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19,396 results on '"Lupi A."'

151. Síndrome de Brooke-Spiegler a propósito de un caso clínico

Author

Maria Belen Mendoza Macias, Carminia Rivas Ulunque, Omar Lupi, and Lisseth Carolina Mosquera Castro

Subjects
síndrome de brooke-spiegler, cilindromas, tricoepiteliomas, espiradenomas, Medicine
Abstract

El síndrome de Brooke Spiegler es resultante de la mutación del gen CYLD, con expresión fenotípica variable, es una enfermedad autosómica dominante asociada a múltiples tumores de piel, con predilección por cabeza y cuello. Las lesiones aparecen a temprana edad con progresión en tamaño y número en el transcurso del tiempo; tiene predilección por el sexo femenino. La presentación clínica incluye cilindromas, espiroadenomas, y tricoepiteliomas1,2.

Published
2024
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153. A fatal respiratory complication of malaria caused by Plasmodium vivax

Author

López, Angie R., Martins, Ezequias B., de Pina-Costa, Anielle, Pacheco-Silva, Ana Beatriz, Ferreira, Marcel T., Mamani, Roxana F., Detepo, Paula J. T., Lupi, Otilia, Bressan, Clarisse S., Calvet, Guilherme A., Silva, Michele F. B., de Fátima Ferreira-da-Cruz, Maria, de Bruycker-Nogueira, Fernanda, Filippis, Ana Maria B., Daniel-Ribeiro, Cláudio Tadeu, Siqueira, André, and Brasil, Patrícia

Published
2023
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156. A Europe-wide inventory of citizen-led energy action with data from 29 countries and over 10000 initiatives

Author

Wierling, August, Schwanitz, Valeria Jana, Zeiss, Jan Pedro, von Beck, Constantin, Paudler, Heather Arghandeh, Koren, Ingrid Knutsdotter, Kraudzun, Tobias, Marcroft, Timothy, Müller, Lukas, Andreadakis, Zacharias, Candelise, Chiara, Dufner, Simon, Getabecha, Melake, Glaase, Grete, Hubert, Wit, Lupi, Veronica, Majidi, Sona, Mohammadi, Shirin, Nosar, Negar Safara, du Pont, Yann Robiou, Roots, Philippa, Rudek, Tadeusz Józef, Sciullo, Alessandro, Sehdev, Gayatri, Ziaabadi, Mehran, and Zoubin, Nahid

Published
2023
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157. Astrophysics with the Laser Interferometer Space Antenna

Author

Amaro-Seoane, Pau, Andrews, Jeff, Arca Sedda, Manuel, Askar, Abbas, Baghi, Quentin, Balasov, Razvan, Bartos, Imre, Bavera, Simone S., Bellovary, Jillian, Berry, Christopher P. L., Berti, Emanuele, Bianchi, Stefano, Blecha, Laura, Blondin, Stéphane, Bogdanović, Tamara, Boissier, Samuel, Bonetti, Matteo, Bonoli, Silvia, Bortolas, Elisa, Breivik, Katelyn, Capelo, Pedro R., Caramete, Laurentiu, Cattorini, Federico, Charisi, Maria, Chaty, Sylvain, Chen, Xian, Chruślińska, Martyna, Chua, Alvin J. K., Church, Ross, Colpi, Monica, D’Orazio, Daniel, Danielski, Camilla, Davies, Melvyn B., Dayal, Pratika, De Rosa, Alessandra, Derdzinski, Andrea, Destounis, Kyriakos, Dotti, Massimo, Duţan, Ioana, Dvorkin, Irina, Fabj, Gaia, Foglizzo, Thierry, Ford, Saavik, Fouvry, Jean-Baptiste, Franchini, Alessia, Fragos, Tassos, Fryer, Chris, Gaspari, Massimo, Gerosa, Davide, Graziani, Luca, Groot, Paul, Habouzit, Melanie, Haggard, Daryl, Haiman, Zoltan, Han, Wen-Biao, Istrate, Alina, Johansson, Peter H., Khan, Fazeel Mahmood, Kimpson, Tomas, Kokkotas, Kostas, Kong, Albert, Korol, Valeriya, Kremer, Kyle, Kupfer, Thomas, Lamberts, Astrid, Larson, Shane, Lau, Mike, Liu, Dongliang, Lloyd-Ronning, Nicole, Lodato, Giuseppe, Lupi, Alessandro, Ma, Chung-Pei, Maccarone, Tomas, Mandel, Ilya, Mangiagli, Alberto, Mapelli, Michela, Mathis, Stéphane, Mayer, Lucio, McGee, Sean, McKernan, Berry, Miller, M. Coleman, Mota, David F., Mumpower, Matthew, Nasim, Syeda S., Nelemans, Gijs, Noble, Scott, Pacucci, Fabio, Panessa, Francesca, Paschalidis, Vasileios, Pfister, Hugo, Porquet, Delphine, Quenby, John, Ricarte, Angelo, Röpke, Friedrich K., Regan, John, Rosswog, Stephan, Ruiter, Ashley, Ruiz, Milton, Runnoe, Jessie, Schneider, Raffaella, Schnittman, Jeremy, Secunda, Amy, Sesana, Alberto, Seto, Naoki, Shao, Lijing, Shapiro, Stuart, Sopuerta, Carlos, Stone, Nicholas C., Suvorov, Arthur, Tamanini, Nicola, Tamfal, Tomas, Tauris, Thomas, Temmink, Karel, Tomsick, John, Toonen, Silvia, Torres-Orjuela, Alejandro, Toscani, Martina, Tsokaros, Antonios, Unal, Caner, Vázquez-Aceves, Verónica, Valiante, Rosa, van Putten, Maurice, van Roestel, Jan, Vignali, Christian, Volonteri, Marta, Wu, Kinwah, Younsi, Ziri, Yu, Shenghua, Zane, Silvia, Zwick, Lorenz, Antonini, Fabio, Baibhav, Vishal, Barausse, Enrico, Bonilla Rivera, Alexander, Branchesi, Marica, Branduardi-Raymont, Graziella, Burdge, Kevin, Chakraborty, Srija, Cuadra, Jorge, Dage, Kristen, Davis, Benjamin, de Mink, Selma E., Decarli, Roberto, Doneva, Daniela, Escoffier, Stephanie, Gandhi, Poshak, Haardt, Francesco, Lousto, Carlos O., Nissanke, Samaya, Nordhaus, Jason, O’Shaughnessy, Richard, Portegies Zwart, Simon, Pound, Adam, Schussler, Fabian, Sergijenko, Olga, Spallicci, Alessandro, Vernieri, Daniele, and Vigna-Gómez, Alejandro

Published
2023
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158. Improved calorimetric particle identification in NA62 using machine learning techniques

Author

Cortina Gil, E., Kleimenova, A., Minucci, E., Padolski, S., Petrov, P., Shaikhiev, A., Volpe, R., Fedorko, W., Numao, T., Petrov, Y., Velghe, B., Wong, V. W. S., Yu, M., Bryman, D., Fu, J., Hives, Z., Husek, T., Jerhot, J., Kampf, K., Zamkovsky, M., De Martino, B., Perrin-Terrin, M., Akmete, A. T., Aliberti, R., Khoriauli, G., Kunze, J., Lomidze, D., Peruzzo, L., Vormstein, M., Wanke, R., Dalpiaz, P., Fiorini, M., Mazzolari, A., Neri, I., Norton, A., Petrucci, F., Soldani, M., Wahl, H., Bandiera, L., Cotta Ramusino, A., Gianoli, A., Romagnoni, M., Sytov, A., Iacopini, E., Latino, G., Lenti, M., Lo Chiatto, P., Panichi, I., Parenti, A., Bizzeti, A., Bucci, F., Antonelli, A., Georgiev, G., Kozhuharov, V., Lanfranchi, G., Martellotti, S., Moulson, M., Spadaro, T., Tinti, G., Ambrosino, F., Capussela, T., Corvino, M., D’Errico, M., Di Filippo, D., Fiorenza, R., Giordano, R., Massarotti, P., Mirra, M., Napolitano, M., Rosa, I., Saracino, G., Anzivino, G., Brizioli, F., Imbergamo, E., Lollini, R., Piandani, R., Santoni, C., Barbanera, M., Cenci, P., Checcucci, B., Lubrano, P., Lupi, M., Pepe, M., Piccini, M., Costantini, F., Di Lella, L., Doble, N., Giorgi, M., Giudici, S., Lamanna, G., Lari, E., Pedreschi, E., Sozzi, M., Cerri, C., Fantechi, R., Pontisso, L., Spinella, F., Mannelli, I., D’Agostini, G., Raggi, M., Biagioni, A., Cretaro, P., Frezza, O., Leonardi, E., Lonardo, A., Turisini, M., Valente, P., Vicini, P., Ammendola, R., Bonaiuto, V., Fucci, A., Salamon, A., Sargeni, F., Arcidiacono, R., Bloch-Devaux, B., Boretto, M., Menichetti, E., Migliore, E., Soldi, D., Biino, C., Filippi, A., Marchetto, F., Briano Olvera, A., Engelfried, J., Estrada-Tristan, N., Reyes Santos, M. A., Boboc, P., Bragadireanu, A. M., Ghinescu, S. A., Hutanu, O. E., Bician, L., Blazek, T., Cerny, V., Kucerova, Z., Bernhard, J., Ceccucci, A., Ceoletta, M., Danielsson, H., De Simone, N., Duval, F., Döbrich, B., Federici, L., Gamberini, E., Gatignon, L., Guida, R., Hahn, F., Holzer, E. B., Jenninger, B., Koval, M., Laycock, P., Lehmann Miotto, G., Lichard, P., Mapelli, A., Marchevski, R., Massri, K., Noy, M., Palladino, V., Pinzino, J., Ryjov, V., Schuchmann, S., Venditti, S., Bache, T., Brunetti, M. B., Duk, V., Fascianelli, V., Fry, J. R., Gonnella, F., Goudzovski, E., Henshaw, J., Iacobuzio, L., Kenworthy, C., Lazzeroni, C., Lurkin, N., Newson, F., Parkinson, C., Romano, A., Sanders, J., Sergi, A., Sturgess, A., Swallow, J., Tomczak, A., Heath, H., Page, R., Trilov, S., Angelucci, B., Britton, D., Graham, C., Protopopescu, D., Carmignani, J., Dainton, J. B., Jones, R. W. L., Ruggiero, G., Fulton, L., Hutchcroft, D., Maurice, E., Wrona, B., Conovaloff, A., Cooper, P., Coward, D., Rubin, P., Baeva, A., Baigarashev, D., Emelyanov, D., Enik, T., Falaleev, V., Fedotov, S., Gorshanov, K., Gushchin, E., Kekelidze, V., Kereibay, D., Kholodenko, S., Khotyantsev, A., Korotkova, A., Kudenko, Y., Kurochka, V., Kurshetsov, V., Litov, L., Madigozhin, D., Medvedeva, M., Mefodev, A., Misheva, M., Molokanova, N., Movchan, S., Obraztsov, V., Okhotnikov, A., Ostankov, A., Polenkevich, I., Potrebenikov, Yu., Sadovskiy, A., Semenov, V., Shkarovskiy, S., Sugonyaev, V., Yushchenko, O., and Zinchenko, A.

Published
2023
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159. Customization of hormone therapy in women with autosomal dominant polycystic kidney disease (ADPKD): actionable strategies and future perspectives

Author

Martina Catania, Micaela Petrone, Liliana Italia De Rosa, Rebecca S. Degliuomini, Kristiana Kola, Chiara Lupi, Matteo Brambilla Pisoni, Stefano Salvatore, Massimo Candiani, Giuseppe Vezzoli, and Maria Teresa Sciarrone Alibrandi

Subjects
ADPKD, Contraception, Female sexual hormones, Fertile age, Hormonal therapy, Menopause transition, Internal medicine, RC31-1245, Diseases of the genitourinary system. Urology, RC870-923
Abstract

Autosomal dominant polycystic kidney disease (ADPKD) is the most common genetically inherited kidney disease and the fourth leading cause of renal replacement therapy worldwide. It is characterized by the development of multiple cysts in the kidneys and in other organs, the increase in renal volume and the progressive loss of renal function. ADPKD outcome seems to be sensitive to hormonal fluctuations, particularly those of sex hormones. Despite the limited literature available, this review presents the first comprehensive overview of contraception and hormonal replacement therapy in women with ADPKD, delving into the risks and benefits associated with different contraceptive methods, including hormonal, intrauterine devices, and non-hormonal approaches. It also explores personalized strategies for contraception based on the severity of renal disease and the presence of comorbidities. Although the protective role of female sex hormones in slowing the progression of renal failure is acknowledged, hormonal therapy in women with ADPKD remains intricate and challenging due to its potential impact on liver disease progression. Women with ADPKD typically experience a slower progression of renal disease compared to men, largely influenced by hormonal dynamics. This literature review underscores the importance of a multidisciplinary assessment and a thorough patient discussion to identify the most suitable contraceptive method for each woman affected by polycystic kidney disease.

Published
2024
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161. Measurement of the K+ → π+γγ decay

Author

E. Cortina Gil, A. Kleimenova, E. Minucci, S. Padolski, P. Petrov, A. Shaikhiev, R. Volpe, T. Numao, Y. Petrov, B. Velghe, V.W.S. Wong, D. Bryman, J. Fu, Z. Hives, T. Husek, J. Jerhot, K. Kampf, M. Zamkovsky, B. De Martino, M. Perrin-Terrin, B. Döbrich, S. Lezki, A.T. Akmete, R. Aliberti, G. Khoriauli, J. Kunze, D. Lomidze, L. Peruzzo, M. Vormstein, R. Wanke, P. Dalpiaz, M. Fiorini, A. Mazzolari, I. Neri, A. Norton, F. Petrucci, M. Soldani, H. Wahl, L. Bandiera, A. Cotta Ramusino, A. Gianoli, M. Romagnoni, A. Sytov, E. Iacopini, G. Latino, M. Lenti, P. Lo Chiatto, I. Panichi, A. Parenti, A. Bizzeti, F. Bucci, A. Antonelli, G. Georgiev, V. Kozhuharov, G. Lanfranchi, S. Martellotti, M. Moulson, T. Spadaro, G. Tinti, F. Ambrosino, T. Capussela, M. Corvino, M. D'Errico, D. Di Filippo, R. Fiorenza, R. Giordano, P. Massarotti, M. Mirra, M. Napolitano, I. Rosa, G. Saracino, G. Anzivino, F. Brizioli, E. Imbergamo, R. Lollini, R. Piandani, C. Santoni, M. Barbanera, P. Cenci, B. Checcucci, P. Lubrano, M. Lupi, M. Pepe, M. Piccini, F. Costantini, L. Di Lella, N. Doble, M. Giorgi, S. Giudici, G. Lamanna, E. Lari, E. Pedreschi, M. Sozzi, C. Cerri, R. Fantechi, L. Pontisso, F. Spinella, I. Mannelli, G. D'Agostini, M. Raggi, A. Biagioni, P. Cretaro, O. Frezza, E. Leonardi, A. Lonardo, M. Turisini, P. Valente, P. Vicini, R. Ammendola, V. Bonaiuto, A. Fucci, A. Salamon, F. Sargeni, R. Arcidiacono, B. Bloch-Devaux, M. Boretto, E. Menichetti, E. Migliore, D. Soldi, C. Biino, A. Filippi, F. Marchetto, A. Briano Olvera, J. Engelfried, N. Estrada-Tristan, M.A. Reyes Santos, K.A. Rodriguez Rivera, P. Boboc, A.M. Bragadireanu, S.A. Ghinescu, O.E. Hutanu, L. Bician, T. Blazek, V. Cerny, Z. Kucerova, J. Bernhard, A. Ceccucci, M. Ceoletta, H. Danielsson, N. De Simone, F. Duval, L. Federici, E. Gamberini, L. Gatignon, R. Guida, F. Hahn, E.B. Holzer, B. Jenninger, M. Koval, P. Laycock, G. Lehmann Miotto, P. Lichard, A. Mapelli, R. Marchevski, K. Massri, M. Noy, V. Palladino, J. Pinzino, V. Ryjov, S. Schuchmann, S. Venditti, T. Bache, M.B. Brunetti, V. Duk, V. Fascianelli, J.R. Fry, F. Gonnella, E. Goudzovski, J. Henshaw, L. Iacobuzio, C. Kenworthy, C. Lazzeroni, N. Lurkin, F. Newson, C. Parkinson, A. Romano, J. Sanders, A. Sergi, A. Sturgess, J. Swallow, A. Tomczak, H. Heath, R. Page, S. Trilov, B. Angelucci, D. Britton, C. Graham, D. Protopopescu, J. Carmignani, J.B. Dainton, R.W.L. Jones, G. Ruggiero, L. Fulton, D. Hutchcroft, E. Maurice, B. Wrona, A. Conovaloff, P. Cooper, D. Coward, P. Rubin, A. Baeva, D. Baigarashev, D. Emelyanov, T. Enik, V. Falaleev, S. Fedotov, K. Gorshanov, E. Gushchin, V. Kekelidze, D. Kereibay, S. Kholodenko, A. Khotyantsev, A. Korotkova, Y. Kudenko, V. Kurochka, V. Kurshetsov, L. Litov, D. Madigozhin, M. Medvedeva, A. Mefodev, M. Misheva, N. Molokanova, S. Movchan, V. Obraztsov, A. Okhotnikov, A. Ostankov, I. Polenkevich, Yu. Potrebenikov, A. Sadovskiy, V. Semenov, S. Shkarovskiy, V. Sugonyaev, O. Yushchenko, and A. Zinchenko

Subjects
Physics, QC1-999
Abstract

A sample of 3984 candidates of the K+→π+γγ decay, with an estimated background of 291±14 events, was collected by the NA62 experiment at CERN during 2017–2018. In order to describe the observed di-photon mass spectrum, the next-to-leading order contribution in chiral perturbation theory was found to be necessary. The decay branching ratio in the full kinematic range is measured to be (9.61±0.17)×10−7. The first search for production and prompt decay of an axion-like particle with gluon coupling in the process K+→π+a, a→γγ is also reported.

Published
2024
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162. Characterizing individual differences in children and adolescents with autism spectrum disorder: a descriptive study

Author

S. Di Vara, S. Guerrera, D. Menghini, F. Scibelli, E. Lupi, G. Valeri, and S. Vicari

Subjects
ASD, sex, psychopathology, cognitive, adaptive functioning, Psychology, BF1-990
Abstract

IntroductionAutism Spectrum Disorder (ASD) is a neurodevelopmental disorder characterized by a higher prevalence in male than in female participants. Recent studies have hypothesized the presence of different phenotypes in male and female participants with ASD. The present study aims to assess possible sex differences in cognitive and adaptive functioning, symptomatology of ASD, and psychopathological comorbidities in a large sample of children and adolescents with ASD.MethodsThe study included a total of 2,146 children and adolescents diagnosed with ASD, comprising 1785 boys (mean age 7.12 ± 3.69 years) and 361 girls (mean age 6.25 ± 3.30 years). The age of the participants ranged from 1.35 to 19.05 years (mean age 9.98 ± 3.64). The study sought to include all children and adolescents diagnosed with Autism or ASD.ResultsPresent results showed that girls with ASD had lower IQs than boys but similar adaptive functioning. The severity of symptoms of ASD was greater in boys than in girls, as were scores on psychopathological measures. With increasing age, boys with ASD showed greater impairment in social communication skills than girls and increased psychopathological comorbidities. Older girls showed fewer restricted and repetitive behaviors.DiscussionExploring phenotypic differences in children and adolescents with ASD fosters an understanding of subtle diagnostic facets that may go unrecognized, allowing for increasingly individualized and tailored interventions.

Published
2024
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163. Development and validation of a parameter-free model chemistry for the computation of reliable reaction rates

Author

Barone, Vincenzo, Lupi, Jacopo, Salta, Zoi, and Tasinato, Nicola

Subjects
Physics - Chemical Physics, Physics - Computational Physics
Abstract

A recently developed model chemistry (jun-Cheap) has been slightly modified and proposed as an effective, reliable and parameter-free scheme for the computation of accurate reaction rates with special reference to astrochemical and atmospheric processes. Benchmarks with different sets of state-of-the-art energy barriers spanning a wide range of values show that, in the absence of strong multi-reference contributions, the proposed model outperforms the most well-known model chemistries, reaching a sub-chemical accuracy without any empirical parameter and with affordable computer times. Some test cases show that geometries, energy barriers, zero point energies and thermal contributions computed at this level can be used in the framework of the master equation approach based on ab-initio transition state theory (AITSTME) for obtaining accurate reaction rates., Comment: JCTC

Published
2021

164. The AGORA High-resolution Galaxy Simulations Comparison Project. III: Cosmological zoom-in simulation of a Milky Way-mass halo

Author

Roca-Fàbrega, Santi, Kim, Ji-hoon, Hausammann, Loic, Nagamine, Kentaro, Powell, Johnny W., Shimizu, Ikkoh, Ceverino, Daniel, Lupi, Alessandro, Primack, Joel R., Quinn, Thomas, Revaz, Yves, Velázquez, Héctor, Abel, Tom, Buehlmann, Michael, Dekel, Avishai, Dong, Bili, Hahn, Oliver, Hummels, Cameron B., Kim, Ki-won, Smith, Britton D., Strawn, Clayton J., Teyssier, Romain, and Turk, Matthew

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

We present a suite of high-resolution cosmological zoom-in simulations to $z=4$ of a $10^{12}\,{\rm M}_{\odot}$ halo at $z=0$, obtained using seven contemporary astrophysical simulation codes widely used in the numerical galaxy formation community. Physics prescriptions for gas cooling, heating, and star formation, are similar to the ones used in our previous {\it AGORA} disk comparison but now account for the effects of cosmological processes. In this work, we introduce the most careful comparison yet of galaxy formation simulations run by different code groups, together with a series of four calibration steps each of which is designed to reduce the number of tunable simulation parameters adopted in the final run. After all the participating code groups successfully completed the calibration steps, we reach a suite of cosmological simulations with similar mass assembly histories down to $z=4$. With numerical accuracy that resolves the internal structure of a target halo, we find that the codes overall agree well with one another in e.g., gas and stellar properties, but also show differences in e.g., circumgalactic medium properties. We argue that, if adequately tested in accordance with our proposed calibration steps and common parameters, the results of high-resolution cosmological zoom-in simulations can be robust and reproducible. New code groups are invited to join this comparison by generating equivalent models by adopting the common initial conditions, the common easy-to-implement physics package, and the proposed calibration steps. Further analyses of the simulations presented here will be in forthcoming reports from our Collaboration., Comment: Accepted for publication to the ApJ. The simulation snapshots used in this paper will be made publicly available in a user-friendly interface. The announcement of the data release will be posted on the AGORA Project webpage (www.agorasimulations.org). Early access to the data can be provided upon request to the authors, or to the project coordinator (sroca01@ucm.es, santacruzgalaxy@gmail.com)

Published
2021
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165. First demonstration of in-beam performance of bent Monolithic Active Pixel Sensors

Author

project, ALICE ITS, Rinella, G. Aglieri, Agnello, M., Alessandro, B., Agnese, F., Akram, R. S., Alme, J., Anderssen, E., Andreou, D., Antinori, F., Apadula, N., Atkinson, P., Baccomi, R., Badalà, A., Balbino, A., Bartels, C., Barthel, R., Baruffaldi, F., Belikov, I., Beole, S., Becht, P., Bhatti, A., Bhopal, M., Bianchi, N., Blidaru, M. B., Boca, G., Bok, J., Bonomi, G., Bonora, M., Borri, M., Borshchov, V., Botta, E., Bruno, G. E., Buckland, M., Bufalino, S., Cai, M., Camerini, P., Cariola, P., Catalano, F., Sanchez, C. Ceballos, Chakaberia, I., Chartier, M., Colamaria, F., Colella, D., Collu, A., Concas, M., Contin, G., Costanza, S., Cui, P., Dainese, A., Dainton, J. B., De Cilladi, L., De Martin, C., De Robertis, G., Deng, W., Di Mauro, A., Ding, Y., Durkac, M., Elia, D., Ersdal, M. R., Faggin, M., Fan, F., Fantoni, A., Fecchio, P., Feliciello, A., Feofilov, G., Ferk, A., Ferencei, J., Fiorenza, G., Flores, A. N., Fragiacomo, E., Gajanana, D., Gal, A., Gao, C., Gargiulo, C., Gianotti, P., Giubilato, P., Grant, A., Greiner, L., Grelli, A., Groettvik, O. S., Grosa, F., Hu, C. Guo, Hannigan, R., Hasenbichler, J. A., Helstrup, H., Hillemanns, H., Hills, C., Hindley, P., Hippolyte, B., Hofman, B., Hong, G. H., Huang, G., Iddon, J. P., Ilyas, H., Imhoff, M. A., Isakov, A., Jadlovska, A., Jadlovska, S., Jadlovsky, J., Jaelani, S., Johnson, T., Junique, A., Kalinak, P., Kalweit, A., Keil, M., Khabanova, Z., Khan, H., Kim, B., Kim, C., Kim, J., Kim, T., Klein, J., Kluge, A., Kobdaj, C., Kotliarov, A., Králik, I., Krizek, F., Kugathasan, T., Kuhn, C., Kuijer, P. G., Kushpil, S., Kweon, M. J., Kwon, J. Y., Kwon, Y., La Rocca, P., Lakrathok, A., Langoy, R., Larionov, P., Laudi, E., Lazareva, T., Lea, R., Lemmon, R. C., Li, X. L., Lien, J., Lim, B., Lim, S. H., Lindsay, S., Liu, A., Liu, J., Lunardon, M., Luparello, G., Lupi, M., Mager, M., Maire, A., Malik, Q. W., Mandaglio, G., Manzari, V., Mao, Y., Margagliotti, G. V., Markert, C., Marras, D., Martinengo, P., Masciocchi, S., Masera, M., Masoni, A., Mastroserio, A., Matuoka, P. F. T., Mazza, G., Mazzaschi, F., Mazzoni, M. A., Morel, F, Muccifora, V., Mulliri, A., Musa, L., Nesbo, S. V., Nesterov, D., Norman, J., Park, J., Patra, R. N, Pastore, C., Pei, H., Peng, X., Piano, S., Pinto, C., Pisano, S., Politano, S., Prakasa, E., Prino, F., Protsenko, M., Puccio, M., Rachevski, A., Ramello, L., Rami, F., Ravasenga, I., Rehman, A., Reidt, F., Riggi, F., Røed, K., Röhrich, D., Ronchetti, F., Rosano, A., Rossewij, M. J., Rossi, A., Rui, R., Russo, R., Sadikin, R., Sarritzu, V., Schambach, J., Senyukov, S., Seo, J. J., Shahoyan, R., Shaukat, S., Siddhanta, S., Sitta, M., Snellings, R. J. M., Snoeys, W., Songmoolnak, A., Sonneveld, J., Soramel, F., Suljic, M., Sumowidagdo, S., Sun, D., Sun, X., Tambave, G. J., Tersimonov, G., Tkacik, M., Toppi, M., Trifiró, A., Trogolo, S., Trubnikov, V., Turrisi, R., Tveter, T. S., Tymchuck, I., Ullaland, K., Urioni, M., Usai, G. L., Valle, N., van Doremalen, L. V. R., Vanat, T., Van Hoorne, J. W., Varga-Kofarago, M., Velure, A., Wang, D., Wang, Y., Wikne, J., Wright, J. R., Xu, R., Yang, P., Yin, Z., Yoo, I. -K., Yoon, J. H., Yuan, S., Zaccolo, V., Zhang, E., Zhang, X., Zherebchevskii, V., Zhou, D., Zhu, J., Zhu, Y., Zinovjev, G., and Zurlo, N.

Subjects
Physics - Instrumentation and Detectors
Abstract

A novel approach for designing the next generation of vertex detectors foresees to employ wafer-scale sensors that can be bent to truly cylindrical geometries after thinning them to thicknesses of 20-40$\mu$m. To solidify this concept, the feasibility of operating bent MAPS was demonstrated using 1.5$\times$3cm ALPIDE chips. Already with their thickness of 50$\mu$m, they can be successfully bent to radii of about 2cm without any signs of mechanical or electrical damage. During a subsequent characterisation using a 5.4GeV electron beam, it was further confirmed that they preserve their full electrical functionality as well as particle detection performance. In this article, the bending procedure and the setup used for characterisation are detailed. Furthermore, the analysis of the beam test, including the measurement of the detection efficiency as a function of beam position and local inclination angle, is discussed. The results show that the sensors maintain their excellent performance after bending to radii of 2cm, with detection efficiencies above 99.9% at typical operating conditions, paving the way towards a new class of detectors with unprecedented low material budget and ideal geometrical properties.

Published
2021

166. Chemical analysis of prestellar cores in Ophiuchus yields short timescales and rapid collapse

Author

Bovino, Stefano, Lupi, Alessandro, Giannetti, Andrea, Sabatini, Giovanni, Schleicher, Dominik R. G., Wyrowski, Friedrich, and Menten, Karl M.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

Sun-like stars form from the contraction of cold and dense interstellar clouds. How the collapse proceeds and what are the main physical processes driving it, however, is still under debate and a final consensus on the timescale of the process has not been reached. Does this contraction proceed slowly, sustained by strong magnetic fields and ambipolar diffusion, or is it driven by fast collapse with gravity dominating the entire process? One way to answer this question is to measure the age of prestellar cores through statistical methods based on observations or via reliable chemical chronometers, which should better reflect the physical conditions of the cores. Here we report APEX observations of ortho-H$_2$D$^+$ and para-D$_2$H$^+$ for six cores in the Ophiuchus complex and combine them with detailed three-dimensional magneto-hydrodynamical simulations including chemistry, providing a range of ages for the observed cores up to 200 kyr. The outcome of our simulations and subsequent analysis provides a good match with the observational results in terms of physical (core masses and volume densities) and dynamical parameters such as the Mach number and the virial parameter. We show that models of fast collapse successfully reproduce the observed range of chemical abundance ratios as the timescales to reach the observed stages is comparable to the dynamical time of the cores (i.e. the free-fall time) and much shorter than the ambipolar diffusion time, measured from the electron fraction in the simulations. To confirm that this ratio can be used to distinguish between different star-formation scenarios a larger (statistically relevant) sample of star-forming cores should be explored., Comment: submitted to A&A, 12 pages, 5 figures, 4 tables

Published
2021
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167. Chemical post-processing of magneto-hydrodynamical simulations of star-forming regions: robustness and pitfalls

Author

Ferrada-Chamorro, Simón, Lupi, Alessandro, and Bovino, Stefano

Subjects
Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

A common approach to model complex chemistry in numerical simulations is via post-processing of existing magneto-hydrodynamic simulations, relying on computing the evolution of chemistry over the dynamic history of a subset of particles from within the raw simulation. Here, we validate such a technique, assessing its ability to recover the abundances of chemical species, using the chemistry package KROME. We also assess, for the first time, the importance of the main free input parameters, by means of a direct comparison with a self-consistent state-of-the-art simulation in which chemistry was directly coupled to hydrodynamics. We have found that the post-processing is highly reliable, with an accuracy at the percent level, even when the most relaxed input parameters are employed. In particular, our results show that the number of particles used does not affect significantly the average properties, although it suppresses the appearance of possibly important spatial features. On the other hand, the choice of the integration time-step plays a crucial role. Longer integration time-steps can produce large errors, as the post-processing solution will be forced towards chemical equilibrium, a condition that does not always necessarily apply. When the interpolation-based reconstruction of chemical properties is performed, the errors further increase up to a factor of $\sim2$. Concluding, our results suggest that this technique is extremely useful when exploring the relative quantitative effect of different chemical parameters and/or networks, without the need of re-running simulations multiple times, but some care should be taken in the choice of particles sub-sample and integration time-step., Comment: 11 pages, 6 figures, 3 tables

Published
2021
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168. Intermediate dose enoxaparin in hospitalized patients with moderate-severe COVID-19: a pilot phase II single-arm study, INHIXACOVID19

Author

B. Cosmi, M. Giannella, G. Fornaro, F. Cristini, A. Patacca, A. Castagna, F. Mazzaferri, S. Testa, A. Pan, M. Lupi, P. Brambilla, A. Montineri, S. Frattima, E. G. Bignami, M. Salvetti, G. De Stefano, E. Grandone, G. Di Perri, R. Rozzini, A. Stella, A. Romagnoli, F. Drago, and P. Viale

Subjects
COVID-19, Enoxaparin, Venous thromboembolism, Thromboprofilaxis, Major bleeding, Infectious and parasitic diseases, RC109-216
Abstract

Abstract Background Randomized clinical trials in non-critically ill COVID-19 patients showed that therapeutic-dose heparin increased survival with reduced organ support as compared with usual-care thromboprophylaxis, albeit with increased bleeding risk. The purpose of the study is to assess the safety of intermediate dose enoxaparin in hospitalized patients with moderate to severe COVID-19. Methods A phase II single-arm interventional prospective study including patients receiving intermediate dose enoxaparin once daily according to body weight: 60 mg for 45–60 kg, 80 mg for 61–100 kg or 100 mg for > 100 kg for 14 days, with dose adjustment according to anti-factor Xa activity (target range: 0.4–0.6 UI/ml); an observational cohort (OC) included patients receiving enoxaparin 40 mg day for comparison. Follow-up was 90 days. Primary outcome was major bleeding within 30 and 90 days after treatment onset. Secondary outcome was the composite of all-cause 30 and 90-day mortality rates, disease severity at the end of treatment, intensive care unit (ICU) admission and length of ICU stay, length of hospitalization. All outcomes were adjudicated by an independent committee and analyzed before and after propensity score matching (PSm). Results Major bleeding was similar in IC (1/98 1.02%) and in the OC (none), with only one event observed in a patient receiving concomitantly anti-platelet therapy. The composite outcome was observed in 53/98 patients (54%) in the IC and 132/203 (65%) patients in the OC (p = 0.07) before PSm, while it was observed in 50/90 patients (55.6%) in the IC and in 56/90 patients (62.2%) in the OC after PSm (p = 0.45). Length of hospitalization was lower in the IC than in OC [median 13 (IQR 8–16) vs 14 (11–21) days, p = 0.001], however it lost statistical significance after PSm (p = 0.08). At 30 days, two patients had venous thrombosis and two pulmonary embolism in the OC. Time to first negative RT-PCR were similar in the two groups. Conclusions Weight adjusted intermediate dose heparin with anti-FXa monitoring is safe with potential positive impact on clinical course in COVID-19 non-critically ill patients. Trial registration The study INHIXACOVID19 was registred on ClinicalTrials.gov with the trial registration number (TRN) NCT04427098 on 11/06/2020.

Published
2023
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169. A fatal respiratory complication of malaria caused by Plasmodium vivax

Author

Angie R. López, Ezequias B. Martins, Anielle de Pina-Costa, Ana Beatriz Pacheco-Silva, Marcel T. Ferreira, Roxana F. Mamani, Paula J. T. Detepo, Otilia Lupi, Clarisse S. Bressan, Guilherme A. Calvet, Michele F. B. Silva, Maria de Fátima Ferreira-da-Cruz, Fernanda de Bruycker-Nogueira, Ana Maria B. Filippis, Cláudio Tadeu Daniel-Ribeiro, André Siqueira, and Patrícia Brasil

Subjects
Malaria, Plasmodium vivax, Respiratory, Fatal complication, Arctic medicine. Tropical medicine, RC955-962, Infectious and parasitic diseases, RC109-216
Abstract

Abstract Background Malaria is endemic and represents an important public health issue in Brazil. Knowledge of risk factors for disease progression represents an important step in preventing and controlling malaria-related complications. Reports of severe forms of Plasmodium vivax malaria are now becoming a common place, but respiratory complications are described in less than 3% of global literature on severe vivax malaria. Case presentation A severe respiratory case of imported vivax malaria in a previously healthy 40-year-old woman has been reported. The patient died after the fifth day of treatment with chloroquine and primaquine due to acute respiratory distress syndrome. Conclusions Respiratory symptoms started 48 h after the initiation of anti-malarial drugs, raising the hypothesis that the drugs may have been involved in the genesis of the complication. The concept that vivax malaria is a benign disease that can sometimes result in the development of serious complications must be disseminated. This report highlights, once more, the crucial importance of malaria early diagnosis, a true challenge in non-endemic areas, where health personnel are not familiar with the disease and do not consider its diagnosis promptly.

Published
2023
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170. Impact of the COVID-19 Pandemic on Iron Overload Assessment by MRI in Patients with Hemoglobinopathies: The E-MIOT Network Experience

Author

Antonella Meloni, Laura Pistoia, Amalia Lupi, Riccardo Righi, Antonino Vallone, Massimiliano Missere, Stefania Renne, Priscilla Fina, Ada Riva, Maria Rita Gamberini, Valerio Cecinati, Francesco Sorrentino, Rosamaria Rosso, Giuseppe Messina, Paolo Ricchi, Vincenzo Positano, Sophie Mavrogeni, Emilio Quaia, Filippo Cademartiri, and Alessia Pepe

Subjects
COVID-19, iron overload, magnetic resonance imaging, Computer applications to medicine. Medical informatics, R858-859.7
Abstract

Background. The E-MIOT (Extension-Myocardial Iron Overload in Thalassemia) project is an Italian Network assuring high-quality quantification of tissue iron overload by magnetic resonance imaging (MRI). We evaluated the impact of the COVID-19 pandemic on E-MIOT services. Methods. The activity of the E-MIOT Network MRI centers in the year 2020 was compared with that of 2019. A survey evaluated whether the availability of MRI slots for patients with hemoglobinopathies was reduced and why. Results. The total number of MRI scans was 656 in 2019 and 350 in 2020, with an overall decline of 46.4% (first MRI: 71.7%, follow-up MRI: 36.9%), a marked decline (86.9%) in the period March–June 2020, and a reduction in the gap between the two years in the period July–September. A new drop (41.4%) was recorded in the period October–December for two centers, due to the general reduction in the total amount of MRIs/day for sanitization procedures. In some centers, patients refused MRI scans for fear of getting COVID. Drops in the MRI services >80% were found for patients coming from a region without an active MRI site. Conclusions. The COVID-19 pandemic had a strong negative impact on MRI multi-organ iron quantification, with a worsening in the management of patients with hemoglobinopathies.

Published
2023
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171. Cubic Fe-bearing majorite synthesized at 18–25 GPa and 1000 °C: implications for element transport, subducted slab rheology and diamond formation

Author

Vincenzo Stagno, Luca Bindi, Barbara Bonechi, Steeve Greaux, Sonja Aulbach, Tetsuo Irifune, Stefano Lupi, Giulia Marras, Catherine A. McCammon, Manuela Nazzari, Federica Piccirilli, Brent Poe, Claudia Romano, and Piergiorgio Scarlato

Subjects
Medicine, Science
Abstract

Abstract The chemistry and mineralogy of slabs subducted into lower mantle control slab rheology and impact the deep volatile cycle. It is known that the metamorphism of little-altered oceanic crust results in eclogite rocks with subequal proportions of garnet and clinopyroxene. With increasing pressure, these minerals react to stabilize pyrope-rich tetragonal majoritic garnet. However, some eclogites contain higher proportions of omphacitic clinopyroxene, caused by Na- and Si-rich metasomatism on the ocean floor or during subduction. The mineralogy of such eclogites is expected to evolve differently. Here, we discuss the results of the crystallization products of omphacitic glass at ~ 18 and ~ 25 GPa and 1000 °C to simulate P–T regimes of cold subduction. The full characterization of the recovered samples indicates evidence of crystallization of Na-, Si-rich cubic instead of tetragonal majorite. This cubic majorite can incorporate large amounts of ferric iron, promoting redox reactions with surrounding volatile-bearing fluids and, ultimately, diamond formation. In addition, the occurrence of cubic majorite in the slab would affect the local density, favoring the continued buoyancy of the slab as previously proposed by seismic observations. Attention must be paid to omphacitic inclusions in sublithospheric diamonds as these might have experienced back-transformation from the HP isochemical cubic phase.

Published
2023
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172. A study of the K + → π 0 e + νγ decay

Author

The NA62 collaboration, E. Cortina Gil, A. Kleimenova, E. Minucci, S. Padolski, P. Petrov, A. Shaikhiev, R. Volpe, T. Numao, Y. Petrov, B. Velghe, V. W. S. Wong, D. Bryman, J. Fu, Z. Hives, T. Husek, J. Jerhot, K. Kampf, M. Zamkovsky, B. De Martino, M. Perrin-Terrin, A. T. Akmete, R. Aliberti, G. Khoriauli, J. Kunze, D. Lomidze, L. Peruzzo, M. Vormstein, R. Wanke, P. Dalpiaz, M. Fiorini, A. Mazzolari, I. Neri, A. Norton, F. Petrucci, M. Soldani, H. Wahl, L. Bandiera, A. Cotta Ramusino, A. Gianoli, M. Romagnoni, A. Sytov, E. Iacopini, G. Latino, M. Lenti, P. Lo Chiatto, I. Panichi, A. Parenti, A. Bizzeti, F. Bucci, A. Antonelli, G. Georgiev, V. Kozhuharov, G. Lanfranchi, S. Martellotti, M. Moulson, T. Spadaro, G. Tinti, F. Ambrosino, T. Capussela, M. Corvino, M. D’Errico, D. Di Filippo, R. Fiorenza, R. Giordano, P. Massarotti, M. Mirra, M. Napolitano, I. Rosa, G. Saracino, G. Anzivino, F. Brizioli, E. Imbergamo, R. Lollini, R. Piandani, C. Santoni, M. Barbanera, P. Cenci, B. Checcucci, P. Lubrano, M. Lupi, M. Pepe, M. Piccini, F. Costantini, L. Di Lella, N. Doble, M. Giorgi, S. Giudici, G. Lamanna, E. Lari, E. Pedreschi, M. Sozzi, C. Cerri, R. Fantechi, L. Pontisso, F. Spinella, I. Mannelli, G. D’Agostini, M. Raggi, A. Biagioni, P. Cretaro, O. Frezza, E. Leonardi, A. Lonardo, M. Turisini, P. Valente, P. Vicini, R. Ammendola, V. Bonaiuto, A. Fucci, A. Salamon, F. Sargeni, R. Arcidiacono, B. Bloch-Devaux, M. Boretto, E. Menichetti, E. Migliore, D. Soldi, C. Biino, A. Filippi, F. Marchetto, A. Briano Olvera, J. Engelfried, N. Estrada-Tristan, M. A. Reyes Santos, P. Boboc, A. M. Bragadireanu, S. A. Ghinescu, O. E. Hutanu, L. Bician, T. Blazek, V. Cerny, Z. Kucerova, J. Bernhard, A. Ceccucci, M. Ceoletta, H. Danielsson, N. De Simone, F. Duval, B. Döbrich, L. Federici, E. Gamberini, L. Gatignon, R. Guida, F. Hahn, E. B. Holzer, B. Jenninger, M. Koval, P. Laycock, G. Lehmann Miotto, P. Lichard, A. Mapelli, R. Marchevski, K. Massri, M. Noy, V. Palladino, J. Pinzino, V. Ryjov, S. Schuchmann, S. Venditti, T. Bache, M. B. Brunetti, V. Duk, V. Fascianelli, J. R. Fry, F. Gonnella, E. Goudzovski, J. Henshaw, L. Iacobuzio, C. Kenworthy, C. Lazzeroni, N. Lurkin, F. Newson, C. Parkinson, A. Romano, J. Sanders, A. Sergi, A. Sturgess, J. Swallow, A. Tomczak, H. Heath, R. Page, S. Trilov, B. Angelucci, D. Britton, C. Graham, D. Protopopescu, J. Carmignani, J. B. Dainton, R. W. L. Jones, G. Ruggiero, L. Fulton, D. Hutchcroft, E. Maurice, B. Wrona, A. Conovaloff, P. Cooper, D. Coward, P. Rubin, A. Baeva, D. Baigarashev, D. Emelyanov, T. Enik, V. Falaleev, S. Fedotov, K. Gorshanov, E. Gushchin, V. Kekelidze, D. Kereibay, S. Kholodenko, A. Khotyantsev, A. Korotkova, Y. Kudenko, V. Kurochka, V. Kurshetsov, L. Litov, D. Madigozhin, M. Medvedeva, A. Mefodev, M. Misheva, N. Molokanova, S. Movchan, V. Obraztsov, A. Okhotnikov, A. Ostankov, I. Polenkevich, Yu. Potrebenikov, A. Sadovskiy, V. Semenov, S. Shkarovskiy, V. Sugonyaev, O. Yushchenko, and A. Zinchenko

Subjects
Branching fraction, Electroweak Interaction, Fixed Target Experiments, Flavour Physics, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Abstract A sample of 1.3 × 105 K + → π 0 e + νγ candidates with less than 1% background was collected by the NA62 experiment at the CERN SPS in 2017–2018. Branching fraction measurements are obtained at percent relative precision in three restricted kinematic regions, improving on existing results by a factor larger than two. An asymmetry, possibly related to T-violation, is investigated with no evidence observed within the achieved precision.

Published
2023
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173. Testing the robustness of a structural model for discerning use and non-use values of ecosystem services

Author

Hyunjung Kim, Frank Lupi, and Charles Towe

Subjects
ecosystem services, Monte Carlo simulation, nonmarket valuation, structural estimation, Q57, Q26, C15, C13, Agriculture (General), S1-972, Economic growth, development, planning, HD72-88
Abstract

A theoretically consistent structural model facilitates definition and measurement of use and non-use benefits of ecosystem services. Unlike many previous approaches that utilize multiple stated choice situations, we apply this conceptual framework to a travel cost random utility model and a consequential single referendum contingent valuation research design for simultaneously estimating use and non-use willingness to pay for environmental quality improvement. We employ Monte Carlo generated data to evaluate properties of key parameters and examine the robustness of this method of measuring use and non-use values associated with quality change. The simulation study confirms that this new method, combined with simulated revealed and stated preference data can generally, but not always, be applied to successfully identify use and non-use values of various ecosystems while consistency is ensured.

Published
2023
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175. Prediction of Mortality and Heart Failure Hospitalization After Transcatheter Tricuspid Valve Interventions: Validation of TRISCORE

Author

Adamo, Marianna, Russo, Giulio, Pagnesi, Matteo, Pancaldi, Edoardo, Alessandrini, Hannes, Andreas, Martin, Badano, Luigi P., Braun, Daniel, Connelly, Kim A., Denti, Paolo, Estevez-Loureiro, Rodrigo, Fam, Neil, Gavazzoni, Mara, Hahn, Rebecca T., Harr, Claudia, Hausleiter, Joerg, Himbert, Dominique, Kalbacher, Daniel, Ho, Edwin, Latib, Azeem, Lubos, Edith, Ludwig, Sebastian, Lupi, Laura, Lurz, Philipp, Monivas, Vanessa, Nickenig, Georg, Pedicino, Daniela, Pedrazzini, Giovanni, Pozzoli, Alberto, Marafon, Denise Pires, Pastorino, Roberta, Praz, Fabien, Rodes-Cabau, Joseph, Besler, Christian, Schöber, Anne Rebecca, Schofer, Joachim, Scotti, Andrea, Piayda, Kerstin, Sievert, Horst, Tang, Gilbert H.L., Sticchi, Alessandro, Messika-Zeitoun, David, Thiele, Holger, Schlotter, Florian, von Bardeleben, Ralph Stephan, Webb, John, Dreyfus, Julien, Windecker, Stephan, Leon, Martin, Maisano, Francesco, Metra, Marco, and Taramasso, Maurizio

Published
2024
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178. The role of bars on the dynamical-friction driven inspiral of massive perturbers

Author

Bortolas, Elisa, Bonetti, Matteo, Dotti, Massimo, Lupi, Alessandro, Capelo, Pedro R., Mayer, Lucio, and Sesana, Alberto

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics, 85A05
Abstract

In this paper, we systematically explore the impact of a galactic bar on the inspiral time-scale of a massive object (MO) within a Milky Way-like galaxy. We integrate the orbit of MOs in a multi-component galaxy model via a semi-analytical approach that accounts for dynamical friction generalized to rotationally supported backgrounds. We compare the MO evolution in a galaxy featuring a Milky Way-like rotating bar to the evolution within an analogous axisymmetric galaxy without the bar. In agreement with previous studies, we find that the bar presence may significantly affect the inspiral, sometimes making it shorter by a factor of a few, sometimes hindering it for a Hubble time. The erratic behaviour is mainly impacted by the relative phase at which the MO encounters the stronger bar-induced resonances. In particular, the effect of the bar is more prominent for initially in-plane, prograde MOs, especially those crossing the bar co-rotation radius or outer Lindblad resonance. In the barred galaxy, we find the sinking of the most massive MOs (>~10^7.5 Msun) approaching the galaxy from large separations (>~8 kpc) to be most efficiently hampered. Neglecting the effect of global torques associated with the non-symmetric mass distribution is thus not advisable even within an idealized, smooth galaxy model; we further note that spiral patterns are unlikely to affect the inspiral due to their transient and fluctuating nature. We speculate that the sinking efficiency of massive black holes involved in minor galaxy mergers may be hampered in barred galaxies, making them less likely to host a gravitational wave signal accessible to low-frequency detectors., Comment: 19 pages, 12 figures, 2 tables. MNRAS, accepted

Published
2021
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179. Hyperbolic Metamaterials via Hierarchical Block Copolymer Nanostructures

Author

Murataj, I., Channab, M., Cara, E., Pirri, C. F., Boarino, L., Angelini, A., and Lupi, F. Ferrarese

Subjects
Condensed Matter - Materials Science, Physics - Optics
Abstract

Hyperbolic metamaterials (HMMs) offer unconventional properties in the field of optics, enabling opportunities for confinement and propagation of light at the nanoscale. In-plane orientation of the optical axis, in the direction coinciding with the anisotropy of the HMMs, is desirable for a variety of novel applications in nanophotonics and imaging. Here, a method for creating localized HMMs with in-plane optical axis, based on block copolymer (BCP) blend instability, is introduced. The dewetting of BCP thin film over topographically defined substrates generates droplets composed of highly ordered lamellar nanostructures in hierarchical configuration. The hierarchical nanostructures represent a valuable platform for the subsequent pattern transfer into a Au/air HMM, exhibiting hyperbolic behavior in a broad wavelength range in the visible spectrum. A computed Purcell factor as high as 32 at 580 nm supports the strong reduction in the fluorescence lifetime of defects in nanodiamonds placed on top of the HMM., Comment: This is the pre-peer reviewed version of the following article: I. Murataj et al. Adv. Optical Mater. 2021, 2001933, which has been published in final form at https://doi.org/10.1002/adom.202001933. This article may be used for non-commercial purposes in accordance with Wiley Terms and Conditions for Use of Self-Archived Versions

Published
2021
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180. Forming massive seed black holes in high-redshift quasar host progenitors

Author

Lupi, Alessandro, Haiman, Zoltan, and Volonteri, Marta

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The presence of massive black holes (BHs) with masses of order $10^9\rm\, M_\odot$, powering bright quasars when the Universe was less than 1 Gyr old, poses strong constraints on their formation mechanism. Several scenarios have been proposed to date to explain massive BH formation, from the low-mass seed BH remnants of the first generation of stars to the massive seed BHs resulting from the rapid collapse of massive gas clouds. However, the plausibility of some of these scenarios to occur within the progenitors of high-z quasars has not yet been thoroughly explored. In this work, we investigate, by combining dark-matter only N-body simulations with a semi-analytic framework, whether the conditions for the formation of massive seed BHs from synchronised atomic-cooling halo pairs and/or dynamically-heated mini-haloes are fulfilled in the overdense regions where the progenitors of a typical high-redshift quasar host form and evolve. Our analysis shows that the peculiar conditions in such regions, i.e. strong halo clustering and high star formation rates, are crucial to produce a non-negligible number of massive seed BH host candidates: we find $\approx1400$ dynamically heated metal-free mini-haloes, including one of these which evolves to a synchronised pair and ends up in the massive quasar-host halo by $z=6$. This demonstrates that the progenitors of high-redshift quasar host haloes can harbour early massive seed BHs. Our results further suggest that multiple massive seed BHs may form in or near the quasar host's progenitors, potentially merging at lower redshifts and yielding gravitational wave events., Comment: 16 pages, 9 figures, 3 tables, matches the published version

Published
2021
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182. Business Models Definition for Next-Generation Vision Inspection Systems

Author

Francesco Lupi, Antonio Maffei, and Michele Lanzetta

Subjects
visual inspection, flexibility, reconfigurability, autonomy, manufacturing, business model, Production capacity. Manufacturing capacity, T58.7-58.8
Abstract

Automated industrial Visual Inspection Systems (VIS) are predominantly designed for specific use cases, resulting in constrained adaptability, high setup requirements, substantial capital investments, and significant knowledge barriers. This paper explores the business potential of recent alternative architectures proposed in the literature for the visual inspection of individual products or complex assemblies within highly variable production environments, utilizing next-generation VIS. These advanced VIS exhibit significant technical (hardware and software) enhancements, such as increased flexibility, reconfigurability, Computer Aided Design (CAD)-based integration, self-X capabilities, and autonomy, as well as economic improvements, including cost-effectiveness, non-invasiveness, and plug-and-produce capabilities. The new trends in VIS have the potential to revolutionize business models by enabling as-a-service approaches and facilitating a paradigm shift towards more sustainable manufacturing and human-centric practices. We extend the discussion to examine how these technological innovations, which reduce the need for extensive coding skills and lengthy reconfiguration activities for operators, can be implemented as a shared resource within a circular lifecycle. This analysis includes detailing the underlying business model that supports shared utilization among different stakeholders, promoting a circular economy in manufacturing by leveraging the capabilities of next-generation VIS. Such an approach not only enhances the sustainability of manufacturing processes but also democratizes access to state-of-the-art inspection technologies, thereby expanding the possibilities for autonomous manufacturing ecosystems.

Published
2024
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183. Aloe vera―An Extensive Review Focused on Recent Studies

Author

Alessia Catalano, Jessica Ceramella, Domenico Iacopetta, Maria Marra, Filomena Conforti, Francesca R. Lupi, Domenico Gabriele, Fernanda Borges, and Maria Stefania Sinicropi

Subjects
Aloe vera L., biological activities, chemical composition, toxicological aspects, Chemical technology, TP1-1185
Abstract

Since ancient times, Aloe vera L. (AV) has attracted scientific interest because of its multiple cosmetic and medicinal properties, attributable to compounds present in leaves and other parts of the plant. The collected literature data show that AV and its products have a beneficial influence on human health, both by topical and oral use, as juice or an extract. Several scientific studies demonstrated the numerous biological activities of AV, including, for instance, antiviral, antimicrobial, antitumor, and antifungal. Moreover, its important antidepressant activity in relation to several diseases, including skin disorders (psoriasis, acne, and so on) and prediabetes, is a growing field of research. This comprehensive review intends to present the most significant and recent studies regarding the plethora of AV’s biological activities and an in-depth analysis exploring the component/s responsible for them. Moreover, its morphology and chemical composition are described, along with some studies regarding the single components of AV available in commerce. Finally, valorization studies and a discussion about the metabolism and toxicological aspects of this “Wonder Plant” are reported.

Published
2024
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184. Anisotropic Optical Response of Ti-Doped VO2 Single Crystals

Author

Salvatore Macis, Lorenzo Mosesso, Annalisa D’Arco, Andrea Perucchi, Paola Di Pietro, and Stefano Lupi

Subjects
vanadium oxide, VO2, Ti doping, anisotropy, infrared spectroscopy, Technology, Electrical engineering. Electronics. Nuclear engineering, TK1-9971, Engineering (General). Civil engineering (General), TA1-2040, Microscopy, QH201-278.5, Descriptive and experimental mechanics, QC120-168.85
Abstract

This study delves into the effects of titanium (Ti) doping on the optical properties of vanadium dioxide (VO2), a material well known for its metal–to–insulator transition (MIT) near room temperature. By incorporating Ti into VO2’s crystal lattice, we aim to uncover the resultant changes in its physical properties, crucial for enhancing its application in smart devices. Utilizing polarized infrared micro–spectroscopy, we examined TixV1−xO2 single crystals with varying Ti concentrations (x = 0.059, x = 0.082, and x = 0.187) across different crystal phases (the conductive rutile phase and insulating monoclinic phases M1 and M2) from the far–infrared to the visible spectral range. Our findings reveal that Ti doping significantly influences the phononic spectra, introducing absorption peaks not attributed to pure VO2 or TiO2. This is especially notable with polarization along the crystal growth axis, mainly in the x = 0.187 sample. Furthermore, we demonstrate that the electronic contribution to optical conductivity in the metallic phase exhibits strong anisotropy, higher along the c axis than the a–b plane. This anisotropy, coupled with the progressive broadening of the zone center infrared active phonon modes with increasing doping, highlights the complex interplay between structural and electronic dynamics in doped VO2. Our results underscore the potential of Ti doping in fine-tuning VO2’s electronic and thermochromic properties, paving the way for its enhanced application in optoelectronic devices and technologies.

Published
2024
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185. Nanofibrous Conductive Sensor for Limonene: One-Step Synthesis via Electrospinning and Molecular Imprinting

Author

Antonella Macagnano, Fabricio Nicolas Molinari, Paolo Papa, Tiziana Mancini, Stefano Lupi, Annalisa D’Arco, Anna Rita Taddei, Simone Serrecchia, and Fabrizio De Cesare

Subjects
molecular imprinting polymer-MIP, molecularly imprinted nanofibers-MINF, electrospinning, PVP-PAA-MWCNT composite sensor, BVOCs, terpenes, Chemistry, QD1-999
Abstract

Detecting volatile organic compounds (VOCs) emitted from different plant species and their organs can provide valuable information about plant health and environmental factors that affect them. For example, limonene emission can be a biomarker to monitor plant health and detect stress. Traditional methods for VOC detection encounter challenges, prompting the proposal of novel approaches. In this study, we proposed integrating electrospinning, molecular imprinting, and conductive nanofibers to fabricate limonene sensors. In detail, polyvinylpyrrolidone (PVP) and polyacrylic acid (PAA) served here as fiber and cavity formers, respectively, with multiwalled carbon nanotubes (MWCNT) enhancing conductivity. We developed one-step monolithic molecularly imprinted fibers, where S(−)-limonene was the target molecule, using an electrospinning technique. The functional cavities were fixed using the UV curing method, followed by a target molecule washing. This procedure enabled the creation of recognition sites for limonene within the nanofiber matrix, enhancing sensor performance and streamlining manufacturing. Humidity was crucial for sensor working, with optimal conditions at about 50% RH. The sensors rapidly responded to S(−)-limonene, reaching a plateau within 200 s. Enhancing fiber density improved sensor performance, resulting in a lower limit of detection (LOD) of 137 ppb. However, excessive fiber density decreased accessibility to active sites, thus reducing sensitivity. Remarkably, the thinnest mat on the fibrous sensors created provided the highest selectivity to limonene (Selectivity Index: 72%) compared with other VOCs, such as EtOH (used as a solvent in nanofiber development), aromatic compounds (toluene), and two other monoterpenes (α-pinene and linalool) with similar structures. These findings underscored the potential of the proposed integrated approach for selective VOC detection in applications such as precision agriculture and environmental monitoring.

Published
2024
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186. The Potential Role of Viral Persistence in the Post-Acute Sequelae of SARS-CoV-2 Infection (PASC)

Author

Lorenzo Lupi, Adriana Vitiello, Cristina Parolin, Arianna Calistri, and Alfredo Garzino-Demo

Subjects
post-acute sequelae of SARS-CoV-2, SARS-CoV-2 persistence, dysbiosis, PASC, Medicine
Abstract

The infection by severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2) is associated not only with the development of acute disease but also with long-term symptoms or post-acute sequelae of SARS-CoV-2 (PASC). Multiple lines of evidence support that some viral antigens and RNA can persist for up to 15 months in multiple organs in the body, often after apparent clearance from the upper respiratory system, possibly leading to the persistence of symptoms. Activation of the immune system to viral antigens is observed for a prolonged time, providing indirect evidence of the persistence of viral elements after acute infection. In the gastrointestinal tract, the persistence of some antigens could stimulate the immune system, shaping the local microbiota with potential systemic effects. All of these interactions need to be investigated, taking into account predisposing factors, multiplicity of pathogenic mechanisms, and stratifying populations of vulnerable individuals, particularly women, children, and immunocompromised individuals, where SARS-CoV-2 may present additional challenges.

Published
2024
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187. A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).IX. The effects of ram pressure stripping down to the scale of individual HII regions in the dwarf galaxy IC 3476

Author

Boselli, A., Lupi, A., Epinat, B., Amram, P., Fossati, M., Anderson, J. P., Boissier, S., Boquien, M., Consolandi, G., Cote, P., Cuillandre, J. C., Ferrarese, L., Galbany, L., Gavazzi, G., Gomez-Lopez, J. A., Gwyn, S., Hensler, G., Hutchings, J., Kuncarayakti, H., Longobardi, A., Peng, E. W., Plana, H., Postma, J., Roediger, J., Roehlly, Y., Schimd, C., Trinchieri, G., and Vollmer, B.

Subjects
Astrophysics - Astrophysics of Galaxies
Abstract

We study the IB(s)m galaxy IC 3476 observed in the context of VESTIGE, a blind narrow-band Halpha+[NII] imaging survey of the Virgo cluster. The deep narrow-band (NB) image reveals a very pertubed ionised gas distribution, characterised by a prominent banana-shaped structure in the front of the galaxy formed of giant HII regions crossing the stellar disc, with star forming structures at ~8 kpc from the edges of the stellar disc, detected also in a deep FUV ASTROSAT/UVIT image. This particular morphology indicates that the galaxy is undergoing an almost edge-on ram pressure stripping event. The NB image also shows that the star formation activity is totally quenched in the leading edge of the disc, where the gas has been removed during the interaction. The SED fitting analysis indicates that this quenching episode is very recent (~50 Myr), and roughly corresponds to an increase of the star formation activity in the inner regions with respect to what expected for secular evolution. The analysis of these data, whose angular resolution allows the study of the induced effects of the perturbation down to the scale of individual HII regions, also suggests that the increase of the star formation activity is due to the compression of the gas along the stellar disc of the galaxy, which is able to increase its mean electron density and boost the star formation process producing bright HII regions. The hydrodynamic interaction has deeply perturbed the velocity field of the ionised gas component while leaving unaffected that of the stellar disc. The comparison of the data with hydrodynamic simulations accounting for the different gas phases (atomic, molecular, ionised) consistently indicates that the perturbing event is very recent, once again confirming that ram pressure stripping is a violent phenomenon able to perturb on short timescales the evolution of galaxies in rich environments., Comment: Accepted for publication on Astronomy & Astrophysics

Published
2020
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188. Non-isotropic feedback from accreting spinning black holes

Author

Sala, Luca, Cenci, Elia, Capelo, Pedro R., Lupi, Alessandro, and Dotti, Massimo

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

Active galactic nuclei (AGN) are massive black holes (BHs) caught in the act of accreting gas at the centre of their host galaxies. Part of the accreting mass is converted to energy and released into the surrounding medium, in a process loosely referred to as AGN feedback. Most numerical simulations include AGN feedback as a sub-grid model, wherein energy or momentum (or both) is coupled to the nearby gas. In this work, we implement a new momentum-driven model in the hydrodynamics code GIZMO, in which accretion from large scales is mediated by a sub-grid accretion disc model, and gas particles are stochastically kicked over a bi-conical region, to mimic observed kinetic winds. The feedback cone's axis can be set either parallel to the angular momentum of the gas surrounding the BH or to the BH spin direction, which is self-consistently evolved within the accretion-disc model. Using a circumnuclear disc (CND) as a test bed, we find that (i) the conical shape of the outflow is always visible and is weakly dependent on the launching orientation and aperture, resulting in comparable mass inflows and outflows; (ii) the cone's orientation is also similar amongst our tests, and it is not always the same as the initial value, due to the interaction with the CND playing a crucial role in shaping the outflow; and (iii) the velocity of the outflow, instead, differs and strongly depends on the interplay with the CND., Comment: 14 pages, 6 figures, accepted for publication in MNRAS. Updated with published version, minimal changes

Published
2020
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189. Black hole spin evolution in warped accretion discs

Author

Cenci, Elia, Sala, Luca, Lupi, Alessandro, Capelo, Pedro R., and Dotti, Massimo

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena
Abstract

Massive black holes (BHs) inhabiting galactic nuclei can be described by two parameters only, i.e. mass and spin, that change through cosmic time in response to accretion and merger events. While most numerical simulations accurately track the BH mass, spin evolution is rarely taken into account. In this work, we implement and validate a self-consistent sub-grid model for the evolution of the BH mass and spin via gas accretion in the hydrodynamics code GIZMO. The model assumes that accretion from resolved scales does not occur instantaneously, but is mediated by a sub-grid geometrically thin $\alpha$-disc. After validating our model semi-analytically, we test it in an idealized environment consisting of a circumnuclear disc, where gas accretion onto the accretion disc is consistently determined by GIZMO. In the absence of any accretion-related feedback, the spin evolution closely traces that observed in the semi-analytical models and depends on the free parameters of our implementation, such as the initial BH spin, angular momentum of the accretion disc, and the radius at which the gas inflow circularises. In GIZMO, we also couple our model with the biconical-outflow model presented in a companion paper, wherein the feedback axis is always aligned with the BH spin. In this last case, the evolution of the central BH differs significantly from the previous cases, since the feedback process modifies the gas dynamics and its inflow rates from resolved scales. Such an interaction cannot be modeled by simple semi-analytical models and should be treated using full N-body hydrodynamical simulations., Comment: 10 pages, 5 figures, accepted for publication in MNRAS. Updated with published version, minimal changes

Published
2020
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190. Remote Configuration of the ProASIC3 on the ALICE Inner Tracking System Readout Unit

Author

Yuan, Shiming, Alme, Johan, Röhrich, Dieter, Richter, Matthias, Ersdal, Magnus Rentsch, Giubilato, Piero, Rinella, Gianluca Aglieri, Velure, Arild, Lupi, Matteo, and Schambach, Johann Joachim

Subjects
Physics - Instrumentation and Detectors, Electrical Engineering and Systems Science - Systems and Control, High Energy Physics - Experiment
Abstract

A Large Ion Collider Experiment (ALICE) is one of the four major experiments conducted at the CERN Large Hadron Collider (LHC). The ALICE detector is currently undergoing an upgrade for the upcoming Run 3 at the LHC. The new Inner Tracking System (ITS) sub-detector is part of this upgrade. The front-end electronics of the ITS is composed by 192 Readout Units, installed in a radiation environment. Single Event Upsets (SEUs) in the SRAM-based Xilinx Kintex Ultrascale FPGAs used in the ITS readout represent a real concern. To clear SEUs affecting the Kintex configuration memory, a secondary Flash-based Microsemi ProASIC3E (PA3) FPGA is used. This device configures and continuously scrubs the Xilinx FPGA while data-taking is ongoing, which avoids accumulation of SEUs. The communication path to the RUs is via the radiation hard Gigabit Transceiver (GBT) system on 100 m long optical links. The PA3 is reachable via the GBT Slow Control Adapter (GBT-SCA) ASIC using a dedicated JTAG bus driving channel. During the course of Run 3, it is foreseeable that the FPGA design of the PA3 will require upgrades to correct possible issues and add new functionality. It is therefore mandatory that the PA3 itself can be configured remotely, for which a dedicated software tool is needed. This paper presents the design and implementation of the distributed tools to re-configure remotely the PA3 FPGAs.

Published
2020

192. Configuration of an AVS/RS Using a Data-Driven Queueing Network Model

Author

Lupi, Giacomo, Accorsi, Riccardo, Battarra, Ilaria, Manzini, Riccardo, Chaari, Fakher, Series Editor, Gherardini, Francesco, Series Editor, Ivanov, Vitalii, Series Editor, Haddar, Mohamed, Series Editor, Cavas-Martínez, Francisco, Editorial Board Member, di Mare, Francesca, Editorial Board Member, Kwon, Young W., Editorial Board Member, Trojanowska, Justyna, Editorial Board Member, Xu, Jinyang, Editorial Board Member, Galizia, Francesco Gabriele, editor, and Bortolini, Marco, editor

Published
2023
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195. Familial hypercholesterolaemia in children and adolescents from 48 countries: a cross-sectional study

Author

Dharmayat, Kanika Inamdar, Vallejo-Vaz, Antonio J., Stevens, Christophe A.T., Brandts, Julia M., Lyons, Alexander R.M., Groselj, Urh, Abifadel, Marianne, Aguilar-Salinas, Carlos A., Alhabib, Khalid, Alkhnifsawi, Mutaz, Almahmeed, Wael, Alnouri, Fahad, Alonso, Rodrigo, Al-Rasadi, Khalid, Ashavaid, Tester F., Banach, Maciej, Béliard, Sophie, Binder, Christoph, Bourbon, Mafalda, Chlebus, Krzysztof, Corral, Pablo, Cruz, Diogo, Descamps, Olivier S., Drogari, Euridiki, Durst, Ronen, Ezhov, Marat V., Genest, Jacques, Harada-Shiba, Mariko, Holven, Kirsten B., Humphries, Steve E., Khovidhunkit, Weerapan, Lalic, Katarina, Laufs, Ulrich, Liberopoulos, Evangelos, Roeters van Lennep, Jeanine, Lima-Martinez, Marcos Miguel, Lin, Jie, Maher, Vincent, März, Winfried, Miserez, André R., Mitchenko, Olena, Nawawi, Hapizah, Panayiotou, Andrie G., Paragh, György, Postadzhiyan, Arman, Reda, Ashraf, Reiner, Željko, Reyes, Ximena, Sadiq, Fouzia, Sahebkar, Amirhossein, Schunkert, Heribert, Shek, Aleksandr B., Stroes, Eric, Su, Ta-Chen, Subramaniam, Tavintharan, Susekov, Andrey, Vázquez Cárdenas, Alejandra, Huong Truong, Thanh, Tselepis, Alexandros D., Vohnout, Branislav, Wang, Luya, Yamashita, Shizuya, Al-Sarraf, Ahmad, Al-Sayed, Nasreen, Davletov, Kairat, Dwiputra, Bambang, Gaita, Dan, Kayikcioglu, Meral, Latkovskis, Gustavs, Marais, A. David, Thushara Matthias, Anne, Mirrakhimov, Erkin, Nordestgaard, Børge G., Petrulioniene, Zaneta, Pojskic, Belma, Sadoh, Wilson, Tilney, Myra, Tomlinson, Brian, Tybjærg-Hansen, Anne, Viigimaa, Margus, Catapano, Alberico L., Freiberger, Tomas, Hovingh, G. Kees, Mata, Pedro, Soran, Handrean, Raal, Frederick, Watts, Gerald F., Schreier, Laura, Bañares, Virginia, Greber-Platzer, Susanne, Baumgartner-Kaut, Margot, de Gier, Charlotte, Dieplinger, Hans, Höllerl, Florian, Innerhofer, Reinhold, Karall, Daniela, Lischka, Julia, Ludvik, Bernhard, Mäser, Martin, Scholl-Bürgi, Sabine, Thajer, Alexandra, Toplak, Hermann, Demeure, Fabian, Mertens, Ann, Balligand, Jean-Luc, Stephenne, Xavier, Sokal, Etienne, Petrov, Ivo, Goudev, Assen, Nikolov, Fedya, Tisheva, Snejana, Yotov, Yoto, Tzvetkov, Ivajlo, Hegele, Robert A, Gaudet, Daniel, Brunham, Liam, Ruel, Isabelle, McCrindle, Brian, Cuevas, Ada, Perica, Dražen, Symeonides, Phivos, Trogkanis, Efstratios, Kostis, Andreas, Ioannou, Andreas, Mouzarou, Angeliki, Georgiou, Anthoula, Stylianou, Andreas, Miltiadous, George, Iacovides, Paris, Deltas, Constantinos, Vrablik, Michal, Urbanova, Zuzana, Jesina, Pavel, Tichy, Lukas, Hyanek, Josef, Dvorakova, Jana, Cepova, Jana, Sykora, Josef, Buresova, Kristyna, Pipek, Michal, Pistkova, Eva, Bartkova, Ivana, S|ulakova, Astrid, Toukalkova, Lenka, Spenerova, Michaela, Maly, Jan, Benn, Marianne, Bendary, Ahmed, Elbahry, Atef, Ferrières, Jean, Ferrieres, Dorota, Peretti, Noel, Bruckert, Eric, Gallo, Antonio, Valero, René, Mourre, Florian, Aouchiche, Karine, Reynaud, Rachel, Tounian, Patrick, Lemale, Julie, Boccara, Franck, Moulin, Philippe, Charrières, Sybil, Di Filippo, Mathilde, Cariou, Bertrand, Paillard, François, Dourmap, Caroline, Pradignac, Alain, Verges, Bruno, Simoneau, Isabelle, Farnier, Michel, Cottin, Yves, Yelnik, Cecile, Hankard, Regis, Schiele, François, Durlach, Vincent, Sultan, Ariane, Carrié, Alain, Rabès, Jean-Pierre, Sanin, Veronika, Schmieder, Raphael S., Ates, Sara, Rizos, Christos V., Skoumas, Ioannis, Tziomalos, Konstantinos, Rallidis, Loukianos, Kotsis, Vasileios, Doumas, Michalis, Skalidis, Emmanouil, Kolovou, Genovefa, Kolovou, Vana, Garoufi, Anastasia, Koutagiar, Iosif, Polychronopoulos, Georgios, Kiouri, Estela, Antza, Christina, Zacharis, Evangelos, Attilakos, Achilleas, Sfikas, George, Koumaras, Charalambos, Anagnostis, Panagiotis, Anastasiou, Georgia, Liamis, George, Adamidis, Petros-Spyridon, Milionis, Haralambos, Lambadiari, Vaia, Stabouli, Stella, Filippatos, Theodosios, Mollaki, Vicky, Tsaroumi, Anastasia, Lamari, Frida, Proyias, Pavlos, Harangi, Mariann, Reddy, Lakshmi Lavanya, Shah, Swarup A. V, Ponde, Chandrashekhar K., Dalal, Jamshed J., Sawhney, Jitendra P.S., Verma, Ishwar C., Hosseini, Susan, Jamialahmadi, Tannaz, Alareedh, Mohammed, Shaghee, Foaad, Rhadi, Sabah Hasan, Abduljalal, Maryam, Alfil, Sarmad, Kareem, Huda, Cohen, Hofit, Leitersdorf, Eran, Schurr, Daniel, Shpitzen, Shoshi, Arca, Marcello, Averna, Maurizio, Bertolini, Stefano, Calandra, Sebastiano, Tarugi, Patrizia, Casula, Manuela, Galimberti, Federica, Gazzotti, Marta, Olmastroni, Elena, Sarzani, Riccardo, Ferri, Claudio, Repetti, Elena, Giorgino, Francesco, Suppressa, Patrizia, Bossi, Antonio Carlo, Borghi, Claudio, Muntoni, Sandro, Cipollone, Francesco, Scicali, Roberto, Pujia, Arturo, Passaro, Angelina, Berteotti, Martina, Pecchioli, Valerio, Pisciotta, Livia, Mandraffino, Giuseppe, Pellegatta, Fabio, Mombelli, Giuliana, Branchi, Adriana, Fiorenza, Anna Maria, Pederiva, Cristina, Werba, José Pablo, Parati, Gianfranco, Nascimbeni, Fabio, Iughetti, Lorenzo, Fortunato, Giuliana, Cavallaro, Raimondo, Iannuzzo, Gabriella, Calabrò, Paolo, Cefalù, Angelo Baldassare, Capra, Maria Elena, Zambon, Alberto, Pirro, Matteo, Sbrana, Francesco, Trenti, Chiara, Minicocci, Ilenia, Federici, Massimo, Del Ben, Maria, Buonuomo, Paola Sabrina, Moffa, Simona, Pipolo, Antonio, Citroni, Nadia, Guardamagna, Ornella, Lia, Salvatore, Benso, Andrea, Biolo, Gianni Biolo, Maroni, Lorenzo, Lupi, Alessandro, Bonanni, Luca, Rinaldi, Elisabetta, Zenti, Maria Grazia, Masuda, Daisaku, Mahfouz, Linda, Jambart, Selim, Ayoub, Carine, Ghaleb, Youmna, Kasim, Noor Alicezah Mohd, Nor, Noor Shafina Mohd, Al-Khateeb, Alyaa, Kadir, Siti Hamimah Sheikh Abdul, Chua, Yung-An, Razman, Aimi Zafira, Nazli, Sukma Azureen, Ranai, Norashikin Mohd, Latif, Ahmad Zubaidi Abd, Torres, María Teresa Magaña, Mehta, Roopa, Martagon, Alexandro J., Ramirez, Gabriela A. Galan, Antonio-Villa, Neftali Eduardo, Vargas-Vazquez, Arsenio, Elias-Lopez, Daniel, Retana, Gustavo Gonzalez, Encinas, Bethsabel Rodrıguez, Macıas, Jose J. Ceballos, Zazueta, Alejandro Romero, Alvarado, Rocio Martinez, Portano, Julieta D. Morales, Lopez, Humberto Alvares, Sauque-Reyna, Leobardo, Gomez Herrera, Laura G., Simental Mendia, Luis E., Aguilar, Humberto Garcia, Cooremans, Elizabeth Ramirez, Aparicio, Berenice Pe~na, Zubieta, Victoria Mendoza, Gonzalez, Perla A. Carrillo, Ferreira-Hermosillo, Aldo, Portilla, Nacu Caracas, Dominguez, Guadalupe Jimenez, Garcia, Alinna Y. Ruiz, Arriaga Cazares, Hector E., Gonzalez Gonzalez, Jesus R., Mendez Valencia, Carla V., Padilla Padilla, Francisco G., Prado, Ramon Madriz, De los Rios Ibarra, Manuel O., Arjona Villica~na, Ruy D., Acevedo Rivera, Karina J., Carrera, Ricardo Allende, Alvarez, Jose A., Amezcua Martinez, Jose C., Barrera Bustillo, Manuel de los Reyes, Vargas, Gonzalo Carazo, Chacon, Roberto Contreras, Figueroa Andrade, Mario H., Ortega, Ashanty Flores, Alcala, Hector Garcia, Garcia de Leon, Laura E., Guzman, Berenice Garcia, Gardu~no Garcia, Jose J., Garnica Cuellar, Juan C., Gomez Cruz, Jose R., Garcia, Anell Hernandez, Holguin Almada, Jesus R., Herrera, Ursulo Juarez, Sobrevilla, Fabiola Lugo, Rodriguez, Eduardo Marquez, Sibaja, Cristina Martinez, Medrano Rodriguez, Alma B., Morales Oyervides, Jose C., Perez Vazquez, Daniel I., Reyes Rodriguez, Eduardo A., Osorio, Ma. Ludivina Robles, Saucedo, Juan Rosas, Tamayo, Margarita Torres, Valdez Talavera, Luis A., Vera Arroyo, Luis E., Zepeda Carrillo, Eloy A., Galema-Boers, Annette, Weigman, Albert, Bogsrud, Martin P., Malik, Munir, Shah, Saeedullah, Khan, Sabeen Abid, Rana, Muhammad Asim, Batool, Hijab, Starostecka, Ewa, Konopka, Agnieszka, Lewek, Joanna, Bielecka-Dąbrowa, Agata, Gach, Agnieszka, Jóźwiak, Jacek, Pajkowski, Marcin, Romanowska-Kocejko, Marzena, Żarczyńska-Buchowiecka, Marta, Hellmann, Marcin, Chmara, Magdalena, Wasąg, Bartosz, Parczewska, Aleksandra, Gilis-Malinowska, Natasza, Borowiec-Wolna, Justyna, Stróżyk, Aneta, Michalska-Grzonkowska, Aleksandra, Chlebus, Izabela, Kleinschmidt, Mariola, Wojtecka, Agnieszka, Zdrojewski, Tomasz, Myśliwiec, Małgorzata, Hennig, Matylda, Medeiros, Ana Margarida, Alves, Ana Catarina, Almeida, Ana Filipa, Lopes, Andreia, Guerra, António, Bilhoto, Carla, Simões, Fernando, Silva, Francisco, Lobarinhas, Goreti, Gama, Guida, Palma, Isabel, Salgado, José Miguel, Matos, Luísa Diogo, Moura, Márcio de, Virtuoso, Maria João, Tavares, Mónica, Ferreira, Patrícia, Pais, Patrícia, Garcia, Paula, Coelho, Raquel, Ribeiro, Raquel, Correia, Susana, Sadykova, Dinara, Slastnikova, Evgenia, Alammari, Dalal, Mawlawi, Horia Ahmed, Alsahari, Atif, Khudary, Alia Abdullah, Alrowaily, Nawal Lafi, Rajkovic, Natasa, Popovic, Ljiljana, Singh, Sandra, Rasulic, Iva, Petakov, Ana, Lalic, Nebojsa M., Peng, Fabian Kok, Vasanwala, Rashida Farhan, Venkatesh, Sreedharan Aravind, Raslova, Katarina, Fabryova, Lubomira, Nociar, Jan, Šaligova, Jana, Potočňáková, Ludmila, Kozárová, Miriam, Varga, Tibor, Kadurova, Michaela, Debreova, Marianna, Novodvorsky, Peter, Gonova, Katarina, Klabnik, Alexander, Buganova, Ingrid, Battelino, Tadej, Bizjan, Barbara Jenko, Debeljak, Marusa, Kovac, Jernej, Mlinaric, Matej, Molk, Neza, Sikonja, Jaka, Sustar, Ursa, Podkrajsek, Katarina Trebusak, Muñiz-Grijalvo, Ovidio, Díaz-Díaz, Jose Luis, de Andrés, Raimundo, Fuentes-Jiménez, Francisco, Blom, Dirk, Miserez, Eleonore B., Shipton, Janine L., Ganokroj, Poranee, Futema, Marta, Ramaswami, Uma, Alieva, Rano B., Fozilov, Khurshid G., Khoshimov, Shavkat U., Nizamov, Ulugbek I., Abdullaeva, Guzal J., Kan, Liliya E., Abdullaev, Alisher A., Zakirova, Daria V., Do, Doan-Loi, Nguyen, Mai-Ngoc-Thi, Kim, Ngoc-Thanh, Le, Thanh-Tung, Le, Hong-An, Santos, Raul, and Ray, Kausik K.

Published
2024
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