier, M. Eriksson, Michael Sholl, Manfred Bester, Richard S. Ellis, Bhuvnesh Jain, D. W. Gerdes, William Carithers, Richard Massey, L. Gladney, D. Vincent, Guofeng Wang, Alain Mazure, Michael Schubnell, Carl W. Akerlof, Rahman Amanullah, Eugene D. Commins, Reynald Pain, Donald E. Groom, J. F. Genat, K. Robinson, Gregory Tarle, Dragan Huterer, Michael E. Brown, J. I. Lamoureux, Ralph C. Bohlin, J. Snyder, N. Kuznetsova, Jason Rhodes, 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), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), California Institute of Technology (CALTECH), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Department of Mathematics [Berkeley], University of California [Berkeley] (UC Berkeley), University of California (UC)-University of California (UC), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), 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), School of Engineering [Edinburgh], University of Edinburgh, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Department of Physics, Stockholm University, Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Harvard-Smithsonian Center for Astrophysics (CfA), Harvard University-Smithsonian Institution, Dispositifs et Instrumentation en Optoélectronique et micro-ondes (DIOM), Université Jean Monnet - Saint-Étienne (UJM), Dept Mat Sci & Engn, Zhejiang University, California Institute of Technology (CALTECH)-NASA, University of California [Berkeley], University of California-University of California, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Harvard University [Cambridge]-Smithsonian Institution, DIOM (DIOM), and Université Jean Monnet [Saint-Étienne] (UJM)

Subjects
Point spread function, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics::High Energy Astrophysical Phenomena, Dark matter, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Cosmology, law.invention, Telescope, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Spitzer Space Telescope, law, 0103 physical sciences, Dark energy, Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, Instrumentation, Weak gravitational lensing, Astrophysics::Galaxy Astrophysics, Physics, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, Astrophysics (astro-ph), Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysics, Supernova
Abstract

A wide field space-based imaging telescope is necessary to fully exploit the technique of observing dark matter via weak gravitational lensing. This first paper in a three part series outlines the survey strategies and relevant instrumental parameters for such a mission. As a concrete example of hardware design, we consider the proposed Supernova/Acceleration Probe (SNAP). Using SNAP engineering models, we quantify the major contributions to this telescope's Point Spread Function (PSF). These PSF contributions are relevant to any similar wide field space telescope. We further show that the PSF of SNAP or a similar telescope will be smaller than current ground-based PSFs, and more isotropic and stable over time than the PSF of the Hubble Space Telescope. We outline survey strategies for two different regimes - a ``wide'' 300 square degree survey and a ``deep'' 15 square degree survey that will accomplish various weak lensing goals including statistical studies and dark matter mapping., 25 pages, 8 figures, 1 table, replaced with Published Version

Published
2004

46. Fully depleted back-illuminated p-channel CCD development

Author

V. Prasad, J. Bercovitz, Chris Bebek, Hakeem M. Oluseyi, R. W. Kadel, Armin Karcher, Donald E. Groom, Bojan T. Turko, William F. Kolbe, Nicholas P. Palaio, Guobin Wang, and Stephen Holland

Subjects
Physics, High resistivity silicon, Fabrication, Silicon, business.industry, chemistry.chemical_element, Radiation, Optics, P channel, Engineering, chemistry, Optoelectronics, National laboratory, business, CCD fully depleted back illuminated radiation damage pointspread function fabrication
Abstract

An overview of CCD development efforts at Lawrence Berkeley National Laboratory is presented. Operation of fully-depleted, back-illuminated CCD's fabricated on high resistivity silicon is described, along with results on the use of such CCD's at ground-based observatories. Radiation damage and point-spread function measurements are described, as well as discussion of CCD fabrication technologies.

Published
2003

47. SNAP NIR detectors

Author

Eric V. Linder, Guobin Wang, Saul Perlmutter, Steven E. Holland, S. Harris, Dragan Huterer, Greg Aldering, Eric Prieto, R. Lafever, A. L. Spadafora, Jason Rhodes, J.F. Genat, George F. Smoot, Michael Levi, H. von der Lippe, S. C. Loken, Mark L. Brown, Alex G. Kim, Anne Ealet, Pierre Astier, B. Krieger, Daniel Levin, William F. Kolbe, Michael Schubnell, Ariel Goobar, R. DiGennaro, Peter Harvey, E. Barrelet, Richard S. Ellis, Alain Bonissent, Alexandre Refregier, Michael Sholl, Timothy A. McKay, David H. Pankow, R. Pratt, E. Moertsell, Michael Lampton, Susana E. Deustua, H. Heetderks, Rahman Amanullah, Donald E. Groom, M. Eriksson, Nicholas P. Palaio, Manfred Bester, Carl W. Akerlof, K. Robinson, Ramon Miquel, Peter Nugent, J.-P. Walder, Gary Bernstein, Shawn McKee, S. Mufson, Gerson Goldhaber, William Carithers, Richard Massey, Roger F. Malina, Andrew S. Fruchter, A. D. Tomasch, D. Vincent, J. I. Lamoureux, Armin Karcher, C. R. Bower, Gregory Tarle, Natalie A. Roe, J. A. Musser, Lars Bergström, C. T. Day, G. Smadja, Hakeem M. Oluseyi, Chris Bebek, Eugene D. Commins, Reynald Pain, J. Bercovitz, Nick Mostek, Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and Flores, Sylvie

Subjects
Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, [SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph], 01 natural sciences, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 010309 optics, Photometry (optics), Acceleration, Integral field spectrograph, Optics, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, media_common, Physics, Zodiacal light, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], business.industry, Near-infrared spectroscopy, Universe, Cardinal point, [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Dark energy, business
Abstract

The SuperNova/Acceleration Probe (SNAP) will measure precisely the cosmological expansion history over both the acceleration and deceleration epochs and thereby constrain the nature of the dark energy that dominates our universe today. The SNAP focal plane contains equal areas of optical CCDs and NIR sensors and an integral field spectrograph. Having over 150 million pixels and a field-of-view of 0.34 square degrees, the SNAP NIR system will be the largest yet constructed. With sensitivity in the range 0.9-1.7 μm, it will detect Type Ia supernovae between z = 1 and 1.7 and will provide follow-up precision photometry for all supernovae. HgCdTe technology, with a cut-off tuned to 1.7 μm, will permit passive cooling at 140 K while maintaining noise below zodiacal levels. By dithering to remove the effects of intrapixel variations and by careful attention to other instrumental effects, we expect to control relative photometric accuracy below a few hundredths of a magnitude. Because SNAP continuously revisits the same fields we will be able to achieve outstanding statistical precision on the photometry of reference stars in these fields, allowing precise monitoring of our detectors. The capabilities of the NIR system for broadening the science reach of SNAP are discussed.

Published
2003

48. SNAP: an integral field spectrograph for supernova identification

Author

Anne Ealet, Eric Prieto, Alain Bonissent, Roger Malina, G. Bernstein, Stephane Basa, Oliver LeFevre, Alain Mazure, Christophe Bonneville, Carl W. Akerlof, Greg Aldering, R. Amanullah, Pierre Astier, E. Barrelet, Christopher Bebek, Lars Bergstrom, John Bercovitz, Manfred Bester, C. R. Bower, William C. Carithers, Jr., Eugene D. Commins, C. Day, Susana E. Deustua, Richard S. DiGennaro, R. Ellis, Mikael Eriksson, Andrew Fruchter, Jean-Francois Genat, Gerson Goldhaber, Ariel Goobar, Donald E. Groom, Stewart E. Harris, Peter R. Harvey, Henry D. Heetderks, Steven E. Holland, Dragan Huterer, Armin Karcher, Alex G. Kim, William F. Kolbe, B. Krieger, R. Lafever, J. Lamoureux, Michael L. Lampton, Michael E. Levi, Daniel S. Levin, Eric V. Linder, Stewart C. Loken, R. Massey, Timothy McKay, Shawn P. McKee, Ramon Miquel, E. Moertsell, N. Mostek, Stuart Mufson, J. A. Musser, Peter E. Nugent, Hakeem M. Oluseyi, Reynald Pain, Nicholas P. Palaio, David H. Pankow, Saul Perlmutter, R. Pratt, Alexandre Refregier, J. Rhodes, Kem E. Robinson, N. Roe, Michael Sholl, Michael S. Schubnell, G. Smadja, George F. Smoot, Anthony Spadafora, Gregory Tarle, Andrew D. Tomasch, H. von der Lippe, D. Vincent, J.-P. Walder, Guobin Wang, and Mather, John C.

Subjects
Physics, Field (physics), business.industry, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Type (model theory), 01 natural sciences, 010309 optics, Supernova, Acceleration, Optics, Integral field spectrograph, 0103 physical sciences, Magnitude (astronomy), Spectral resolution, business, 010303 astronomy & astrophysics, Spectrograph
Abstract

A well-adapted spectrograph concept has been developed for the SNAP (SuperNova/Acceleration Probe) experiment. The goal is to ensure proper identification of Type Ia supernovae and to standardize the magnitude of each candidate by determining explosion parameters. An instrument based on an integral field method with the powerful concept of imager slicing has been designed and is presented in this paper. The spectrograph concept is optimized to have very high efficiency and low spectral resolution (R {approx} 100), constant through the wavelength range (0.35-1.7{micro}m), adapted to the scientific goals of the mission.

Published
2003

49. A low power, wide dynamic range multigain signal processor for the SNAP CCD

Author

G. Chao, H. von der Lippe, Armin Karcher, B. Krieger, J. Steckert, J.-P. Walder, J. F. Genat, and S. Kurz

Subjects
Nuclear and High Energy Physics, Engineering, business.industry, Dynamic range, Electrical engineering, Chip, Signal, Noise (electronics), Signal-to-noise ratio, Nuclear Energy and Engineering, CMOS, Integrator, Wide dynamic range, Electrical and Electronic Engineering, business
Abstract

A four-channel custom chip designed for reading out the CCDs of the proposed SNAP satellite visible imager is presented. Each channel consists of a single-ended to differential converter followed by a correlated double sampler and a novel multislope integrator. The output signal is differentially brought out of the chip by an output buffer. This circuit is designed to operate at room temperature for test purpose and at 140 K, which will be the operating temperature. The readout speed is 100 kHz. The 16-bit dynamic range is covered using 3 gains each with a 12-bit signal to noise ratio. The prototype chip, implemented in a 0.25 /spl mu/m CMOS technology, has a measured readout noise of 7 /spl mu/V rms at 100 kHz readout speed, a measured nonlinearity of /spl plusmn/0.0025% and a power consumption of 6.5 mW, with a 3.3 V supply voltage.

Published
2003

50. SNAP Telescope

Author

Michael L. Lampton, Carl W. Akerlof, Greg Aldering, R. Amanullah, Pierre Astier, E. Barrelet, Christopher Bebek, Lars Bergstrom, John Bercovitz, G. Bernstein, Manfred Bester, Alain Bonissent, C. R. Bower, William C. Carithers, Jr., Eugene D. Commins, C. Day, Susana E. Deustua, Richard S. DiGennaro, Anne Ealet, Richard S. Ellis, Mikael Eriksson, Andrew Fruchter, Jean-Francois Genat, Gerson Goldhaber, Ariel Goobar, Donald E. Groom, Stewart E. Harris, Peter R. Harvey, Henry D. Heetderks, Steven E. Holland, Dragan Huterer, Armin Karcher, Alex G. Kim, William F. Kolbe, B. Krieger, R. Lafever, J. Lamoureux, Michael E. Levi, Daniel S. Levin, Eric V. Linder, Stewart C. Loken, Roger Malina, R. Massey, Timothy McKay, Shawn P. McKee, Ramon Miquel, E. Mortsell, N. Mostek, Stuart Mufson, J. A. Musser, Peter E. Nugent, Hakeem M. Oluseyi, Reynald Pain, Nicholas P. Palaio, David H. Pankow, Saul Perlmutter, R. Pratt, Eric Prieto, Alexandre Refregier, J. Rhodes, Kem E. Robinson, N. Roe, Michael Sholl, Michael S. Schubnell, G. Smadja, George F. Smoot, A. Spadafora, Gregory Tarle, Andrew D. Tomasch, H. von der Lippe, R. Vincent, J.-P. Walder, Guobin Wang, Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), MacEwen, Howard A., and Flores, Sylvie

Subjects
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 010309 optics, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics::High Energy Astrophysical Phenomena, 0103 physical sciences, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, [SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, 01 natural sciences, Astrophysics::Galaxy Astrophysics
Abstract

The SuperNova/Acceleration Probe (SNAP) mission will require a two-meter class telescope delivering diffraction limited images spanning a one degree field in the visible and near infrared wavelength regime. This requirement, equivalent to nearly one billion pixel resolution, places stringent demands on its optical system in terms of field flatness, image quality, and freedom from chromatic aberration. We discuss the advantages of annular-field three-mirror anastigmat (TMA) telescopes for applications such as SNAP, and describe the features of the specific optical configuration that we have baselined for the SNAP mission. We discuss the mechanical design and choice of materials for the telescope. Then we present detailed ray traces and diffraction calculations for our baseline optical design. We briefly discuss stray light and tolerance issues, and present a preliminary wavefront error budget for the SNAP Telescope. We conclude by describing some of tasks to be carried out during the upcoming SNAP research and development phase.

Published
2002

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