SYNTHESIS AND CHARACTERIZATION BY INFRARED AND MOSSBAUER SPECTROSCOPIES OF SOME NEW SnR2 (R = Me, Ph, Bu) RESIDUE CONTAINING ARBOXYALKYLPHOSPHONATE ADDUCTS AND DERIVATIVES by MOUHAMADOU SEMBENE BOYE, MOUHAMADOU BIRAME DIOP, MODOU SARR, AMINATA DIASSE-SARR, LIBASSE DIOP, ALAIN WATTIAUX

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Managing Liver Cirrhosis: a Multidisciplinary Approach by V. M. Durleshter, S. A. Gabriel, N. V. Korochanskaya, O. V. Kovalevskaya, S. N. Serikova, P. V. Markov, O. A. Usova, D. S. Murashko, V. Yu. Dyn'ko, A. Yu. Bukhtoyarov, M. A. Basenko

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Escherichia coli in septic arthritis: prevalence and antibiotics susceptibility patterns by Masroora Ali Khan, Muhammad Kamran Taj, Zahid Khan, Imran Taj, Muhammad Naeem, Saima Azam

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Comprehensive Overview - Outcomes and Challenges of Bariatric Surgery - Physical, Psychological and Nutritional Considerations by Katarzyna Doman, Dawid Komada, Kamil Hermanowicz, Daria Oleksy, Agnieszka Najdek, Urszula Kaczmarska, Aleksandra Woźniak, Marcin Mycyk, Julia Nowak, Michał Jakub Cioch

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Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy [version 2; peer review: 2 approved] by Pamela Klaassen, Maria Beltrán, Alessio Traficante, Mark Booth, Kate Pattle, Jonathan Marshall, Joshua Lovell, Brandt Gaches, Alvaro Hacar, Nicolas Peretto, Caroline Bot, Doris Arzoumanian, Thomas Stanke, Gaspard Duchêne, Ana Duarte Cabral, Antonio Hales, David Eden, Patricia Luppe, Jens Kauffmann, Elena Redaelli, Sebastian Marino, Álvaro Sánchez-Monge, Andrew Rigby, Dmitry Semenov, Eugenio Schisano, Mark Thompson, Silvia Spezzano, Claudia Cicone, Friedrich Wyrowski, Martin Cordiner, Tony Mroczkowski, Doug Johnstone, Luca Di Mascolo, Minju Lee, Eelco van Kampen, Thomas Maccarone, Daizhong Liu, Matthew Smith, Amélie Saintonge, Sven Wedemeyer, Alexander Thelen

“…Because we are deeply embedded in the plane of our Galaxy, it takes up a significant fraction of the sky, with complex dust lanes scattered throughout the optically recognizable bands of the Milky Way. These bands become bright at (sub-)millimetre wavelengths, where we can study dust thermal emission and the chemical and kinematic signatures of the gas. …”
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