Mostrando 421 - 440 Resultados de 591 Para Buscar '"supernova"', tiempo de consulta: 0.17s Limitar resultados
  1. 421
    “…The high haplotyping precision (∼99.7%) and recall (∼95.9%) represents a substantial improvement over the commonly used tool for assembling cobarcoded reads (Supernova), and is comparable to a trio-binning-based third generation long-read-based assembly method (TrioCanu) but with a significantly higher single-base accuracy [up to 99.99997% (Q65)]. …”
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  2. 422
    “…Galactic Cosmic Rays (GCRs) are charged particles, originating from galactic and/or extra-galactic Supernova Remnants (SNR), that continuously permeate the Heliosphere. …”
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  3. 423
    “…Since the first Edition of this book published in 2011 with the title Astronomy with Radioactivities, long-awaited new direct observations of supernova radioactivity have been made and are now addressed in two updated chapters dealing with supernovae. …”
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  4. 424
  5. 425
    “…Data were obtained at 100 K from new in-house diffractometers Rigaku Synergy-S (Mo and Ag source, HyPix100 detector) and Stoe Stadivari (Mo source, EIGER2 1M CdTe detector), and an older Oxford Diffraction Supernova (Mo source, Atlas CCD detector). The synchrotron data were obtained at 25 K from BL02B1 beamline at SPring-8 in Japan (λ = 0.2480 Å, Pilatus3 X 1M CdTe detector). …”
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  6. 426
    “…We apply a novel statistical method15, 16 to quantify the evolutionary timeline and find that star formation is regulated by efficient stellar feedback, driving GMC dispersal on short timescales (~1.5 Myr) due to radiation and stellar winds, prior to supernova explosions. This feedback limits GMC lifetimes to about one dynamical timescale (~10 Myr), with integrated star formation efficiencies of only 2–3%. …”
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  7. 427
    “…Interpreting high-energy, astrophysical phenomena, such as supernova explosions or neutron-star collisions, requires a robust understanding of matter at supranuclear densities. …”
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  8. 428
  9. 429
    “…Type Ia supernovae are cosmic distance indicators(1,2), and the main source of iron in the Universe(3,4), but their formation paths are still debated. …”
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  10. 430
    por Sizun, P Y, Brunner, J W
    Publicado 2002
    “…Potential sources of neutrino are galactic (e.g supernova remnants, micro-quasars) and extra-galactic (e.g active galactic nuclei, gamma-ray bursters). …”
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  11. 431
    “…These data are compared with the respective meteoritic and Ryugu data and spectroscopic observations of other comets and extra-solar environments; Cl, Br, and Kr data are also evaluated in the context of a potential late supernova contribution, as suggested by the Si- and S-isotopic data of 67P/CG.…”
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  12. 432
    “…With a phased assembly approach, we targeted a heterozygous F(1) derived from a wide cross to assess the ability to derive both haplotypes and characterize a pungency gene with a large insertion/deletion. The Supernova software generated a highly ordered, more contiguous sequence assembly than all currently available C. annuum reference genomes. …”
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  13. 433
    por Stahl, A, Wiebusch, C, Guler, A M, Kamiscioglu, M, Sever, R, Yilmazer, A U, Gunes, C, Yilmaz, D, Del Amo Sanchez, P, Duchesneau, D, Pessard, H, Marcoulaki, E, Papazoglou, I A, Berardi, V, Cafagna, F, Catanesi, M G, Magaletti, L, Mercadante, A, Quinto, M, Radicioni, E, Ereditato, A, Kreslo, I, Pistillo, C, Weber, M, Ariga, A, Ariga, T, Strauss, T, Hierholzer, M, Kawada, J, Hsu, C, Haug, S, Jipa, A, Lazanu, I, Cardini, A, Lai, A, Oldeman, R, Thomson, M, Blake, A, Prest, M, Auld, A, Elliot, J, Lumbard, J, Thompson, C, Gornushkin, Y A, Pascoli, S, Collins, R, Haworth, M, Thompson, J, Bencivenni, G, Domenici, D, Longhin, A, Blondel, A, Bravar, A, Dufour, F, Karadzhov, Y, Korzenev, A, Noah, E, Ravonel, M, Rayner, M, Asfandiyarov, R, Haesler, A, Martin, C, Scantamburlo, E, Cadoux, F, Bayes, R, Soler, F J P, Aalto-Setälä, L, Enqvist, K, Huitu, K, Rummukainen, K, Nuijten, G, Eskola, K J, Kainulainen, K, Kalliokoski, T, Kumpulainen, J, Loo, K, Maalampi, J, Manninen, M, Moore, I, Suhonen, J, Trzaska, W H, Tuominen, K, Virtanen, A, Bertram, I, Finch, A, Grant, N, Kormos, L L, Ratoff, P, Christodoulou, G, Coleman, J, Touramanis, C, Mavrokoridis, K, Murdoch, M, McCauley, N, Payne, D, Jonsson, P, Kaboth, A, Long, K, Malek, M, Scott, M, Uchida, Y, Wascko, M O, Di Lodovico, F, Wilson, J R, Still, B, Sacco, R, Terri, R, Campanelli, M, Nichol, R, Thomas, J, Izmaylov, A, Khabibullin, M, Khotjantsev, A, Kudenko, Y, Matveev, V, Mineev, O, Yershov, N, Palladino, V, Evans, J, Söldner-Rembold, S, Yang, U K, Bonesini, M, Pihlajaniemi, T, Weckström, M, Mursula, K, Enqvist, T, Kuusiniemi, P, Räihä, T, Sarkamo, J, Slupecki, M, Hissa, J, Kokko, E, Aittola, M, Barr, G, Haigh, M D, de Jong, J, O'Keeffe, H, Vacheret, A, Weber, A, Galvanin, G, Temussi, M, Caretta, O, Davenne, T, Densham, C, Ilic, J, Loveridge, P, Odell, J, Wark, D, Robert, A, Andrieu, B, Popov, B, Giganti, C, Levy, J -M, Dumarchez, J, Buizza-Avanzini, M, Cabrera, A, Dawson, J, Franco, D, Kryn, D, Obolensky, M, Patzak, T, Tonazzo, A, Vanucci, F, Orestano, D, Di Micco, B, Tortora, L, Bésida, O, Delbart, A, Emery, S, Galymov, V, Mazzucato, E, Vasseur, G, Zito, M, Kudryavtsev, V A, Thompson, L F, Tsenov, R, Kolev, D, Rusinov, I, Bogomilov, M, Vankova, G, Matev, R, Vorobyev, A, Novikov, Yu, Kosyanenko, S, Suvorov, V, Gavrilov, G, Baussan, E, Dracos, M, Jollet, C, Meregaglia, A, Vallazza, E, Agarwalla, S K, Li, T, Autiero, D, Chaussard, L, Déclais, Y, Marteau, J, Pennacchio, E, Rondio, E, Lagoda, J, Zalipska, J, Przewlocki, P, Grzelak, K, Barker, G J, Boyd, S, Harrison, P F, Litchfield, R P, Ramachers, Y, Badertscher, A, Curioni, A, Degunda, U, Epprecht, L, Gendotti, A, Knecht, L, Di Luise, S, Horikawa, S, Lussi, D, Murphy, S, Natterer, G, Petrolo, F, Periale, L, Rubbia, A, Sergiampietri, F, Viant, T
    Publicado 2012
    “…Below 100~MeV, neutrinos from a new galactic supernova burst would be recorded with large statistics, addressing the astrophysics of the supernova and neutrino flavor oscillations through the SN and Earth matter. …”
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  14. 434
    por Botao, L, Dieminger, T, Franks, M, Gendotti, A, Kose, U, Rubbia, A, Sgalaberna, D, Zhao, X, Wuthrich, J, Bronner, C, Hayato, Y, Hiraide, K, Ieki, K, Kataoka, Y, Noguchi, Y, Shiozawa, M, Takemoto, Y, Radicioni, E, Boiano, A, De Rosa, G, Di Nitto, A, Langella, A, Lavitola, L, Ricciardi, G, Tortone, G, Bortolato, G, Collazuol, G, D'Ago, D, Feltre, M, Levorato, S, Longhin, A, Mattiazzi, M, Pari, M, Pupilli, F, Lamanna, G, Morescalchi, L, Pinzino, J, Sozzi, M, Ameli, F, Ludovici, L, Rescigno, M, Bolognesi, S, Calvet, D, Daret, T, Emery, S, Gonzalez, E M, Hassani, S, Joshi, S, Vasseur, G, Zietara, K, Di Lodovico, F, Hayashida, S, Hayrapetyan, K, Migenda, J, Dumarchez, J, Diaz Lopez, G, Giganti, C, Guigue, M, Popov, B, Russo, S, Saenz-Arevalo, W, Zito, M, Bernardi, L, Drapier, O, Buizza-Avanzini, M, Magniette, F, Mueller, T, Paganini, P, Quilain, B, Dealtry, T, Kormos, L, O'Keeffe, H M, Suchenek, M, Ziembicki, M, Bozza, C, Fusco, L, Ballester Merelo, F, Esteve Bosch, R, Gomez Gambin, A, Herrero Bosch, V, Mora Mas, F J, Toledo Alarcon, J F, Sanchez, F, Lam, V G C, Litchfield, R P, Machado, L N, Mikola, V, Naik, S, Riley, D, Soler, F J P, Bubak, A, Holeczek, J, Kisiel, J, Yokoyama, M, O'Flaherty, M, Richards, B, Buchowicz, A, Dygnarowicz, K, Galinski, G, Kurjata, R, Marzec, J, Obrebski, W, Pastuszak, G, Rychter, A, Zaremba, K, Ioannisian, A
    Publicado 2023
    “…Beyond the physics of neutrino oscillations, Hyper-Kamiokande will achieve unprecedented sensitivities to the detection of proton decays and supernova burst and relic neutrinos and will look for other types of astrophysical neutrinos, indirect evidence of dark matter and sterile neutrinos. …”
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  15. 435
    por Quintieri, L
    Publicado 2002
    “…However, even the largest hypothetical signal, such as a supernova occurring in our Galaxy, would produce a strain $\Delta L/L$ in the bar of the order of the GW amplitude \textit{h} $\sim$ 10$^{-18}$. …”
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  16. 436
    por Jain, Pankaj
    Publicado 2015
    “…IntroductionOverviewScales and DimensionsNight SkyConstellationsEarth, Sun, and the Solar SystemRetrograde Motion of PlanetsSidereal TimeAstronomical Catalogs and SoftwareObservationsElectromagnetic WavesElectromagnetic SpectrumTelescopesRefractor TelescopeReflecting TelescopeObservations at Visible FrequenciesTheoretical Limit on ResolutionSeeingMounting of TelescopeEquatorial MountAzimuthal MountInterferometerObservations at Other WavelengthsAstrometryCoordinate SystemsThe Horizontal SystemEquatorial Coordinate SystemEcliptic SystemGalactic Coordinate SystemSupergalactic Coordinate SystemSpace Velocity and Proper Motion of StarsDoppler EffectParallaxAberrationCoordinate TransformationsTransformation between Equatorial and Ecliptic Coordinate SystemsPrecession of EquinoxesEquatorial Mounting of a TelescopePhotometryIntroductionFlux Density and IntensityBlackbody RadiationEnergy Density in an Isotropic Radiation FieldMagnitude ScaleApparent MagnitudeAbsolute MagnitudeThe Color IndexBolometric MagnitudeStellar TemperaturesEffective TemperatureColor TemperatureAppendix: Solid AngleGravitation and Kepler's LawsTwo-Body ProblemApplication to Solar SystemVirial TheoremTidal Forces and Roche LimitStars, Stellar Spectra, and ClassificationIntroductionStellar Spectra Harvard Classification of Stellar SpectraSaha Equation Derivation of the Saha Equation Number of States of a Free Particle in a BoxHR DiagramStar Clusters and AssociationsDistance and Age Determination of Clusters using Color-Magnitude DiagramRadiation from Astronomical SourcesContinuous SpectraSynchrotron RadiationBremsstrahlungCompton ScatteringBound-Free TransitionsAbsorption and Emission Line SpectrumRadial Velocity due to Doppler EffectCauses of Finite Width of Spectral LinesMolecular Band SpectraExtinctionExtinction CoefficientColor ExcessStellar StructurePressure GradientMass DistributionEnergy ProductionTemperature GradientRadiative TransportConvective TransportBoundary ConditionsRosseland Mean OpacityEquation of StateIdeal Gas LawStellar Energy SourcesAppendix: Maxwell-Boltzmann DistributionStellar Nuclear ReactionsFundamental InteractionsFundamental ParticlesA Brief Introduction to NeutrinosPP Chain Nuclear Reaction RateNuclear Reaction Rate: DerivationNuclear Cross-SectionEstimating the Nuclear Reaction RateEnergy Released in Nuclear ReactionsStandard Solar ModelStar Formation and Stellar EvolutionEarly Stage of Star FormationFragmentationEvolution on the Main SequenceDegenerate Free Electron GasEvolution beyond the Main SequencePopulation I and II StarsWhite DwarfsNeutron StarBlack HolesSupernovaThe SunSolar AtmospherePhotosphereChromosphereCoronaDynamo Mechanism for Magnetic Field EnhancementSunspots and the Solar CycleSome Transient Phenomena The Solar SystemOrbital Properties of PlanetsRetrograde Motion of PlanetsAlbedo and Temperature of PlanetsTerrestrial Planets: Interior StructureJovian PlanetsThe MoonEclipses and OccultationsWhy Did Pluto Lose Its Planetship?…”
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  17. 437
    por Abe, K., Akutsu, R., Ali, A., Alt, C., Andreopoulos, C., Anthony, L., Antonova, M., Aoki, S., Ariga, A., Ashida, Y., Atkin, E.T., Awataguchi, Y., Ban, S., Barbi, M., Barker, G.J., Barr, G., Barry, C., Batkiewicz-Kwasniak, M., Beloshapkin, A., Bench, F., Berardi, V., Berkman, S., Berns, L., Bhadra, S., Bienstock, S., Blondel, A., Bolognesi, S., Bourguille, B., Boyd, S.B., Brailsford, D., Bravar, A., Bravo Berguño, D., Bronner, C., Bubak, A., Buizza Avanzini, M., Calcutt, J., Campbell, T., Cao, S., Cartwright, S.L., Catanesi, M.G., Cervera, A., Chappell, A., Checchia, C., Cherdack, D., Chikuma, N., Christodoulou, G., Coleman, J., Collazuol, G., Cook, L., Coplowe, D., Cudd, A., Dabrowska, A., De Rosa, G., Dealtry, T., Denner, P.F., Dennis, S.R., Densham, C., Di Lodovico, F., Dokania, N., Dolan, S., Drapier, O., Dumarchez, J., Dunne, P., Eklund, L., Emery-Schrenk, S., Ereditato, A., Fernandez, P., Feusels, T., Finch, A.J., Fiorentini, G.A., Fiorillo, G., Francois, C., Friend, M., Fujii, Y., Fujita, R., Fukuda, D., Fukuda, R., Fukuda, Y., Gameil, K., Giganti, C., Golan, T., Gonin, M., Gorin, A., Guigue, M., Hadley, D.R., Haigh, J.T., Hamacher-Baumann, P., Hartz, M., Hasegawa, T., Hastings, N.C., Hayashino, T., Hayato, Y., Hiramoto, A., Hogan, M., Holeczek, J., Hong Van, N.T., Iacob, F., Ichikawa, A.K., Ikeda, M., Ishida, T., Ishii, T., Ishitsuka, M., Iwamoto, K., Izmaylov, A., Jamieson, B., Jenkins, S.J., Jesús-Valls, C., Jiang, M., Johnson, S., Jonsson, P., Jung, C.K., Kabirnezhad, M., Kaboth, A.C., Kajita, T., Kakuno, H., Kameda, J., Karlen, D., Kasetti, S.P., Kataoka, Y., Katori, T., Kato, Y., Kearns, E., Khabibullin, M., Khotjantsev, A., Kikawa, T., Kim, H., Kim, J., King, S., Kisiel, J., Knight, A., Knox, A., Kobayashi, T., Koch, L., Koga, T., Konaka, A., Kormos, L.L., Koshio, Y., Kowalik, K., Kubo, H., Kudenko, Y., Kukita, N., Kuribayashi, S., Kurjata, R., Kutter, T., Kuze, M., Labarga, L., Lagoda, J., Lamoureux, M., Laveder, M., Lawe, M., Licciardi, M., Lindner, T., Litchfield, R.P., Liu, S.L., Li, X., Longhin, A., Ludovici, L., Lu, X., Lux, T., Machado, L.N., Magaletti, L., Mahn, K., Malek, M., Manly, S., Maret, L., Marino, A.D., Martin, J.F., Maruyama, T., Matsubara, T., Matsushita, K., Matveev, V., Mavrokoridis, K., Mazzucato, E., McCarthy, M., McCauley, N., McFarland, K.S., McGrew, C., Mefodiev, A., Metelko, C., Mezzetto, M., Minamino, A., Mineev, O., Mine, S., Miura, M., Molina Bueno, L., Moriyama, S., Morrison, J., Mueller, Th.A., Munteanu, L., Murphy, S., Nagai, Y., Nakadaira, T., Nakahata, M., Nakajima, Y., Nakamura, A., Nakamura, K.G., Nakamura, K., Nakayama, S., Nakaya, T., Nakayoshi, K., Nantais, C., Ngoc, T.V., Niewczas, K., Nishikawa, K., Nishimura, Y., Nonnenmacher, T.S., Nova, F., Novella, P., Nowak, J., Nugent, J.C., O'Keeffe, H.M., O'Sullivan, L., Odagawa, T., Okumura, K., Okusawa, T., Oser, S.M., Owen, R.A., Oyama, Y., Palladino, V., Palomino, J.L., Paolone, V., Parker, W.C., Paudyal, P., Pavin, M., Payne, D., Penn, G.C., Pickering, L., Pidcott, C., Pinzon Guerra, E.S., Pistillo, C., Popov, B., Porwit, K., Posiadala-Zezula, M., Pritchard, A., Quilain, B., Radermacher, T., Radicioni, E., Radics, B., Ratoff, P.N., Reinherz-Aronis, E., Riccio, C., Rondio, E., Roth, S., Rubbia, A., Ruggeri, A.C., Rychter, A., Sakashita, K., Sánchez, F., Schloesser, C.M., Scholberg, K., Schwehr, J., Scott, M., Seiya, Y., Sekiguchi, T., Sekiya, H., Sgalaberna, D., Shah, R., Shaikhiev, A., Shaker, F., Shaykina, A., Shiozawa, M., Shorrock, W., Shvartsman, A., Smirnov, A., Smy, M., Sobczyk, J.T., Sobel, H., Soler, F.J.P., Sonoda, Y., Steinmann, J., Suvorov, S., Suzuki, A., Suzuki, S.Y., Suzuki, Y., Sztuc, A.A., Tada, M., Tajima, M., Takeda, A., Takeuchi, Y., Tanaka, H.K., Tanaka, H.A., Tanaka, S., Thompson, L.F., Toki, W., Touramanis, C., Tsui, K.M., Tsukamoto, T., Tzanov, M., Uchida, Y., Uno, W., Vagins, M., Valder, S., Vallari, Z., Vargas, D., Vasseur, G., Vilela, C., Vinning, W.G.S., Vladisavljevic, T., Volkov, V.V., Wachala, T., Walker, J., Walsh, J.G., Wang, Y., Wark, D., Wascko, M.O., Weber, A., Wendell, R., Wilking, M.J., Wilkinson, C., Wilson, J.R., Wilson, R.J., Wood, K., Wret, C., Yamada, Y., Yamamoto, K., Yanagisawa, C., Yang, G., Yano, T., Yasutome, K., Yen, S., Yershov, N., Yokoyama, M., Yoshida, T., Yu, M., Zalewska, A., Zalipska, J., Zaremba, K., Zarnecki, G., Ziembicki, M., Zimmerman, E.D., Zito, M., Zsoldos, S., Zykova, A.
    Publicado 2019
    “…The impact on evaluation of backgrounds to searches for supernova relic neutrinos at present and future water Cherenkov detectors is also discussed.…”
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  18. 438
    por Acciari, V.A., Ansoldi, S., Antonelli, L.A., Engels, A. Arbet, Baack, D., Babić, A., Banerjee, B., Barres de Almeida, U., Barrio, J.A., Becerra González, J., Bednarek, W., Bellizzi, L., Bernardini, E., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Biland, A., Blanch, O., Bonnoli, G., Bošnjak, Ž., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S.M., Colin, U., Colombo, E., Contreras, J.L., Cortina, J., Covino, S., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Depaoli, D., Di Pierro, F., Di Venere, L., Espiñeira, E. Souto, Do., Dominis Prester, D., Donini, A., Dorner, D., Doro, M., Elsaesser, D., Fallah Ramazani, V., Fattorini, A., Ferrara, G., Foffano, L., Fonseca, M.V., Font, L., Fruck, C., Fukami, S., López, R.J. García, Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinović, N., Green, D., Hadasch, D., Hahn, A., Herrera, J., Hoang, J., Hrupec, D., Hütten, M., Inada, T., Inoue, S., Ishio, K., Iwamura, Y., Jouvin, L., Kajiwara, Y., Karjalainen, M., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Lombardi, S., Longo, F., López, M., López-Coto, R., López-Oramas, A., Loporchio, S., de Oliveira Fraga, B. Machado, Masuda, S., Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Martínez, M., Mazin, D., Mender, S., Mićanović, S., Miceli, D., Miener, T., Minev, M., Miranda, J.M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Munar-Adrover, P., Neustroev, V., Nigro, C., Nilsson, K., Ninci, D., Nishijima, K., Noda, K., Nogués, L., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J.M., Pavletić, L., Peñil, P., Peresano, M., Persic, M., Prada Moroni, P.G., Prandini, E., Puljak, I., Rhode, W., Ribó, M., Rico, J., Righi, C., Rugliancich, A., Saha, L., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Schleicher, B., Schmidt, K., Schweizer, T., Sitarek, J., Šnidarić, I., Sobczynska, D., Spolon, A., Stamerra, A., Strom, D., Strzys, M., Suda, Y., Surić, T., Takahashi, M., Tavecchio, F., Temnikov, P., Terzić, T., Teshima, M., Torres-Albà, N., Tosti, L., van Scherpenberg, J., Vanzo, G., Vazquez Acosta, M., Ventura, S., Verguilov, V., Vigorito, C.F., Vitale, V., Vovk, I., Will, M., Zarić, D., authors, External, Celli, S., Morlino, G.
    Publicado 2020
    “…Diffusive shock acceleration (DSA) is the most promising mechanism to accelerate Galactic cosmic rays (CRs) in the shocks of supernova remnants (SNRs). The turbulence upstream is supposedly generated by the CRs, but this process is not well understood. …”
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  19. 439
    Publicado 2002
    “…\item Atmospheric neutrino oscillations - Long base-line neutrino oscillations \item Magnetic monopoles - Supernova detection \item The Unexpected \end{itemize}…”
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  20. 440
    por Caratelli, D., Foreman, W., Friedland, A., Gardiner, S., Gil-Botella, I., Karagiorgi, G., Kirby, M., Lehmann Miotto, G., Littlejohn, B.R., Mooney, M., Reichenbacher, J., Sousa, A., Scholberg, K., Yu, J., Yang, T., Asaadi, J., Bezerra, T.J.C., Capozzi, F., Cavanna, F., Church, E., Himmel, A., Junk, T., Klein, J., Lepetic, I., Li, S., Sala, P., Schellman, H., Sorel, M., Wang, J., Wang, M.H.L.S., Wu, W., Zennamo, J., Adames, M.R., Amar, H., Andrade, D.A., Andreopoulos, C., Ankowski, A.M., Arroyave, M.A., Aushev, V., Ayala-Torres, M.A., Baldi, P., Backhouse, C., Balantekin, A.B., Barkhouse, W.A., Barham Alzás, P., Barrow, J.L., Battat, J.B.R., Bazetto, M.C.Q., Beacom, J.F., Behera, B., Bellettini, G., Berger, J., Bezerra, A.T., Bian, J., Bilki, B., Bles, B., Bolton, T., Bomben, L., Bonesini, M., Bonilla-Diaz, C., Boran, F., Borkum, A.N., Bostan, N., Brailsford, D., Branca, A., Brunetti, G., Cai, T., Chappell, A., Charitonidis, N., Cintra, P.H.P., Conley, E., Coan, T.E., Cova, P., Cremaldi, L.M., Crespo-Anadón, J.I., Cuesta, C., Cui, Y., Dallavalle, R., Davies, G.S., De, S., Dedin Neto, P., Delgado, M., Delmonte, N., Denton, P.B., De Roeck, A., Dharmapalan, R., Djurcic, Z., Dolek, F., Doran, S., Dorrill, R., Duffy, K.E., Dutta, B., Dvornikov, O., Edayath, S., Evans, J.J., Ezeribe, A.C., Falcone, A., Fani, M., Felix, J., Feng, Y., Fields, L., Filip, P., Fiorillo, G., Franco, D., Garcia-Gamez, D., Giri, A., Gogota, O., Gollapinni, S., Goodman, M., Gramellini, E., Gran, R., Granger, P., Grant, C., Greenberg, S.E., Groh, M., Guenette, R., Guffanti, D., Harris, D.A., Hatzikoutelis, A., Heeger, K.M., Morquecho, M. Hernandez, Herner, K., Ho, J., Holanda, P.C., Ilic, N., Jackson, C.M., Jang, W., Janka, H.-Th., Jo, J.H., Joaquim, F.R., Jones, R.S., Jovančević, N., Jwa, Y.-J., Kalra, D., Kaplan, D.M., Katsioulas, I., Kearns, E., Kelly, K.J., Kemp, E., Ketchum, W., Kish, A., Koerner, L.W., Kosc, T., Kothekar, K., Kreslo, I., Kubota, S., Kudryavtsev, V.A., Kumar, P., Kutter, T., Kvasnicka, J., Lazanu, I., LeCompte, T., Li, Y., Liu, Y., Lokajicek, M., Louis, W.C., Luk, K.B., Luo, X., Machado, P.A.N., Machulin, I.M., Mahn, K., Man, M., Mandujano, R.C., Maneira, J., Corchado, S. Manthey, Marchionni, A., Marfatia, D., Maricic, J., Marinho, F., Mariani, C., Marshall, C.M., López, F. Martínez, Martinez Caicedo, D.A., Mastbaum, A., Matheny, M., McConkey, N., Mehta, P., Messer, O.E.B., Minotti, A., Miranda, O.G., Mishra, P., Mocioiu, I., Mogan, A., Mohanta, R., Mohayai, T., Montanari, C., Montano Zetina, L.M., Moor, A.F., Moretti, D., Moura, C.A., Mualem, L.M., Nachtman, J., Narita, S., Navrer-Agasson, A., Nebot-Guinot, M., Newby, J., Nikolov, J., Nowak, J.A., Ochoa-Ricoux, J.P., O'Connor, E., Onel, Y., Onishchuk, Y., Orebi Gann, G.D., Pandey, V., Parozzi, E.G., Parveen, S., Parvu, M., Patterson, R.B., Paulucci, L., Pec, V., Peeters, S.J.M., Pompa, F., Poonthottathil, N., Poudel, S.S., Psihas, F., Rafique, A., Rajaoalisoa, M., Ramson, B.J., Razafinime, S.H., Real, J.S., Rikalo, A., Ross-Lonergan, M., Russell, B., Sacerdoti, S., Sahoo, S.K., Sahu, N., Sanders, D.A., Santoro, D., Santos, M.V., Schmitz, D.W., Senise, Jr.C.R., Shanahan, P.N., Sharma, H.R., Sharma, R.K., Shi, W., Shin, S., Singh, J., Nagu, S., Singh, L., Singh, P., Singh, V., Soderberg, M., Solano Salinas, C.J., Spurgeon, C., Spurgeon, K., Steklain, A.F., Stocker, F., Stokes, T., Strait, J., Strait, M., Strauss, T., Suter, L., Svoboda, R., Szelc, A.M., Szydagis, M., Tarpara, E., Tatar, E., Terranova, F., Testera, G., Chithirasree, N., Todorović, N., Tonazzo, A., Torti, M., Tortorici, F., Toups, M., Tran, D.Q., Travar, M., Tsai, Y.-D., Tsai, Y.-T., Tu, S.Z., Urheim, J., Utaegbulam, H., Valder, S., Valdiviesso, G.A., Valentim, R., Vergani, S., Viren, B., Vraničar, A., Wang, B., Waters, D., Weatherly, P., Weber, M., Wei, H., Wenzel, H., Westerdale, S., Whitehead, L.H., Whittington, D., Wilkinson, A., Wilson, R.J., Worcester, M., Wresilo, K., Yaeggy, B., Yang, G., Zalesak, J., Zamorano, B., Zuklin, J.
    Publicado 2022
    “…These include novel charge enhancement and readout systems, enhanced photon detection, low radioactivity argon, and xenon doping. 7) Low-energy signatures, whether steady-state or part of a supernova burst or larger GeV-scale event topology, have specific triggering, DAQ and reconstruction requirements that must be addressed outside the scope of conventional GeV-scale data collection and analysis pathways.…”
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