3,470 results on '"Villar, J."'
Search Results
2. Calibration for in vivo monitoring of thyroid of exposed population at risk of intakes of radioiodine isotopes due to a nuclear or radiological emergency
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Pérez López, B., Valencia Villar, J., Navarro Amaro, J.F., and López Ponte, M.A.
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- 2024
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3. Análisis y aspectos técnicos de las preguntas asociadas a imágenes radiológicas en el examen para médico interno residente en España, convocatoria 2022
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Murias Quintana, E., Costilla García, S.M., Curbelo García, J.J., Calvo Blanco, J., Vega Villar, J., and Baladrón Romero, J.
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- 2024
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4. Ferroptosis as a Biological Phase Transition I: avascular and vascular tumor growth
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Nieto-Villar, J. M. and Mansilla, R.
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Physics - Biological Physics ,Nonlinear Sciences - Chaotic Dynamics ,Quantitative Biology - Biomolecules ,Quantitative Biology - Quantitative Methods - Abstract
Herewith we discuss a network model of the ferroptosis avascular and vascular tumor growth based on our previous proposed framework. Chiefly, ferroptosis should be viewed as a first order phase transition characterized by a supercritical Andronov Hopf bifurcation, with the emergence of limit cycle. The increase of the population of the oxidized PUFA fragments, take as the control parameter, involves an inverse Feigenbaum, (a cascade of saddle foci Shilnikov's bifurcations) scenario, which results in the stabilization of the dynamics and in a decrease of complexity., Comment: 13 pages, 3 figures
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- 2021
5. Rationale and study design for an Individualized PeriopeRative Open lung VEntilatory approach in Emergency Abdominal Laparotomy/scopy: study protocol for a prospective international randomized controlled trial
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Laguna, G., Suárez-Sipmann, F., Tusman, G., Ripollés, J., Díaz-Cambronero, O., Pujol, R., Rivas, E., Garutti, I., Mellado, R., Vallverdú, J., Jacas, A., Fervienza, A., Marrero, R., Librero, J., Villar, J., and Ferrando, C.
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- 2024
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6. Fundamento y diseño del estudio para una estrategia ventilatoria de pulmón abierto perioperatoria individualizada en laparotomía/laparoscopia abdominal urgente (iPROVE): protocolo del estudio para ensayo controlado aleatorizado prospectivo internacional
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Laguna, G., Suárez-Sipmann, F., Tusman, G., Ripollés, J., Díaz-Cambronero, O., Pujol, R., Rivas, E., Garutti, I., Mellado, R., Vallverdú, J., Jacas, A., Fervienza, A., Marrero, R., Librero, J., Villar, J., and Ferrando, C.
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- 2024
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7. Metastasis Models: Thermodynamics and Complexity
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Guerra, A., primary, Betancourt-Mar, J. A., additional, Llanos-Pérez, J. A., additional, Mansilla, R., additional, and Nieto-Villar, J. M., additional
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- 2023
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8. Correction: Efficacy and safety assessment of different dosage of benznidazol for the treatment of Chagas disease in chronic phase in adults (MULTIBENZ study): study protocol for a multicenter randomized Phase II non-inferiority clinical trial
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Molina-Morant, D., Fernández, M. L., Bosch-Nicolau, P., Sulleiro, E., Bangher, M., Salvador, F., Sanchez-Montalva, A., Ribeiro, A. L. P., de Paula, A. M. B., Eloi, S., Correa-Oliveira, R., Villar, J. C., Sosa-Estani, S., and Molina, I.
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- 2023
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9. Lignocellulosic biomass pre-treatments by diluted sulfuric acid and ethanol-water mixture: A comparative techno-economic analysis
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Gutierrez, Soledad, Mangone, Franco, Vergara, Priscilla, Gonzalez, Valeria, Ferreira, Joao Pedro, Villar, J. Carlos, and Garcia-Ochoa, Felix
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- 2023
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10. NMR-based metabolomics to determine the fluctuation of metabolites in hydroponic purslane crops at different harvesting times
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Montoya-García, César Omar, García-Mateos, Rosario, Magdaleno-Villar, J. Jesús, Volke-Haller, Víctor Hugo, Villa-Ruano, Nemesio, Zepeda-Vallejo, L. Gerardo, and Becerra-Martínez, Elvia
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- 2023
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11. SISTEMA DE EMISIÓN Y DETECCIÓN DE PULSOS ÓPTICOS EN EL ORDEN DE LOS NANOSEGUNDOS
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Raymond, S., Del Villar, J., Stolik, S., Jimenez, D., Valor, A., and de la Rosa, J.M.
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- 2023
12. Effect of the concentration of the nutrient solution on the nutrient content of chrysanthemum (Dendranthema grandiflorum (Ramat.)
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Quevedo-Ortiz, Betsy, Juarez-Hernandez, Ma. de Jesus, Magdaleno-Villar, J. Jesus, Perez-Vivar, Marcelino, Valdez-Hernandez, Edna Fabiola, and Mejfa-Munoz, Jose Merced
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- 2022
13. First results on dark matter annual modulation from ANAIS-112 experiment
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Amaré, J., Cebrián, S., Coarasa, I., Cuesta, C., García, E., Martínez, M., Oliván, M. A., Ortigoza, Y., de Solórzano, A. Ortiz, Puimedón, J., Salinas, A., Sarsa, M. L., Villar, P., and Villar, J. A.
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Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment ,Physics - Instrumentation and Detectors - Abstract
ANAIS is a direct detection dark matter experiment aiming at the testing of the DAMA/LIBRA annual modulation result, which standing for about two decades has neither been confirmed nor ruled out by any other experiment in a model independent way. ANAIS-112, consisting of 112.5 kg of sodium iodide crystals, is taking data at the Canfranc Underground Laboratory, Spain, since August 2017. This letter presents the annual modulation analysis of 1.5 years of data, amounting to 157.55 kg$\times$y. We focus on the model independent analysis searching for modulation and the validation of our sensitivity prospects. ANAIS-112 data are consistent with the null hypothesis (p-values of 0.65 and 0.16 for [2-6] and [1-6] keV energy regions, respectively). The best fits for the modulation hypothesis are consistent with the absence of modulation ($S_m$=-0.0044$\pm$0.0058 cpd/kg/keV and -0.0015$\pm$0.0063 cpd/kg/keV, respectively). They are in agreement with our estimated sensitivity for the accumulated exposure, supporting our projected goal of reaching a 3$\sigma$ sensitivity to the DAMA/LIBRA result in 5 years of data taking., Comment: 6 pages, 4 figures
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- 2019
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14. Bioactive compounds of purslane (Portulaca oleracea L.) according to the production system: A review
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Montoya-García, César Omar, García-Mateos, Rosario, Becerra-Martínez, Elvia, Toledo-Aguilar, Rocío, Volke-Haller, Víctor Hugo, and Jesús Magdaleno-Villar, J.
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- 2023
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15. ANAIS-112 sensitivity in the search for dark matter annual modulation
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Coarasa, I., Amaré, J., Cebrián, S., Cuesta, C., García, E., Martínez, M., Oliván, M. A., Ortigoza, Y., de Solórzano, A. Ortiz, Puimedón, J., Salinas, A., Sarsa, M. L., Villar, P., and Villar, J. A.
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Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment ,Physics - Instrumentation and Detectors - Abstract
The annual modulation measured by the DAMA/LIBRA experiment can be explained by the interaction of dark matter WIMPs in NaI(Tl) scintillator detectors. Other experiments, with different targets or techniques, exclude the region of parameters singled out by DAMA/LIBRA, but the comparison of their results relies on several hypotheses regarding the dark matter model. ANAIS-112 is a dark matter search with 112.5 kg of NaI(Tl) scintillators at the Canfranc Underground Laboratory (LSC) to test the DAMA/LIBRA result in a model independent way. We analyze its prospects in terms of the a priori critical and detection limits of the experiment. A simple figure of merit has been obtained to compare the different experiments looking for the annual modulation observed by DAMA/LIBRA. We conclude that after 5 years of measurement, ANAIS-112 can detect the annual modulation in the 3$\sigma$ region compatible with the DAMA/LIBRA result., Comment: 8 pages, 5 figures, 2 tables. arXiv admin note: substantial text overlap with arXiv:1704.06861
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- 2018
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16. Analysis of backgrounds for the ANAIS-112 dark matter experiment
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Amare, J., Cebrian, S., Coarasa, I., Cuesta, C., Garcia, E., Martinez, M., Olivan, M. A., Ortigoza, Y., de Solorzano, A. Ortiz, Puimedon, J., Salinas, A., Sarsa, M. L., Villar, J. A., and Villar, P.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment ,Physics - Instrumentation and Detectors - Abstract
The ANAIS (Annual modulation with NaI(Tl) Scintillators) experiment aims at the confirmation or refutation of theDAMA/LIBRA positive annual modulation signal in the low energy detection rate, using the same target and technique, at the Canfranc Underground Laboratory (LSC) in Spain. ANAIS-112, consisting of nine 12.5 kg NaI(Tl) modules produced by Alpha Spectra Inc. in a 3x3matrix configuration, is taking data smoothly in "dark matter search" mode since August, 2017, after a commissioning phase and operation of the first detectors during the last years in various setups. A large effort has been carried out withinANAIS to characterize the background of sodium iodide detectors, before unblinding the data and performing the first annual modulation analysis. Here, the background models developed for all the nine ANAIS-112 detectors are presented. Measured spectra from threshold to high energy in different conditions are well described by the models based on quantified activities independently estimated following several approaches. In the region from 1 to 6 keVee the measured, efficiency corrected background level is 3.58+-0.02 keV-1 kg-1 day-1; NaI crystal bulk contamination is the dominant background source being 210Pb, 40K, 22Na and 3H contributions the most relevant ones. This background level, added to the achieved 1 keVee analysis threshold (thanks to the outstanding light collection and robust filtering procedures developed), allow ANAIS-112 to be sensitive to the modulation amplitude measured by DAMA/LIBRA, and able to explore at three sigma level in 5 years the WIMP parameter region singled out by this experiment., Comment: Final version for publication
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- 2018
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17. Performance of ANAIS-112 experiment after the first year of data taking
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Amaré, J., Cebrián, S., Coarasa, I., Cuesta, C., García, E., Martínez, M., Oliván, M. A., Ortigoza, Y., de Solórzano, A. Ortiz, Puimedón, J., Salinas, A., Sarsa, M. L., Villar, P., and Villar, J. A.
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Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment ,Physics - Instrumentation and Detectors - Abstract
ANAIS is a direct detection dark matter experiment aiming at the study of the annual modulation expected in the interaction rate. It uses same target and technique than DAMA/LIBRA experiment, which reported a highly significant positive modulation compatible with that expected for dark matter particles distributed in the galactic halo. However, other very sensitive experiments do not find any hint of particles with the required properties, although comparison is model dependent. In 2017, ANAIS-112 experiment was installed at the Canfranc Underground Laboratory (LSC), in Spain, and after the commissioning run for calibration and general assessment, ANAIS-112 started data taking in dark matter mode on August 3$^{rd}$, 2017. It consists of nine NaI(Tl) modules, amounting 112.5 kg of mass in total. ANAIS-112 will be able to test the DAMA/LIBRA result with the achieved background and threshold at three sigma level in five years of data taking. Here we report on the experimental apparatus and detector performance after the first year of data taking. Total live time available amounts to 341.72 days, being the corresponding exposure 105.32 kg x yr., Comment: 27 pages, 40 figures
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- 2018
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18. Characteristics and outcomes of COVID-19 patients admitted to hospital with and without respiratory symptoms
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Citarella, B, Kartsonaki, C, Ibanez-Prada, E, Goncalves, B, Baruch, J, Escher, M, Pritchard, M, Wei, J, Philippy, F, Dagens, A, Hall, M, Lee, J, Kutsogiannis, D, Wils, E, Fernandes, M, Tirupakuzhi Vijayaraghavan, B, Panda, P, Martin-Loeches, I, Ohshimo, S, Fatoni, A, Horby, P, Dunning, J, Rello, J, Merson, L, Rojek, A, Vaillant, M, Olliaro, P, Reyes, L, Moharam, S, Abdalasalam, S, Abdalhadi, A, Abdalla, N, Abdalla, W, Abdalrheem, A, Abdalsalam, A, Abdeewi, S, Abdelgaum, E, Abdelhalim, M, Abdelkabir, M, Abdelrahman, I, Abdukahil, S, Abdulbaqi, L, Abdulhamid, S, Abdulhamid, W, Abdulkadir, N, Abdulwahed, E, Abdunabi, R, Abe, R, Abel, L, Abodina, A, Abrous, A, Absil, L, Jabal, K, Salah, N, Abusalama, A, Abuzaid, T, Acharya, S, Acker, A, Adam, E, Adem, S, Ademnou, M, Adewhajah, F, Adriao, D, Afum-Adjei Awuah, A, Agbogbatey, M, Al Ageel, S, Ahmed, A, Ahmed, M, Ahmed, S, Alaraji, Z, Elhefnawy Enan, A, Ahmed Khalil, R, Ahmed Mohamed Abdelaziz, A, Ainscough, K, Airlangga, E, Aisa, T, Aisha, A, Aisha, B, Hssain, A, Tamlihat, Y, Akimoto, T, Akmal, E, Akwani, C, Al Qasim, E, Alajeeli, A, Alali, A, Alalqam, R, Alameen, A, Al-Aquily, M, Albakry, K, Albatni, S, Alberti, A, Aldabbourosama, O, Al-dabbous, T, Aldhalia, A, Aldoukali, A, Alegesan, S, Alessi, M, Alex, B, Alexandre, K, Al-Fares, A, Alflite, A, Alfoudri, H, Alhadad, Q, Alhaddad, H, Mohamed Abdalla Alhasan, M, Alhouri, A, Alhouri, H, Ali, A, Ali, I, TagElser Mohammed Ali, M, Abbas, S, Abdelghafar, Y, Sheikh, N, Alidjnou, K, Aljadi, M, Aljamal, S, Alkahlout, M, Alkaseek, A, Alkhafajee, Q, Allavena, C, Allou, N, Almasri, L, Almjersah, A, Alqandouz, R, Alrfaea, W, Alrifaee, M, Alsaadi, R, Al-Saba'a, Y, Alshareea, E, Alshenawy, E, Altaf, A, Alves, J, Alves, R, Cabrita, J, Amaral, M, Amer, A, Amira, N, Adusei, A, Amuasi, J, Andini, R, Andrejak, C, Angheben, A, Angoulvant, F, Ankrah, S, Ansart, S, Anthonidass, S, Antonelli, M, Antunes de Brito, C, Apriyana, A, Arabi, Y, Aragao, I, Arancibia, F, Araujo, C, Arcadipane, A, Archambault, P, Arenz, L, Arlet, J, Arnold-Day, C, Arora, L, Arora, R, Artaud-Macari, E, Aryal, D, Asensio, A, Ashley, E, Ashraf, M, Ben Ashur, A, Asiedu-Bekoe, F, Asif, N, Asim, M, Assi, G, Assie, J, Asyraf, A, Atangana, F, Atia, A, Atif, M, Abdelrhman Abdallahrs, A, Atique, A, Atlowly, M, Attanyake, A, Auchabie, J, Aumaitre, H, Auvet, A, Ali Mohammed, A, Axelsen, E, Ayad, A, Hassan Helmi, A, Azemar, L, Azizeldin, M, Azoulay, C, Babatunde, H, Bach, B, Bachelet, D, Badr, C, Baevre-Jensen, R, Baig, N, Baillie, J, Baird, J, Bak, E, Bakakos, A, Bakar, N, Bakeer, H, Bakri, A, Bal, A, Balakrishnan, M, Bandoh, I, Bani-Sadr, F, Barbalho, R, Barbosa, N, Barclay, W, Barnett, S, Barnikel, M, Barrasa, H, Barrigoto, C, Bartoli, M, Basmaci, R, Basri, M, Batool, A, Battaglini, D, Bauer, J, Bautista Rincon, D, Dow, D, Beane, A, Bedossa, A, Bee, K, Begum, H, Behilill, S, Beishuizen, A, Beljantsev, A, Bellemare, D, Beltrame, A, Beltrao, B, Beluze, M, Benech, N, Benjiman, L, Bennett, S, Bento, L, Berdal, J, Berdeweel, L, Bergeaud, D, Bergin, H, Bertoli, G, Bertolino, L, Bessis, S, Bevilcaqua, S, Bezulier, K, Bhatt, A, Bhavsar, K, Bianchi, I, Bianco, C, Bichoka, S, Bidin, F, Humaid, F, Bin Kamarudin, M, Binnawara, M, Bisoffi, Z, Biston, P, Bitker, L, Bittaye, M, Bitton, J, Blanco-Schweizer, P, Blier, C, Bloos, F, Blot, M, Boccia, F, Bodenes, L, Bogaert, D, Boivin, A, Bolanga, A, Bolanos, I, Bolze, P, Bompart, F, Bonifasius, A, Bonney, J, Borges, D, Borie, R, Bosse, H, Botelho-Nevers, E, Bouadma, L, Bouchaud, O, Bouchez, S, Bouhour, D, Bouiller, K, Bouillet, L, Bouisse, C, Bountthasavong, L, Boureau, A, Bourke, J, Bouscambert, M, Bousquet, A, Boyer-Besseyre, M, Boylan, M, Bozza, F, Braconnier, A, Braga, C, Brandenburger, T, Monteiro, F, Brazzi, L, Breen, D, Breen, P, Brewster, D, Brickell, K, Broadley, T, Brotherton, H, Browne, A, Brozzi, N, Brunvoll, S, Brusse-Keizer, M, Bryda, P, Buchtele, N, Bugaeva, P, Buisson, M, Buonsenso, D, Burhan, E, Buri, D, Burrell, A, Bustos, I, Butnaru, D, Cabie, A, Cabral, S, Caceres, E, Cadoz, C, Garces, R, Calligy, K, Calvache, J, Camoes, J, Campana, V, Campbell, P, Campisi, J, Canepa, C, Cantero, M, Caoili, J, Caraux-Paz, P, Carcel, S, Cardoso, F, Cardoso, N, Cardoso, S, Carelli, S, Carlier, N, Carmoi, T, Carney, G, Carqueja, I, Carret, M, Carrier, F, Carroll, I, Carson, G, Casanova, M, Cascao, M, Casey, S, Casimiro, J, Cassandra, B, Castaneda, S, Castanheira, N, Castor-Alexandre, G, Castro, I, Catarino, A, Catherine, F, Cattaneo, P, Cavalin, R, Cavalli, G, Cavayas, A, Ceccato, A, Ceesay, M, Cerkovnik, S, Cervantes-Gonzalez, M, Cevik, M, Chair, A, Chakveatze, C, Chan, A, Chand, M, Chapplain, J, Charpentier, C, Chas, J, Chaudry, M, Chavez Iniguez, J, Chen, A, Chen, Y, Chenard, L, Cheng, M, Cheret, A, Chiarabini, T, Chica, J, Chidambaram, S, Tho, L, Chirouze, C, Chiumello, D, Cho, S, Cholley, B, Chommanam, D, Chopin, M, Chow, Y, Chow, T, Christy, N, Chua, H, Chua, J, Cidade, J, Cisneros Herreros, J, Ciullo, A, Clarke, J, Claure-Del Granado, R, Clohisey, S, Codan, C, Cody, C, Coles, J, Coles, M, Colin, G, Collins, M, Combs, P, Connolly, J, Connor, M, Conrad, A, Conway, E, Cooke, G, Cordel, H, Corley, A, Cornelis, S, Cornet, A, Corpuz, A, Cortegiani, A, Corvaisier, G, Couffignal, C, Couffin-Cadiergues, S, Courtois, R, Cousse, S, Cowan, J, Cregan, R, Crowl, G, Crump, J, Cruz, C, Csete, M, Cullen, A, Cummings, M, Curley, G, Curlier, E, Curran, C, Custodio, P, da Silva Filipe, A, Da Silveira, C, Dabaliz, A, Dahl, J, Dahly, D, D'Alessandro, U, Daley, P, Dalloul, Z, Dalton, H, Dalton, J, Daly, S, Damas, J, Dame, J, Damien, C, Daneman, N, Dantas, J, D'Aragon, F, de Loughry, G, de Mendoza, D, De Montmollin, E, Franca, R, Isabel de Pinho Oliveira, A, De Rosa, R, De Rose, C, de Silva, T, de Vries, P, Deacon, J, Dean, D, Debard, A, Debenedictis, B, Debray, M, Decastro, N, Dechert, W, Decours, R, Defous, E, Delacroix, I, Delamou, A, Delaveuve, E, Delavigne, K, Delfos, N, Deligiannis, I, Dell'Amore, A, Delmas, C, Delobel, P, Delsing, C, Demonchy, E, Denis, E, Deplanque, D, Depuydt, P, Descamps, D, Desvallees, M, Dewayanti, S, Dhangar, P, Diallo, A, Diallo, S, Diamantis, S, Dias, A, Da Silva, F, Diaz, R, Diaz, J, Diaz, P, Dibba, B, Didier, K, Diehl, J, Dieperink, W, Dimet, J, Dinot, V, Diop, F, Diouf, A, Dishon, Y, Djadda, C, Djossou, F, Docherty, A, Doherty, H, Dondorp, A, Donnelly, C, Donohue, Y, Donohue, S, Doran, P, Dorival, C, D'Ortenzio, E, Doshi, Y, Douangdala, P, Douglas, J, Douma, R, Dournon, N, Downey, J, Downing, M, Drake, T, Driscoll, A, Duah, I, Fonseca, C, Dubee, V, Dubos, F, Dubot-Peres, A, Ducancelle, A, Duculan, T, Dudman, S, Duggal, A, Dunand, P, Duplaix, M, Durante-Mangoni, E, Durham, L, Dussol, B, Duthoit, J, Duval, X, Dyrhol-Riise, A, Ean, S, Ebo, A, Echeverria-Villalobos, M, Edelstein, M, Egan, S, Eggesbo, L, Ehzaz, K, Eira, C, El Sanharawi, M, El Sayed, M, Elabid, M, Elagili, M, Elapavaluru, S, Elbahnasawy, M, Elboshra, S, Elharrar, B, Ellerbroek, J, Ellingjord-Dale, M, 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U., Barnikel M., Barrasa H., Barrigoto C., Bartoli M., Basmaci R., Basri M. F. H., Batool A., Battaglini D., Bauer J., Bautista Rincon D. F., Dow D. B., Beane A., Bedossa A., Bee K. H., Begum H., Behilill S., Beishuizen A., Beljantsev A., Bellemare D., Beltrame A., Beltrao B. A., Beluze M., Benech N., Benjiman L. E., Bennett S., Bento L., Berdal J. -E., Berdeweel L., Bergeaud D., Bergin H., Bertoli G., Bertolino L., Bessis S., Bevilcaqua S., Bezulier K., Bhatt A., Bhavsar K., Bianchi I., Bianco C., Bichoka S., Bidin F. N., Humaid F. B., Bin Kamarudin M. N., Binnawara M., Bisoffi Z., Biston P., Bitker L., Bittaye M., Bitton J., Blanco-Schweizer P., Blier C., Bloos F., Blot M., Boccia F., Bodenes L., Bogaert D., Boivin A. -H., Bolanga A., Bolanos I., Bolze P. -A., Bompart F., Bonifasius A., Bonney J., Borges D., Borie R., Bosse H. M., Botelho-Nevers E., Bouadma L., Bouchaud O., Bouchez S., Bouhour D., Bouiller K., Bouillet L., Bouisse C., Bountthasavong L., Boureau A. -S., Bourke J., Bouscambert M., Bousquet A., Boyer-Besseyre M., Boylan M., Bozza F. A., Braconnier A., Braga C., Brandenburger T., Monteiro F. B., Brazzi L., Breen D., Breen P., Brewster D., Brickell K., Broadley T., Brotherton H., Browne A., Brozzi N., Brunvoll S. H., Brusse-Keizer M., Bryda P., Buchtele N., Bugaeva P., Buisson M., Buonsenso D., Burhan E., Buri D., Burrell A., Bustos I. G., Butnaru D., Cabie A., Cabral S., Cabrita J., Caceres E., Cadoz C., Garces R. C., Calligy K., Calvache J. A., Camoes J., Campana V., Campbell P., Campisi J., Canepa C., Cantero M., Caoili J., Caraux-Paz P., Carcel S., Cardoso F., Cardoso N., Cardoso S., Carelli S., Carlier N., Carmoi T., Carney G., Carqueja I., Carret M. -C., Carrier F. 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J., Cortegiani A., Corvaisier G., Couffignal C., Couffin-Cadiergues S., Courtois R., Cousse S., Cowan J., Cregan R., Crowl G., Crump J., Cruz C., Csete M., Cullen A., Cummings M., Curley G., Curlier E., Curran C., Custodio P., da Silva Filipe A., Da Silveira C., Dabaliz A. -A., Dahl J. A., Dahly D., D'Alessandro U., Daley P., Dalloul Z., Dalton H., Dalton J., Daly S., Damas J., Dame J., Damien C., Daneman N., Dantas J., D'Aragon F., de Loughry G., de Mendoza D., De Montmollin E., Franca R. F. D. O., Isabel de Pinho Oliveira A., De Rosa R., De Rose C., de Silva T., de Vries P., Deacon J., Dean D., Debard A., DeBenedictis B., Debray M. -P., DeCastro N., Dechert W., Decours R., Defous E., Delacroix I., Delamou A., Delaveuve E., Delavigne K., Delfos N. M., Deligiannis I., Dell'Amore A., Delmas C., Delobel P., Delsing C., Demonchy E., Denis E., Deplanque D., Depuydt P., Descamps D., Desvallees M., Dewayanti S., Dhangar P., Diallo A., Diallo S. T., Diamantis S., Dias A., Da Silva F. D., Diaz R., Diaz J. J., Diaz P., Dibba B. K., Didier K., Diehl J. -L., Dieperink W., Dimet J., Dinot V., Diop F., Diouf A., Dishon Y., Djadda C., Djossou F., Docherty A. B., Doherty H., Dondorp A. M., Donnelly C. A., Donohue Y., Donohue S., Doran P., Dorival C., D'Ortenzio E., Doshi Y., Douangdala P., Douglas J. J., Douma R., Dournon N., Downey J., Downing M., Drake T., Driscoll A., Duah I. K., Fonseca C. D., Dubee V., Dubos F., Dubot-Peres A., Ducancelle A., Duculan T., Dudman S., Duggal A., Dunand P., Duplaix M., Durante-Mangoni E., Durham L., Dussol B., Duthoit J., Duval X., Dyrhol-Riise A. M., Ean S. C., Ebo A., Echeverria-Villalobos M., Edelstein M., Egan S., Eggesbo L. M., Ehzaz K., Eira C., El Sanharawi M., El Sayed M., Elabid M., Elagili M. B., Elapavaluru S., Elbahnasawy M., Elboshra S., Elharrar B., Ellerbroek J., Ellingjord-Dale M., ELMagrahi H., Elmubark M. M., Elotmani L., Eloundou L., Eloy P., Elshaikhy B., Elshazly T., Elsokni W., Eltayeb A. A., Elyazar I., Emad Z. K., Embarek H., Enderle I., Endo T., Eneli G., Eng C. C., Engelmann I., Enouf V., Epaulard O., Esaadi H., Esperatti M., Esperou H., Santo C. E., Esposito-Farese M., Essaka R., Essuman L., Estevao J., Etienne M., Everding A. G., Evers M., Fabre I., Fabre M., Fadera I., Abdalla Fadlalla A. O., Faheem A., Fahy A., Fairfield C. J., Fakar Z., Fareed K., Faria P., Farooq A., Fateena H., Fathi M., Fatima S., Faure K., Favory R., Fayed M., Feely N., Fernandes J., Fernandes S., Ferrand F. -X., Devouge E. F., Ferrao J., Ferraz M., Ferreira B., Ferreira I., Ferreira S., Ferriere N., Ficko C., Figueiredo-Mello C., Finlayson W., Flament T., Fletcher T., Florence A. -M., Florio L. L., Flynn B., Flynn D., Foley J., Fomin V., Fonseca T., Fontela P., Forrest K., Forsyth S., Foster D., Foti G., Fotso B., Fourn E., Fowler R. A., Fraher M., Franch-Llasat D., Fraser C., Fraser J. F., Freire M. V., Ribeiro A. F., French C., Friedrich C., Fritz R., Fry S., Fuentes N., Fukuda M., Argin G., Gaborieau V., Gaci R., Gagliardi M., Gagnard J. -C., Gagneux-Brunon A., Gai A., Gaiao S., Skeie L. G., Galal Mohamed Ramadan A. M., Gallagher P., Gamble C., Gani Y., Garan A., Garcia R., Garcia-Diaz J., Garcia-Gallo E., Garimella N., Garot D., Garrait V., Gauli B., Gavrylov A., Gaymard A., Gebauer J., Geraud E., Morlaes L. G., Germano N., Ghemmeid M., Ghisulal P. K., Ghosn J., Giani M., Gigante T., Gilroy E., Giordano G., Girvan M., Gissot V., Giwangkancana G., Glikman D., Glybochko P., Gnall E., Goco G., Goehringer F., Goepel S., Goffard J. -C., Goh J. Y., Golacs B., Golob J., Gomez K., Gomez-Junyent J., Gominet M., Gonzalez A., Gordon P., Gorenne I., Goubert L., Goujard C., Goulenok T., Grable M., Graf J., Grandin E. W., Granier P., Grasselli G., Grazioli L., Green C. A., Greene C., Greenhalf W., Greffe S., Grieco D. L., Griffee M., Griffiths F., Grigoras I., Groenendijk A., Grovogui F. M., Gruner H., Gu Y., Guedj J., Guego M., Guerguerian A. -M., Guerreiro D., Guery R., Guillaumot A., Guilleminault L., Guimaraes de Castro M., Guimard T., Haalboom M., Haber D., Hachemi A., Haddud A., Hadri N., Hafez W., Haidri F. R., Rida Hajij F. M., Hakak S., Hall A., Halpin S., Hamdan S., Hamdi A., Hameed J., Hamer A., Hamers R. L., Hamidfar R., Hammarstrom B., Hammond N., Hammond T., Han L. Y., Hanan M., Haniffa R., Hao K. W., Hardwick H., Harrison E. M., Harrison J., Ekow Harrison S. B., Hartman A., Hasan S., Nabil Hasan M. A., Hasan M. S., Hashmi J., Hashmi M., Hassan A., Hassanin E., Hayat M., Hayes A., Hays L., Heerman J., Heggelund L., Helmi A., Hendry R., Hennessy M., Henriquez-Trujillo A. R., Hentzien M., Hernandez D., Hershey A., Hesstvedt L., Hidayah A., Higgins E., Higgins R., Hinton S., Hiraiwa H., Hirkani H., Hitoto H., Ho A., Ho Y. B., Hoctin A., Hoffmann I., Hoh W. H., Hoiting O., Holt R., Holter J. C., Horcajada J. P., Houas I., Houderi M., Hough C. L., Houltham S., Ming-Yang Hsu J., Hulot J. -S., Hurd A., Hussain I., Hussein A. M., Hussein M., Ibrahim F., Ibran B., Ijaz S., Ikram M. A., Illana C. C., Imbert P., Ansari M. I., Sikander R. I., Inacio H., Dominguez C. I., Ing Y. S., Ippolito M., Irawany V., Isgett S., Isidoro T., Ismail N., Isnard M., Istre M. S., Itai J., Ivulich D., Jaafar D., Jaafoura S., Jaber H., Jabot J., Jackson C., Jagne A., Jaureguiberry S., Jaworsky D., Jego F., Jelani A. M., Jenum S., Jimbo-Sotomayor R., Joe O. Y., Jorge Garcia R. N., Jorgensen S. B., Joseph C., Joseph M., Joshi S., Jourdain M., Jouvet P., Jung A., Jung H., Juzar D., Kafif O., Kaguelidou F., Kaisbain N., Kaleesvran T., Kali S., Kalleberg K. T., Kalomoiri S., Ayadi Kamaluddin M. A., Kamano A. S., Che Kamaruddin Z. A., Kamarudin N., Kamineni K., Kandamby D. H., Kang K. Y., Kanwal D., Kanyawati D., Karghul M., Karpayah P., Karsies T., Kasugai D., Katz K., Kay C., Kayyali L., Keating S., Kedia P., Kelly A., Kelly C., Kelly N., Kelly S., Kelly Y., Kelsey M., Kennon K., Keomany S., Kernan M., Kerroumi Y., Keshav S., Khail S., Khaled S., Khalid I., Khalil A., Khan I., Khan Q. A., Khanal S., Khatak A., Kherajani K., Kho M. E., Khoo D., Khoo R., Khoo S., Khoso M. N., Khuwaja A., Kiat K. H., Kida Y., Kiiza P., Granerud B. K., Kildal A. B., Kim J. B., Kimmoun A., Kindgen-Milles D., Kitamura N., Kjetland Kjetland E. F., Klenerman P., Klont R., Bekken G. K., Knight S. R., Kobbe R., Forson P. K., Kodippily C., Vasconcelos M. K., Koirala S., Komatsu M., Abebrese F. K., Korten V., Kouba S., Kourouma M. L., Kourouma K., Kpangon A., Krawczyk K., Kredan A., Krishnan V., Krishnan S., Kruglova O., Krund A., Kuan P. X., Kumar A., Kumar D., Kumar G., Kumar M., Kuriakose D., Kurtzman E., Kutsogiannis D., Kutsyna G., Bedu-Addo A. K., Kwedi S., Kyriakoulis K., Lachatre M., Lacoste M., Laffey J. G., Lafhej N., Lagrange M., Laine F., Lairez O., Lakhey S., Lambert M., Lamontagne F., Langelot-Richard M., Langlois V., Lantang E. Y., Lanza M., Laouenan C., Laribi S., Lariviere D., Lasry S., Lath S., Latif N., Latifeh Y., Launay O., Laureillard D., Lavie-Badie Y., Law A., Lawrence C., Lawrence T., Le M., Le Bihan C., Le Bris C., Le Falher G., Le Fevre L., Le Hingrat Q., Le Marechal M., Le Mestre S., Le Moal G., Le Moing V., Le Nagard H., Leal E., Santos M. L., Lee B. H., Lee H. G., Lee S. H., Lee T. C., Lee Y. L., Leeming G., Lefebvre B., Lefebvre L., Lefevre B., LeGac S., Lehiste M. -H., Lelievre J. -D., Lellouche F., Lemaignen A., Lemee V., Lemeur A., Lemmink G., Lene H. S., Lennon J., Leon R., Leone M., Lepik T., Lepiller Q., Lescure F. -X., Lesens O., Lesouhaitier M., Lester-Grant A., Letizia A., Letrou S., Levy B., Levy Y., Levy-Marchal C., Lewandowska K., L'Her E., Bassi G. 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E., Martinot M., Martin-Quiros A., Martins A., Martins J., Martins N., Rego C. M., Martucci G., Martynenko O., Marwali E. M., Marzukie M., Maslove D., Mason S., Masood S., Masoud F., Massoma M., Masumbe P., Mat Nor M. B., Matan M., Fernandes H. M., Mathew M., Mathew C., Mattei M., Maulin L., May J., Maynar J., Mayxay M., Mazzoni T., Sweeney L. M., McArthur C., McCann N., McCanny P., McCarthy A., McCloskey C., McConnochie R., McDermott S., McDonald S. E., McElroy A., McElwee S., McEvoy N., McGeer A., McLean K. A., McNally P., McNicholas B., Meaney E., Mear-Passard C., Mechlin M., Medombou N., Mehkri O., Mele F., Melo L., Memon K. A., Mendes J. J., Menkiti O., Menon K., Mentre F., Mentzer A. J., Mercier E., Mercier N., Merckx A., Mergeay-Fabre M., Mergler B., Mesquita A., Meta R., Metwally O., Meybeck A., Meyer D., Meynert A. M., Meysonnier V., Mezidi M., Michelanglei C., Michelet I., Mihelis E., Mihnovit V., Abdullah D. M., Miller J., Miranda-Maldonado H., Misnan N. A., Eliza Mohamed N. N., Mohamed N., Mohamed T. J., Ads A. M., Mohamed Elsayed Abdelhalim A. R., Mohammed L., Mohammed Mostafa S. F., Abdelrahman Mohammedahmed M. O., Mohammedelhassan O. A., Moin A., Mokhtar W., Molinos E., Molloy B., Mone M., Monteiro A., Montes C., Montrucchio G., Moore S., Moore S. C., Cely L. M., Morgom M., Moro L., Motherway C., Motos A., Mouquet H., Perrot C. M., Moyet J., Mualla S. H., Muftah M., Mufti A. K., Muh N. Y., Muhaisen M., Muhamad D., Mullaert J., Muller F., Muller K. E., Munblit D., Ali S. M., Munir N., Munshi L., Murphy A., Murray P., Murris M., Murthy S., Musaab H., Mustafa A., Mustafa M., Mustafa D., Muvindi H., Myrodia D. M., Mohd-Hanafiah F. N., Nadjm B., Nagpal D., Nagrebetsky A., Nagybanyai-Nagy B., Boudoin H. N., Narasimhan M., Narayanan N., Nasa P., Khan R. N., Nasrallah A., Nassif Metri A. G., Nazerali-Maitland A., Neant N., Neb H., Nekliudov N., Nelder M., Nelwan E., Neto R., Neumann E., Ng W. Y., Ng P. Y., Nghi A., Nguyen D., Choileain O. N., Leathlobhair N. N., Niba N., Nichol A. D., Nitayavardhana P., Nonas S., Mohd Noordin N. A., Izzati Norharizam N. F., North A., Notari A., Noursadeghi M., Nowinski A., Nseir S., Numfor L., Nurnaningsih N., Nusantara D. U., Nyamankolly E., Nygaard A. B., Brien F. O., Callaghan A. O., O'Callaghan A., Occhipinti G., OConnor D., O'Donnell M., Ofori-Boadu L., Ogston T., Ogura T., Oh T. -H., O'Halloran S., O'Hearn K., Ohene S. -A., Oliveira J., Oliveira L., Olliaro P. L., Rageh Elnaggar C. O., Mohammed Omer A. A., Ondobo P., Ong D. S. Y., Ong J. Y., Oosthuyzen W., Opavsky A., Openshaw P., Orakzai S., Orozco-Chamorro C. M., Ortoleva J., Elsayed Soliman M. O., Osatnik J., O'Shea L., O'Sullivan M., Othman E., Othman S. Z., Ouamara N., Ouissa R., Owusu M., Owusu-Asare A. A., Oziol E., Pagadoy M., Pages J., Palacios A., Palmarini M., Panarello G., Paneru H., Pang L. H., Panigada M., Pansu N., Papadopoulos A., Parke R., Parker M., Pasquier J., Pastene B., Patauner F., Patel D., Pathmanathan M. D., Patrao L., Patricio P., Patterson L., Pattnaik R., Paul C., Paul M., Paulos J., Paxton W. A., Payen J. -F., Peake S. L., Peariasamy K., Peek G. J., Peelman F., Peiffer-Smadja N., Peigne V., Pejkovska M., Pelosi P., Peltan I. D., Pereira R., Perez D., Perpoint T., Pesenti A., Pestre V., Petrou L., Petrovic M., Petrov-Sanchez V., Pettersen F. O., Peytavin G., Philips R. O., Phonemixay O., Phoutthavong S., Piagnerelli M., Picard W., Picone O., de Piero M., Piersma D., Pimentel C., Pinto R., Pires C., Piroth L., Pitaloka A., Piubelli C., Pius R., Piva S., Plantier L., Png H. S., Poissy J., Pokeerbux R., Poli S., Pollakis G., Ponscarme D., Porto D. B., Post A. -M., Postma D. F., Povoa P., Povoas D., Powis J., Prapa S., Praphasiri V., Preau S., Prebensen C., Preiser J. -C., Prinssen A., Dilanthi Priyadarshani G. D., Proenca L., Pudota S., Semedi B. 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M., Botelho-Nevers E., Bouadma L., Bouchaud O., Bouchez S., Bouhour D., Bouiller K., Bouillet L., Bouisse C., Bountthasavong L., Boureau A. -S., Bourke J., Bouscambert M., Bousquet A., Boyer-Besseyre M., Boylan M., Bozza F. A., Braconnier A., Braga C., Brandenburger T., Monteiro F. B., Brazzi L., Breen D., Breen P., Brewster D., Brickell K., Broadley T., Brotherton H., Browne A., Brozzi N., Brunvoll S. H., Brusse-Keizer M., Bryda P., Buchtele N., Bugaeva P., Buisson M., Buonsenso D., Burhan E., Buri D., Burrell A., Bustos I. G., Butnaru D., Cabie A., Cabral S., Cabrita J., Caceres E., Cadoz C., Garces R. C., Calligy K., Calvache J. A., Camoes J., Campana V., Campbell P., Campisi J., Canepa C., Cantero M., Caoili J., Caraux-Paz P., Carcel S., Cardoso F., Cardoso N., Cardoso S., Carelli S., Carlier N., Carmoi T., Carney G., Carqueja I., Carret M. -C., Carrier F. M., Carroll I., Carson G., Casanova M. -L., Cascao M., Casey S., Casimiro J., Cassandra B., Castaneda S., Castanheira N., Castor-Alexandre G., Castro I., Catarino A., Catherine F. -X., Cattaneo P., Cavalin R., Cavalli G. G., Cavayas A., Ceccato A., Ceesay M., Cerkovnik S., Cervantes-Gonzalez M., Cevik M., Chair A., Chakveatze C., Chan A., Chand M., Chapplain J. -M., Charpentier C., Chas J., Chaudry M. M., Chavez Iniguez J. S., Chen A., Chen Y. -S., Chenard L., Cheng M. P., Cheret A., Chiarabini T., Chica J., Chidambaram S. K., Tho L. C., Chirouze C., Chiumello D., Cho S. -M., Cholley B., Chommanam D., Chopin M. -C., Chow Y. P., Chow T. S., Christy N., Chua H. J., Chua J., Cidade J. P., Cisneros Herreros J. M., Ciullo A., Clarke J., Claure-Del Granado R., Clohisey S., Codan C., Cody C., Coles J., Coles M., Colin G., Collins M., Combs P., Connolly J., Connor M., Conrad A., Conway E., Cooke G. S., Cordel H., Corley A., Cornelis S., Cornet A. D., Corpuz A. J., Cortegiani A., Corvaisier G., Couffignal C., Couffin-Cadiergues S., Courtois R., Cousse S., Cowan J., Cregan R., Crowl G., Crump J., Cruz C., Csete M., Cullen A., Cummings M., Curley G., Curlier E., Curran C., Custodio P., da Silva Filipe A., Da Silveira C., Dabaliz A. -A., Dahl J. A., Dahly D., D'Alessandro U., Daley P., Dalloul Z., Dalton H., Dalton J., Daly S., Damas J., Dame J., Damien C., Daneman N., Dantas J., D'Aragon F., de Loughry G., de Mendoza D., De Montmollin E., Franca R. F. D. O., Isabel de Pinho Oliveira A., De Rosa R., De Rose C., de Silva T., de Vries P., Deacon J., Dean D., Debard A., DeBenedictis B., Debray M. -P., DeCastro N., Dechert W., Decours R., Defous E., Delacroix I., Delamou A., Delaveuve E., Delavigne K., Delfos N. M., Deligiannis I., Dell'Amore A., Delmas C., Delobel P., Delsing C., Demonchy E., Denis E., Deplanque D., Depuydt P., Descamps D., Desvallees M., Dewayanti S., Dhangar P., Diallo A., Diallo S. T., Diamantis S., Dias A., Da Silva F. D., Diaz R., Diaz J. J., Diaz P., Dibba B. K., Didier K., Diehl J. -L., Dieperink W., Dimet J., Dinot V., Diop F., Diouf A., Dishon Y., Djadda C., Djossou F., Docherty A. B., Doherty H., Dondorp A. M., Donnelly C. A., Donohue Y., Donohue S., Doran P., Dorival C., D'Ortenzio E., Doshi Y., Douangdala P., Douglas J. J., Douma R., Dournon N., Downey J., Downing M., Drake T., Driscoll A., Duah I. K., Fonseca C. D., Dubee V., Dubos F., Dubot-Peres A., Ducancelle A., Duculan T., Dudman S., Duggal A., Dunand P., Duplaix M., Durante-Mangoni E., Durham L., Dussol B., Duthoit J., Duval X., Dyrhol-Riise A. M., Ean S. C., Ebo A., Echeverria-Villalobos M., Edelstein M., Egan S., Eggesbo L. M., Ehzaz K., Eira C., El Sanharawi M., El Sayed M., Elabid M., Elagili M. B., Elapavaluru S., Elbahnasawy M., Elboshra S., Elharrar B., Ellerbroek J., Ellingjord-Dale M., ELMagrahi H., Elmubark M. M., Elotmani L., Eloundou L., Eloy P., Elshaikhy B., Elshazly T., Elsokni W., Eltayeb A. A., Elyazar I., Emad Z. K., Embarek H., Enderle I., Endo T., Eneli G., Eng C. C., Engelmann I., Enouf V., Epaulard O., Esaadi H., Esperatti M., Esperou H., Santo C. E., Esposito-Farese M., Essaka R., Essuman L., Estevao J., Etienne M., Everding A. G., Evers M., Fabre I., Fabre M., Fadera I., Abdalla Fadlalla A. O., Faheem A., Fahy A., Fairfield C. J., Fakar Z., Fareed K., Faria P., Farooq A., Fateena H., Fathi M., Fatima S., Faure K., Favory R., Fayed M., Feely N., Fernandes J., Fernandes S., Ferrand F. -X., Devouge E. F., Ferrao J., Ferraz M., Ferreira B., Ferreira I., Ferreira S., Ferriere N., Ficko C., Figueiredo-Mello C., Finlayson W., Flament T., Fletcher T., Florence A. -M., Florio L. L., Flynn B., Flynn D., Foley J., Fomin V., Fonseca T., Fontela P., Forrest K., Forsyth S., Foster D., Foti G., Fotso B., Fourn E., Fowler R. A., Fraher M., Franch-Llasat D., Fraser C., Fraser J. F., Freire M. V., Ribeiro A. F., French C., Friedrich C., Fritz R., Fry S., Fuentes N., Fukuda M., Argin G., Gaborieau V., Gaci R., Gagliardi M., Gagnard J. -C., Gagneux-Brunon A., Gai A., Gaiao S., Skeie L. G., Galal Mohamed Ramadan A. M., Gallagher P., Gamble C., Gani Y., Garan A., Garcia R., Garcia-Diaz J., Garcia-Gallo E., Garimella N., Garot D., Garrait V., Gauli B., Gavrylov A., Gaymard A., Gebauer J., Geraud E., Morlaes L. G., Germano N., Ghemmeid M., Ghisulal P. K., Ghosn J., Giani M., Gigante T., Gilroy E., Giordano G., Girvan M., Gissot V., Giwangkancana G., Glikman D., Glybochko P., Gnall E., Goco G., Goehringer F., Goepel S., Goffard J. -C., Goh J. Y., Golacs B., Golob J., Gomez K., Gomez-Junyent J., Gominet M., Gonzalez A., Gordon P., Gorenne I., Goubert L., Goujard C., Goulenok T., Grable M., Graf J., Grandin E. W., Granier P., Grasselli G., Grazioli L., Green C. A., Greene C., Greenhalf W., Greffe S., Grieco D. L., Griffee M., Griffiths F., Grigoras I., Groenendijk A., Grovogui F. M., Gruner H., Gu Y., Guedj J., Guego M., Guerguerian A. -M., Guerreiro D., Guery R., Guillaumot A., Guilleminault L., Guimaraes de Castro M., Guimard T., Haalboom M., Haber D., Hachemi A., Haddud A., Hadri N., Hafez W., Haidri F. R., Rida Hajij F. M., Hakak S., Hall A., Halpin S., Hamdan S., Hamdi A., Hameed J., Hamer A., Hamers R. L., Hamidfar R., Hammarstrom B., Hammond N., Hammond T., Han L. Y., Hanan M., Haniffa R., Hao K. W., Hardwick H., Harrison E. M., Harrison J., Ekow Harrison S. B., Hartman A., Hasan S., Nabil Hasan M. A., Hasan M. S., Hashmi J., Hashmi M., Hassan A., Hassanin E., Hayat M., Hayes A., Hays L., Heerman J., Heggelund L., Helmi A., Hendry R., Hennessy M., Henriquez-Trujillo A. R., Hentzien M., Hernandez D., Hershey A., Hesstvedt L., Hidayah A., Higgins E., Higgins R., Hinton S., Hiraiwa H., Hirkani H., Hitoto H., Ho A., Ho Y. B., Hoctin A., Hoffmann I., Hoh W. H., Hoiting O., Holt R., Holter J. C., Horcajada J. P., Houas I., Houderi M., Hough C. L., Houltham S., Ming-Yang Hsu J., Hulot J. -S., Hurd A., Hussain I., Hussein A. M., Hussein M., Ibrahim F., Ibran B., Ijaz S., Ikram M. A., Illana C. C., Imbert P., Ansari M. I., Sikander R. I., Inacio H., Dominguez C. I., Ing Y. S., Ippolito M., Irawany V., Isgett S., Isidoro T., Ismail N., Isnard M., Istre M. S., Itai J., Ivulich D., Jaafar D., Jaafoura S., Jaber H., Jabot J., Jackson C., Jagne A., Jaureguiberry S., Jaworsky D., Jego F., Jelani A. M., Jenum S., Jimbo-Sotomayor R., Joe O. Y., Jorge Garcia R. N., Jorgensen S. B., Joseph C., Joseph M., Joshi S., Jourdain M., Jouvet P., Jung A., Jung H., Juzar D., Kafif O., Kaguelidou F., Kaisbain N., Kaleesvran T., Kali S., Kalleberg K. T., Kalomoiri S., Ayadi Kamaluddin M. A., Kamano A. S., Che Kamaruddin Z. A., Kamarudin N., Kamineni K., Kandamby D. H., Kang K. Y., Kanwal D., Kanyawati D., Karghul M., Karpayah P., Karsies T., Kasugai D., Katz K., Kay C., Kayyali L., Keating S., Kedia P., Kelly A., Kelly C., Kelly N., Kelly S., Kelly Y., Kelsey M., Kennon K., Keomany S., Kernan M., Kerroumi Y., Keshav S., Khail S., Khaled S., Khalid I., Khalil A., Khan I., Khan Q. A., Khanal S., Khatak A., Kherajani K., Kho M. E., Khoo D., Khoo R., Khoo S., Khoso M. N., Khuwaja A., Kiat K. H., Kida Y., Kiiza P., Granerud B. K., Kildal A. B., Kim J. B., Kimmoun A., Kindgen-Milles D., Kitamura N., Kjetland Kjetland E. F., Klenerman P., Klont R., Bekken G. K., Knight S. R., Kobbe R., Forson P. K., Kodippily C., Vasconcelos M. K., Koirala S., Komatsu M., Abebrese F. K., Korten V., Kouba S., Kourouma M. L., Kourouma K., Kpangon A., Krawczyk K., Kredan A., Krishnan V., Krishnan S., Kruglova O., Krund A., Kuan P. X., Kumar A., Kumar D., Kumar G., Kumar M., Kuriakose D., Kurtzman E., Kutsogiannis D., Kutsyna G., Bedu-Addo A. K., Kwedi S., Kyriakoulis K., Lachatre M., Lacoste M., Laffey J. G., Lafhej N., Lagrange M., Laine F., Lairez O., Lakhey S., Lambert M., Lamontagne F., Langelot-Richard M., Langlois V., Lantang E. Y., Lanza M., Laouenan C., Laribi S., Lariviere D., Lasry S., Lath S., Latif N., Latifeh Y., Launay O., Laureillard D., Lavie-Badie Y., Law A., Lawrence C., Lawrence T., Le M., Le Bihan C., Le Bris C., Le Falher G., Le Fevre L., Le Hingrat Q., Le Marechal M., Le Mestre S., Le Moal G., Le Moing V., Le Nagard H., Leal E., Santos M. L., Lee B. H., Lee H. G., Lee S. H., Lee T. C., Lee Y. L., Leeming G., Lefebvre B., Lefebvre L., Lefevre B., LeGac S., Lehiste M. -H., Lelievre J. -D., Lellouche F., Lemaignen A., Lemee V., Lemeur A., Lemmink G., Lene H. S., Lennon J., Leon R., Leone M., Lepik T., Lepiller Q., Lescure F. -X., Lesens O., Lesouhaitier M., Lester-Grant A., Letizia A., Letrou S., Levy B., Levy Y., Levy-Marchal C., Lewandowska K., L'Her E., Bassi G. L., Liang J., Liaquat A., Liegeon G., Lim K. C., Lim W. S., Lima C., Lina B., Lina L., Lind A., Lingad M. K., Lingas G., Lion-Daolio S., Liu K., Livrozet M., Lizotte P., Loforte A., Lolong N., Loon L. C., Lopes D., Lopez-Colon D., Loschner A. L., Loubet P., Loufti B., Louis G., Lourenco S., Lovelace-Macon L., Lee Low L., Lowik M., Loy J. S., Lucet J. C., Luna C. M., Lungu O., Lunn M., Luong L., Luque N., Luton D., Maasikas O., Machado M., Machado S., Macheda G., Magzoub M., Mahieu R., Mahy S., Maia A. R., Maier L. S., Ascofare O. M., Maillet M., Maitre T., Majeed N. A., Malfertheiner M., Malik N., Mallon P., Maltez F., Malvy D., Manda V., Mandelbrot L., Manetta F., Mankikian J., Manning E., Manuel A., Maraczi V., Sant'Ana Malaque C. M., Marino F., Markowicz S., Marques A., Marquis C., Marsh L., Marsh B., Marshal M., Marshall J., Martelli C. T., Martin D. -A., Martin E., Martin-Blondel G., Martinelli A., Martinez F. E., Martinot M., Martin-Quiros A., Martins A., Martins J., Martins N., Rego C. M., Martucci G., Martynenko O., Marwali E. M., Marzukie M., Maslove D., Mason S., Masood S., Masoud F., Massoma M., Masumbe P., Mat Nor M. B., Matan M., Fernandes H. M., Mathew M., Mathew C., Mattei M., Maulin L., May J., Maynar J., Mayxay M., Mazzoni T., Sweeney L. M., McArthur C., McCann N., McCanny P., McCarthy A., McCloskey C., McConnochie R., McDermott S., McDonald S. E., McElroy A., McElwee S., McEvoy N., McGeer A., McLean K. A., McNally P., McNicholas B., Meaney E., Mear-Passard C., Mechlin M., Medombou N., Mehkri O., Mele F., Melo L., Memon K. A., Mendes J. J., Menkiti O., Menon K., Mentre F., Mentzer A. J., Mercier E., Mercier N., Merckx A., Mergeay-Fabre M., Mergler B., Mesquita A., Meta R., Metwally O., Meybeck A., Meyer D., Meynert A. M., Meysonnier V., Mezidi M., Michelanglei C., Michelet I., Mihelis E., Mihnovit V., Abdullah D. M., Miller J., Miranda-Maldonado H., Misnan N. A., Eliza Mohamed N. N., Mohamed N., Mohamed T. J., Ads A. M., Mohamed Elsayed Abdelhalim A. R., Mohammed L., Mohammed Mostafa S. F., Abdelrahman Mohammedahmed M. O., Mohammedelhassan O. A., Moin A., Mokhtar W., Molinos E., Molloy B., Mone M., Monteiro A., Montes C., Montrucchio G., Moore S., Moore S. C., Cely L. M., Morgom M., Moro L., Motherway C., Motos A., Mouquet H., Perrot C. M., Moyet J., Mualla S. H., Muftah M., Mufti A. K., Muh N. Y., Muhaisen M., Muhamad D., Mullaert J., Muller F., Muller K. E., Munblit D., Ali S. M., Munir N., Munshi L., Murphy A., Murray P., Murris M., Murthy S., Musaab H., Mustafa A., Mustafa M., Mustafa D., Muvindi H., Myrodia D. M., Mohd-Hanafiah F. N., Nadjm B., Nagpal D., Nagrebetsky A., Nagybanyai-Nagy B., Boudoin H. N., Narasimhan M., Narayanan N., Nasa P., Khan R. N., Nasrallah A., Nassif Metri A. G., Nazerali-Maitland A., Neant N., Neb H., Nekliudov N., Nelder M., Nelwan E., Neto R., Neumann E., Ng W. Y., Ng P. Y., Nghi A., Nguyen D., Choileain O. N., Leathlobhair N. N., Niba N., Nichol A. D., Nitayavardhana P., Nonas S., Mohd Noordin N. A., Izzati Norharizam N. F., North A., Notari A., Noursadeghi M., Nowinski A., Nseir S., Numfor L., Nurnaningsih N., Nusantara D. U., Nyamankolly E., Nygaard A. B., Brien F. O., Callaghan A. O., O'Callaghan A., Occhipinti G., OConnor D., O'Donnell M., Ofori-Boadu L., Ogston T., Ogura T., Oh T. -H., O'Halloran S., O'Hearn K., Ohene S. -A., Oliveira J., Oliveira L., Olliaro P. L., Rageh Elnaggar C. O., Mohammed Omer A. A., Ondobo P., Ong D. S. Y., Ong J. Y., Oosthuyzen W., Opavsky A., Openshaw P., Orakzai S., Orozco-Chamorro C. M., Ortoleva J., Elsayed Soliman M. O., Osatnik J., O'Shea L., O'Sullivan M., Othman E., Othman S. Z., Ouamara N., Ouissa R., Owusu M., Owusu-Asare A. A., Oziol E., Pagadoy M., Pages J., Palacios A., Palmarini M., Panarello G., Paneru H., Pang L. H., Panigada M., Pansu N., Papadopoulos A., Parke R., Parker M., Pasquier J., Pastene B., Patauner F., Patel D., Pathmanathan M. D., Patrao L., Patricio P., Patterson L., Pattnaik R., Paul C., Paul M., Paulos J., Paxton W. A., Payen J. -F., Peake S. L., Peariasamy K., Peek G. J., Peelman F., Peiffer-Smadja N., Peigne V., Pejkovska M., Pelosi P., Peltan I. D., Pereira R., Perez D., Perpoint T., Pesenti A., Pestre V., Petrou L., Petrovic M., Petrov-Sanchez V., Pettersen F. O., Peytavin G., Philips R. O., Phonemixay O., Phoutthavong S., Piagnerelli M., Picard W., Picone O., de Piero M., Piersma D., Pimentel C., Pinto R., Pires C., Piroth L., Pitaloka A., Piubelli C., Pius R., Piva S., Plantier L., Png H. S., Poissy J., Pokeerbux R., Poli S., Pollakis G., Ponscarme D., Porto D. B., Post A. -M., Postma D. F., Povoa P., Povoas D., Powis J., Prapa S., Praphasiri V., Preau S., Prebensen C., Preiser J. -C., Prinssen A., Dilanthi Priyadarshani G. D., Proenca L., Pudota S., Semedi B. P., Pulicken M., Puplampu P., Purcell G., Quesada L., Quinones-Cardona V., Quist-Paulsen E., Quraishi M., Qutishat F., Rabaa M., Rabaud C., Rabindrarajan E., Rafael A., Rafiq M., Ragab A., Rahardjani M., Ullah A. R., Haji Ab Rahman A. K., Rahman R. A., Rainieri F., Rajahram G. S., Ramachandran P., Ramakrishnan N., Ramalho J., Ramli A. A., Rammaert B., Ramos G. V., Rana A., Rangappa R., Ranjan R., Rapp C., Rashan A., Rashan T., Rasheed G., Rasmin M., Ratsep I., Rau C., Ravi T., Raza A., Real A., Rebaudet S., Redl S., Reeve B., Rehman A., Rehman Khalid M. O., Reikvam D. H., Reis R., Remppis J., Remy M., Ren H., Renk H., Resseguier A. -S., Revest M., Rewa O., Ribeiro M. I., Ricchiuto A., Richardson D., Richier L., Atikah Ahmad Ridzuan S. N., Rios A. L., Rishu A., Rispal P., Risso K., Rivera Nunez M. A., Robba C., Roberto A., Roberts S., Roberts C., Robertson D. L., Robineau O., Roca A., Roche-Campo F., Rodari P., Rodeia S., Roessler B., Roger C., Roger P. -M., Roncon-Albuquerque R., Roriz M., Rosa-Calatrava M., Rose M., Rosenberger D., Rossanese A., Rossetti M., Rossignol P., Roy C., Roze B., Rusmawatiningtyas D., Russell C. D., Ryan M., Ryckaert S., Holten A. R., Saba I., Sadaf S., Sadat M., Sahraei V., Said A., Saidani N., Sakiyalak P., Sako F. B., Salah M., Salah Eldin Mohamed Abbas A. A., Salahuddin N., Salazar L., Saleem J., Alyasiri M. S., Abu Salem T. A., Sales G., Gandonniere C. S., Salvator H., Samardali D., Samardali S., Shaaban Aly Orabi Y. S., Sanchez E., Sanchez O., Sanchez de Oliveira K., Sanchez-Miralles A., Sancho-Shimizu V., Sandhu G., Sandhu Z., Sandrine P. -F., Sandulescu O., Santos M., Sarfo-Mensah S., Banheiro B. S., Sarmiento I. C. E., Sarton B., Satya A., Satyapriya S., Satyawati R., Saviciute E., Saw Y. T., Schaffer J., Schermer T., Scherpereel A., Schneider M., Schnur J., Schroll S., Schwameis M., Schwartz G., Scott J. T., Scott-Brown J., Sedillot N., Seitz T., Selvanayagam J., Selvarajoo M., Semple M. G., Senian R. B., Senneville E., Sepulveda C., Sequeira F., Sequeira T., Neto A. S., Shadowitz E., Shahidan S. A., Shahla H., Shalabi L., Shames H., Shankar A., Sharjeel S., Sharma P., Shaw C. A., Shaw V., Sheenan J. R., Mohan Shetty D. R., Shetty R., Shiekh M., Shime N., Shimizu K., Shrapnel S., Shrestha S. K., Shrestha P. S., Shum H. P., Mohammed N. S., Siang N. Y., Siaw-Frimpong M., Sibiude J., Sibounheuang B., Siddig N., Siddiqui A., Siddiqui M. A., Sigfrid L., Sillah F., Sillaots P., Silva C., Silva M. J., Silva R., Lim Heng B. S., Sin W. C., Sinatti D., Singh M., Singh P., Sitompul P. A., Sivam K., Skogen V., Smith S., Smood B., Smyth C., Snacken M., So D., Soh T. V., Solberg L. B., Solomon J., Solomon T., Somers E., Sommet A., Song M. J., Song R., Song T., Chia J. S., Soraas A., Sotto A., Soum E., Sousa A. C., Sousa M., Uva M. S., Souza-Dantas V., Sow M. S., Sperry A., Spinuzza E., Ruwan Sri Darshana B. P. S., Sriskandan S., Stabler S., Staudinger T., Stecher S. -S., Steinsvik T., Stienstra Y., Stiksrud B., Stolz E., Stone A., Streinu-Cercel A., Strong G., Stuart A., Stuart D., Su R., Subekti D., Suen G., Suen J. Y., Sukumar P., Sultana A., Summers C., Supic D., Suppiah D., Surovcova M., Suwarti A., Svistunov A., Syahrin S., Sylverken A., Syrigos K., Sztajnbok J., Szuldrzynski K., Tabrizi S., Taccone F. S., Tagherset L., Taib S. M., Taleb S., Talla C., Talsma J., Tamisier R., Tampubolon M. L., Tan K. K., Tan Y. C., Tanaka H., Tanaka T., Taniguchi H., Taqdees H., Taqi A., Tardivon C., Kamal Mostafa Y. T., Tarhabat A., Tattevin P., Taufik M. A., Tawfik H., Tee T. Y., Teixeira J., Tejada S., Tellier M. -C., Teoh S. K., Teotonio V., Teoule F., Terrier O., Terzi N., Tessier-Grenier H., Tey A., Mohd Thabit A. A., Thakur A., Tham Z. D., Thangavelu S., Theron E., Thibault V., Thiberville S. -D., Thill B., Thirumanickam J., Thompson N., Thompson S., Thomson E. C., Thomson D., Thorpe M., Thurai S. R. T., Thwaites R. S., Tierney P., Tieroshyn V., Timashev P. S., Timsit J. -F., Tissot N., Toal F., Yang Toh J. Z., Toki M., Tonby K., Tonnii S. L., Torre M., Torres A., Torres M., Santos-Olmo R. M. T., Torres-Zevallos H., Tounkara A., Towers M., Traore F. A., Trapani T., Tromeur C., Trontzas I., Trouillon T., Truong J., Tual C., Tubiana S., Tuite H., Turgeon A. F., Turmel J. -M., Turtle L. C. W., Tveita A., Twardowski P., Uchiyama M., Udayanga P. I., Udy A., Ullrich R., Uribe A., Usman A., Usuf E., Uyeki T. M., Vajdovics C., Valentini P., Val-Flores L., Van de Velde S., van den Berge M., van der Feltz M., van der Palen J., van der Valk P., Van Der Vekens N., Van der Voort P., Van Der Werf S., van Gulik L., Van Hattem J., van Netten C., van Veen I., Vanel N., Vanoverschelde H., Varrone M., Vasudayan S. R., Vauchy C., Vecham P. K., Veeran S., Veislinger A., Vencken S., Ventura S., Verbon A., Vidal J. E., Vieira C., Vijayan D., Villar J., Villeneuve P. -M., Villoldo A., Vishwanathan G., Visseaux B., Visser H., Vitiello C., Vongsouvath M., Vonkeman H., Vuotto F., Wahab S. A., Wahab N. H., Wahid N. A., Wainstein M., Walsh L., Shukeri W. F. W. M., Wang C. -H., Webb S., Weil K., Wen T. P., Wesam H., Wesselius S., West T. E., Wham M., Whelan B., White N., Wicky P. H., Wiedemann A., Wijaya S. O., Wille K., Willems S., Williams B., Williams P. J., Williams V., Wittman J., Wong C., Wong X. C., Wong Y. S., Wong T. F., Wright N., Xian L. S., Xynogalas I., Binti Mohd Yakop S. R., Yamazaki M., Yarad E., Yazdanpanah Y., Hing N. Y. L., Mahmoud Abdelaal A. Y., Yelnik C., Yeoh C. H., Yerkovich S., Yiaye T., Yokoyama T., Yonis H., Yousif O., Yuliarto S., Zaaqoq A., Zabbe M., Zabert G. E., Zacharowski K., Zahid M., Zahran M., Binti Zaidan N. Z., Zambon M., Zambrano M., Zanella A., Zaynah N., Zayyad H., Zoufaly A., and Zucman D.
- Abstract
Background: COVID-19 is primarily known as a respiratory illness; however, many patients present to hospital without respiratory symptoms. The association between non-respiratory presentations of COVID-19 and outcomes remains unclear. We investigated risk factors and clinical outcomes in patients with no respiratory symptoms (NRS) and respiratory symptoms (RS) at hospital admission. Methods: This study describes clinical features, physiological parameters, and outcomes of hospitalised COVID-19 patients, stratified by the presence or absence of respiratory symptoms at hospital admission. RS patients had one or more of: cough, shortness of breath, sore throat, runny nose or wheezing; while NRS patients did not. Results: Of 178,640 patients in the study, 86.4 % presented with RS, while 13.6 % had NRS. NRS patients were older (median age: NRS: 74 vs RS: 65) and less likely to be admitted to the ICU (NRS: 36.7 % vs RS: 37.5 %). NRS patients had a higher crude in-hospital case-fatality ratio (NRS 41.1 % vs. RS 32.0 %), but a lower risk of death after adjusting for confounders (HR 0.88 [0.83–0.93]). Conclusion: Approximately one in seven COVID-19 patients presented at hospital admission without respiratory symptoms. These patients were older, had lower ICU admission rates, and had a lower risk of in-hospital mortality after adjusting for confounders.
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- 2024
19. Effect of metering systems and drying methods on the barrier properties of paper coated with multiple layers of cellulose nanofibres
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Agencia Estatal de Investigación (España), Ministerio de Ciencia e Innovación (España), Comunidad de Madrid, Universidade de Coimbra, Gómez Hernández, Nuria [0000-0002-0797-6474], Vergara, Priscilla [0000-0003-2876-649X], Fillat, Ursula [0000-0002-8512-0356], Villar, J. C. [0000-0001-6850-9792], Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72], Gómez Hernández, Nuria, Vergara, Priscilla, Fillat, Ursula, Villar, J. C., Agencia Estatal de Investigación (España), Ministerio de Ciencia e Innovación (España), Comunidad de Madrid, Universidade de Coimbra, Gómez Hernández, Nuria [0000-0002-0797-6474], Vergara, Priscilla [0000-0003-2876-649X], Fillat, Ursula [0000-0002-8512-0356], Villar, J. C. [0000-0001-6850-9792], Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72], Gómez Hernández, Nuria, Vergara, Priscilla, Fillat, Ursula, and Villar, J. C.
- Abstract
Developing environmentally friendly barrier coatings as an alternative to petroleum-based polymer packaging is a challenge. Cellulose nanofibres (CNF) films have exhibited great potential as water and gas barrier layers. Recycled paper was multi-layer coated with three commercial CNF (mechanical (M-CNF), TEMPO (T-CNF) and carboxymethylated (C-CNF)) using two metering systems (wound rod and blade micrometer) and two drying methods (tension-free contact drying and air drying). The coatability and rheological behaviour of the CNF suspensions were analysed. The gas, water and grease barrier properties of the CNF coated papers were determined and compared with the results of paper coated with cationic starch. The three CNF suspensions and the starch suspension were successfully coated using both metering systems. In the multi-layer coating, air drying yielded higher coat weights than contact drying, and the difference was more noticeable in M-CNF and T-CNF coated samples. A lack of uniformity observed in CNF coatings increased with the number of coating layers. M-CNF coated samples had a whitish surface with a uniform appearance, but coating was insufficiently compact to provide barrier properties. T-CNF coating exhibited a cracked surface and consequently provided no barrier properties. Drying stresses caused breakage of T-CNF coating, which could be explained by the drop in apparent viscosity at much lower rheological shear stresses in the T-CNF suspension. C-CNF showed successful coatability and provided barrier properties to paper with both metering systems and drying methods. Air permeance decreased considerably and the water wettability of the paper decreased by 60% compared to the reference paper, even with a single coating layer (about 1 g·m−2). In addition, a greaseproof paper (grease resistance >1800 s and kit no >10) was obtained with multi-layer C-CNF coating. Although water vapour permeability at 90 % RH and 20 °C decreased slightly with a single layer of CN
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- 2024
20. The ANAIS-112 experiment at the Canfranc Underground Laboratory
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Amare, J, Cebrian, S, Coarasa, I, Cuesta, C, Garcia, E, Martinez, M, Olivan, M A, Ortigoza, Y, de Solorzano, A Ortiz, Puimedon, J, Salinas, A, Sarsa, M L, Villar, P, and Villar, J A
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Physics - Instrumentation and Detectors ,Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment - Abstract
The ANAIS experiment aims at the confirmation of the DAMA/LIBRA signal at the Canfranc Underground Laboratory (LSC). Several 12.5 kg NaI(Tl) modules produced by Alpha Spectra Inc. have been operated there during the last years in various set-ups; an outstanding light collection at the level of 15 photoelectrons per keV, which allows triggering at 1 keV of visible energy, has been measured for all of them and a complete characterization of their background has been achieved. In the first months of 2017, the full ANAIS-112 set-up consisting of nine Alpha Spectra detectors with a total mass of 112.5 kg was commissioned at LSC and the first dark matter run started in August, 2017. Here, the latest results on the detectors performance and measured background from the commissioning run will be presented and the sensitivity prospects of the ANAIS-112 experiment will be discussed., Comment: To appear in the Proceedings of the XV International Conference on Topics in Astroparticle and Underground Physics (TAUP2017) at Journal of Physics: Conference Series (JPCS)
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- 2017
21. Cosmogenic production of tritium in dark matter detectors
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Amare, J., Castel, J., Cebrian, S., Coarasa, I., Cuesta, C., Dafni, T., Galan, J., Garcia, E., Garza, J. G., Iguaz, F. J., Irastorza, I. G., Luzon, G., Martinez, M., Mirallas, H., Olivan, M. A., Ortigoza, Y., de Solorzano, A. Ortiz, Puimedon, J., Ruiz-Choliz, E., Sarsa, M. L., Villar, J. A., and Villar, P.
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Physics - Instrumentation and Detectors ,Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment - Abstract
The direct detection of dark matter particles requires ultra-low background conditions at energies below a few tens of keV. Radioactive isotopes are produced via cosmogenic activation in detectors and other materials and those isotopes constitute a background source which has to be under control. In particular, tritium is specially relevant due to its decay properties (very low endpoint energy and long half-life) when induced in the detector medium, and because it can be generated in any material as a spallation product. Quantification of cosmogenic production of tritium is not straightforward, neither experimentally nor by calculations. In this work, a method for the calculation of production rates at sea level has been developed and applied to some of the materials typically used as targets in dark matter detectors (germanium, sodium iodide, argon and neon); it is based on a selected description of tritium production cross sections over the entire energy range of cosmic nucleons. Results have been compared to available data in the literature, either based on other calculations or from measurements. The obtained tritium production rates, ranging from a few tens to a few hundreds of nuclei per kg and per day at sea level, point to a significant contribution to the background in dark matter experiments, requiring the application of specific protocols for target material purification, material storing underground and limiting the time the detector is on surface during the building process in order to minimize the exposure to the most dangerous cosmic ray components., Comment: Final version as published
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- 2017
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22. Radiopurity assessment of the energy readout for the NEXT double beta decay experiment
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Cebrián, S., Pérez, J., Bandac, I., Labarga, L., Álvarez, V., Azevedo, C. D. R., Benlloch-Rodríguez, J. M., Borges, F. I. G. M., Botas, A., Cárcel, S., Carrión, J. V., Conde, C. A. N., Díaz, J., Diesburg, M., Escada, J., Esteve, R., Felkai, R., Fernandes, L. M. P., Ferrario, P., Ferreira, A. L., Freitas, E. D. C., Goldschmidt, A., Gómez-Cadenas, J. J., González-Díaz, D., Gutiérrez, R. M., Hauptman, J., Henriques, C. A. O., Hernandez, A. I., Morata, J. A. Hernando, Herrero, V., Jones, B. J. P., Laing, A., Lebrun, P., Liubarsky, I., López-March, N., Losada, M., Martín-Albo, J., Martínez-Lema, G., Martínez, A., McDonald, A. D., Monrabal, F., Monteiro, C. M. B., Mora, F. J., Moutinho, L. M., Vidal, J. Muñoz, Musti, M., Nebot-Guinot, M., Novella, P., Nygren, D. R., Palmeiro, B., Para, A., Querol, M., Renner, J., Ripoll, L., Rodríguez, o J., Rogers, L., Santos, F. P., Santos, J. M. F. dos, Simón, A., Sofka, C., Sorel, M., Stiegler, T., Toledo, p J. F., Torrent, J., Tsamalaidze, Z., Veloso, J. F. C. A., Villar, J. A., Webb, R., White, J. T., and Yahlali, N.
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Physics - Instrumentation and Detectors ,High Energy Physics - Experiment ,Nuclear Experiment - Abstract
The Neutrino Experiment with a Xenon Time-Projection Chamber (NEXT) experiment intends to investigate the neutrinoless double beta decay of 136Xe, and therefore requires a severe suppression of potential backgrounds. An extensive material screening and selection process was undertaken to quantify the radioactivity of the materials used in the experiment. Separate energy and tracking readout planes using different sensors allow us to combine the measurement of the topological signature of the event for background discrimination with the energy resolution optimization. The design of radiopure readout planes, in direct contact with the gas detector medium, was especially challenging since the required components typically have activities too large for experiments demanding ultra-low background conditions. After studying the tracking plane, here the radiopurity control of the energy plane is presented, mainly based on gamma-ray spectroscopy using ultra-low background germanium detectors at the Laboratorio Subterr\'aneo de Canfranc (Spain). All the available units of the selected model of photomultiplier have been screened together with most of the components for the bases, enclosures and windows. According to these results for the activity of the relevant radioisotopes, the selected components of the energy plane would give a contribution to the overall background level in the region of interest of at most 2.4 x 10-4 counts keV-1 kg-1 y-1, satisfying the sensitivity requirements of the NEXT experiment., Comment: Final version for publication
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- 2017
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23. Annual modulation of dark matter: The ANAIS-112 case
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Coarasa, I., Amaré, J., Cebrián, S., Cuesta, C., García, E., Martínez, M., Oliván, M. A., Ortigoza, Y., de Solórzano, A. Ortiz, Puimedón, J., Sarsa, M. L., Villar, J. A., and Villar, P.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Nuclear Experiment ,Physics - Instrumentation and Detectors - Abstract
The annual modulation measured by the DAMA/LIBRA experiment can be explained by the interaction of dark matter WIMPs in NaI(Tl) scintillator detectors. Other experiments, with different targets or techniques, exclude the region of parameters singled out by DAMA/LIBRA, but the comparison of their results relies on several hypotheses regarding the dark matter model. ANAIS-112 is a dark matter search with 112.5 kg of NaI(Tl) scintillators under commissioning at the Canfranc Underground Laboratory (LSC) to test the DAMA/LIBRA result in a model independent way. We analyze its prospects in terms of the a priori critical and detection limits of the experiment. The analysis is based on the detector response and the background level measured for the first modules operated in Canfranc.
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- 2017
24. EVALUACIÓN DE DOSIS, PERIODOS DE APLICACIÓN Y RESIDUALIDAD DE PACLOBUTRAZOL EN TOMATE
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Juárez-Rodríguez, Lucia, Pérez-Grajales, Mario, Castro-Brindis, Rogelio, Segura-Miranda, Antonio, Magaña-Lira, Natanae, and Magdaleno-Villar, J. Jesús
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- 2022
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25. Light yield determination in large sodium iodide detectors applied in the search for dark matter
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Oliván, M. A., Amaré, J., Cebrián, S., Cuesta, C., García, E., Martínez, M., Ortigoza, Y., de Solórzano, A. Ortiz, Pobes, C., Puimedón, J., Sarsa, M. L., Villar, J. A., and Villar, P.
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Physics - Instrumentation and Detectors ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Application of NaI(Tl) detectors in the search for galactic dark matter particles through their elastic scattering off the target nuclei is well motivated because of the long standing DAMA/LIBRA highly significant positive result on annual modulation, still requiring confirmation. For such a goal, it is mandatory to reach very low threshold in energy (at or below the keV level), very low radioactive background (at a few counts/keV/kg/day), and high detection mass (at or above the 100 kg scale). One of the most relevant technical issues is the optimization of the crystal intrinsic scintillation light yield and the efficiency of the light collecting system for large mass crystals. In the frame of the ANAIS (Annual modulation with NaI Scintillators) dark matter search project large NaI(Tl) crystals from different providers coupled to two photomultiplier tubes (PMTs) have been tested at the Canfranc Underground Laboratory. In this paper we present the estimates of the NaI(Tl) scintillation light collected using full-absorption peaks at very low energy from external and internal sources emitting gammas/electrons, and single-photoelectron events populations selected by using very low energy pulses tails. Outstanding scintillation light collection at the level of 15~photoelectrons/keV can be reported for the final design and provider chosen for ANAIS detectors. Taking into account the Quantum Efficiency of the PMT units used, the intrinsic scintillation light yield in these NaI(Tl) crystals is above 40~photoelectrons/keV for energy depositions in the range from 3 up to 25~keV. This very high light output of ANAIS crystals allows triggering below 1~keV, which is very important in order to increase the sensitivity in the direct detection of dark matter.
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- 2017
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26. Assessment of backgrounds of the ANAIS experiment for dark matter direct detection
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Amare, J., Cebrian, S., Cuesta, C., Garcia, E., Martinez, M., Olivan, M. A., Ortigoza, Y., de Solorzano, A. Ortiz, Puimedon, J., Sarsa, M. L., Villar, J. A., and Villar, P.
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Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment ,Nuclear Experiment ,Physics - Instrumentation and Detectors - Abstract
A large effort has been carried out to characterize the background of sodium iodide crystals within the ANAIS (Annual modulation with NaI Scintillators) project. In this paper, the background models developed for three 12.5-kg NaI(Tl) scintillators produced by Alpha Spectra Inc. and operated at the Canfranc Underground Laboratory are presented together with an evaluation of the background prospects for the full experiment. Measured spectra from threshold to high energy in different conditions are well described by the models based on quantified activities. At the region of interest, crystal bulk contamination is the dominant background source. Contributions from 210Pb, 40K, 22Na and 3H are the most relevant. Those from 40K and 22Na could be efficiently suppressed thanks to anticoincidence operation in a crystals matrix or inside a Liquid Scintillator Veto (LSV), while that from 210Pb has been reduced by improving crystal production methods and 3H production could be reduced by shielding against cosmic rays during production. Assuming the activities of the last characterized detector, for nine crystals with a total mass of 112.5 kg the expected background rate is 2.5 counts/(keV kg d) in the region from 1 to 4 keV, which could be reduced at 1.4 counts/(keV kg d) by using a LSV., Comment: Version as accepted for publication in Eur. Phys. J. C
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- 2016
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27. The satisfactory growth and development at 2 years of age of the INTERGROWTH-21st Fetal Growth Standards cohort support its appropriateness for constructing international standards
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Villar, José, Ismail, Leila Cheikh, Urias, Eleonora Staines, Giuliani, Francesca, Ohuma, Eric O, Victora, Cesar G, Papageorghiou, Aris T, Altman, Douglas G, Garza, Cutberto, Barros, Fernando C, Puglia, Fabien, Ochieng, Roseline, Jaffer, Yasmin A, Noble, Julia A, Bertino, Enrico, Purwar, Manorama, Pang, Ruyan, Lambert, Ann, Chumlea, Cameron, Stein, Alan, Fernandes, Michelle, Bhutta, Zulfiqar A, Kennedy, Stephen H, Katz, M, Bhan, MK, Garza, C, Zaidi, S, Langer, A, Rothwell, PM, Weatherall, D, Bhutta, ZA, Villar, J, Kennedy, S, Altman, DG, Barros, FC, Bertino, E, Burton, F, Carvalho, M, Ismail, L Cheikh, Chumlea, WC, Gravett, MG, Jaffer, YA, Lambert, A, Lumbiganon, P, Noble, JA, Pang, RY, Papageorghiou, AT, Purwar, M, Rivera, J, Victora, C, Shorten, M, Hoch, L, Knight, HE, Ohuma, EO, Cosgrove, C, Blakey, I, Urias, E Staines, Roseman, F, Kunnawar, N, Gu, SH, Wang, JH, Wu, MH, Domingues, M, Gilli, P, Juodvirsiene, L, Musee, N, Al-Jabri, H, Waller, S, Muninzwa, D, Yellappan, D, Carter, A, Reade, D, Miller, R, Salomon, L, Leston, A, Mitidieri, A, Al-Aamri, F, Paulsene, W, Sande, J, Al-Zadjali, WKS, Batiuk, C, Bornemeier, S, Dighe, M, Gaglioti, P, Jacinta, N, Jaiswal, S, Oas, K, Oberto, M, Olearo, E, Owende, MG, Shah, J, Sohoni, S, Todros, T, Venkataraman, M, Vinayak, S, Wang, L, Wilson, D, Wu, QQ, Zhang, Y, and Chamberlain, P
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Pediatric ,Conditions Affecting the Embryonic and Fetal Periods ,Infant Mortality ,Clinical Research ,Preterm ,Low Birth Weight and Health of the Newborn ,Nutrition ,Prevention ,Perinatal Period - Conditions Originating in Perinatal Period ,2.4 Surveillance and distribution ,Aetiology ,Reproductive health and childbirth ,Good Health and Well Being ,Brazil ,Cephalometry ,Child Development ,China ,Female ,Fetal Development ,Growth Charts ,Health Status ,Humans ,India ,Infant ,Infant ,Newborn ,Italy ,Kenya ,Longitudinal Studies ,Male ,Motor Skills ,Nutritional Status ,Oman ,Pregnancy ,United Kingdom ,United States ,World Health Organization ,International Fetal and Newborn Growth Consortium for the 21(st) Century (INTERGROWTH-21(st)) ,INTERGROWTH-21(st) fetal growth standards ,development ,postnatal growth ,Paediatrics and Reproductive Medicine ,Obstetrics & Reproductive Medicine - Abstract
BackgroundThe World Health Organization recommends that human growth should be monitored with the use of international standards. However, in obstetric practice, we continue to monitor fetal growth using numerous local charts or equations that are based on different populations for each body structure. Consistent with World Health Organization recommendations, the INTERGROWTH-21st Project has produced the first set of international standards to date pregnancies; to monitor fetal growth, estimated fetal weight, Doppler measures, and brain structures; to measure uterine growth, maternal nutrition, newborn infant size, and body composition; and to assess the postnatal growth of preterm babies. All these standards are based on the same healthy pregnancy cohort. Recognizing the importance of demonstrating that, postnatally, this cohort still adhered to the World Health Organization prescriptive approach, we followed their growth and development to the key milestone of 2 years of age.ObjectiveThe purpose of this study was to determine whether the babies in the INTERGROWTH-21st Project maintained optimal growth and development in childhood.Study designIn the Infant Follow-up Study of the INTERGROWTH-21st Project, we evaluated postnatal growth, nutrition, morbidity, and motor development up to 2 years of age in the children who contributed data to the construction of the international fetal growth, newborn infant size and body composition at birth, and preterm postnatal growth standards. Clinical care, feeding practices, anthropometric measures, and assessment of morbidity were standardized across study sites and documented at 1 and 2 years of age. Weight, length, and head circumference age- and sex-specific z-scores and percentiles and motor development milestones were estimated with the use of the World Health Organization Child Growth Standards and World Health Organization milestone distributions, respectively. For the preterm infants, corrected age was used. Variance components analysis was used to estimate the percentage variability among individuals within a study site compared with that among study sites.ResultsThere were 3711 eligible singleton live births; 3042 children (82%) were evaluated at 2 years of age. There were no substantive differences between the included group and the lost-to-follow up group. Infant mortality rate was 3 per 1000; neonatal mortality rate was 1.6 per 1000. At the 2-year visit, the children included in the INTERGROWTH-21st Fetal Growth Standards were at the 49th percentile for length, 50th percentile for head circumference, and 58th percentile for weight of the World Health Organization Child Growth Standards. Similar results were seen for the preterm subgroup that was included in the INTERGROWTH-21st Preterm Postnatal Growth Standards. The cohort overlapped between the 3rd and 97th percentiles of the World Health Organization motor development milestones. We estimated that the variance among study sites explains only 5.5% of the total variability in the length of the children between birth and 2 years of age, although the variance among individuals within a study site explains 42.9% (ie, 8 times the amount explained by the variation among sites). An increase of 8.9 cm in adult height over mean parental height is estimated to occur in the cohort from low-middle income countries, provided that children continue to have adequate health, environmental, and nutritional conditions.ConclusionThe cohort enrolled in the INTERGROWTH-21st standards remained healthy with adequate growth and motor development up to 2 years of age, which supports its appropriateness for the construction of international fetal and preterm postnatal growth standards.
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- 2018
28. International estimated fetal weight standards of the INTERGROWTH‐21st Project
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Stirnemann, J, Villar, J, Salomon, LJ, Ohuma, E, Ruyan, P, Altman, DG, Nosten, F, Craik, R, Munim, S, Cheikh Ismail, L, Barros, FC, Lambert, A, Norris, S, Carvalho, M, Jaffer, YA, Noble, JA, Bertino, E, Gravett, MG, Purwar, M, Victora, CG, Uauy, R, Bhutta, Z, Kennedy, S, Papageorghiou, AT, Katz, M, Bhan, MK, Garza, C, Zaidi, S, Langer, A, Rothwell, PM, Weatherall, Sir D, Bhutta, ZA, Burton, F, Ismail, L Cheikh, Chumlea, WC, Lumbiganon, P, Pang, RY, Rivera, J, Victora, C, Berkley, J, Shorten, M, Hoch, L, Knight, HE, Ohuma, EO, Cosgrove, C, Blakey, I, Ash, S, Urias, E Staines, Roseman, F, Kunnawar, N, Gu, SH, Wang, JH, and Wu, MH
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Conditions Affecting the Embryonic and Fetal Periods ,Prevention ,Perinatal Period - Conditions Originating in Perinatal Period ,Clinical Research ,Preterm ,Low Birth Weight and Health of the Newborn ,Pediatric ,Infant Mortality ,Reproductive health and childbirth ,Adult ,Birth Weight ,Cross-Sectional Studies ,Female ,Femur ,Fetal Weight ,Gestational Age ,Head ,Humans ,Pregnancy ,Prospective Studies ,Ultrasonography ,Prenatal ,International Fetal and Newborn Growth Consortium for the 21st Century ,Scientific Advisory Committee ,Steering Committees ,INTERGROWTH-21st ,INTERBIO-21st ,Executive Committee ,In addition for INTERBIO 21st ,Project Coordinating Unit ,Data Analysis Group ,Data Management Group ,Ultrasound Group ,In addition for INTERBIO-21st: ,Anthropometry Group ,Laboratory Processing Group ,Neonatal Group ,Environmental Health Group ,Neurodevelopment Group ,Participating countries and local investigators ,birth weight ,fetal growth ,gestational age ,screening ,ultrasound ,Paediatrics and Reproductive Medicine ,Obstetrics & Reproductive Medicine - Abstract
ObjectiveEstimated fetal weight (EFW) and fetal biometry are complementary measures used to screen for fetal growth disturbances. Our aim was to provide international EFW standards to complement the INTERGROWTH-21st Fetal Growth Standards that are available for use worldwide.MethodsWomen with an accurate gestational-age assessment, who were enrolled in the prospective, international, multicenter, population-based Fetal Growth Longitudinal Study (FGLS) and INTERBIO-21st Fetal Study (FS), two components of the INTERGROWTH-21st Project, had ultrasound scans every 5 weeks from 9-14 weeks' until 40 weeks' gestation. At each visit, measurements of fetal head circumference (HC), biparietal diameter, occipitofrontal diameter, abdominal circumference (AC) and femur length (FL) were obtained blindly by dedicated research sonographers using standardized methods and identical ultrasound machines. Birth weight was measured within 12 h of delivery by dedicated research anthropometrists using standardized methods and identical electronic scales. Live babies without any congenital abnormality, who were born within 14 days of the last ultrasound scan, were selected for inclusion. As most births occurred at around 40 weeks' gestation, we constructed a bootstrap model selection and estimation procedure based on resampling of the complete dataset under an approximately uniform distribution of birth weight, thus enriching the sample size at extremes of fetal sizes, to achieve consistent estimates across the full range of fetal weight. We constructed reference centiles using second-degree fractional polynomial models.ResultsOf the overall population, 2404 babies were born within 14 days of the last ultrasound scan. Mean time between the last scan and birth was 7.7 (range, 0-14) days and was uniformly distributed. Birth weight was best estimated as a function of AC and HC (without FL) as log(EFW) = 5.084820 - 54.06633 × (AC/100)3 - 95.80076 × (AC/100)3 × log(AC/100) + 3.136370 × (HC/100), where EFW is in g and AC and HC are in cm. All other measures, gestational age, symphysis-fundus height, amniotic fluid indices and interactions between biometric measures and gestational age, were not retained in the selection process because they did not improve the prediction of EFW. Applying the formula to FGLS biometric data (n = 4231) enabled gestational age-specific EFW tables to be constructed. At term, the EFW centiles matched those of the INTERGROWTH-21st Newborn Size Standards but, at
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- 2017
29. Could pulmonary low-dose radiation therapy be an alternative treatment for patients with COVID-19 pneumonia? Preliminary results of a multicenter SEOR-GICOR nonrandomized prospective trial (IPACOVID trial)
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Arenas, M., Algara, M., De Febrer, G., Rubio, C., Sanz, X., de la Casa, M. A., Vasco, C., Marín, J., Fernández-Letón, P., Villar, J., Torres-Royo, L., Villares, P., Membrive, I., Acosta, J., López-Cano, M., Araguas, P., Quera, J., Rodríguez-Tomás, F., and Montero, A.
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- 2021
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30. The ANAIS Dark Matter Project: Status and Prospects
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Amaré, J., Cebrián, S., Cuesta, C., García, E., Martínez, M., Oliván, M. A., Ortigoza, Y., de Solórzano, A. Ortiz, Pobes, C., Puimedón, J., Sarsa, M. L., Villar, J. A., and Villar, P.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Physics - Instrumentation and Detectors - Abstract
The ANAIS (Annual modulation with NaI(Tl) Scintillators) experiment aims at the confirmation of the DAMA/LIBRA positive annual modulation signal using the same target and technique at the Canfranc Underground Laboratory (LSC). A first step, named ANAIS-25 (two 12.5 kg NaI(Tl) modules) taking data from December 2012 to February 2015, provided interesting outcomes: very high light collection efficiency, that could allow to lower the analysis energy threshold down to the level of 1 keVee, and a good understanding of the different background components, in particular the cosmogenic activated isotopes in the crystal bulk and other radioactive contaminations of the NaI crystal/powder. But those prototypes clearly pointed to the need for improved crystal radiopurity, in particular for $^{210}$Pb contamination. Since then, improvements in the purification and growing procedures in order to reduce background in the very low energy region have been implemented and a new 12.5 kg module has been constructed and installed between the former two crystals, forming the ANAIS-37 setup. Very preliminary results of this setup evidence the improvement on radiopurity of the new crystal and are presented here. In addition, background simulations and prospects for the full experiment are discussed., Comment: 7 pages, 6 figures. Proceeding of the MG14 conference, July 2015, Rome
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- 2016
31. Status of the ANAIS Dark Matter Project at the Canfranc Underground Laboratory
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Amaré, J., Cebrián, S., Cuesta, C., García, E., Martínez, M., Oliván, M. A., Ortigoza, Y., de Solórzano, A. Ortiz, Pobes, C., Puimedón, J., Sarsa, M. L., Villar, J. A., and Villar, P.
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Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Experiment ,Physics - Instrumentation and Detectors - Abstract
The ANAIS (Annual modulation with NaI(Tl) Scintillators) experiment aims at the confirmation of the DAMA/LIBRA signal using the same target and technique at the Canfranc Underground Laboratory (LSC). Along 2016, 112.5 kg of ultra pure NaI(Tl) crystals will be installed at LSC in a 3x3 modules matrix configuration. The ANAIS-25 and ANAIS-37 set-ups have been taking data at the LSC testing the detector performance, the DAQ and analysis systems, and assessing the background. Main results coming from both set-ups will be summarized in this paper, focusing on the excellent detector performance and background understanding. Prospects for the experiment will be also briefly revised., Comment: To appear in Journal of Physics: Conference Series. TAUP2015 Proceedings
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- 2015
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32. Background model of NaI(Tl) detectors for the ANAIS Dark Matter Project
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Amare, J., Cebrian, S., Cuesta, C., Garcia, E., Martinez, M., Olivan, M. A., Ortigoza, Y., de Solorzano, A. Ortiz, Pobes, C., Puimedon, J., Sarsa, M. L., Villar, J. A., and Villar, P.
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Physics - Instrumentation and Detectors ,High Energy Physics - Experiment - Abstract
A thorough understanding of the background sources is mandatory in any experiment searching for rare events. The ANAIS (Annual Modulation with NaI(Tl) Scintillators) experiment aims at the confirmation of the DAMA/LIBRA signal at the Canfranc Underground Laboratory (LSC). Two NaI(Tl) crystals of 12.5 kg each produced by Alpha Spectra have been taking data since December 2012. The complete background model of these detectors and more precisely in the region of interest will be described. Preliminary background analysis of a new 12.5 kg crystal received at Canfranc in March 2015 will be presented too. Finally, the power of anticoincidence rejection in the region of interest has been analyzed in a 4x 5 12.5 kg detector matrix., Comment: Contributed to the 11th Patras Workshop on Axions, WIMPs and WISPs, Zaragoza, June 22 to 26, 2015
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- 2015
33. First proof of topological signature in the high pressure xenon gas TPC with electroluminescence amplification for the NEXT experiment
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NEXT Collaboration, Ferrario, P., Laing, A., López-March, N., Gómez-Cadenas, J. J., Álvarez, V., Azevedo, C. D. R., Borges, F. I. G., Cárcel, S., Cebrián, S., Cervera, A., Conde, C. A. N., Dafni, T., Díaz, J., Diesburg, M., Esteve, R., Fernandes, L. M. P., Ferreira, A. L., Freitas, E. D. C., Gehman, V. M., Goldschmidt, A., González-Díaz, D., Gutiérrez, R. M., Hauptman, J., Henriques, C. A. O., Morata, J. A. Hernando, Irastorza, I. G., Labarga, L., Lebrun, P., Liubarsky, I., Lorca, D., Losada, M., Luzón, G., Marí, A., Martín-Albo, J., Martínez-Lema, G., Martínez, A., Miller, T., Monrabal, F., Monserrate, M., Monteiro, C. M. B., Mora, F. J., Moutinho, L. M., Vidal, J. Muñoz, Nebot-Guinot, M., Novella, P., Nygren, D., Para, A., Pérez, J., Aparicio, J. L. Pérez, Querol, M., Renner, J., Ripoll, L., Rodríguez, J., Santos, F. P., Santos, J. M. F. dos, Serra, L., Shuman, D., Simón, A., Sofka, C., Sorel, M., Toledo, J. F., Torrent, J., Tsamalaidze, Z., Veloso, J. F. C. A., Villar, J. A., Webb, R., White, J. T., Yahlali, N., and Yepes-Ramírez, H.
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Physics - Instrumentation and Detectors ,High Energy Physics - Experiment - Abstract
The NEXT experiment aims to observe the neutrinoless double beta decay of xenon in a high-pressure Xe136 gas TPC using electroluminescence (EL) to amplify the signal from ionization. One of the main advantages of this technology is the possibility to reconstruct the topology of events with energies close to Qbb. This paper presents the first demonstration that the topology provides extra handles to reject background events using data obtained with the NEXT-DEMO prototype. Single electrons resulting from the interactions of Na22 1275 keV gammas and electron-positron pairs produced by conversions of gammas from the Th228 decay chain were used to represent the background and the signal in a double beta decay. These data were used to develop algorithms for the reconstruction of tracks and the identification of the energy deposited at the end-points, providing an extra background rejection factor of 24.3 +- 1.4 (stat.)%, while maintaining an efficiency of 66.7 +- 1% for signal events.
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- 2015
34. Background analysis and status of the ANAIS dark matter project
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Amaré, J., Cebrián, S., Cuesta, C., García, E., Ginestra, C., Martínez, M., Oliván, M. A., Ortigoza, Y., de Solórzano, A. Ortiz, Pobes, C., Puimedón, J., Sarsa, M. L., Villar, J. A., and Villar, P.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Physics - Instrumentation and Detectors - Abstract
ANAIS (Annual modulation with NaI Scintillators) is a project aiming to set up at the new facilities of the Canfranc Underground Laboratory (LSC), a large scale NaI(Tl) experiment in order to explore the DAMA/LIBRA annual modulation positive result using the same target and technique. Two 12.5 kg each NaI(Tl) crystals provided by Alpha Spectra took data at the LSC in the ANAIS-25 set-up. The comparison of the background model for the ANAIS-25 prototypes with the experimental results is presented. ANAIS crystal radiopurity goals have been achieved for Th-232 and U-238 chains, but a Pb-210 contamination out-of-equilibrium was identified, whose origin has been studied. The high light collection efficiency obtained with these prototypes allows to anticipate an energy threshold of the order of 1 keVee. A new detector, with improved performances, was received in March 2015 and very preliminary results are shown., Comment: 6 pages, 7 figures
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- 2015
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35. Radon and material radiopurity assessment for the NEXT double beta decay experiment
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Cebrián, S., Pérez, J., Bandac, I., Labarga, L., Álvarez, V., Barrado, A. I., Bettini, A., Borges, F. I. G. M., Camargo, M., Cárcel, S., Cervera, A., Conde, C. A. N., Conde, E., Dafni, T., Díaz, J., Esteve, R., Fernandes, L. M. P., Fernández, M., Ferrario, P., Freitas, E. D. C., Gehman, V. M., Goldschmidt, A., Gómez-Cadenas, J. J., González-Díaz, D., Gutiérrez, R. M., Hauptman, J., Morata, J. A. Hernando, Herrera, D. C., Irastorza, I. G., Laing, A., Liubarsky, I., López-March, N., Lorca, D., Losada, M., Luzón, G., Marí, A., Martín-Albo, J., Martínez, A., Martínez-Lema, G., Miller, T., Monrabal, F., Monserrate, M., Monteiro, C. M. B., Mora, F. J., Moutinho, L. M., Vidal, J. Muñoz, Nebot-Guinot, M., Nygren, D., Oliveira, C. A. B., de Solórzano, A. Ortiz, Aparicio, J. L. Pérez, Querol, M., Renner, J., Ripoll, L., Rodríguez, J., Santos, F. P., Santos, J. M. F. dos, Serra, L., Shuman, D., Simón, A., Sofka, C., Sorel, M., Toledo, J. F., Torrent, J., Tsamalaidze, Z., Veloso, J. F. C. A., Villar, J. A., Webb, R. C., White, J. T., and Yahlali, N.
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Physics - Instrumentation and Detectors ,High Energy Physics - Experiment ,Nuclear Experiment - Abstract
The Neutrino Experiment with a Xenon TPC (NEXT), intended to investigate the neutrinoless double beta decay using a high-pressure xenon gas TPC filled with Xe enriched in 136Xe at the Canfranc Underground Laboratory in Spain, requires ultra-low background conditions demanding an exhaustive control of material radiopurity and environmental radon levels. An extensive material screening process is underway for several years based mainly on gamma-ray spectroscopy using ultra-low background germanium detectors in Canfranc but also on mass spectrometry techniques like GDMS and ICPMS. Components from shielding, pressure vessel, electroluminescence and high voltage elements and energy and tracking readout planes have been analyzed, helping in the final design of the experiment and in the construction of the background model. The latest measurements carried out will be presented and the implication on NEXT of their results will be discussed. The commissioning of the NEW detector, as a first step towards NEXT, has started in Canfranc; in-situ measurements of airborne radon levels were taken there to optimize the system for radon mitigation and will be shown too., Comment: Proceedings of the Low Radioactivity Techniques 2015 workshop (LRT2015), Seattle, March 2015
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- 2015
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36. Production and relevance of cosmogenic radionuclides in NaI(Tl) crystals
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Amare, J., Cebrian, S., Cuesta, C., Garcia, E., Ginestra, C., Martinez, M., Olivan, M. A., Ortigoza, Y., de Solorzano, A. Ortiz, Pobes, C., Puimedon, J., Sarsa, M. L., Villar, J. A., and Villar, P.
- Subjects
Physics - Instrumentation and Detectors ,High Energy Physics - Experiment ,Nuclear Experiment - Abstract
The cosmogenic production of long-lived radioactive isotopes in materials is an hazard for experiments demanding ultra-low background conditions. Although NaI(Tl) scintillators have been used in this context for a long time, very few activation data were available. We present results from two 12.5 kg NaI(Tl) detectors, developed within the ANAIS project and installed at the Canfranc Underground Laboratory. The prompt data taking starting made possible a reliable quantification of production of some I, Te and Na isotopes with half-lives larger than ten days. Initial activities underground were measured and then production rates at sea level were estimated following the history of detectors; a comparison of these rates with calculations using typical cosmic neutron flux at sea level and a selected description of excitation functions was also carried out. After including the contribution from the identified cosmogenic products in the detector background model, we found that the presence of 3H in the crystal bulk would help to fit much better our background model and experimental data. We have analyzed the cosmogenic production of 3H in NaI, and although precise quantification has not been attempted, we can conclude that it could imply a very relevant contribution to the total background below 15 keV in NaI detectors., Comment: Proceedings of the Low Radioactivity Techniques 2015 workshop, March 2015, Seattle (US)
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- 2015
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37. Accurate gamma and MeV-electron track reconstruction with an ultra-low diffusion Xenon/TMA TPC at 10 atmospheres
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Gonzalez-Diaz, Diego, Alvarez, V., Borges, F. I. G., Camargo, M., Carcel, S., Cebrian, S., Cervera, A., Conde, C. A. N., Dafni, T., Diaz, J., Esteve, R., Fernandes, L. M. P., Ferrario, P., Ferreira, A. L., Freitas, E. D. C., Gehman, V. M., Goldschmidt, A., Gomez-Cadenas, J. J., Gutierrez, R. M., Hauptman, J., Morata, J. A. Hernando, Herrera, D. C., Irastorza, I. G., Labarga, L., Laing, A., Liubarsky, I., Lopez-March, N., Lorca, D., Losada, M., Luzon, G., Mari, A., Martin-Albo, J., Martinez-Lema, G., Martinez, A., Miller, T., Monrabal, F., Monserrate, M., Monteiro, C. M. B., Mora, F. J., Moutinho, L. M., Vidal, J. Munoz, Nebot-Guinot, M., Nygren, D., Oliveira, C. A. B., Perez, J., Aparicio, J. L. Perez, Querol, M., Renner, J., Ripoll, L., Rodriguez, J., Santos, F. P., Santos, J. M. F. dos, Serra, L., Shuman, D., Simon, A., Sofka, C., Sorel, M., Toledo, J. F., Torrent, J., Tsamalaidze, Z., Veloso, J. F. C. A., Villar, J. A., Webb, R., White, J. T., Yahlali, N., Azevedo, C., Aznar, F., Calvet, D., Castel, J., Ferrer-Ribas, E., Garcia, J. A., Giomataris, I., Gomez, H., Iguaz, F. J., Lagraba, A., Coguie, A. Le, Mols, J. P., Sahin, O., Rodriguez, A., Ruiz-Choliz, E., Segui, L., Tomas, A., and Veenhof, R.
- Subjects
Physics - Instrumentation and Detectors - Abstract
We report the performance of a 10 atm Xenon/trimethylamine time projection chamber (TPC) for the detection of X-rays (30 keV) and gamma-rays (0.511-1.275 MeV) in conjunction with the accurate tracking of the associated electrons. When operated at such a high pressure and in 1%-admixtures, trimethylamine (TMA) endows Xenon with an extremely low electron diffusion (1.3 +-0.13 mm-sigma (longitudinal), 0.8 +-0.15 mm-sigma (transverse) along 1 m drift) besides forming a convenient Penning-Fluorescent mixture. The TPC, that houses 1.1 kg of gas in its active volume, operated continuously for 100 live-days in charge amplification mode. The readout was performed through the recently introduced microbulk Micromegas technology and the AFTER chip, providing a 3D voxelization of 8mm x 8mm x 1.2mm for approximately 10 cm/MeV-long electron tracks. This work was developed as part of the R&D program of the NEXT collaboration for future detector upgrades in the search of the 0bbnu decay in 136Xe, specifically those based on novel gas mixtures. Therefore we ultimately focus on the calorimetric and topological properties of the reconstructed MeV-electron tracks.
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- 2015
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38. Parameters of Physical and Physiological Quality in Tomato Seeds Produced under High Temperature Condition during Different Periods of Development
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Ruiz-Nieves, Juan M., Magdaleno-Villar, J. Jesus, Sanchez-Alonso, Mariana G., Delgado-Vargas, Victoria A., Helene, Gautier, and Ayala-Garay, Oscar J.
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- 2021
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39. The popularity of neurology in Spain: an analysis of specialty selection
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Curbelo, J., Romeo, J.M., Galván-Román, J.M., Vega-Villar, J., Martinez-Lapiscina, E.H., Jiménez-Fonseca, P., Villacampa, T., Sánchez-Lasheras, F., Fernández-Somoano, A., and Baladrón, J.
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- 2020
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40. Popularidad de Neurología en España: análisis de la elección de la especialidad
- Author
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Curbelo, J., Romeo, J.M., Galván-Román, J.M., Vega-Villar, J., Martinez-Lapiscina, E.H., Jiménez-Fonseca, P., Villacampa, T., Sánchez-Lasheras, F., Fernández-Somoano, A., and Baladrón, J.
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- 2020
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41. EFECTO DEL PACLOBUTRAZOL SOBRE EL CRECIMIENTO DE LA PLANTA, RENDIMIENTO Y CALIDAD DEL FRUTO EN TOMATE
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Ramos-Fernández, Josúe, Ayala-Garay, Oscar J., Pérez-Grajales, Mario, Castillo, Felipe Sánchez-del, and Magdaleno-Villar, J. Jesús
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- 2021
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42. Low dose anti-inflammatory radiotherapy for the treatment of pneumonia by covid-19: A proposal for a multi-centric prospective trial
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Algara, M., Arenas, M., Marin, J., Vallverdu, I., Fernandez-Letón, P., Villar, J., Fabrer, G., Rubio, C., and Montero, A.
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- 2020
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43. Achieving accurate estimates of fetal gestational age and personalised predictions of fetal growth based on data from an international prospective cohort study: a population-based machine learning study
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Norris, S, Abbott, SE, Abubakar, A, Acedo, J, Ahmed, I, Al-Aamri, F, Al-Abduwani, J, Al-Abri, J, Alam, D, Albernaz, E, Algren, H, Al-Habsi, F, Alija, M, Al-Jabri, H, Al-Lawatiya, H, Al-Rashidiya, B, Altman, DG, Al-Zadjali, WK, Andersen, HF, Aranzeta, L, Ash, S, Baricco, M, Barros, FC, Barsosio, H, Batiuk, C, Batra, M, Berkley, J, Bertino, E, Bhan, MK, Bhat, BA, Bhutta, ZA, Blakey, I, Bornemeier, S, Bradman, A, Buckle, M, Burnham, O, Burton, F, Capp, A, Cararra, VI, Carew, R, Carrara, VI, Carter, AA, Carvalho, M, Chamberlain, P, Cheikh, Ismail L, Cheikh Ismail, L, Choudhary, A, Choudhary, S, Chumlea, WC, Condon, C, Corra, LA, Cosgrove, C, Craik, R, da Silveira, MF, Danelon, D, de Wet, T, de Leon, E, Deshmukh, S, Deutsch, G, Dhami, J, Di, Nicola P, Dighe, M, Dolk, H, Domingues, M, Dongaonkar, D, Enquobahrie, D, Eskenazi, B, Farhi, F, Fernandes, M, Finkton, D, Fonseca, S, Frederick, IO, Frigerio, M, Gaglioti, P, Garza, C, Gilli, G, Gilli, P, Giolito, M, Giuliani, F, Golding, J, Gravett, MG, Gu, SH, Guman, Y, He, YP, Hoch, L, Hussein, S, Ibanez, D, Ioannou, C, Jacinta, N, Jackson, N, Jaffer, YA, Jaiswal, S, Jimenez-Bustos, JM, Juangco, FR, Juodvirsiene, L, Katz, M, Kemp, B, Kennedy, S, Ketkar, M, Khedikar, V, Kihara, M, Kilonzo, J, Kisiang'ani, C, Kizidio, J, Knight, CL, Knight, HE, Kunnawar, N, Laister, A, Lambert, A, Langer, A, Lephoto, T, Leston, A, Lewis, T, Liu, H, Lloyd, S, Lumbiganon, P, Macauley, S, Maggiora, E, Mahorkar, C, Mainwaring, M, Malgas, L, Matijasevich, A, McCormick, K, McGready, R, Miller, R, Min, A, Mitidieri, A, Mkrtychyan, V, Monyepote, B, Mota, D, Mulik, I, Munim, S, Muninzwa, D, Musee, N, Mwakio, S, Mwangudzah, H, Napolitano, R, Newton, CR, Ngami, V, Noble, JA, Norris, T, Nosten, F, Oas, K, Oberto, M, Occhi, L, Ochieng, R, Ohuma, EO, Olearo, E, Olivera, I, Owende, MG, Pace, C, Pan, Y, Pang, RY, Papageorghiou, AT, Patel, B, Paul, V, Paulsene, W, Puglia, F, Purwar, M, Rajan, V, Raza, A, Reade, D, Rivera, J, Rocco, DA, Roseman, F, Roseman, S, Rossi, C, Rothwell, PM, Rovelli, I, Saboo, K, Salam, R, Salim, M, Salomon, L, Sanchez, Luna M, Sande, J, Sarris, I, Savini, S, Sclowitz, IK, Seale, A, Shah, J, Sharps, M, Shembekar, C, Shen, YJ, Shorten, M, Signorile, F, Singh, A, Sohoni, S, Somani, A, Sorensen, TK, Soria- Frisch, A, Staines Urias, E, Stein, A, Stones, W, Taori, V, Tayade, K, Todros, T, Uauy, R, Varalda, A, Venkataraman, M, Victora, C, Villar, J, Vinayak, S, Waller, S, Walusuna, L, Wang, JH, Wang, L, Wanyonyi, S, Weatherall, D, Wiladphaingern, S, Wilkinson, A, Wilson, D, Wu, MH, Wu, QQ, Wulff, K, Yellappan, D, Yuan, Y, Zaidi, S, Zainab, G, Zhang, JJ, Zhang, Y, Fung, Russell, Villar, Jose, Dashti, Ali, Ismail, Leila Cheikh, Staines-Urias, Eleonora, Ohuma, Eric O, Salomon, Laurent J, Victora, Cesar G, Barros, Fernando C, Lambert, Ann, Carvalho, Maria, Jaffer, Yasmin A, Noble, J Alison, Gravett, Michael G, Purwar, Manorama, Pang, Ruyan, Bertino, Enrico, Munim, Shama, Min, Aung Myat, McGready, Rose, Norris, Shane A, Bhutta, Zulfiqar A, Kennedy, Stephen H, Papageorghiou, Aris T, and Ourmazd, Abbas
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- 2020
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44. Search for chameleons with CAST
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Anastassopoulos, V., Arik, M., Aune, S., Barth, K., Belov, A., Bräuninger, H., Cantatore, G., Carmona, J. M., Cetin, S. A., Christensen, F., Collar, J. I., Dafni, T., Davenport, M., Desch, K., Dermenev, A., Eleftheriadis, C., Fanourakis, G., Ferrer-Ribas, E., Friedrich, P., Galán, J., García, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Geralis, T., Giomataris, I., Hailey, C., Haug, F., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jacoby, J., Jakobsen, A., Jakovčić, K., Kaminski, J., Karuza, M., Kavuk, M., Krčmar, M., Krieger, C., Krüger, A., Lakić, B., Laurent, J. M., Liolios, A., Ljubičić, A., Luzón, G., Neff, S., Ortega, I., Papaevangelou, T., Pivovarov, M. J., Raffelt, G., Riege, H., Rosu, M., Ruz, J., Savvidis, I., Solanki, S. K., Vafeiadis, T., Villar, J. A., Vogel, J. K., Yildiz, S. C., Zioutas, K., Brax, P., Lavrentyev, I., and Upadhye, A.
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Astrophysics - Solar and Stellar Astrophysics ,High Energy Physics - Phenomenology ,Physics - Instrumentation and Detectors - Abstract
In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ($\beta_{\rm m}$) and to photons ($\beta_{\gamma}$) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1$\,$keV to 400$\,$eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600$\,$eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of $\beta_{\gamma}\!\lesssim\!10^{11}$ for $1<\beta_{\rm m}<10^6$., Comment: 8 pages, 12 figures
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- 2015
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45. New solar axion search in CAST with $^4$He filling
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Arik, M., Aune, S., Barth, K., Belov, A., Bräuninger, H., Bremer, J., Burwitz, V., Cantatore, G., Carmona, J. M., Cetin, S. A., Collar, J. I., Da Riva, E., Dafni, T., Davenport, M., Dermenev, A., Eleftheriadis, C., Elias, N., Fanourakis, G., Ferrer-Ribas, E., Galán, J., García, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Geralis, T., Georgiopoulou, E., Giomataris, I., Gninenko, S., Marzoa, M. Gómez, Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jacoby, J., Jakovčić, K., Karuza, M., Kavuk, M., Krčmar, M., Kuster, M., Lakić, B., Laurent, J. M., Liolios, A., Ljubičić, A., Luzón, G., Neff, S., Niinikoski, T., Nordt, A., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Rodríguez, G. Raffelt A., Rosu, M., Ruz, J., Savvidis, I., Shilon, I., Solanki, S. K., Stewart, L., Tomás, A., Vafeiadis, T., Villar, J., Vogel, J. K., Yildiz, S. C., and Zioutas, K.
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High Energy Physics - Experiment ,Physics - Instrumentation and Detectors - Abstract
The CERN Axion Solar Telescope (CAST) searches for $a\to\gamma$ conversion in the 9 T magnetic field of a refurbished LHC test magnet that can be directed toward the Sun. Two parallel magnet bores can be filled with helium of adjustable pressure to match the X-ray refractive mass $m_\gamma$ to the axion search mass $m_a$. After the vacuum phase (2003--2004), which is optimal for $m_a\lesssim0.02$ eV, we used $^4$He in 2005--2007 to cover the mass range of 0.02--0.39 eV and $^3$He in 2009--2011 to scan from 0.39--1.17 eV. After improving the detectors and shielding, we returned to $^4$He in 2012 to investigate a narrow $m_a$ range around 0.2 eV ("candidate setting" of our earlier search) and 0.39--0.42 eV, the upper axion mass range reachable with $^4$He, to "cross the axion line" for the KSVZ model. We have improved the limit on the axion-photon coupling to $g_{a\gamma}< 1.47\times10^{-10} {\rm GeV}^{-1}$ (95% C.L.), depending on the pressure settings. Since 2013, we have returned to vacuum and aim for a significant increase in sensitivity., Comment: CAST Collaboration 6 pages 3 figures
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- 2015
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46. COMPLEX ABDOMINAL WALL HERNIAS: A MULTICENTER COHORT STUDY
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Nieto Martos, R, primary, Blázquez Hernando, L, additional, Martos Meléndez, S, additional, Andrés Andrade Yagual, A, additional, López Monclús, J, additional, Robín Valle de Lersundi, A, additional, Muñoz Rodríguez, J, additional, Porrero Guerrero, B, additional, Román García de Leon, L, additional, Manuel Molina Villar, J, additional, María Fernández Cebrian, J, additional, and Ángel García Ureña, M, additional
- Published
- 2024
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47. ABDOMINAL WALL PSEUDOHERNIA AFTER SHOCK WAVE LITHOTRIPSY: A RARE CAUSE OF ABDOMINAL WALL BULGING
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Santana Valenciano, Á, primary, del Carmen Ortega Ferrete, A, additional, Zaborras Buill, J, additional, López Monclús, J, additional, Porrero Guerrero, B, additional, Valle de Lersundi, A R, additional, Muñoz Rodriguez, J, additional, Molina Villar, J M, additional, Garcia de León, L R, additional, Fernández Cebrian, J M, additional, Garcia Ureña, M Á, additional, and Blazquez Hernando, L, additional
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- 2024
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48. VERY LONG-TERM QUALITY OF LIFE AFTER FOLLOWING MADRID'S MODIFICATION OF TAR FOR COMPLETE BILATERAL ABDOMINAL WALL SECTION AFTER A HIGH-ENERGY TRAUMA. HOW CAN WE FIX IT?
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Nieto Martos, R, primary, Blázquez Hernando, L, additional, Divina Juez Sáez, L, additional, Manuel Molina Villar, J, additional, Martos Meléndez, S, additional, Andrés Andrade Yagual, A, additional, and María Fernández Cebrián, J, additional
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- 2024
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49. An improved measurement of electron-ion recombination in high-pressure xenon gas
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NEXT Collaboration, Serra, L., Sorel, M., Álvarez, V., Borges, F. I. G., Camargo, M., Cárcel, S., Cebrián, S., Cervera, A., Conde, C. A. N., Dafni, T., Díaz, J., Esteve, R., Fernandes, L. M. P., Ferrario, P., Ferreira, A. L., Freitas, E. D. C., Gehman, V. M., Goldschmidt, A., Gómez-Cadenas, J. J., González-Díaz, D., Gutiérrez, R. M., Hauptman, J., Morata, J. A. Hernando, Herrera, D. C., Irastorza, I. G., Labarga, L., Laing, A., Liubarsky, I., Lopez-March, N., Lorca, D., Losada, M., Luzón, G., Marí, A., Martín-Albo, J., Martínez-Lema, G., Martínez, A., Miller, T., Monrabal, F., Monserrate, M., Monteiro, C. M. B., Mora, F. J., Moutinho, L. M., Vidal, J. Muñoz, Nebot-Guinot, M., Nygren, D., Oliveira, C. A. B., Pérez, J., Aparicio, J. L. Pérez, Querol, M., Renner, J., Ripoll, L., Rodríguez, A., Rodríguez, J., Santos, F. P., Santos, J. M. F. dos, Shuman, D., Simón, A., Sofka, C., Toledo, J. F., Torrent, J., Tsamalaidze, Z., Veloso, J. F. C. A., Villar, J. A., Webb, R., White, J. T., and Yahlali, N.
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Physics - Instrumentation and Detectors ,High Energy Physics - Experiment - Abstract
We report on results obtained with the NEXT-DEMO prototype of the NEXT-100 high-pressure xenon gas time projection chamber (TPC), exposed to an alpha decay calibration source. Compared to our previous measurements with alpha particles, an upgraded detector and improved analysis techniques have been used. We measure event-by-event correlated fluctuations between ionization and scintillation due to electron-ion recombination in the gas, with correlation coeffcients between -0.80 and -0.56 depending on the drift field conditions. By combining the two signals, we obtain a 2.8 % FWHM energy resolution for 5.49 MeV alpha particles and a measurement of the optical gain of the electroluminescent TPC. The improved energy resolution also allows us to measure the specific activity of the radon in the gas due to natural impurities. Finally, we measure the average ratio of excited to ionized atoms produced in the xenon gas by alpha particles to be $0.561\pm 0.045$, translating into an average energy to produce a primary scintillation photon of $W_{\rm ex}=(39.2\pm 3.2)$ eV., Comment: 22 pages, 11 figures, 1 table
- Published
- 2014
- Full Text
- View/download PDF
50. Radiopurity assessment of the tracking readout for the NEXT double beta decay experiment
- Author
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Cebrián, S., Pérez, J., Bandac, I., Labarga, L., Álvarez, V., Barrado, A. I., Bettini, A., Borges, F. I. G. M., Camargo, M., Cárcel, S., Cervera, A., Conde, C. A. N., Conde, E., Dafni, T., Díaz, J., Esteve, R., Fernandes, L. M. P., Fernández, M., Ferrario, P., Ferreira, A. L., Freitas, E. D. C., Gehman, V. M., Goldschmidt, A., Gómez-Cadenas, J. J., González-Díaz, D., Gutiérrez, R. M., Hauptman, J., Morata, J. A. Hernando, Herrera, D. C., Irastorza, I. G., Laing, A., Liubarsky, I., López-March, N., Lorca, D., Losada, M., Luzón, G., Marí, A., Martín-Albo, J., Martínez, A., Martínez-Lema, G., Miller, T., Monrabal, F., Monserrate, M., Monteiro, C. M. B., Mora, F. J., Moutinho, L. M., Vidal, J. Muñoz, Nebot-Guinot, M., Nygren, D., Oliveira, C. A. B., de Solórzano, A. Ortiz, Aparicio, J. L. Pérez, Querol, M., Renner, J., Ripoll, L., Rodríguez, J., Santos, F. P., Santos, J. M. F. dos, Serra, L., Shuman, D., Simón, A., Sofka, C., Sorel, M., Toledo, J. F., Torrent, J., Tsamalaidze, Z., Veloso, J. F. C. A., Villar, J. A., Webb, R. C., White, J. T., and Yahlali, N.
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Physics - Instrumentation and Detectors ,High Energy Physics - Experiment ,Nuclear Experiment - Abstract
The Neutrino Experiment with a Xenon Time-Projection Chamber (NEXT) is intended to investigate the neutrinoless double beta decay of 136Xe, which requires a severe suppression of potential backgrounds; therefore, an extensive screening and selection process is underway to control the radiopurity levels of the materials to be used in the experimental set-up of NEXT. The detector design combines the measurement of the topological signature of the event for background discrimination with the energy resolution optimization. Separate energy and tracking readout planes are based on different sensors: photomultiplier tubes for calorimetry and silicon multi-pixel photon counters for tracking. The design of a radiopure tracking plane, in direct contact with the gas detector medium, was specially challenging since the needed components like printed circuit boards, connectors, sensors or capacitors have typically, according to available information in databases and in the literature, activities too large for experiments requiring ultra-low background conditions. Here, the radiopurity assessment of tracking readout components based on gamma-ray spectroscopy using ultra-low background germanium detectors at the Laboratorio Subterraneo de Canfranc (Spain) is described. According to the obtained results, radiopure enough printed circuit boards made of kapton and copper, silicon photomultipliers and other required components, fulfilling the requirement of an overall background level in the region of interest of at most 8 10-4 counts keV-1 kg-1 y-1, have been identified.
- Published
- 2014
- Full Text
- View/download PDF
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