Com essas Palavras Maria Orientou Seus Corações para o Bem (Ev. de Maria 9,19) by Sandro Gallazzi

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State of the Art in the Standardization of Stromal Vascular Fraction Processing by Martina Cremona, Matteo Gallazzi, Giulio Rusconi, Luca Mariotta, Mauro Gola, Gianni Soldati

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A Large Dataset to Enhance Skin Cancer Classification With Transformer-Based Deep Neural Networks by Mirco Gallazzi, Sara Biavaschi, Alessandro Bulgheroni, Tommaso M. Gatti, Silvia Corchs, Ignazio Gallo

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Gravitational lens candidates in the E-CDFS by More, A, Jahnke, K, More, S, Gallazzi, A, Bell, E, Barden, M, Haeussler, B

Qualitative flood risk assessment for road and railway infrastructures: the experience of the MOVIDA project by N. Petruccelli, L. Mantecchini, A. Gallazzi, D. Molinari, M. Hammouti, M. Zazzeri, S. Sterlacchini, F. Ballio, A. Brath, A. Domeneghetti

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Differences in Trabecular bone morphology between patients with non progressive and progressive osteoporotic vertebral compression fractures by E. Gallazzi, G.A. La Maida, A. Della Valle, M. Ferraro, D. Cecconi, A. Cicatelli, D.R. Peroni, B. Misaggi

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Contemporary Advances in Cardiac Remote Monitoring: A Comprehensive, Updated Mini-Review by Alberto Preda, Raffaele Falco, Chiara Tognola, Marco Carbonaro, Sara Vargiu, Michela Gallazzi, Matteo Baroni, Lorenzo Gigli, Marisa Varrenti, Giulia Colombo, Gabriele Zanotto, Cristina Giannattasio, Patrizio Mazzone, Fabrizio Guarracini

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CT Arthrography of the Elbow: What Radiologists Should Know by Gianluca Folco, Carmelo Messina, Salvatore Gitto, Stefano Fusco, Francesca Serpi, Andrea Zagarella, Mauro Battista Gallazzi, Paolo Arrigoni, Alberto Aliprandi, Marco Porta, Paolo Vitali, Luca Maria Sconfienza, Domenico Albano

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Dental pulp mesenchymal stem cell (DPSCs)-derived soluble factors, produced under hypoxic conditions, support angiogenesis via endothelial cell activation and generation of M2-like... by Ludovica Barone, Martina Cucchiara, Maria Teresa Palano, Barbara Bassani, Matteo Gallazzi, Federica Rossi, Mario Raspanti, Piero Antonio Zecca, Gianluca De Antoni, Christina Pagiatakis, Roberto Papait, Giovanni Bernardini, Antonino Bruno, Rosalba Gornati

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From Halos to Galaxies. IX. Estimate of Halo Assembly History for SDSS Galaxy Groups by Cheqiu Lyu, Yingjie Peng, Yipeng Jing, Xiaohu Yang, Luis C. Ho, Alvio Renzini, Dingyi Zhao, Filippo Mannucci, Houjun Mo, Kai Wang, Bitao Wang, Bingxiao Xu, Jing Dou, Anna R. Gallazzi, Qiusheng Gu, Roberto Maiolino, Enci Wang, Feng Yuan

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The Gas-phase Mass–Metallicity Relation for Massive Galaxies at z ∼ 0.7 with the LEGA-C Survey by Zach J. Lewis, Brett H. Andrews, Rachel Bezanson, Michael Maseda, Eric F. Bell, Romeel Davé, Francesco D’Eugenio, Marijn Franx, Anna Gallazzi, Anna de Graaff, Yasha Kaushal, Angelos Nersesian, Jeffrey A. Newman, Arjen van der Wel, Po-Feng Wu

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Stellar metallicity from optical and UV spectral indices: test case for WEAVE-StePS by Ditrani, FR, Longhetti, M, La Barbera, F, Iovino, A, Costantin, L, Zibetti, S, Gallazzi, A, Fossati, M, Angthopo, J, Ascasibar, Y, Poggianti, B, Sánchez-Blázquez, P, Balcells, M, Bianconi, M, Bolzonella, M, Cassarà, LP, Cucciati, O, Dalton, GB, Jin, S, Spiniello, C

From Halos to Galaxies. X. Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction by Zeyu Gao, Yingjie Peng, Kai Wang, Luis C. Ho, Alvio Renzini, Anna R. Gallazzi, Filippo Mannucci, Houjun Mo, Yipeng Jing, Xiaohu Yang, Enci Wang, Dingyi Zhao, Jing Dou, Qiusheng Gu, Cheqiu Lyu, Roberto Maiolino, Bitao Wang, Yu-Chen Wang, Bingxiao Xu, Feng Yuan, Xingye Zhu

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From Halos to Galaxies. VI. Improved Halo Mass Estimation for SDSS Groups and Measurement of the Halo Mass Function by Dingyi Zhao, Yingjie Peng, Yipeng Jing, Xiaohu Yang, Luis C. Ho, Alvio Renzini, Anna R. Gallazzi, Cheqiu Lyu, Roberto Maiolino, Jing Dou, Zeyu Gao, Qiusheng Gu, Filippo Mannucci, Houjun Mo, Bitao Wang, Enci Wang, Kai Wang, Yu-Chen Wang, Bingxiao Xu, Feng Yuan, Xingye Zhu

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Obscured star formation in intermediate-density environments: A Spitzer study of the Abell 901/902 supercluster by Gallazzi, A, Bell, E, Wolf, C, Gray, M, Papovich, C, Barden, M, Peng, C, Meisenheimer, K, Heymans, C, Kampen, E, Gilmour, R, Balogh, M, McIntosh, D, Bacon, D, Barazza, F, Boehm, A, Caldwell, J, Haeussler, B, Jahnke, K, Jogee, S, Lane, K, Robaina, A, Sanchez, S, Taylor, A, Wisotzki, L

The STAGES view of red spirals and dusty red galaxies: Mass-dependent quenching of star-formation in cluster infall by Wolf, C, Aragon-Salamanca, A, Balogh, M, Barden, M, Bell, E, Gray, M, Peng, C, Bacon, D, Barazza, F, Boehm, A, Caldwell, J, Gallazzi, A, Haeussler, B, Heymans, C, Jahnke, K, Jogee, S, Kampen, E, Lane, K, McIntosh, D, Meisenheimer, K, Papovich, C, Sanchez, S, Taylor, A, Wisotzki, L, Zheng, X

Optically-passive spirals: The missing link in gradual star formation suppression upon cluster infall by Wolf, C, Aragón-Salamanca, A, Balogh, M, Barden, M, Bell, E, Gray, M, Peng, C, Bacon, D, Barazza, F, Böhm, A, Caldwell, J, Gallazzi, A, ler, B, Heymans, C, Jahnke, K, Jogee, S, Kampen, E, Lane, K, McIntosh, D, Meisenheimer, K, Papovich, C, Sánchez, S, Taylor, A, Wisotzki, L, Zheng, X

LESS THAN 10 PERCENT OF STAR FORMATION IN z similar to 0.6 MASSIVE GALAXIES IS TRIGGERED BY MAJOR INTERACTIONS by Robaina, A, Bell, E, Skelton, R, McIntosh, D, Somerville, R, Zheng, X, Rix, H, Bacon, D, Balogh, M, Barazza, F, Barden, M, Boehm, A, Caldwell, J, Gallazzi, A, Gray, M, Haeussler, B, Heymans, C, Jahnke, K, Jogee, S, van Kampen, E, Lane, K, Meisenheimer, K, Papovich, C, Peng, C, Sanchez, S

A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate-redshift galaxies with WEAVE by Costantin, L, Lovino, A, Zibetti, S, Longhetti, M, Gallazzi, A, Mercurio, A, Lonoce, I, Balcells, M, Bolzonella, M, Busarello, G, Dalton, G, Ferre-Mateu, A, Garcia-Benito, R, Gargiulo, A, Haines, C, Jin, S, Barbera, FL, Mcgee, S, Merluzzi, P, Morelli, L, Murphy, DNA, L Peralta de Arriba, Pizzella, A, Poggianti, BM, Pozzetti, L, Sanchez-Blazquez, P, Talia, M, Tortora, C, Trager, SC, Vazdekis, A, Vergani, D, Vulcani, B