Results 41 to 50 of about 279,129 (320)
Mitigation of LEO Satellite Brightness and Trail Effects on the Rubin Observatory LSST [PDF]
Astronomical Journal, 2020 We report studies on the mitigation of optical effects of bright low-Earth-orbit (LEO) satellites on Vera C. Rubin Observatory and its Legacy Survey of Space and Time (LSST).J. A. Tyson, Ž. Ivezić, A. Bradshaw, M. Rawls, B. Xin, P. Yoachim, J. Parejko, J. Greene, M. Sholl, Timothy M. C. Abbott, D. Polin +10 moresemanticscholar +1 more sourceThe IceCube Neutrino Observatory: Instrumentation and Online Systems [PDF]
, 2016 The IceCube Neutrino Observatory is a cubic-kilometer-scale high-energy neutrino detector built into the ice at the South Pole. Construction of IceCube, the largest neutrino detector built to date, was completed in 2011 and enabled the discovery of high ...I. C. M. Aartsen, M. Ackermann, J. Adams, J. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, K. Andeen, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, R. Auer, J. Auffenberg, S. Axani, J. Baccus, X. Bai, S. Barnet, S. Barwick, V. Baum, R. Bay, K. Beattie, J. Beatty, J. Tjus, K. Becker, T. Bendfelt, S. Benzvi, D. Berley, E. Bernardini, A. Bernhard, D. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, S. Blot, D. Boersma, C. Bohm, M. Borner, F. Bos, D. Bose, S. Boser, O. Botner, A. Bouchta, J. Braun, L. Brayeur, H. Bretz, S. Bron, A. Burgman, C. Burreson, T. Carver, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, G. Collin, J. Conrad, D. Cowen, R. Cross, C. Day, M. Day, J. Andr'e, C. Clercq, E. del Pino Rosendo, H. Dembinski, S. Ridder, F. Descamps, P. Desiati, K. D. Vries, G. Wasseige, M. With, T. DeYoung, J. C. D'iaz-V'elez, V. Lorenzo, H. Dujmovic, J. Dumm, M. Dunkman, B. Eberhardt, W. Edwards, T. Ehrhardt, B. Eichmann, P. Eller, S. Euler, P. Evenson, S. Fahey, A. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, S. Flis, C.-C. Fosig, A. Franckowiak, M. Frere, E. Friedman, T. Fuchs, T. Gaisser, J. Gallagher, L. Gerhardt, K. Ghorbani, W. Giang, L. Gladstone, T. Glauch, D. Glowacki, T. Glusenkamp, A. Goldschmidt, J. G. Gonzalez, D. Grant, Z. Griffith, L. Gustafsson, C. Haack, A. Hallgren, F. Halzen, E. Hansen, T. Hansmann, K. Hanson, J. Haugen, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, R. Heller, S. Hickford, J. Hignight, G. Hill, K. Hoffman, R. Hoffmann, K. Hoshina, F. Huang, M. Huber, P. O. Hulth, K. Hultqvist, S. In, M. Inaba, A. Ishihara, E. Jacobi, J. Jacobsen, G. Japaridze, M. Jeong, K. Jero, A. Jones, B. Jones, J. Joseph, W. Kang, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. Kelley, J. Kemp, A. Kheirandish, J. Kim, M. Kim, T. Kintscher, J. Kiryluk, N. Kitamura, T. Kittler, S. Klein, S. Kleinfelder, M. Kleist, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Kopke, C. Kopper, S. Kopper, D. Koskinen, M. Kowalski, M. Krasberg, K. Krings, M. Kroll, G. Kruckl, C. Kruger, J. Kunnen, S. Kunwar, N. Kurahashi, T. Kuwabara, M. Labare, K. Laihem, H. Landsman, J. Lanfranchi, M. Larson, F. Lauber, A. Laundrie, D. Lennarz, H. Leich, M. Lesiak-Bzdak, M. Leuermann, L. Lu, J. Ludwig, J. Lunemann, C. Mackenzie, J. Madsen, G. Maggi, K. Mahn, S. Mancina, M. Mandelartz, R. Maruyama, K. Mase, H. Matis, R. Maunu, F. McNally, C. Mcparland, P. Meade, K. Meagher, M. Medici, M. Meier, A. Meli, T. Menne, G. Merino, T. Meures, S. Miarecki, R. Minor, T. Montaruli, M. Moulai, T. Murray, R. Nahnhauer, U. Naumann, G. Neer, M. Newcomb, H. Niederhausen, S. Nowicki, D. Nygren, A. Pollmann, A. Olivas, A. O'Murchadha, T. Palczewski, H. Pandya, D. Pankova, S. Patton, P. Peiffer, O. Penek, J. Pepper, C. Heros, C. Pettersen, D. Pieloth, E. Pinat, P. Price, G. Przybylski, M. Quinnan, C. Raab, L. Radel, M. Rameez, K. Rawlins, R. Reimann, B. Relethford, M. Relich, E. Resconi, W. Rhode, M. Richman, B. Riedel, S. Robertson, M. Rongen, C. Roucelle, C. Rott, T. Ruhe, D. Ryckbosch, D. Rysewyk, L. Sabbatini, S. Herrera, A. Sandrock, J. Sandroos, P. Sandstrom, S. Sarkar, K. Satalecka, P. Schlunder, T. Schmidt, S. Schoenen, S. Schoneberg, A. Schukraft, L. Schumacher, D. Seckel, S. Seunarine, M. Solarz, D. Soldin, M. Song, G. Spiczak, C. Spiering, T. Stanev, Alexander Stasik, J. Stettner, A. Steuer, T. Stezelberger, R. Stokstad, A. Stossl, R. Strom, N. Strotjohann, K. Sulanke, G. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, F. Tenholt, S. Ter-Antonyan, A. Terliuk, G. Tevsi'c, L. Thollander, S. Tilav, P. Toale, M. Tobin, S. Toscano, D. Tosi, M. Tselengidou, A. Turcati, E. Unger, M. Usner, J. Vandenbroucke, N. Eijndhoven, S. Vanheule, M. Rossem, J. Santen, M. Vehring, M. Voge, E. Vogel, M. Vraeghe, D. Wahl, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, C. Weaver, M. Weiss, C. Wendt, S. Westerhoff, D. Wharton, B. Whelan, S. Wickmann, K. Wiebe, C. Wiebusch, L. Wille, D. Williams, L. Wills, P. Wisniewski, M. Wolf, T. R. Wood, E. Woolsey, K. Woschnagg, D. Xu, X. Xu, Y. Xu, J. Yáñez, G. Yodh, S. Yoshida, M. Zoll +351 moresemanticscholar +1 more sourceObservation of the Crab Nebula with the HAWC Gamma-Ray Observatory [PDF]
, 2017 The Crab Nebula is the brightest TeV gamma-ray source in the sky and has been used for the past 25 years as a reference source in TeV astronomy, for calibration and verification of new TeV instruments. The High Altitude Water Cherenkov Observatory (HAWC),A. Abeysekara, A. Albert, R. Alfaro, C. Alvarez, J. Álvarez, R. Arceo, J. C. Arteaga-Vel'azquez, H. Solares, A. Barber, N. Bautista-Elivar, A. Becerril, E. Belmont-Moreno, S. Benzvi, D. Berley, J. Braun, C. Brisbois, K. Caballero-Mora, T. Capistr'an, A. Carramiñana, S. Casanova, M. Castillo, U. Cotti, J. Cotzomi, S. C. D. Le'on, E. D. L. Fuente, C. D. Le'on, T. DeYoung, B. Dingus, M. DuVernois, J. C. D'iaz-V'elez, R. Ellsworth, D. Fiorino, N. Fraija, J. A. Garc'ia-Gonz'alez, M. Gerhardt, A. G. Muñoz, M. Gonz'alez, J. Goodman, Z. Hampel-Arias, J. P. Harding, S. Hernández, A. Hernández-Almada, J. Hinton, C. Hui, P. Hüntemeyer, A. Iriarte, A. Jardin-Blicq, V. Joshi, S. Kaufmann, D. Kieda, A. Lara, R. Lauer, W. Lee, D. Lennarz, H. L. Vargas, J. Linnemann, A. Longinotti, G. Raya, R. Luna-Garc'ia, R. L'opez-Coto, K. Malone, S. Marinelli, O. Martinez, I. Martinez-Castellanos, J. Mart'inez-Castro, H. Mart'inez-Huerta, J. Matthews, P. Miranda-Romagnoli, E. Moreno, M. Mostaf'a, L. Nellen, M. Newbold, M. Nisa, R. Noriega-Papaqui, R. Pelayo, J. Pretz, E. G. P'erez-P'erez, Z. Ren, C. Rho, C. Rivière, D. Rosa-González, M. Rosenberg, E. Ruiz-Velasco, H. Salazar, F. Greus, A. Sandoval, Michael Schneider, H. Schoorlemmer, G. Sinnis, A. Smith, R. Springer, P. Surajbali, I. Taboada, O. Tibolla, K. Tollefson, I. Torres, T. Ukwatta, L. Villaseñor, T. Weisgarber, S. Westerhoff, I. Wisher, J. Wood, T. Yapici, G. Yodh, P. Younk, A. Zepeda, H. Zhou +106 moresemanticscholar +1 more sourceCosmic-Ray Extremely Distributed Observatory [PDF]
Symmetry, 2020 The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a newly formed, global collaboration dedicated to observing and studying cosmic rays (CR) and cosmic-ray ensembles (CRE): groups of at least two CR with a common primary interaction vertex or ...P. Homola, D. Beznosko, G. Bhatta, L. Bibrzycki, Michalina Borczyńska, L. Bratek, N. Budnev, Dariusz Burakowski, D. Alvarez-Castillo, K. A. Cheminant, A. Ćwikła, Punsiri Dam-O, N. Dhital, A. Duffy, Piotr Głownia, K. Gorzkiewicz, D. Góra, Alok C. Gupta, Z. Hlávková, Martin Homola, J. Jałocha, R. Kaminski, M. Karbowiak, M. Kasztelan, R. Kierepko, M. Knap, P. Kovács, S. Kuliński, B. Lozowski, M. Magrys, M. Medvedev, J. Mędrala, J. Mietelski, J. Miszczyk, A. Mozgova, A. Napolitano, V. Nazari, Y. Ng, M. Niedźwiecki, C. Oancea, B. Ogan, G. Opila, K. Oziomek, M. Pawlik, M. Piekarczyk, Bozena Poncyliusz, Jerzy Pryga, Matías Rosas, K. Rzecki, J. Zamora-Saá, K. Smelcerz, K. Smolek, Weronika K Stanek, J. Stasielak, S. Stuglik, J. Sulma, O. Sushchov, M. Svanidze, Kyle Tam, A. Tursunov, J. Vaquero, T. Wibig, K. Wozniak +62 moresemanticscholar +1 more sourceThe Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO)
, 2012 The Helioseismic and Magnetic Imager (HMI) instrument and investigation as a part of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone dynamics and the solar dynamo, the origin and evolution of sunspots, active regions, and ...P. Scherrer, J. Schou, R. Bush, A. Kosovichev, R. Bogart, J. Hoeksema, Yang Liu, T. Duvall, Junwei Zhao, A. Title, C. Schrijver, T. Tarbell, S. Tomczyk +12 moresemanticscholar +1 more sourceDesign of Waveguide NbN‐Based Superconductor–Insulator–Superconductor Mixer for 650 GHz
Advanced Photonics Research, EarlyView.This research work focuses on a waveguide NbN‐based superconductor–insulator–superconductor mixer operating at 650 GHz. The signal coupling circuit is designed using a waveguide‐microstrip coupling structure, and the return loss obtained is lower than −16 dB. For the mixing circuit, its return loss is less than −7.5 dB, and the return loss reduces with Lianhao He, Fangting Lin, Xiaoyong Hewiley +1 more source
