Author: "Cheng, K." - Searchworks@Jio Institute Digital Library Search Results

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13,348 results on '"Cheng, K."'

101. Vascular and neurological outcomes in patients with atrial fibrillation treated with edoxaban; effects of cancer

Author: Cheng, K, primary, Tu, H P T, additional, Scherrer-Crosbie, M S C, additional, Cheng, K C C, additional, and Hsu, T Y H, additional
Published: 2023
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102. Our choice is not binary between lockdown and herd immunity

Author: Cheng, K K
Published: 2020

103. Pseudocapacitance enhanced by N-defects in Na3MnTi(PO4)3/N-doped carbon composite for symmetric full sodium-ion batteries

Author: Li, H., Zhang, W., Han, Z., Sun, K., Gao, C., Cheng, K., Liu, Z., Chen, Q., Zhang, J., Lai, Y., Zhang, Z., and Sun, H.
Published: 2021
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104. Covid-19 : risk factors for severe disease and death

Author: Jordan, Rachel E, Adab, Peymane, and Cheng, K K
Published: 2020

105. The mediating role of emotional eating in the relationship between perceived stress and dietary intake quality in Hispanic/Latino adolescents

Author: Bell, Brooke M., Spruijt-Metz, Donna, Naya, Christine H., Lane, Christianne J., Wen, Cheng K. Fred, Davis, Jaimie N., and Weigensberg, Marc J.
Published: 2021
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106. Proletarian revolution and the crisis of modernity : German orthodox Marxism and French revolutionary syndicalism, 1889-1914

Author: Cheng, K.
Subjects: 940
Abstract: This study develops a close-textual and comparative analysis of two influential doctrines of "proletarian revolution" that appeared during the Second International period (1889-1914): "German orthodox Marxism" and "French revolutionary syndicalism." It considers the effect of the dramatic mass-organizational development of the European workers' movement upon both doctrines - in particular, how this shaped the key concepts of "scientific socialism" and "direct action." In this light, the first chapter of the study examines the relationship of both doctrines to "classical" Marxist and anarchist ideology. The main body of the study then outlines the historical development of both tendencies - their "formation" and "decomposition." This analysis challenges prevailing historiographical interpretations of several significant revolutionary thinkers: on the Marxist side, Friedrich Engels, Karl Kautsky, and Rosa Luxemburg; on the syndicalist side, Fernand Pelloutier, Émile Pouget, and Georges Sorel. It also reframes the political history of two major pre-First World War institutions: the Sozialdemokratische Partei Deutschlands and the Confédération générale du travail.
Published: 2017

107. Contributions of the Cherenkov Telescope Array (CTA) to the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016)

Author: Consortium, The CTA, Abchiche, A., Abeysekara, U., Abril, Ó., Acero, F., Acharya, B. S., Adams, C., Agnetta, G., Aharonian, F., Akhperjanian, A., Albert, A., Alcubierre, M., Alfaro, J., Alfaro, R., Allafort, A. J., Aloisio, R., Amans, J. -P., Amato, E., Ambrogi, L., Ambrosi, G., Ambrosio, M., Anderson, J., Anduze, M., Angüner, E. O., Antolini, E., Antonelli, L. A., Antonucci, M., Antonuccio, V., Antoranz, P., Aramo, C., Aravantinos, A., Araya, M., Arcaro, C., Arezki, B., Argan, A., Armstrong, T., Arqueros, F., Arrabito, L., Arrieta, M., Asano, K., Ashley, M., Aubert, P., Singh, C. B., Babic, A., Backes, M., Bais, A., Bajtlik, S., Balazs, C., Balbo, M., Balis, D., Balkowski, C., Ballester, O., Ballet, J., Balzer, A., Bamba, A., Bandiera, R., Barber, A., Barbier, C., Barcelo, M., Barkov, M., Barnacka, A., de Almeida, U. Barres, Barrio, J. A., Basso, S., Bastieri, D., Bauer, C., Becciani, U., Becherini, Y., Tjus, J. Becker, Beckmann, V., Bednarek, W., Benbow, W., Ventura, D. Benedico, Berdugo, J., Berge, D., Bernardini, E., Bernardini, M. G., Bernhard, S., Bernlöhr, K., Bertucci, B., Besel, M. -A., Beshley, V., Bhatt, N., Bhattacharjee, P., Bhattacharyya, W., Bhattachryya, S., Biasuzzi, B., Bicknell, G., Bigongiari, C., Biland, A., Bilinsky, A., Bilnik, W., Biondo, B., Bird, R., Bird, T., Bissaldi, E., Bitossi, M., Blanch, O., Blasi, P., Blazek, J., Bockermann, C., Boehm, C., Bogacz, L., Bogdan, M., Bohacova, M., Boisson, C., Boix, J., Bolmont, J., Bonanno, G., Bonardi, A., Bonavolontà, C., Bonifacio, P., Bonnarel, F., Bonnoli, G., Borkowski, J., Bose, R., Bosnjak, Z., Böttcher, M., Bousquet, J. -J., Boutonnet, C., Bouyjou, F., Bowman, L., Braiding, C., Brantseg, T., Brau-Nogué, S., Bregeon, J., Briggs, M., Brigida, M., Bringmann, T., Brisken, W., Bristow, D., Britto, R., Brocato, E., Bron, S., Brook, P., Brooks, W., Brown, A. M., Brügge, K., Brun, F., Brun, P., Brunetti, G., Brunetti, L., Bruno, P., Buanes, T., Bucciantini, N., Buchholtz, G., Buckley, J., Bugaev, V., Bühler, R., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Buson, S., Buss, J., Byrum, K., Cadoux, F., Tovar, J. Calvo, Cameron, R., Canelli, F., Canestrari, R., Capalbi, M., Capasso, M., Capobianco, G., Caproni, A., Caraveo, P., Cardenzana, J., Cardillo, M., Carius, S., Carlile, C., Carosi, A., Carosi, R., Carquín, E., Carr, J., Carroll, M., Carter, J., Carton, P. -H., Casandjian, J. -M., Casanova, S., Cascone, E., Casiraghi, M., Castellina, A., Mora, J. Castroviejo, Catalani, F., Catalano, O., Catalanotti, S., Cauz, D., Cavazzani, S., Cerchiara, P., Chabanne, E., Chadwick, P., Chaleil, T., Champion, C., Chatterjee, A., Chaty, S., Chaves, R., Chen, A., Chen, X., Cheng, K., Chernyakova, M., Chiappetti, L., Chikawa, M., Chinn, D., Chitnis, V. R., Cho, N., Christov, A., Chudoba, J., Cieślar, M., Ciocci, M. A., Clay, R., Colafrancesco, S., Colin, P., Colley, J. -M., Colombo, E., Colome, J., Colonges, S., Conforti, V., Connaughton, V., Connell, S., Conrad, J., Contreras, J. L., Coppi, P., Corbel, S., Coridian, J., Cornat, R., Corona, P., Corti, D., Cortina, J., Cossio, L., Costa, A., Costantini, H., Cotter, G., Courty, B., Covino, S., Covone, G., Crimi, G., Criswell, S. J., Crocker, R., Croston, J., Cuadra, J., Cumani, P., Cusumano, G., Da Vela, P., Dale, Ø., D'Ammando, F., Dang, D., Dang, V. T., Dangeon, L., Daniel, M., Davids, I., Dawson, B., Dazzi, F., Costa, B. de Aguiar, De Angelis, A., Cardoso, R. F. de Araujo, De Caprio, V., Anjos, R. de Cássia dos, De Cesare, G., De Franco, A., De Frondat, F., Pino, E. M. de Gouveia Dal, de la Calle, I., De Lisio, C., Lopez, R. de los Reyes, De Lotto, B., De Luca, A., Neto, J. R. T. de Mello, de Naurois, M., Wilhelmi, E. de Oña, De Palma, F., De Persio, F., de Souza, V., Decock, G., Decock, J., Deil, C., Del Santo, M., Delagnes, E., Deleglise, G., Delgado, C., Delgado, J., della Volpe, D., Deloye, P., Detournay, M., Dettlaff, A., Devin, J., Di Girolamo, T., Di Giulio, C., Di Paola, A., Di Pierro, F., Diaz, M. A., Díaz, C., Dib, C., Dick, J., Dickinson, H., Diebold, S., Digel, S., Dipold, J., Disset, G., Distefano, A., Djannati-Ataï, A., Doert, M., Dohmke, M., Domínguez, A., Dominik, N., Dominique, J. -L., Prester, D. Dominis, Donat, A., Donnarumma, I., Dorner, D., Doro, M., Dournaux, J. -L., Downes, T., Doyle, K., Drake, G., Drappeau, S., Drass, H., Dravins, D., Drury, L., Dubus, G., Ducci, L., Dumas, D., Morå, K. Dundas, Durand, D., D'Urso, D., Dwarkadas, V., Dyks, J., Dyrda, M., Ebr, J., Edy, E., Egberts, K., Eger, P., Egorov, A., Einecke, S., Eisch, J., Eisenkolb, F., Eleftheriadis, C., Elsaesser, D., Elsässer, D., Emmanoulopoulos, D., Engelbrecht, C., Engelhaupt, D., Ernenwein, J. -P., Escarate, P., Eschbach, S., Espinoza, C., Evans, P., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Ramazani, V. Fallah, Fantinel, D., Farakos, K., Farnier, C., Farrell, E., Fasola, G., Favre, Y., Fede, E., Fedora, R., Fedorova, E., Fegan, S., Ferenc, D., Fernandez-Alonso, M., Fernández-Barral, A., Ferrand, G., Ferreira, O., Fesquet, M., Fetfatzis, P., Fiandrini, E., Fiasson, A., Filipčič, A., Filipovic, M., Fink, D., Finley, C., Finley, J. P., Finoguenov, A., Fioretti, V., Fiorini, M., Fleischhack, H., Flores, H., Florin, D., Föhr, C., Fokitis, E., Fonseca, M. V., Font, L., Fontaine, G., Fontes, B., Fornasa, M., Förster, A., Fortin, P., Fortson, L., Fouque, N., Franckowiak, A., Franco, F. J., Albuquerque, I. Freire Mota, Coromina, L. Freixas, Fresnillo, L., Fruck, C., Fuessling, M., Fugazza, D., Fujita, Y., Fukami, S., Fukazawa, Y., Fukuda, T., Fukui, Y., Funk, S., Furniss, A., Gäbele, W., Gabici, S., Gadola, A., Galindo, D., Gall, D. D., Gallant, Y., Galloway, D., Gallozzi, S., Galvez, J. A., Gao, S., Garcia, A., Garcia, B., Gil, R. García, López, R. Garcia, Garczarczyk, M., Gardiol, D., Gargano, C., Gargano, F., Garozzo, S., Garrecht, F., Garrido, L., Garrido-Ruiz, M., Gascon, D., Gaskins, J., Gaudemard, J., Gaug, M., Gaweda, J., Gebhardt, B., Gebyehu, M., Geffroy, N., Genolini, B., Gerard, L., Ghalumyan, A., Ghedina, A., Ghislain, P., Giammaria, P., Giannakaki, E., Gianotti, F., Giarrusso, S., Giavitto, G., Giebels, B., Gieras, T., Giglietto, N., Gika, V., Gimenes, R., Giomi, M., Giommi, P., Giordano, F., Giovannini, G., Girardot, P., Giro, E., Giroletti, M., Gironnet, J., Giuliani, A., Glicenstein, J. -F., Gnatyk, R., Godinovic, N., Goldoni, P., Gomez, G., Gonzalez, M. M., González, A., Gora, D., Gothe, K. S., Gotz, D., Goullon, J., Grabarczyk, T., Graciani, R., Graham, J., Grandi, P., Granot, J., Grasseau, G., Gredig, R., Green, A. J., Green, A. M., Greenshaw, T., Grenier, I., Griffiths, S., Grillo, A., Grondin, M. -H., Grube, J., Grudzinska, M., Grygorczuk, J., Guarino, V., Guberman, D., Gunji, S., Gyuk, G., Hadasch, D., Hagedorn, A., Hagge, L., Hahn, J., Hakobyan, H., Hara, S., Hardcastle, M. J., Hassan, T., Hatanaka, K., Haubold, T., Haupt, A., Hayakawa, T., Hayashida, M., Heller, M., Heller, R., Helo, J. C., Henault, F., Henri, G., Hermann, G., Hermel, R., Llorente, J. Herrera, Herrero, A., Hervet, O., Hidaka, N., Hinton, J., Hirai, W., Hirotani, K., Hnatyk, B., Hoang, J., Hoffmann, D., Hofmann, W., Holch, T., Holder, J., Hooper, S., Horan, D., Hörandel, J., Hörbe, M., Horns, D., Horvath, P., Hose, J., Houles, J., Hovatta, T., Hrabovsky, M., Hrupec, D., Huet, J. -M., Huetten, M., Hughes, G., Hui, D., Humensky, T. B., Hussein, M., Iacovacci, M., Ibarra, A., Ikeno, Y., Illa, J. M., Impiombato, D., Inada, T., Incorvaia, S., Infante, L., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Iocco, F., Ioka, K., Iori, M., Ishio, K., Israel, G. L., Iwamura, Y., Jablonski, C., Jacholkowska, A., Jacquemier, J., Jamrozy, M., Janecek, P., Janiak, M., Jankowsky, D., Jankowsky, F., Jean, P., Jegouzo, I., Jenke, P., Jimenez, J. J., Jingo, M., Jocou, L., Jogler, T., Johnson, C. A., Jones, M., Josselin, M., Journet, L., Jung, I., Kaaret, P., Kagaya, M., Kakuwa, J., Kalekin, O., Kalkuhl, C., Kamon, H., Kankanyan, R., Karastergiou, A., Kärcher, K., Karczewski, M., Karkar, S., Karn, P., Kasperek, J., Katagiri, H., Kataoka, J., Katarzyński, K., Kato, S., Katz, U., Kawanaka, N., Kaye, L., Kazanas, D., Kelley-Hoskins, N., Kersten, J., Khélifi, B., Kieda, D. B., Kihm, T., Kimeswenger, S., Kisaka, S., Kishida, S., Kissmann, R., Klepser, S., Kluźniak, W., Knapen, J., Knapp, J., Knödlseder, J., Koch, B., Köck, F., Kocot, J., Kohri, K., Kokkotas, K., Kolitzus, D., Komin, N., Kominis, I., Kong, A., Konno, Y., Kosack, K., Koss, G., Kossatz, M., Kowal, G., Koyama, S., Kozioł, J., Kraus, M., Krause, J., Krause, M., Krawzcynski, H., Krennrich, F., Kretzschmann, A., Kruger, P., Kubo, H., Kudryavtsev, V., Mezek, G. Kukec, Kuklis, M., Kuroda, H., Kushida, J., La Barbera, A., La Palombara, N., La Parola, V., La Rosa, G., Laffon, H., Lahmann, R., Lakicevic, M., Lalik, K., Lamanna, G., Landriu, D., Landt, H., Lang, R. G., Lapington, J., Laporte, P., Fèvre, J. -P. Le, Flour, T. Le, Sidaner, P. Le, Lee, S. -H., Lee, W. H., Lees, J. -P., Lefaucheur, J., Leffhalm, K., Leich, H., de Oliveira, M. A. Leigui, Lelas, D., Lemière, A., Lemoine-Goumard, M., Lenain, J. -P., Leonard, R., Leoni, R., Lessio, L., Leto, G., Leveque, A., Lieunard, B., Limon, M., Lindemann, R., Lindfors, E., Linhoff, L., Liolios, A., Lipniacka, A., Lockart, H., Lohse, T., Łokas, E., Lombardi, S., Longo, F., Lopatin, A., Lopez, M., Loreggia, D., Louge, T., Louis, F., Louys, M., Lucarelli, F., Lucchesi, D., Lüdecke, H., Luigi, T., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maccarone, T., Maccarone, T. J., Mach, E., Madejski, G. M., Madonna, A., Magniette, F., Magniez, A., Mahabir, M., Maier, G., Majumdar, P., Makariev, M., Malaguti, G., Malaspina, G., Mallot, A. K., Malouf, A., Maltezos, S., Malyshev, D., Mancilla, A., Mandat, D., Maneva, G., Manganaro, M., Mangano, S., Manigot, P., Mankushiyil, N., Mannheim, K., Maragos, N., Marano, D., Marchegiani, P., Marcomini, J. A., Marcowith, A., Mariotti, M., Marisaldi, M., Markoff, S., Martens, C., Martí, J., Martin, J. -M., Martin, L., Martin, P., Martínez, G., Martínez, M., Martínez, O., Martynyuk-Lototskyy, K., Marx, R., Masetti, N., Massimino, P., Mastichiadis, A., Mastroianni, S., Mastropietro, M., Masuda, S., Matsumoto, H., Matsuoka, S., Matthews, N., Mattiazzo, S., Maurin, G., Maxted, N., Maya, J., Mayer, M., Mazin, D., Mazziotta, M. N., Comb, L. Mc, McCubbin, N., McHardy, I., Medina, C., Mehrez, F., Melioli, C., Melkumyan, D., Melse, T., Mereghetti, S., Merk, M., Mertsch, P., Meunier, J. -L., Meures, T., Meyer, M., Meyrelles jr, J. L., Miccichè, A., Michael, T., Michałowski, J., Mientjes, P., Mievre, I., Mihailidis, A., Miller, J., Mineo, T., Minuti, M., Mirabal, N., Mirabel, F., Miranda, J. M., Mirzoyan, R., Mitchell, A., Mizuno, T., Moderski, R., Mognet, I., Mohammed, M., Moharana, R., Mohrmann, L., Molinari, E., Molyneux, P., Monmarthe, E., Monnier, G., Montaruli, T., Monte, C., Monteiro, I., Mooney, D., Moore, P., Moralejo, A., Morello, C., Moretti, E., Mori, K., Morris, P., Morselli, A., Moscato, F., Motohashi, D., Mottez, F., Moudden, Y., Moulin, E., Mueller, S., Mukherjee, R., Munar, P., Munari, M., Mundell, C., Mundet, J., Muraishi, H., Murase, K., Muronga, A., Murphy, A., Nagar, N., Nagataki, S., Nagayoshi, T., Nagesh, B. K., Naito, T., Nakajima, D., Nakamori, T., Nakayama, K., Nanni, J., Naumann, D., Nayman, P., Nellen, L., Nemmen, R., Neronov, A., Neyroud, N., Nguyen, T., Nguyen, T. T., Trung, T. Nguyen, Nicastro, L., Nicolau-Kukliński, J., Niederwanger, F., Niedźwiecki, A., Niemiec, J., Nieto, D., Nievas-Rosillo, M., Nikolaidis, A., Nikołajuk, M., Nishijima, K., Nishikawa, K. -I., Nishiyama, G., Noda, K., Nogues, L., Nolan, S., Northrop, R., Nosek, D., Nöthe, M., Novosyadlyj, B., Nozka, L., Nunio, F., Oakes, L., O'Brien, P., Ocampo, C., Occhipinti, G., Ochoa, J. P., de Bhroithe, A. OFaolain, Oger, R., Ohira, Y., Ohishi, M., Ohm, S., Ohoka, H., Okazaki, N., Okumura, A., Olive, J. -F., Olszowski, D., Ong, R. A., Ono, S., Orienti, M., Orito, R., Orlati, A., Osborne, J., Ostrowski, M., Ottaway, D., Otte, N., Öttl, S., Ovcharov, E., Oya, I., Ozieblo, A., Padovani, M., Pagano, I., Paiano, S., Paizis, A., Palacio, J., Palatka, M., Pallotta, J., Panagiotidis, K., Panazol, J. -L., Paneque, D., Panter, M., Panzera, M. R., Paoletti, R., Paolillo, M., Papayannis, A., Papyan, G., Paravac, A., Paredes, J. M., Pareschi, G., Park, N., Parsons, D., Paśko, P., Pavy, S., Pech, M., Peck, A., Pedaletti, G., Pe'er, A., Peet, S., Pelat, D., Pepato, A., Perez, M. d. C., Perri, L., Perri, M., Persic, M., Petrashyk, A., Petrucci, P. -O., Petruk, O., Peyaud, B., Pfeifer, M., Pfeiffer, G., Piano, G., Pieloth, D., Pierre, E., de Pinho, F. Pinto, García, C. Pio, Piret, Y., Pisarski, A., Pita, S., Platos, Ł., Platzer, R., Podkladkin, S., Pogosyan, L., Pohl, M., Poinsignon, P., Pollo, A., Porcelli, A., Porthault, J., Potter, W., Poulios, S., Poutanen, J., Prandini, E., Prast, J., Pressard, K., Principe, G., Profeti, F., Prokhorov, D., Prokoph, H., Prouza, M., Pruchniewicz, R., Pruteanu, G., Pueschel, E., Pühlhofer, G., Puljak, I., Punch, M., Pürckhauer, S., Pyzioł, R., Queiroz, F., Quel, E. J., Quinn, J., Quirrenbach, A., Rafighi, I., Rainò, S., Rajda, P. J., Rameez, M., Rando, R., Rannot, R. C., Rataj, M., Ravel, T., Razzaque, S., Reardon, P., Reichardt, I., Reimann, O., Reimer, A., Reimer, O., Reisenegger, A., Renaud, M., Renner, S., Reposeur, T., Reville, B., Rezaeian, A., Rhode, W., Ribeiro, D., Prado, R. Ribeiro, Ribó, M., Richards, G., Richer, M. G., Richtler, T., Rico, J., Ridky, J., Rieger, F., Riquelme, M., Ristori, P. R., Rivoire, S., Rizi, V., Roache, E., Rodriguez, J., Fernandez, G. Rodriguez, Vázquez, J. J. Rodríguez, Rojas, G., Romano, P., Romeo, G., Roncadelli, M., Rosado, J., Rose, J., Rosen, S., Lees, S. Rosier, Ross, D., Rouaix, G., Rousselle, J., Rovero, A. C., Rowell, G., Roy, F., Royer, S., Rubini, A., Rudak, B., Rugliancich, A., Rujopakarn, W., Rulten, C., Rupiński, M., Russo, F., Rutkowski, K., Saavedra, O., Sabatini, S., Sacco, B., Sadeh, I., Saemann, E. O., Safi-Harb, S., Saggion, A., Sahakian, V., Saito, T., Sakaki, N., Sakurai, S., Salamon, A., Salega, M., Salek, D., Greus, F. Salesa, Salgado, J., Salina, G., Salinas, L., Salini, A., Sanchez, D., Sanchez-Conde, M., Sandaker, H., Sandoval, A., Sangiorgi, P., Sanguillon, M., Sano, H., Santander, M., Santangelo, A., Santos, E. M., Santos-Lima, R., Sanuy, A., Sapozhnikov, L., Sarkar, S., Satalecka, K., Sato, Y., Savalle, R., Sawada, M., Sayède, F., Schanne, S., Schanz, T., Schioppa, E. J., Schlenstedt, S., Schmid, J., Schmidt, T., Schmoll, J., Schneider, M., Schoorlemmer, H., Schovanek, P., Schubert, A., Schullian, E. -M., Schultze, J., Schulz, A., Schulz, S., Schure, K., Schussler, F., Schwab, T., Schwanke, U., Schwarz, J., Schweizer, T., Schwemmer, S., Schwendicke, U., Schwerdt, C., Sciacca, E., Scuderi, S., Segreto, A., Seiradakis, J. -H., Sembroski, G. H., Semikoz, D., Sergijenko, O., Serre, N., Servillat, M., Seweryn, K., Shafi, N., Shalchi, A., Sharma, M., Shayduk, M., Shellard, R. C., Shibata, T., Shigenaka, A., Shilon, I., Shum, E., Sidoli, L., Sidz, M., Sieiro, J., Siejkowski, H., Silk, J., Sillanpää, A., Simone, D., Simpson, H., Singh, B. B., Sinha, A., Sironi, G., Sitarek, J., Sizun, P., Sliusar, V., Smith, A., Sobczyńska, D., Sol, H., Sottile, G., Sowiński, M., Spanier, F., Spengler, G., Spiga, R., Stadler, R., Stahl, O., Stamerra, A., Stanič, S., Starling, R., Staszak, D., Stawarz, Ł., Steenkamp, R., Stefanik, S., Stegmann, C., Steiner, S., Stella, C., Stephan, M., Stergioulas, N., Sternberger, R., Sterzel, M., Stevenson, B., Stinzing, F., Stodulska, M., Stodulski, M., Stolarczyk, T., Stratta, G., Straumann, U., Stringhetti, L., Strzys, M., Stuik, R., Sulanke, K. -H., Suomijärvi, T., Supanitsky, A. D., Suric, T., Sushch, I., Sutcliffe, P., Sykes, J., Szanecki, M., Szepieniec, T., Szwarnog, P., Tacchini, A., Tachihara, K., Tagliaferri, G., Tajima, H., Takahashi, H., Takahashi, K., Takahashi, M., Takalo, L., Takami, S., Takata, J., Takeda, J., Talbot, G., Tam, T., Tanaka, M., Tanaka, S., Tanaka, T., Tanaka, Y., Tanci, C., Tanigawa, S., Tavani, M., Tavecchio, F., Tavernet, J. -P., Tayabaly, K., Taylor, A., Tejedor, L. A., Telezhinsky, I., Temme, F., Temnikov, P., Tenzer, C., Terada, Y., Terrazas, J. C., Terrier, R., Terront, D., Terzic, T., Tescaro, D., Teshima, M., Testa, V., Tezier, D., Thayer, J., Thornhill, J., Thoudam, S., Thuermann, D., Tibaldo, L., Tiengo, A., Timpanaro, M. C., Tiziani, D., Tluczykont, M., Peixoto, C. J. Todero, Tokanai, F., Tokarz, M., Toma, K., Tomastik, J., Tomono, Y., Tonachini, A., Tonev, D., Torii, K., Tornikoski, M., Torres, D. F., Torres, M., Torresi, E., Toso, G., Tosti, G., Totani, T., Tothill, N., Toussenel, F., Tovmassian, G., Toyama, T., Travnicek, P., Trichard, C., Trifoglio, M., Pujadas, I. Troyano, Trzeciak, M., Tsinganos, K., Tsujimoto, S., Tsuru, T., Uchiyama, Y., Umana, G., Umetsu, Y., Upadhya, S. S., Uslenghi, M., Vagelli, V., Vagnetti, F., Valdes-Galicia, J., Valentino, M., Vallania, P., Valore, L., van Driel, W., van Eldik, C., van Soelen, B., Vandenbroucke, J., Vanderwalt, J., Vasileiadis, G., Vassiliev, V., Vázquez, J. R., Acosta, M. L. Vázquez, Vecchi, M., Vega, A., Vegas, I., Veitch, P., Venault, P., Venema, L., Venter, C., Vercellone, S., Vergani, S., Verma, K., Verzi, V., Vettolani, G. P., Veyssiere, C., Viana, A., Viaux, N., Vicha, J., Vigorito, C., Vincent, P., Vincent, S., Vink, J., Vittorini, V., Vlahakis, N., Vlahos, L., Voelk, H., Voisin, V., Vollhardt, A., Volpicelli, A., von Brand, H., Vorobiov, S., Vovk, I., Vrastil, M., Vu, L. V., Vuillaume, T., Wagner, R., Wagner, S. J., Wakely, S. P., Walstra, T., Walter, R., Walther, T., Ward, J. E., Ward, M., Warda, K., Warren, D., Wassberg, S., Watson, J. J., Wawer, P., Wawrzaszek, R., Webb, N., Wegner, P., Weiner, O., Weinstein, A., Wells, R., Werner, F., Wetteskind, H., White, M., White, R., Więcek, M., Wierzcholska, A., Wiesand, S., Wijers, R., Wilcox, P., Wild, N., Wilhelm, A., Wilkinson, M., Will, M., Williams, D. A., Williams, J. T., Willingale, R., Wilson, N., Winde, M., Winiarski, K., Winkler, H., Winter, M., Wischnewski, R., Witt, E., Wojcik, P., Wolf, D., Wood, M., Wörnlein, A., Wu, E., Wu, T., Yadav, K. K., Yamamoto, H., Yamamoto, T., Yamane, N., Yamazaki, R., Yanagita, S., Yang, L., Yelos, D., Yoshida, A., Yoshida, M., Yoshida, T., Yoshiike, S., Yoshikoshi, T., Yu, P., Zabalza, V., Zaborov, D., Zacharias, M., Zaharijas, G., Zajczyk, A., Zampieri, L., Zandanel, F., Sanchez, R. Zanmar, Zaric, D., Zavrtanik, D., Zavrtanik, M., Zdziarski, A., Zech, A., Zechlin, H., Zhao, A., Zhdanov, V., Ziegler, A., Ziemann, J., Ziętara, K., Zink, A., Ziółkowski, J., Zitelli, V., Zoli, A., Zorn, J., and Żychowski, P.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: List of contributions from the Cherenkov Telescope Array (CTA) Consortium presented at the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016), July 11-15, 2016, in Heidelberg, Germany., Comment: Index of CTA conference proceedings for the Gamma 2016, Heidelberg, Germany
Published: 2016

108. Constraining warm dark matter mass with cosmic reionization and gravitational wave

Author: Tan, W. W., Wang, F. Y., and Cheng, K. S.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We constrain the warm dark matter (WDM) particle mass with the observations of cosmic reionization and CMB optical depth. We suggest that the GWs from stellar mass black holes (BHs) could give a further constraint on WDM particle mass for future observations. The star formation rates (SFRs) of Population I/II (Pop I/II) and Population III (Pop III) stars are also derived. If the metallicity of the universe have been enriched beyond the critical value of $Z_{\rm crit}=10^{-3.5}Z_{\odot}$, the star formation shift from Pop III to Pop I/II stars. Our results show that the SFRs are quite dependent on the WDM particle mass, especially at high redshifts. Combing with the reionization history and CMB optical depth derived from the recent \emph{Planck} mission, we find that the current data requires the WDM particle mass in a narrow range of $1 < m_x < 3$ keV. Furthermore, we suggest that the stochastic gravitational wave background (SGWB) produced by stellar BHs could give a further constraint on the WDM particle mass for future observations. For $m_{x}=3$ keV with Salpeter (Chabrier) initial mass function (IMF), the SGWB from Pop I/II BHs has a peak amplitude of $\Omega_{\rm GW}\approx2.8\times 10^{-9}~(5.0\times 10^{-9})$ at $f= 316 {\rm Hz}$, while the GW radiation at $f<10$Hz is seriously suppressed. For $m_{\rm x}=1$ keV, the SGWB peak amplitude is the same as that of $m_{\rm x}=1$ keV, but a little lower at low frequencies. Therefore, it is hard to constrain the WDM particle mass by the SGWB from Pop I/II BHs. To assess the detectability of GW signal, we also calculate the signal to noise ratio (SNR), which are $\rm SNR=37.7~ (66.5)$ and $27~(47.7)$ for $m_{\rm x}=3$ keV and $m_{\rm x}=1$ keV for Einstein Telescope (ET) with Salpeter (Chabrier) IMF, respectively., Comment: 11 pages, 5 figures, accepted for publication in ApJ
Published: 2016
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109. Studying the SGR 1806-20/Cl* 1806-20 region using the \emph{Fermi} Large Area Telescope

Author: Yeung, Paul K. H., Kong, Albert K. H., Tam, P. H. Thomas, Lin, Lupin C. C., Hui, C. Y., Hu, Chin-Ping, and Cheng, K. S.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: The region around SGR 1806-20 and its host stellar cluster Cl* 1806-20 is a potentially important site of particle acceleration. The soft $\gamma-$ray repeater and Cl* 1806-20, which also contains several very massive stars including a luminous blue variable hypergiant LBV 1806-20, are capable of depositing a large amount of energy to the surroundings. Using the data taken with the \emph{Fermi} Large Area Telescope (LAT), we identified an extended LAT source to the south-west of Cl* 1806-20. The centroid of the 1-50~GeV emission is consistent with that of HESS J1808-204 (until now unidentified). The LAT spectrum is best-fit by a broken power-law with the break energy $E_\mathrm{b}=297\pm15$ MeV. The index above $E_\mathrm{b}$ is $2.60\pm0.04$, and is consistent with the flux and spectral index above 100 GeV for HESS J1808-204, suggesting an association between the two sources. Meanwhile, the interacting supernova remnant SNR G9.7-0.0 is also a potential contributor to the LAT flux. A tentative flux enhancement at the MeV band during a 45-day interval (2011 Jan 21 - 2011 Mar 7) is also reported. We discuss possible origins of the extended LAT source in the context of both leptonic and hadronic scenarios., Comment: Accepted for publication in ApJ
Published: 2016
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110. Observation and Simulation of the Variable Gamma-ray Emission from PSR~J2021+4026

Author: Ng, C. W., Takata, J., and Cheng, K. S.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Pulsars are rapidly spinning and highly magnetized neutron stars, with highly stable rotational period and gradual spin-down over a long timescale due to the loss of radiation. Glitches refer to the events that suddenly increase the rotational speed of a pulsar. The exact causes of glitches and the resulting processes are not fully understood. It is generally believed that couplings between the normal matter and the superfluid components, and the starquakes, are the common causes of glitches. In this study, one famous glitching pulsar, PSR~J2021+4026, is investigated. PSR~J2021+4026 is the first variable gamma-ray pulsar observed by Fermi. From the gamma-ray observations, it is found that the pulsar experienced a significant flux drop, an increase in the spin-down rate, a change in the pulse profile and a shift in the spectral cut-off to a lower energy, simultaneously around 2011 October 16. To explain these effects on the high-energy emissions by the glitch of PSR~J2021+4026, we hypothesized the glitch to be caused by the rearrangement of the surface magnetic field due to the crustal plate tectonic activities on the pulsar which is triggered by a starquake. In this glitch event, the inclination angle of the magnetic dipole axis is slightly shifted. This proposition is then tested by numerical modeling using a three-dimensional two-layer outer gap model. The simulation results indicate that a modification of the inclination angle can affect the pulse profile and the spectral properties, which can explain the observation changes after the glitch., Comment: 20 pages, 6 figures. Accepted for publication in ApJ
Published: 2016
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111. Observing two dark accelerators around the Galactic Centre with Fermi Large Area Telescope

Author: Hui, C. Y., Yeung, P. K. H., Ng, C. W., Lin, L. C. C., Tam, P. H. T., Cheng, K. S., Kong, A. K. H., Chernyshov, D. O., and Dogiel, V. A.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We report the results from a detailed $\gamma-$ray investigation in the field of two "dark accelerators", HESS J1745-303 and HESS J1741-302, with $6.9$ years of data obtained by the Fermi Large Area Telescope. For HESS J1745-303, we found that its MeV-GeV emission is mainly originated from the "Region A" of the TeV feature. Its $\gamma-$ray spectrum can be modeled with a single power-law with a photon index of $\Gamma\sim2.5$ from few hundreds MeV to TeV. Moreover, an elongated feature, which extends from "Region A" toward northwest for $\sim1.3^{\circ}$, is discovered for the first time. The orientation of this feature is similar to that of a large scale atomic/molecular gas distribution. For HESS J1741-302, our analysis does not yield any MeV-GeV counterpart for this unidentified TeV source. On the other hand, we have detected a new point source, Fermi J1740.1-3013, serendipitously. Its spectrum is apparently curved which resembles that of a $\gamma-$ray pulsar. This makes it possibly associated with PSR B1737-20 or PSR J1739-3023., Comment: 11 pages, 7 figures, 2 tables, accepted for publication in MNRAS
Published: 2016
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112. X-Ray afterglow of SWIFT J1644+57: a Compton echo?

Author: Cheng, K. S., Chernyshov, D. O., Dogiel, V. A., Kong, Albert K. H., and Ko, C. M.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Swift, Chandra and XMM have found a weak but nearly constant X-ray component from Swift J1644+57 that appeared at ~500 days and was visible at least until ~ 1400 days after the stellar capture, which cannot be explained by standard tidal disruption theories. We suggest that this X-ray afterglow component may result from Thomson scattering between the primary X-rays and its surrounding plasma, i.e. the Compton echo effect. Similar phenomena has also been observed from molecular clouds in our Galactic Center, which were caused by the past activity of Srg A*. If this interpretation of Swift J1644+57 afterglow is correct, this is the first Compton Echo effect observed in the cosmological distances., Comment: To be published in ApJL, accepted
Published: 2015
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113. Probing gamma-ray emissions of Fermi-LAT pulsars with a non-stationary outer gap model

Author: Takata, J., Ng, C. W., and Cheng, K. S.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We explore a non-stationary outer gap scenario for gamma-ray emission process in pulsar magnetosphere. Electrons/positrons that migrate along the magnetic field line and enter the outer gap from the outer/inner boundaries activate the pair-creation cascade and high-energy emission process. In our model, the rate of the particle injection at the gap boundaries is key physical quantity to control the gap structure and properties of the gamma-ray spectrum. Our model assumes that the injection rate is time variable and the observed gamma-ray spectrum are superposition of the emissions from different gap structures with different injection rates at the gap boundaries. The calculated spectrum superposed by assuming power law distribution of the particle injection rate can reproduce sub-exponential cut-off feature in the gamma-ray spectrum observed by Fermi-LAT. We fit the phase-averaged spectra for 43 young/middle-age pulsars and 14 millisecond pulsars with the model. Our results imply that (1) a larger particle injection at the gap boundaries is more frequent for the pulsar with a larger spin down power and (2) outer gap with an injection rate much smaller than the Goldreich-Julian value produces observe $>10$GeV emissions. Fermi-LAT gamma-ray pulsars show that (i) the observed gamma-ray spectrum below cut-off energy tends to be softer for the pulsar with a higher spin down rate and (ii) the second peak is more prominent in higher energy bands. Based on the results of the fitting, we describe possible theoretical interpretations for these observational properties. We also briefly discuss Crab-like millisecond pulsars that show phase-aligned radio and gamma-ray pulses., Comment: 38 pages, accepted for publication in MNRAS
Published: 2015
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114. Thermochemical valorization of oil palm biomass to value-added products: A biorefinery concept

Author: Ayodele, Bamidele V., primary, Mustapa, Siti I., additional, Alsaffar, May A., additional, Cheng, Cheng K., additional, and Patinvoh, Regina J., additional
Published: 2022
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115. Contributors

Author: Alsaffar, May A., primary, Alsultan, G. Abdulkareem, additional, Ansari, Khursheed B., additional, Arun, Jayaseelan, additional, Ayodele, Bamidele V., additional, Ayoub, Muhammad, additional, Banerjee, Arghya, additional, Barbiero, Chiara, additional, Berruti, Franco, additional, Cheng, Cheng K., additional, Dalai, Ajay K., additional, Danish, Mohd., additional, Dawn, Shanmuganantham S., additional, Derawi, Darfizzi, additional, Dinh, Duy Khoe, additional, Ghenai, Chaouki, additional, Gopinath, Kannappan P., additional, Guan, Guoqing, additional, Hassan, Saeikh Z., additional, Huyen, Pham Thanh, additional, Inayat, Abrar, additional, Jamil, Farrukh, additional, Karnjanakom, Surachai, additional, Khan, Mohd S., additional, Khan, Zakir, additional, Kongparakul, Suwadee, additional, Lee, Dae Hoon, additional, Lee, Won Gyu, additional, Mastuli, M.S., additional, Asikin-Mijan, N., additional, Mohapatro, Rudra N., additional, Mok, Young Sun, additional, Mustapa, Siti I., additional, Nanda, Sonil, additional, Naqvi, Salman R., additional, Nguyen, Duc Ba, additional, Nirmala, Narasiman, additional, Osman, Ahmed I., additional, Patinvoh, Regina J., additional, Patra, Biswa R., additional, Pham, Le K.H., additional, Phan, Thi To Nga, additional, Ravindran, Megan X.Y., additional, Azira Abdul Razak, N., additional, Reubroycharoen, Prasert, additional, Routray, Sunita, additional, Sahayaraj, Daniel V., additional, Salih, Nadia, additional, Salimon, Jumat, additional, Samart, Chanatip, additional, Shahbaz, Muhammad, additional, Shyam, Sivaprasad, additional, Subathra, Munusamy, additional, Swain, Ranjita, additional, Tariq, Rumaisa, additional, Trinh, Quang Thang, additional, and Trinh, Quang Hung, additional
Published: 2022
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116. Investigating vibration characteristics at concrete pavement joints using distributed optical fiber sensors

Author: Bian, Z.Y., primary, Zeng, M.Y., additional, Zhao, H.D., additional, Chen, H., additional, and Cheng, K., additional
Published: 2021
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117. Factors Influencing the Length of Hospital Stay Among Patients with Chronic Obstructive Pulmonary Disease (COPD) in Macao Population: A Retrospective Study of Inpatient Health Record

Author: Li M, Cheng K, Ku K, Li J, Hu H, and Ung COL
Subjects: chronic obstructive pulmonary disease, macao, length of hospital stay, blood test results, clinical therapy, inhaled medications, acute exacerbation, Diseases of the respiratory system, RC705-779
Abstract: Meng Li,1,* Kun Cheng,2,* Keisun Ku,2 Junlei Li,1 Hao Hu,1 Carolina Oi Lam Ung1 1State Key Laboratory of Quality Research in Chinese Medicine, Institute of Chinese Medical Sciences, University of Macau, Macao SAR, China; 2Internal Medicine Department, Kiang Wu Hospital, Macao SAR, China*These authors contributed equally to this workCorrespondence: Hao Hu; Carolina Oi Lam UngState Key Laboratory of Quality Research in Chinese Medicine, Institute of Chinese Medical Sciences, University of Macau, N22-2058, Macao SAR, ChinaTel +853 8822 8538Email haohu@um.edu.mo; carolinaung@um.edu.moPurpose: This study aims to identify the effects of patient and clinical therapy factors on the length of hospital stay (LOS) for admission due to chronic obstructive pulmonary disease (COPD) in Macao.Patients and Methods: Health record of patients with COPD admitted to Kiang Wu Hospital from January 2017 to December 2019 was retrospectively analyzed. Demographic information, blood test results, clinical therapies, and LOS were described and analyzed by multivariable regression.Results: A total of 1116 admissions were included with the average LOS being 12.28 (± 9.23) days. Among them, 735 (66.6%) were male with mean age 79.42 (± 10.35) years old, 697 were current or previous smokers (62.5%), and 360 (32.2%) had 3 or more comorbidities. During hospitalization, the most common treatments received were oxygen therapy (n=991,88.8%), antibiotics (n=828,74.2%), and systemic steroids (n=596,53.4%); only 120 (10.8%) had pulmonary rehabilitation (PR) and 128 (11.5%) received noninvasive ventilation (NIV). Inhaled medications were used during nearly 95% of hospitalization cases, while 2 and 3 types of inhaled medications were used during 230 (20.6%) and 582 (52.2%) hospitalization cases, respectively. Patient factors including age (B=0.178, 95% CI:0.535– 1.072), being female (B=− 1.147, 95% CI:-0.138– 0.056), being current (B=− 0.086, 95% CI:-0.124– 0.018) or previous smoker (B=0.072, 95% CI:0.004– 0.087), having 1, 2, 3 and over 3 comorbidities (B=0.126, 95% CI:0.034– 0.147; B=0.125, 95% CI:0.031– 0.144; B=0.116, 95% CI:0.028– 0.146, B=0.090, 95% CI:0.021– 0.166) and having low hemoglobin level (B=− 0.118, 95% CI:-0.629- − 0.214) exhibited significant associations with LOS. The use of NIV (B=0.080, 95% CI:0.022– 0.138), pulmonary rehabilitation (B=0.269, 95% CI:0.212– 0.327), two and three types of inhaled medications (B=0.109, 95% CI:0.003– 0.166, B=0.255, 95% CI:0.083– 0.237) were significantly associated with longer LOS (P< 0.05).Conclusion: NIV, PR and combined inhaled medications, which are often used for AECOPD, are the main clinical therapies associated with longer LOS in Macao. Smoking cessation, early treatments of comorbidities may be crucial to avoiding AECOPD and reducing LOS and disease burden.Keywords: chronic obstructive pulmonary disease, Macao, length of hospital stay, blood test results, clinical therapy, inhaled medications, acute exacerbation
Published: 2021

118. Corrigendum: A multiply-add engine with monolithically integrated 3D memristor crossbar/CMOS hybrid circuit.

Author: Chakrabarti, B, Lastras-Montaño, M, Adam, G, Prezioso, M, Hoskins, B, Payvand, M, Madhavan, A, Ghofrani, A, Cheng, K-T, Strukov, D, and Theogarajan, Luke
Abstract: This corrects the article DOI: 10.1038/srep42429.
Published: 2017

119. A multiply-add engine with monolithically integrated 3D memristor crossbar/CMOS hybrid circuit

Author: Chakrabarti, B, Lastras-Montaño, MA, Adam, G, Prezioso, M, Hoskins, B, Payvand, M, Madhavan, A, Ghofrani, A, Theogarajan, L, Cheng, K-T, and Strukov, DB
Subjects: Information and Computing Sciences, Engineering, Nanotechnology, Physical Sciences, Affordable and Clean Energy
Abstract: Silicon (Si) based complementary metal-oxide semiconductor (CMOS) technology has been the driving force of the information-technology revolution. However, scaling of CMOS technology as per Moore's law has reached a serious bottleneck. Among the emerging technologies memristive devices can be promising for both memory as well as computing applications. Hybrid CMOS/memristor circuits with CMOL (CMOS + "Molecular") architecture have been proposed to combine the extremely high density of the memristive devices with the robustness of CMOS technology, leading to terabit-scale memory and extremely efficient computing paradigm. In this work, we demonstrate a hybrid 3D CMOL circuit with 2 layers of memristive crossbars monolithically integrated on a pre-fabricated CMOS substrate. The integrated crossbars can be fully operated through the underlying CMOS circuitry. The memristive devices in both layers exhibit analog switching behavior with controlled tunability and stable multi-level operation. We perform dot-product operations with the 2D and 3D memristive crossbars to demonstrate the applicability of such 3D CMOL hybrid circuits as a multiply-add engine. To the best of our knowledge this is the first demonstration of a functional 3D CMOL hybrid circuit.
Published: 2017

120. Hypoxia Accelerate β-actin Expression through Transcriptional Activation of ACTB by Nuclear Respiratory Factor-1

Author: Wang, X. T., Cheng, K., and Zhu, L.
Published: 2021
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121. An Intelligent Denoising Method for Jamming Pattern Recognition under Noisy Conditions

Author: Yao, C. H., Li, Y., Chen, Y. F., Cheng, K. X., Yao, C. H., Li, Y., Chen, Y. F., and Cheng, K. X.
Abstract: Accurate identification of jamming patterns is a crucial decision-making basis for anti-jamming in wireless communication systems. Current works still face challenges in fully considering the substantial influence of environmental noise on identification performance. To address the issue, this paper proposes an automatic threshold denoising-based deep learning model. The proposed method aims to mitigate the impact of noise on recognition performance within the feature space. Considering the challenges posed by non-linear transformations in deep denoising, a shallow denoising approach based on deep learning is proposed. By constructing a dataset of 12 jamming patterns under noisy conditions, the proposed method exhibits excellent recognition performance and maintains a low computational cost.
Published: 2024

122. No evidence for a volcanic trigger for late Cambrian carbon-cycle perturbations

Author: Frieling, J., Mather, T. A., Fendley, I. M., Jenkyns, H. C., Zhao, Z., Dahl, T. W., Bergquist, B. A., Cheng, K., Nielsen, Arne T., Dickson, A. J., Frieling, J., Mather, T. A., Fendley, I. M., Jenkyns, H. C., Zhao, Z., Dahl, T. W., Bergquist, B. A., Cheng, K., Nielsen, Arne T., and Dickson, A. J.
Abstract: The early Paleozoic was marked by several carbon-cycle perturbations and associated carbon-isotope excursions (CIEs). Whether these CIEs are connected to significant (external) triggers, as is commonly considered to be the case for CIEs in the Mesozoic and Cenozoic, or result from small carbon-cycle imbalances that became amplified through lack of efficient silicate weathering or other feedbacks remains unclear. We present concentration and isotope data for sedimentary mercury (Hg) and osmium (Os) to assess the impact of subaerial and submarine volcanism and weathering during the late Cambrian and early Ordovician. Data from the Alum Shale Formation (Sweden) cover the Steptoean positive carbon-isotope excursion (SPICE; ca. 497-494 Ma), a period marked by marine anoxia and biotic overturning, and several smaller CIEs extending into the early Ordovician. Our Hg and Os data offer no strong evidence that the CIEs present in our record were driven by (globally) elevated volcanism or continental weathering. Organic-carbon and Hg concentrations covary cyclically, providing further evidence of an unperturbed Hg cycle. Mesozoic and Cenozoic CIEs are commonly linked to enhanced volcanic activity and weathering, but similar late Cambrian-early Ordovician events cannot easily be connected to such external triggers. Our results are more consistent with reduced early Paleozoic carbon-cycle resilience that allowed small imbalances to develop into large CIEs.
Published: 2024

123. Measuring dark energy with the $E_{\rm iso}-E_{\rm p}$ correlation of gamma-ray bursts using model-independent methods

Author: Wang, J. S., Wang, F. Y., Cheng, K. S., and Dai, Z. G.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: In this paper, we use two model-independent methods to standardize long gamma-ray bursts (GRBs) using the $E_{\rm iso}-E_{\rm p}$ correlation, where $E_{\rm iso}$ is the isotropic-equivalent gamma-ray energy and $E_{\rm p}$ is the spectral peak energy. We update 42 long GRBs and try to make constraint on cosmological parameters. The full sample contains 151 long GRBs with redshifts from 0.0331 to 8.2. The first method is the simultaneous fitting method. The extrinsic scatter $\sigma_{\rm ext}$ is taken into account and assigned to the parameter $E_{\rm iso}$. The best-fitting values are $a=49.15\pm0.26$, $b=1.42\pm0.11$, $\sigma_{\rm ext}=0.34\pm0.03$ and $\Omega_m=0.79$ in the flat $\Lambda$CDM model. The constraint on $\Omega_m$ is $0.55<\Omega_m<1$ at the 1$\sigma$ confidence level. If reduced $\chi^2$ method is used, the best-fit results are $a=48.96\pm0.18$, $b=1.52\pm0.08$ and $\Omega_m=0.50\pm0.12$. The second method is using type Ia supernovae (SNe Ia) to calibrate the $E_{\rm iso}-E_{\rm p}$ correlation. We calibrate 90 high-redshift GRBs in the redshift range from 1.44 to 8.1. The cosmological constraints from these 90 GRBs are $\Omega_m=0.23^{+0.06}_{-0.04}$ for flat $\Lambda$CDM, and $\Omega_m=0.18\pm0.11$ and $\Omega_{\Lambda}=0.46\pm0.51$ for non-flat $\Lambda$CDM. For the combination of GRB and SNe Ia sample, we obtain $\Omega_m=0.271\pm0.019$ and $h=0.701\pm0.002$ for the flat $\Lambda$CDM, and for the non-flat $\Lambda$CDM, the results are $\Omega_m=0.225\pm0.044$, $\Omega_{\Lambda}=0.640\pm0.082$ and $h=0.698\pm0.004$. These results from calibrated GRBs are consistent with that of SNe Ia. Meanwhile, the combined data can improve cosmological constraints significantly, comparing to SNe Ia alone. Our results show that the $E_{\rm iso}-E_{\rm p}$ correlation is promising to probe the high-redshift universe., Comment: 10 pages, 6 figures, 4 table, accepted by A&A. Table 4 contains calibrated distance moduli of GRBs
Published: 2015
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124. Searches for millisecond pulsar candidates among the unidentified Fermi objects

Author: Hui, C. Y., Park, S. M., Hu, C. P., Lin, L. C. C., Li, K. L., Kong, A. K. H., Tam, P. H. T., Takata, J., Cheng, K. S., Jin, Ruolan, Yen, T. -C., and Kim, Chunglee
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Here we report the results of searching millisecond pulsar (MSP) candidates from the Fermi LAT second source catalog (2FGL). Seven unassociated $\gamma-$ray sources in this catalog are identified as promising MSP candidates based on their $\gamma$-ray properties. Through the X-ray analysis, we have detected possible X-ray counterparts, localized to an arcsecond accuracy. We have systematically estimated their X-ray fluxes and compared with the corresponding $\gamma$-ray fluxes. The X-ray to $\gamma$-ray flux ratios for 2FGL J1653.6-0159 and 2FGL J1946.4-5402 are comparable with the typical value for pulsars. For 2FGL J1625.2-0020, 2FGL J1653.6-0159 and 2FGL J1946.4-5402, their candidate X-ray counterparts are bright enough for performing a detailed spectral and temporal analysis to discriminate their thermal/non thermal nature and search for the periodic signal. We have also searched for possible optical/IR counterparts at the X-ray positions. For the optical/IR source coincident with the brightest X-ray object that associated with 2FGL J1120.0-2204, its spectral energy distribution is comparable with a late-type star. Evidence for the variability has also been found by examining its optical light curve. All the aforementioned 2FGL sources resemble a pulsar in one or more aspects, which make them as the promising targets for follow-up investigations., Comment: 37 pages, 12 figures, 6 tables, accepted for publication in ApJ
Published: 2015
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125. Spectrum of Relativistic and Subrelativistic Cosmic Rays in the 100 pc Central Region

Author: Dogiel, V. A., Chernyshov, D. O., Kiselev, A. M., Nobukawa, M., Cheng, K. S., Hui, C. Y., Ko, C. M., Nobukawa, K. K., and Tsuru, T. G.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: From the rate of hydrogen ionization and the gamma ray flux, we derived the spectrum of relativistic and subrelativistic cosmic rays (CRs) nearby and inside the molecular cloud Sgr B2 near the Galactic Center (GC). We studied two cases of CR propagation in molecular clouds: free propagation and scattering of particles by magnetic fluctuations excited by the neutral gas turbulence. We showed that in the latter case CR propagation inside the cloud can be described as diffusion with the coefficient $\sim 3\times 10^{27}$ cm$^2$ s$^{-1}$. For the case of hydrogen ionization by subrelativistic protons, we showed that their spectrum outside the cloud is quite hard with the spectral index $\delta>-1$. The energy density of subrelativistic protons ($>50$ eV cm$^{-3}$) is one order of magnitude higher than that of relativistic CRs. These protons generate the 6.4 keV emission from Sgr B2, which was about 30\% of the flux observed by Suzaku in 2013. Future observations for the period after 2013 may discover the background flux generated by subrelativistic CRs in Sgr B2. Alternatively hydrogen ionization of the molecular gas in Sgr B2 may be caused by high energy electrons. We showed that the spectrum of electron bremsstrahlung is harder than the observed continuum from Sgr B2, and in principle this X-ray component provided by electrons could be seen from the INTEGRAL data as a stationary high energy excess above the observed spectrum $E_x^{-2}$., Comment: 42 pages, 6 figures, accepted by ApJ
Published: 2015
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126. An unexpectedly low-redshift excess of Swift gamma-ray burst rate

Author: Yu, H., Wang, F. Y., Dai, Z. G., and Cheng, K. S.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Gamma-ray bursts (GRBs) are the most violent explosions in the Universe and can be used to explore the properties of high-redshift universe. It is believed that the long GRBs are associated with the deaths of massive stars. So it is possible to use GRBs to investigate the star formation rate (SFR). In this paper, we use Lynden-Bell's $c^-$ method to study the luminosity function and rate of \emph{Swift} long GRBs without any assumptions. We find that the luminosity of GRBs evolves with redshift as $L(z)\propto g(z)=(1+z)^k$ with $k=2.43_{-0.38}^{+0.41}$. After correcting the redshift evolution through $L_0(z)=L(z)/g(z)$, the luminosity function can be expressed as $\psi(L_0)\propto L_0^{-0.14\pm0.02}$ for dim GRBs and $\psi(L_0)\propto L_0^{-0.70\pm0.03}$ for bright GRBs, with the break point $L_{0}^{b}=1.43\times10^{51}~{\rm erg~s^{-1}}$. We also find that the formation rate of GRBs is almost constant at $z<1.0$ for the first time, which is remarkably different from the SFR. At $z>1.0$, the formation rate of GRB is consistent with the SFR. Our results are dramatically different from previous studies. Some possible reasons for this low-redshift excess are discussed. We also test the robustness of our results with Monte Carlo simulations. The distributions of mock data (i.e., luminosity-redshift distribution, luminosity function, cumulative distribution and $\log N-\log S$ distribution) are in good agreement with the observations. Besides, we also find that there are remarkable difference between the mock data and the observations if long GRB are unbiased tracers of SFR at $z<1.0$., Comment: 33 pages, 10 figures, 1 table, accepted by ApJS
Published: 2015
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127. Multi-wavelength Emission from the Fermi Bubble III. Stochastic (Fermi) Re-Acceleration of Relativistic Electrons Emitted by SNRs

Author: Cheng, K. S., Chernyshov, D. O., Dogiel, V. A., and Ko, C. M.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We analyse the model of stochastic re-acceleration of electrons, which are emitted by supernova remnants (SNRs) in the Galactic Disk and propagate then into the Galactic halo, in order to explain the origin on nonthermal (radio and gamma-ray) emission from the Fermi Bubbles (FB). We assume that the energy for re-acceleration in the halo is supplied by shocks generated by processes of star accretion onto the central black hole. Numerical simulations show that regions with strong turbulence (places for electron re-acceleration) are located high up in the Galactic Halo about several kpc above the disk. The energy of SNR electrons that reach these regions does not exceed several GeV because of synchrotron and inverse Compton energy losses. At appropriate parameters of re-acceleration these electrons can be re-accelerated up to the energy 10E12 eV which explains in this model the origin of the observed radio and gamma-ray emission from the FB. However although the model gamma-ray spectrum is consistent with the Fermi results, the model radio spectrum is steeper than the observed by WMAP and Planck. If adiabatic losses due to plasma outflow from the Galactic central regions are taken into account, then the re-acceleration model nicely reproduces the Planck datapoints., Comment: 33 pages, 8 figures, accepted by ApJ
Published: 2015
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128. Exploring the intrabinary shock from the redback millisecond pulsar PSR J2129-0429

Author: Hui, C. Y., Hu, C. P., Park, S. M., Takata, J., Li, K. L., Tam, P. H. T., Lin, L. C. C., Kong, A. K. H., Cheng, K. S., and Kim, Chunglee
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We have investigated the intrabinary shock emission from the redback millisecond pulsar PSR J2129-0429 with XMM-Newton and Fermi. Orbital modulation in X-ray and UV can be clearly seen. Its X-ray modulation has a double-peak structure with a dip in between. The observed X-rays are non-thermal dominant which can be modeled by a power-law with a photon index of ~1.2. Intrabinary shock can be the origin of the observed X-rays. The UV light curve is resulted from the ellipsoidal modulation of the companion. Modeling the UV light curve prefers a large viewing angle. The heating effect of the UV light curve is found to be negligible which suggests the high energy radiation beam of PSR J2129-0429 does not direct toward its companion. On the other hand, no significant orbital modulation can be found in gamma-ray which suggests the majority of the gamma-rays come from the pulsar., Comment: 14 pages, 3 figures, 1 table, accepted for publication in ApJ Letter
Published: 2015
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129. Constraining the bulk Lorentz factor from the photosphere emission

Author: Zou, Yuan-Chuan, Cheng, K. S., and Wang, F. Y.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We propose a direct and model-independent method to constrain the Lorentz factor of a relativistically expanding object, like gamma-ray bursts. Only the measurements, such as thermal component of the emission, the distance and the variable time scale of the light curve, are used. If the uncertainties are considered, we will obtain lower limits of the Lorentz factor instead. We apply this method to GRB 090618 and get a lower limit of the Lorentz factor to be 22. The method can be used to any relativistically moving object, such as gamma-ray bursts, blazars, and soft gamma-ray repeaters, providing the thermal component of the emission being observed., Comment: 10 pages, 1 figure
Published: 2015
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130. The birth of radio millisecond pulsars and their high-energy signature

Author: Tam, P. H. T., Li, K. L., Kong, A. K. H., Takata, J., Leung, G. C. K., Cheng, K. S., and Hui, C. Y.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
Abstract: Millisecond pulsars (MSPs) are thought to born in low-mass X-ray binaries when the neutron star has gained enough angular momentum from the accreting materials of its companion star. It is generally believed that a radio MSP is born when the neutron star stops accreting and enters a rotation-powered state. Exactly what happens during the transition time was poorly understood until a year ago. In the past year, observations have revealed a few objects that not only switched from one state to the other (as predicted in the above picture), but also have swung between the two states within weeks to years. In this work, we present observations of two of these transition objects (PSR J1023+0038 and XSS J12270-4859) and a theoretical framework that tries to explain their high-energy radiation., Comment: 7 pages, 6 figures; presented at the 10th INTEGRAL Workshop: 'A Synergistic View of the High Energy Sky' - Integral2014, held 15-19 September 2014, Annapolis, MD
Published: 2014

131. Origin of Hydrogen Ionization in the 1 pc Galactic Central Region

Author: Chernyshov, D. O., Leung, Gene C. K., Cheng, K. S., Dogiel, V. A., and Tatischeff, V.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena
Abstract: We study a possible connection between processes of gamma-ray emission and hydrogen ionization in a few pc of central region around Sgr A*. Previous investigations showed there is a discrepancy between interpretation of gamma-ray and ionization data if gamma-rays are generated by proton-proton collisions. Here we provided analysis of processes of ionization and emission basing on analytical and numerical calculations of kinetic equations which describe processes of particle propagation and their energy losses. The origin of gamma rays could be either due to collisions of relativistic protons with the dense gas of the surrounding circumnuclear disk (CND) or bremsstrahlung and inverse Compton scattering of relativistic electrons. The hydrogen ionization in this case is produced by a low energy component of the CR spectrum. We found that if ionization is produced by protons the expected ionization rate of hydrogen in the CND is of the same order as derived from IR observations. So we do not see any discrepancy between the gamma-ray and ionization data for the hadronic model. In the case of ionization by electrons we obtained the ionization rate one order of magnitude higher than follows from the IR data. In principle, a selection between the leptonic and hadronic interpretations can be performed basing on measurements of radio and X-ray fluxes from this region because the leptonic and hadronic models give different values of the fluxes from there. We do not exclude that gamma-ray production and hydrogen ionization in the CND are due to a past activity of Sgr A* which occurred about 100 year ago. Then we hypothesize that there may be connection between a past proton eruption and a flux of hard X-rays emitted by Sgr A* hundred years ago as follows from the observed time variability of the iron line seen in the direction of GC molecular clouds., Comment: 21 pages, 10 figures. Submitted
Published: 2014

132. Fermi bubbles as a source of cosmic rays above 10^{15} eV

Author: Chernyshov, D. O., Cheng, K. S., Dogiel, V. A., and Ko, C. M.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Fermi bubbles are giant gamma-ray structures extended north and south of the Galactic center with characteristic sizes of order of 10 kpc recently discovered by Fermi Large Area Telescope. Good correlation between radio and gamma-ray emission in the region covered by Fermi bubbles implies the presence of high-energy electrons in this region. Since it is relatively difficult for relativistic electrons of this energy to travel all the way from the Galactic sources toward Fermi bubbles one can assume that they accelerated in-situ. The corresponding acceleration mechanism should also affect the distribution of the relativistic protons in the Galaxy. Since protons have much larger lifetimes the effect may even be observed near the Earth. In our model we suggest that Fermi bubbles are created by acceleration of electrons on series of shocks born due to periodic star accretions by supermassive black hole Sgr A*. We propose that hadronic CR within the "knee" of the observed CR spectrum are produced by Galactic supernova remnants distributed in the Galactic disk. Reacceleration of these particles in the Fermi Bubble produces CRs beyond the knee. This model provides a natural explanation of the observed CR flux, spectral indexes, and matching of spectra at the knee., Comment: 7 pages, 3 figures. Published in Nuclear Physics B, oral talk at the conference "Cosmic ray origin - beyond the standard models" San-Vito di Cadore, Italy, March 16-22, 2014
Published: 2014
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133. Multi-wavelength Emission from the Fermi Bubble II. Secondary Electrons and the Hadronic Model of the Bubble

Author: Cheng, K. -S., Chernyshov, D. O., Dogiel, V. A., and Ko, C. -M.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena
Abstract: We analyse the origin of the gamma-ray flux from the Fermi Bubbles (FBs) in the framework of the hadronic model in which gamma-rays are produced by collisions of relativistic protons with the protons of background plasma in the Galactic halo. It is assumed in this model that the observed radio emission from the FBs is due to synchrotron radiation of secondary electrons produced by $pp$ collisions. However, if these electrons loose their energy by the synchrotron and inverse-Compton, the spectrum of secondary electrons is too soft, and an additional arbitrary component of primary electrons is necessary in order to reproduce the radio data. Thus, a mixture of the hadronic and leptonic models is required for the observed radio flux. It was shown that if the spectrum of primary electrons is $\propto E_e^{-2}$, the permitted range of the magnetic field strength is within 2 - 7 $\mu$G region. The fraction of gamma-rays produced by $pp$ collisions can reach about 80% of the total gamma-ray flux from the FBs. If magnetic field is <2 $\mu$G or >7 $\mu$G the model is unable to reproduce the data. Alternatively, the electrons in the FBs may lose their energy by adiabatic energy losses if there is a strong plasma outflow in the GC. Then, the pure hadronic model is able to reproduce characteristics of the radio and gamma-ray flux from the FBs. However, in this case the required magnetic field strength in the FBs and the power of CR sources are much higher than those followed from observations., Comment: 18 pages, 4 figures. Accepted for publication in ApJ
Published: 2014
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134. A detailed X-ray investigation of PSR J2021+4026 and $\gamma$-Cygni supernova remnant

Author: Hui, C. Y., Seo, K. A., Lin, L. C. C., Huang, R. H. H., Hu, C. P., Wu, J. H. K., Trepl, L., Takata, J., Wang, Y., Chou, Y., Cheng, K. S., and Kong, A. K. H.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We have investigated the field around the radio-quiet $\gamma$-ray pulsar, PSR J2021+4026, with a ~140 ks XMM-Newton observation and a ~56 ks archival Chandra data. Through analyzing the pulsed spectrum, we show that the X-ray pulsation is purely thermal in nature which suggests the pulsation is originated from a hot polar cap with $T\sim3\times10^{6}$ K on the surface of a rotating neutron star. On the other hand, the power-law component that dominates the pulsar emission in the hard band is originated from off-pulse phases, which possibly comes from a pulsar wind nebula. In re-analyzing the Chandra data, we have confirmed the presence of bow-shock nebula which extends from the pulsar to west by ~10 arcsec. The orientation of this nebular feature suggests that the pulsar is probably moving eastward which is consistent with the speculated proper motion by extrapolating from the nominal geometrical center of the supernova remnant (SNR) G78.2+2.1 to the current pulsar position. For G78.2+2.1, our deep XMM-Newton observation also enables a study of the central region and part of the southeastern region with superior photon statistics. The column absorption derived for the SNR is comparable with that for PSR J2021+4026, which supports their association. The remnant emission in both examined regions are in an non-equilibrium ionization state. Also, the elapsed time of both regions after shock-heating is apparently shorter than the Sedov age of G78.2+2.1. This might suggest the reverse shock has reached the center not long ago. Apart from PSR J2021+4026 and G78.2+2.1, we have also serendipitously detected an X-ray flash-like event XMM J202154.7+402855 from this XMM-Newton observation., Comment: 45 pages, 10 figures, 2 tables, accepted for publication in ApJ
Published: 2014
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135. Multi-channel nanowire devices for efficient power conversion

Author: Nela, L., Ma, J., Erine, C., Xiang, P., Shen, T.-H., Tileli, V., Wang, T., Cheng, K., and Matioli, E.
Published: 2021
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136. Enhancing Axial Fan Noise Reduction through Innovative Wavy Blade Configurations.

Author: Qi, W. C., Cheng, K., Li, P. C., and Li, J. Y.
Subjects: NOISE control, AXIAL flow, AERODYNAMIC noise, VORTEX shedding, LARGE eddy simulation models
Abstract: Noise is one of the key indicators to evaluate axial flow fans, and in many cases, it is also the only indicator for determining their suitability for use. In this study, a new method to reduce axial fan's noise was proposed for changing the section chord length to transform the blades of two axial fans with the same design parameters but distinct chord lengths to wavy blades. The aerodynamic calculations and noise reduction mechanism of the wavy configuration of the two fans were studied by combining CFD of large eddy simulation with the Lighthill acoustic analogy method. The results showed that the main mechanism contributing to noise reduction through wavy configuration was the promotion of transformation of the blade surface's layered vortex structure into an uncorrelated comb vortex structure. For fan blades with smaller chord lengths, the comb structure with low spanwise correlation was still maintained after the trailing edge, while for fan blades with larger chord lengths, the comb structure of the shedding vortex rapidly dissipated downstream of the trailing edge. Under the rated design conditions, the implementation of wavy leading edge blades resulted in noise reductions of 1.9 dB and 1.5 dB for the two fans, respectively, while wavy trailing edge blades yielded reductions of 2.6 dB and 2.1 dB, respectively. Furthermore, the adoption of wavy configuration induced a phenomenon of pressure increase and efficiency decrease in both axial fans at medium and low flow rates, with minimal impact at high flow rates. These outcomes underscored the superior noise reduction efficacy of the wavy trailing edge blades, offering a promising way for the noise reduction design of axial flow fans. [ABSTRACT FROM AUTHOR]
Published: 2024
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137. Empirical Model of the Lowest Cutoff Altitude of Global Hiss Near Magnetic Equator.

Author: Li, L. Y., Yang, L., Cheng, K. X., Cao, J. B., Yang, J. Y., and Berthelier, J. J.
Subjects: ALTITUDES, RADIATION belts, TERRESTRIAL radiation, HYDROGEN ions
Abstract: Van Allen Probe observations indicate that whistler‐mode hiss waves below 1 kHz are absorbed at low altitudes near magnetic equator. The lowest cutoff frequency of equatorial hiss is close to the gyrofrequency of hydrogen ions. The lowest cutoff altitude of global hiss is extracted when its occurrence rate is equal to 0.005 on the plane of altitude (L in RE) and magnetic local time (MLT). By fitting the lowest cutoff altitude of global hiss, we constructed the empirical model of the lowest cutoff altitude of equatorial hiss under geomagnetically quiet (AE < 200 nT) and active (AE ≥ 200 nT) conditions. The enhanced substorm activities reduce the lowest cutoff altitude of hiss waves on the dawnside (MLT ∼ 1–5 hr), whereas the lowest cutoff altitude of the dayside hiss is nearly fixed at ∼1.1 RE (MLT ∼ 6–20 hr). From the dayside to the nightside (MLT ∼ 0–6 hr and 20–24 hr), the lowest cutoff altitude of equatorial hiss raises gradually from 1.1 RE to 1.4 RE. Plain Language Summary: Plasmaspheric hiss can cause the scattering loss of Earth's radiation belt electrons via wave‐particle resonant interactions and creates a slot region relatively safe for satellites. Thus, their spatial distribution is a key parameter controlling the dynamics of radiation belts. Although the outer boundary of hiss waves can be estimated with the empirical plasmapause location, there is no any empirical model to quantificationally describe their inner boundary. Here, based on the Van Allen Probe observations, we constructed empirical models to estimate the lowest cutoff altitude of global hiss under different geomagnetic conditions. The new empirical models provide an inner boundary for simulating the resonant interactions between hiss waves and high‐energy electrons. Key Points: The lowest cutoff altitude of global hiss is quantificationally examined with Van Allen Probes observations near the magnetic equatorThe lowest cutoff altitude of equatorial hiss is nearly fixed at L ∼ 1.1 on the dayside, but changes between L ∼ 1.1–1.4 on the nightsideNew empirical models are constructed to estimate the lowest cutoff altitude of global hiss under different geomagnetic conditions [ABSTRACT FROM AUTHOR]
Published: 2024
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138. Erratum to: Measurement of the top quark mass with lepton+jets final states using pp collisions at s=13TeV

Author: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Erö, J., Valle, A. Escalante Del, Flechl, M., Friedl, M., Frühwirth, R., Ghete, V. M., Hrubec, J., Jeitler, M., Krammer, N., Krätschmer, I., Liko, D., Madlener, T., Mikulec, I., Rad, N., Rohringer, H., Schieck, J., Schöfbeck, R., Spanring, M., Spitzbart, D., Taurok, A., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, De Wolf, E. A., Croce, D. Di, Janssen, X., Lauwers, J., Pieters, M., De Klundert, M. Van, Haevermaet, H. Van, Mechelen, P. Van, Remortel, N. Van, Zeid, S. Abu, Blekman, F., D’Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Marchesini, I., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Doninck, W. Van, Mulders, P. Van, Parijs, I. Van, Beghin, D., Bilin, B., Brun, H., Clerbaux, B., De Lentdecker, G., Delannoy, H., Dorney, B., Fasanella, G., Favart, L., Goldouzian, R., Grebenyuk, A., Kalsi, A. K., Lenzi, T., Luetic, J., Seva, T., Starling, E., Velde, C. Vander, Vanlaer, P., Vannerom, D., Yonamine, R., Cornelis, T., Dobur, D., Fagot, A., Gul, M., Khvastunov, I., Poyraz, D., Roskas, C., Trocino, D., Tytgat, M., Verbeke, W., Vermassen, B., Vit, M., Zaganidis, N., Bakhshiansohi, H., Bondu, O., Brochet, S., Bruno, G., Caputo, C., Caudron, A., David, P., De Visscher, S., Delaere, C., Delcourt, M., Francois, B., Giammanco, A., Krintiras, G., Lemaitre, V., Magitteri, A., Mertens, A., Musich, M., Piotrzkowski, K., Quertenmont, L., Saggio, A., Marono, M. Vidal, Wertz, S., Zobec, J., Júnior, W. L. Aldá, Alves, F. L., Alves, G. A., Brito, L., Silva, G. Correia, Hensel, C., Moraes, A., Pol, M. E., Teles, P. Rebello, Chagas, E. Belchior Batista Das, Carvalho, W., Chinellato, J., Coelho, E., Da Costa, E. M., Da Silveira, G. G., De Jesus Damiao, D., De Souza, S. Fonseca, Malbouisson, H., Jaime, M. Medina, De Almeida, M. Melo, Herrera, C. Mora, Mundim, L., Nogima, H., Rosas, L. J. Sanchez, Santoro, A., Sznajder, A., Thiel, M., Manganote, E. J. Tonelli, Da Silva De Araujo, F. Torres, Pereira, A. Vilela, Ahuja, S., Bernardes, C. A., Calligaris, Luigi, Tomei, T. R. Fernandez Perez, Gregores, E. M., Mercadante, P. G., Novaes, S. F., Padula, Sandra S., Abad, D. Romero, Vargas, J. C. Ruiz, Aleksandrov, A., Hadjiiska, R., Iaydjiev, P., Marinov, A., Misheva, M., Rodozov, M., Shopova, M., Sultanov, G., Dimitrov, A., Litov, L., Pavlov, B., Petkov, P., Fang, W., Gao, X., Yuan, L., Ahmad, M., Bian, J. G., Chen, G. M., Chen, H. S., Chen, M., Chen, Y., Jiang, C. H., Leggat, D., Liao, H., Liu, Z., Romeo, F., Shaheen, S. M., Spiezia, A., Tao, J., Wang, C., Wang, Z., Yazgan, E., Zhang, H., Zhao, J., Ban, Y., Chen, G., Li, J., Li, Q., Liu, S., Mao, Y., Qian, S. J., Wang, D., Xu, Z., Wang, Y., Avila, C., Cabrera, A., Montoya, C. A. Carrillo, Sierra, L. F. Chaparro, Florez, C., Hernández, C. F. González, Delgado, M. A. Segura, Courbon, B., Godinovic, N., Lelas, D., Puljak, I., Sculac, T., Antunovic, Z., Kovac, M., Brigljevic, V., Ferencek, D., Kadija, K., Mesic, B., Starodumov, A., Susa, T., Ather, M. W., Attikis, A., Mavromanolakis, G., Mousa, J., Nicolaou, C., Ptochos, F., Razis, P. A., Rykaczewski, H., Finger, M., Finger, Jr., M., Jarrin, E. Carrera, Mahmoud, M. A., Mohamed, Elgammal A., Salama, E., Bhowmik, S., Dewanjee, R. K., Kadastik, M., Perrini, L., Raidal, M., Veelken, C., Eerola, P., Kirschenmann, H., Pekkanen, J., Voutilainen, M., Havukainen, J., Heikkilä, J. K., Järvinen, T., Karimäki, V., Kinnunen, R., Lampén, T., Lassila-Perini, K., Laurila, S., Lehti, S., Lindén, T., Luukka, P., Mäenpää, T., Siikonen, H., Tuominen, E., Tuominiemi, J., Tuuva, T., Besancon, M., Couderc, F., Dejardin, M., Denegri, D., Faure, J. 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Published: 2022
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139. Erratum to: Measurement of exclusive ΥsNN=5.02TeV photoproduction from protons in pPb collisions at ΥsNN=5.02TeV

Author: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Erö, J., Valle, A. Escalante Del, Flechl, M., Friedl, M., Frühwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., König, A., Krammer, N., Krätschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rad, N., Rohringer, H., Schieck, J., Schöfbeck, R., Spanring, M., Spitzbart, D., Taurok, A., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, De Wolf, E. A., Croce, D. Di, Janssen, X., Lauwers, J., Pieters, M., De Klundert, M. Van, Haevermaet, H. Van, Mechelen, P. Van, Remortel, N. Van, Zeid, S. Abu, Blekman, F., D’Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Marchesini, I., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Doninck, W. Van, Mulders, P. Van, Parijs, I. 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Published: 2022
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140. Erratum to: Search for new physics in dijet angular distributions using proton-proton collisions at s=13TeV and constraints on dark matter and other models

Author: Sirunyan, A. M., Tumasyan, A., Adam, W., Ambrogi, F., Asilar, E., Bergauer, T., Brandstetter, J., Brondolin, E., Dragicevic, M., Erö, J., Valle, A. Escalante Del, Flechl, M., Friedl, M., Frühwirth, R., Ghete, V. M., Grossmann, J., Hrubec, J., Jeitler, M., König, A., Krammer, N., Krätschmer, I., Liko, D., Madlener, T., Mikulec, I., Pree, E., Rad, N., Rohringer, H., Schieck, J., Schöfbeck, R., Spanring, M., Spitzbart, D., Taurok, A., Waltenberger, W., Wittmann, J., Wulz, C.-E., Zarucki, M., Chekhovsky, V., Mossolov, V., Gonzalez, J. Suarez, De Wolf, E. A., Croce, D. Di, Janssen, X., Lauwers, J., Pieters, M., De Klundert, M. Van, Haevermaet, H. Van, Mechelen, P. Van, Remortel, N. Van, Zeid, S. Abu, Blekman, F., D’Hondt, J., De Bruyn, I., De Clercq, J., Deroover, K., Flouris, G., Lontkovskyi, D., Lowette, S., Marchesini, I., Moortgat, S., Moreels, L., Python, Q., Skovpen, K., Tavernier, S., Doninck, W. Van, Mulders, P. Van, Parijs, I. 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M., Mason, D., McBride, P., Merkel, P., Mrenna, S., Nahn, S., O’Dell, V., Pedro, K., Prokofyev, O., Rakness, G., Ristori, L., Savoy-Navarro, A., Schneider, B., Sexton-Kennedy, E., Soha, A., Spalding, W. J., Spiegel, L., Stoynev, S., Strait, J., Strobbe, N., Taylor, L., Tkaczyk, S., Tran, N. V., Uplegger, L., Vaandering, E. W., Vernieri, C., Verzocchi, M., Vidal, R., Wang, M., Weber, H. A., Whitbeck, A., Wu, W., Acosta, D., Avery, P., Bortignon, P., Bourilkov, D., Brinkerhoff, A., Carnes, A., Carver, M., Curry, D., Field, R. D., Furic, I. K., Gleyzer, S. V., Joshi, B. M., Konigsberg, J., Korytov, A., Kotov, K., Ma, P., Matchev, K., Mei, H., Mitselmakher, G., Shi, K., Sperka, D., Terentyev, N., Thomas, L., Wang, J., Wang, S., Yelton, J., Joshi, Y. R., Linn, S., Markowitz, P., Rodriguez, J. L., Ackert, A., Adams, T., Askew, A., Hagopian, S., Hagopian, V., Johnson, K. F., Kolberg, T., Martinez, G., Perry, T., Prosper, H., Saha, A., Santra, A., Sharma, V., Yohay, R., Baarmand, M. M., Bhopatkar, V., Colafranceschi, S., Hohlmann, M., Noonan, D., Roy, T., Yumiceva, F., Adams, M. R., Apanasevich, L., Berry, D., Betts, R. R., Cavanaugh, R., Chen, X., Dittmer, S., Evdokimov, O., Gerber, C. E., Hangal, D. A., Hofman, D. J., Jung, K., Kamin, J., Gonzalez, I. D. Sandoval, Tonjes, M. B., Varelas, N., Wang, H., Wu, Z., Zhang, J., Bilki, B., Clarida, W., Dilsiz, K., Durgut, S., Gandrajula, R. P., Haytmyradov, M., Khristenko, V., Merlo, J.-P., Mermerkaya, H., Mestvirishvili, A., Moeller, A., Nachtman, J., Ogul, H., Onel, Y., Ozok, F., Penzo, A., Snyder, C., Tiras, E., Wetzel, J., Yi, K., Blumenfeld, B., Cocoros, A., Eminizer, N., Fehling, D., Feng, L., Gritsan, A. V., Hung, W. T., Maksimovic, P., Roskes, J., Sarica, U., Swartz, M., Xiao, M., You, C., Al-bataineh, A., Baringer, P., Bean, A., Boren, S., Bowen, J., Castle, J., Khalil, S., Kropivnitskaya, A., Majumder, D., Mcbrayer, W., Murray, M., Rogan, C., Royon, C., Sanders, S., Schmitz, E., Takaki, J. D. Tapia, Wang, Q., Ivanov, A., Kaadze, K., Maravin, Y., Modak, A., Mohammadi, A., Saini, L. K., Skhirtladze, N., Rebassoo, F., Wright, D., Baden, A., Baron, O., Belloni, A., Eno, S. C., Feng, Y., Ferraioli, C., Hadley, N. J., Jabeen, S., Jeng, G. Y., Kellogg, R. G., Kunkle, J., Mignerey, A. C., Ricci-Tam, F., Shin, Y. H., Skuja, A., Tonwar, S. C., Abercrombie, D., Allen, B., Azzolini, V., Barbieri, R., Baty, A., Bauer, G., Bi, R., Brandt, S., Busza, W., Cali, I. A., D’Alfonso, M., Demiragli, Z., Ceballos, G. Gomez, Goncharov, M., Harris, P., Hsu, D., Hu, M., Iiyama, Y., Innocenti, G. M., Klute, M., Kovalskyi, D., Lee, Y.-J., Levin, A., Luckey, P. D., Maier, B., Marini, A. C., Mcginn, C., Mironov, C., Narayanan, S., Niu, X., Paus, C., Roland, C., Roland, G., Stephans, G. S. F., Sumorok, K., Tatar, K., Velicanu, D., Wang, J., Wang, T. W., Wyslouch, B., Zhaozhong, S., Benvenuti, A. C., Chatterjee, R. M., Evans, A., Hansen, P., Kalafut, S., Kubota, Y., Lesko, Z., Mans, J., Nourbakhsh, S., Ruckstuhl, N., Rusack, R., Turkewitz, J., Wadud, M. A., Acosta, J. G., Oliveros, S., Avdeeva, E., Bloom, K., Claes, D. R., Fangmeier, C., Golf, F., Suarez, R. Gonzalez, Kamalieddin, R., Kravchenko, I., Monroy, J., Siado, J. E., Snow, G. R., Stieger, B., Godshalk, A., Harrington, C., Iashvili, I., Nguyen, D., Parker, A., Rappoccio, S., Roozbahani, B., Alverson, G., Barberis, E., Freer, C., Hortiangtham, A., Massironi, A., Morse, D. M., Orimoto, T., De Lima, R. Teixeira, Wamorkar, T., Wang, B., Wisecarver, A., Wood, D., Bhattacharya, S., Charaf, O., Hahn, K. A., Mucia, N., Odell, N., Schmitt, M. H., Sung, K., Trovato, M., Velasco, M., Bucci, R., Dev, N., Hildreth, M., Anampa, K. Hurtado, Jessop, C., Karmgard, D. J., Kellams, N., Lannon, K., Li, W., Loukas, N., Marinelli, N., Meng, F., Mueller, C., Musienko, Y., Planer, M., Reinsvold, A., Ruchti, R., Siddireddy, P., Smith, G., Taroni, S., Wayne, M., Wightman, A., Wolf, M., Woodard, A., Alimena, J., Antonelli, L., Bylsma, B., Durkin, L. S., Flowers, S., Francis, B., Hart, A., Hill, C., Ji, W., Ling, T. Y., Luo, W., Winer, B. L., Wulsin, H. W., Cooperstein, S., Driga, O., Elmer, P., Hardenbrook, J., Hebda, P., Higginbotham, S., Kalogeropoulos, A., Lange, D., Luo, J., Marlow, D., Mei, K., Ojalvo, I., Olsen, J., Palmer, C., Piroué, P., Salfeld-Nebgen, J., Stickland, D., Tully, C., Malik, S., Norberg, S., Barker, A., Barnes, V. E., Das, S., Gutay, L., Jones, M., Jung, A. W., Khatiwada, A., Miller, D. H., Neumeister, N., Peng, C. C., Qiu, H., Schulte, J. F., Sun, J., Wang, F., Xiao, R., Xie, W., Cheng, T., Dolen, J., Parashar, N., Chen, Z., Ecklund, K. M., Freed, S., Geurts, F. J. M., Guilbaud, M., Kilpatrick, M., Li, W., Michlin, B., Padley, B. P., Roberts, J., Rorie, J., Shi, W., Tu, Z., Zabel, J., Zhang, A., Bodek, A., de Barbaro, P., Demina, R., Duh, Y. t., Ferbel, T., Galanti, M., Garcia-Bellido, A., Han, J., Hindrichs, O., Khukhunaishvili, A., Lo, K. H., Tan, P., Verzetti, M., Ciesielski, R., Goulianos, K., Mesropian, C., Agapitos, A., Chou, J. P., Gershtein, Y., Espinosa, T. A. Gómez, Halkiadakis, E., Heindl, M., Hughes, E., Kaplan, S., Elayavalli, R. Kunnawalkam, Kyriacou, S., Lath, A., Montalvo, R., Nash, K., Osherson, M., Saka, H., Salur, S., Schnetzer, S., Sheffield, D., Somalwar, S., Stone, R., Thomas, S., Thomassen, P., Walker, M., Delannoy, A. G., Heideman, J., Riley, G., Rose, K., Spanier, S., Thapa, K., Bouhali, O., Hernandez, A. Castaneda, Celik, A., Dalchenko, M., De Mattia, M., Delgado, A., Dildick, S., Eusebi, R., Gilmore, J., Huang, T., Kamon, T., Mueller, R., Pakhotin, Y., Patel, R., Perloff, A., Perniè, L., Rathjens, D., Safonov, A., Tatarinov, A., Akchurin, N., Damgov, J., De Guio, F., Dudero, P. R., Faulkner, J., Gurpinar, E., Kunori, S., Lamichhane, K., Lee, S. W., Mengke, T., Muthumuni, S., Peltola, T., Undleeb, S., Volobouev, I., Wang, Z., Greene, S., Gurrola, A., Janjam, R., Johns, W., Maguire, C., Melo, A., Ni, H., Padeken, K., Alvarez, J. D. Ruiz, Sheldon, P., Tuo, S., Velkovska, J., Xu, Q., Arenton, M. W., Barria, P., Cox, B., Hirosky, R., Joyce, M., Ledovskoy, A., Li, H., Neu, C., Sinthuprasith, T., Wang, Y., Wolfe, E., Xia, F., Harr, R., Karchin, P. E., Poudyal, N., Sturdy, J., Thapa, P., Zaleski, S., Brodski, M., Buchanan, J., Caillol, C., Carlsmith, D., Dasu, S., Dodd, L., Duric, S., Gomber, B., Grothe, M., Herndon, M., Hervé, A., Hussain, U., Klabbers, P., Lanaro, A., Levine, A., Long, K., Loveless, R., Rekovic, V., Ruggles, T., Savin, A., Smith, N., Smith, W. H., and Woods, N.
Published: 2022
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141. 89Zr-Labeled Multifunctional Liposomes Conjugate Chitosan for PET-Trackable Triple-Negative Breast Cancer Stem Cell Targeted Therapy

Author: Yang R, Lu M, Ming L, Chen Y, Cheng K, Zhou J, Jiang S, Lin Z, and Chen D
Subjects: radionuclide, pet, cs, cd44, molecular docking, molecular dynamics simulations, Medicine (General), R5-920
Abstract: Rui Yang,1,* Mudan Lu,2,* Lan Ming,1,* Yu Chen,1 Kai Cheng,1 Jie Zhou,1 Shiwen Jiang,1 Zhenyu Lin,3 Daozhen Chen1 1Research Institute for Reproductive Health and Genetic Diseases, Affiliated Wuxi Maternity and Child Health Care Hospital of Nanjing Medical University, Wuxi 214002, People’s Republic of China; 2Internal Medicine, Affiliated Wuxi Maternity and Child Health Care Hospital of Nanjing Medical University, Wuxi 214002, People’s Republic of China; 3Ministry of Education Key Laboratory for Analytical Science of Food Safety and Biology, Fujian Provincial Key Laboratory of Analysis and Detection for Food Safety, College of Chemistry, Fuzhou University, Fuzhou 350116, People’s Republic of China*These authors contributed equally to this workCorrespondence: Daozhen ChenResearch Institute for Reproductive Health and Genetic Diseases, Affiliated Wuxi Maternity and Child Health Care Hospital of Nanjing Medical University, Wuxi 214002, People’s Republic of ChinaTel +86-13584189188Fax +86-510-82725094Email chendaozhen@163.comPurpose: Therapy for triple-negative breast cancer (TNBC) is a global problem due to lack of specific targets for treatment selection. Cancer stem cells (CSCs) are responsible for tumor formation and recurrence but also offer a promising target for TNBC-targeted therapy. Here, zirconium-89 (89Zr)-labelled multifunctional liposomes (MLPs) surface-decorated with chitosan (CS) were fabricated to specifically target and trace cluster of differentiation 44+ (CD44+) TNBC CSCs specifically.Patients and Methods: The biological basis of CS targeting CD44 for cancer therapy was investigated by detecting the expression of CD44 in TNBC CSCs and TNBC tissues. Molecular docking and dynamics simulations were performed to investigate the molecular basis of CS targeting CD44 for cancer therapy. Gambogic acid (GA)-loaded, 89Zr@CS-MLPs (89Zr-CS-GA-MLPs) were prepared, and their uptake and biodistribution were observed. The anti-tumor efficacy of 89Zr@CS-GA-MLPs was investigated in vivo.Results: CD44 is overexpressed in TNBC CSCs and tissues. Molecular docking and dynamics simulations showed that CS could be stably docked into the active site of CD44 in a reasonable conformation. Furthermore, 89Zr@CS-GA-MLPs were able to bind specifically to CD44+ TNBC stem-like cells and accumulated in tumors of xenograft-bearing mice with excellent radiochemical stability. 89Zr@CS-GA-MLPs loaded with GA showed remarkable anti-tumor efficacy in vivo.Conclusion: The GA-loaded, 89Zr-labelled, CS-decorated MLPs developed in this study represent a novel strategy for TNBC imaging and therapy.Keywords: radionuclide, PET, CS, CD44, molecular docking, molecular dynamics simulation
Published: 2020

142. Analysis of the Risk Factors for Nosocomial Bacterial Infection in Patients with COVID-19 in a Tertiary Hospital

Author: Cheng K, He M, Shu Q, Wu M, Chen C, and Xue Y
Subjects: covid-19, nosocomial bacterial infection, risk factor, Public aspects of medicine, RA1-1270
Abstract: Keping Cheng,1 Miao He,2 Qin Shu,3 Ming Wu,3 Cuifang Chen,2 Yulei Xue4 1Department of Infection Management, Zhongda Hospital Affiliated to Southeast University, Nanjing 210009, People’s Republic of China; 2Department of Public Health, Huangshi Central Hospital, Huangshi 435000, People’s Republic of China; 3Department of Infection Prevention and Control, Huangshi Traditional Chinese Medicine Hospital, Huangshi 435004, Republic of China; 4Department of Infectious Diseases, Jiangsu Provincial Hospital of Traditional Chinese Medicine, Nanjing 210029, People’s Republic of ChinaCorrespondence: Keping ChengZhongda Hospital Affiliated to Southeast University, No. 87 Dingjiaqiao, Nanjing, People’s Republic of ChinaEmail chengkeping@sina.comBackground: Infection surveillance and risk factor analysis are among the most important prerequisites for the prevention and treatment of nosocomial bacteria infections, which are the demands for both infected and non-infected patients.Purpose: To explore the risk factors for nosocomial bacterial infection of patients with COVID-19, and further to provide a theoretical basis for scientific prevention and control of nosocomial bacterial infection.Methods: Between 10 January 2020 and 9 March 2020, we collected data of 212 patients with COVID-19 and then explored the influence of age, gender, length of stay, use of ventilator, urinary catheterization, central venous catheterization, white blood cell (WBC) count and procalcitonin on the nosocomial bacterial infection of patients with COVID-19 by a retrospective study.Results: There were 212 confirmed cases of COVID-19, of which 31 cases had nosocomial bacterial infections, with an incidence of 14.62%. The most common types of nosocomial bacterial infections were lower respiratory tract (12 cases, 38.71%), which was the most frequent site, followed by urinary tract (10 cases, 32.26%), blood stream (7 cases, 22.58%), upper respiratory tract (1 case, 3.23%) and gastrointestinal tract infection (1 case, 3.23%). The incidence of nosocomial bacterial infection was significantly correlated with age, arteriovenous catheterization, urinary catheterization, WBC count and procalcitonin. Moreover, multivariate analysis confirmed that WBC (OR 8.38, 95% CI 1.07 to 65.55), procalcitonin (OR 4.92, 95% CI 1.39 to 17.33) and urinary catheterization (OR 25.38, 95% CI 5.09 to 126.53) were independent risk factors for the nosocomial bacterial infection of patients with COVID-19.Conclusion: Understanding the risk factors for nosocomial bacterial infection of patients with COVID-19 and strengthening the monitoring of various susceptible factors are helpful to control the occurrence of nosocomial bacterial infection in the COVID-19 isolation wards.Keywords: COVID-19, nosocomial bacterial infection, risk factor
Published: 2020

143. P-006: SICKLE RED BLOOD CELL (RBC)-DERIVED EXTRACELLULAR VESICLES ACTIVATE ENDOTHELIAL CELLS AND ENHANCE SICKLE RBC ADHESION MEDIATED BY VON WILLEBRAND FACTOR

Author: AN R., MAN Y., CHENG K., ZHANG T., CHEN C., KUCUKAL E., WULFTANGE W., GOREKE U., BODE A., NAYAK L., VERCELLOTTI G., BELCHER J., LITTLE J., and GURKAN U.
Subjects: Diseases of the blood and blood-forming organs, RC633-647.5
Published: 2022
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144. Effects of Group-delivered Stress-reduction Guided Imagery on Salivary Cortisol, Salivary Amylase, and Stress Mood in Urban, Predominantly Latino Adolescents

Author: Marc J. Weigensberg MD, Cheng K. Fred Wen PhD, Donna Spruijt-Metz PhD, and Christianne Joy Lane PhD
Subjects: Medicine (General), R5-920, Public aspects of medicine, RA1-1270
Abstract: Objectives To determine acute effects of stress-reduction guided imagery delivered in group format on stress biomarkers salivary cortisol and salivary amylase, and on self-reported stress mood, in healthy, predominantly Latino adolescents. Study Design 111 adolescent participants (94% Latino), a subset from a large, randomized controlled lifestyle intervention to improve obesity-related health behaviors, received either 4 weekly lifestyle education sessions (Lifestyle group; LS) or the same weekly lifestyle education sessions plus an additional weekly stress-reduction guided imagery session delivered in group format (Guided imagery group; GI). Salivary cortisol, salivary amylase, and self-reported stress moods were assessed before and after sessions on intervention weeks 3 and 4. Statistics: Linear mixed effects models examined within- and between-session and group differences in pre- to post-session changes. Results Both groups showed decreases in salivary cortisol, 5% decrease in LS group and 32% in GI group (within-group differences all P < .05), with between-group difference in salivary cortisol of moderate size ( P = .05; Cohen’s d = .44). Within the GI group alone, salivary cortisol decrease was similar following either the lifestyle or GI sessions ( P = .64). There were no statistically significant amylase changes within or between groups. All 5 individual stress moods declined by 27% to 46% in the GI group (all P < .05), while only 1 of the 5 declined in LS group. Conclusions Group stress-reduction guided imagery reduces the stress biomarker salivary cortisol, as well as reducing subjective stress mood states, making it a viable modality for large scale stress-reduction interventions.
Published: 2022
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145. P1202 Genome wide association study result for inflammatory bowel disease: A single institute experience in Taiwan

Author: Huang, P J, primary, Sun, T H, additional, Hsu, K C, additional, Wang, C P, additional, Wu, Y H, additional, Chou, J W, additional, and Cheng, K S, additional
Published: 2024
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146. P1163 Incidence and risk of hip replacement rate in patients with inflammatory bowel disease in Taiwan

Author: Lai, H C, primary, Wu, Y H, additional, Wang, C P, additional, Huang, P J, additional, Cheng, K S, additional, and Chou, J W, additional
Published: 2024
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147. P264 The utility of ANCA in Ulcerative Colitis and Crohn’s Disease: A Retrospective Cohort Study in Taiwan

Author: Wu, Y H, primary, Wang, C P, additional, Huang, P J, additional, Lai, H C, additional, Cheng, K S, additional, and Chou, J W, additional
Published: 2024
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148. Cortical bone laminar analysis reveals increased midcortical and periosteal porosity in type 2 diabetic postmenopausal women with history of fragility fractures compared to fracture-free diabetics

Author: Heilmeier, U, Cheng, K, Pasco, C, Parrish, R, Nirody, J, Patsch, JM, Zhang, CA, Joseph, GB, Burghardt, AJ, Schwartz, AV, Link, TM, and Kazakia, G
Subjects: Biomedical and Clinical Sciences, Clinical Sciences, Osteoporosis, Aging, Diabetes, Clinical Research, Aged, Bone Density, Cortical Bone, Diabetes Mellitus, Type 2, Female, Fractures, Bone, Humans, Middle Aged, Porosity, Postmenopause, Radius, Tibia, Tomography, X-Ray Computed, Cortical bone laminar analysis, Cortical pore distribution, Cortical pore number, Cortical porosity, Diabetic bone disease, Type 2 diabetes, Biomedical Engineering, Public Health and Health Services, Endocrinology & Metabolism, Clinical sciences, Epidemiology
Abstract: UnlabelledWe investigated the characteristics and spatial distribution of cortical bone pores in postmenopausal women with type 2 diabetes (T2D). High porosity in the midcortical and periosteal layers in T2D subjects with fragility fractures suggests that these cortical zones might be particularly susceptible to T2D-induced toxicity and may reflect cortical microangiopathy.IntroductionElevated cortical porosity is regarded as one of the main contributors to the high skeletal fragility in T2D. However, to date, it remains unclear if diabetic cortical porosity results from vascular cortical changes or from an expansion in bone marrow space. Here, we used a novel cortical laminar analysis technique to investigate the characteristics and spatial radial distribution of cortical pores in a T2D group with prior history of fragility fractures (DMFx, assigned high-risk group) and a fracture-free T2D group (DM, assigned low-risk group) and to compare their results to non-diabetic controls with (Fx) and without fragility fractures (Co).MethodsEighty postmenopausal women (n = 20/group) underwent high-resolution peripheral quantitative computed tomography (HR-pQCT) of the distal tibia and radius. Cortical bone was divided into three layers of equal width including an endosteal, midcortical, and periosteal layer. Within each layer, total pore area (TPA), total pore number (TPN), and average pore area (APA) were calculated. Statistical analysis employed Mann-Whitney tests and ANOVA with post hoc tests.ResultsCompared to the DM group, DMFx subjects exhibited +90 to +365 % elevated global porosity (p = 0.001). Cortical laminar analysis revealed that this increased porosity was for both skeletal sites confined to the midcortical layer, followed by the periosteal layer (midcortical +1327 % TPA, p ≤ 0.001, periosteal +634 % TPA, p = 0.002), and was associated in both layers and skeletal sites with high TPN (+430 % TPN, p
Published: 2016

149. Investigating the Cutting Mechanics in 2 Dimensional Ultrasonic Vibration Assisted Milling towards Chip Thickness and Chip Formation

Author: Rasidi I., I., primary, Rafai, N. H., additional, Rahim, E. A., additional, Kamaruddin, S. A., additional, Ding, H., additional, and Cheng, K., additional
Published: 2021
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150. Performance of the joint LST-1 and MAGIC observations evaluated with Crab Nebula data

Author: Abe, H., primary, Abe, K., additional, Abe, S., additional, Acciari, V. A., additional, Aguasca-Cabot, A., additional, Agudo, I., additional, Alvarez Crespo, N., additional, Aniello, T., additional, Ansoldi, S., additional, Antonelli, L. A., additional, Aramo, C., additional, Arbet-Engels, A., additional, Arcaro, C., additional, Artero, M., additional, Asano, K., additional, Aubert, P., additional, Baack, D., additional, Babić, A., additional, Baktash, A., additional, Bamba, A., additional, Baquero Larriva, A., additional, Baroncelli, L., additional, Barres de Almeida, U., additional, Barrio, J. A., additional, Batković, I., additional, Baxter, J., additional, Becerra González, J., additional, Bednarek, W., additional, Bernardini, E., additional, Bernardos, M. I., additional, Bernete Medrano, J., additional, Berti, A., additional, Besenrieder, J., additional, Bhattacharjee, P., additional, Biederbeck, N., additional, Bigongiari, C., additional, Biland, A., additional, Bissaldi, E., additional, Blanch, O., additional, Bonnoli, G., additional, Bordas, P., additional, Bošnjak, Ž., additional, Bulgarelli, A., additional, Burelli, I., additional, Burmistrov, L., additional, Buscemi, M., additional, Busetto, G., additional, Campoy Ordaz, A., additional, Cardillo, M., additional, Caroff, S., additional, Carosi, A., additional, Carosi, R., additional, Carrasco, M. S., additional, Carretero-Castrillo, M., additional, Cassol, F., additional, Castro-Tirado, A. J., additional, Cauz, D., additional, Cerasole, D., additional, Ceribella, G., additional, Chai, Y., additional, Cheng, K., additional, Chiavassa, A., additional, Chikawa, M., additional, Chytka, L., additional, Cifuentes, A., additional, Cikota, S., additional, Colombo, E., additional, Contreras, J. L., additional, Cornelia, A., additional, Cortina, J., additional, Costantini, H., additional, Covino, S., additional, D’Amico, G., additional, D’Elia, V., additional, Da Vela, P., additional, Dalchenko, M., additional, Dazzi, F., additional, De Angelis, A., additional, de Bony de Lavergne, M., additional, De Lotto, B., additional, De Lucia, M., additional, de Menezes, R., additional, Del Peral, L., additional, Del Popolo, A., additional, Deleglise, G., additional, Delfino, M., additional, Delgado Mendez, C., additional, Delgado Mengual, J., additional, della Volpe, D., additional, Dellaiera, M., additional, Depaoli, D., additional, Di Piano, A., additional, Di Pierro, F., additional, Di Pilato, A., additional, Di Tria, R., additional, Di Venere, L., additional, Dominik, R. M., additional, Dominis Prester, D., additional, Donini, A., additional, Dorner, D., additional, Doro, M., additional, Díaz, C., additional, Eisenberger, L., additional, Elsässer, D., additional, Emery, G., additional, Escudero, J., additional, Fallah Ramazani, V., additional, Fariña, L., additional, Fattorini, A., additional, Ferrara, G., additional, Ferrarotto, F., additional, Fiasson, A., additional, Foffano, L., additional, Font, L., additional, Freixas Coromina, L., additional, Fröse, S., additional, Fukami, S., additional, Fukazawa, Y., additional, Garcia López, R. J., additional, Garcia, E., additional, Garczarczyk, M., additional, García López, R. J., additional, Gasbarra, C., additional, Gasparrini, D., additional, Gasparyan, S., additional, Gaug, M., additional, Geyer, D., additional, Giesbrecht Paiva, J. G., additional, Giglietto, N., additional, Giordano, F., additional, Gliwny, P., additional, Godinović, N., additional, Grau, R., additional, Green, D., additional, Green, J. G., additional, Gunji, S., additional, Günther, P., additional, Hackfeld, J., additional, Hadasch, D., additional, Hahn, A., additional, Hashiyama, K., additional, Hassan, T., additional, Hayashi, K., additional, Heckmann, L., additional, Heller, M., additional, Herrera Llorente, J., additional, Hirotani, K., additional, Hoffmann, D., additional, Horns, D., additional, Houles, J., additional, Hrabovsky, M., additional, Hrupec, D., additional, Hui, D., additional, Hütten, M., additional, Iarlori, M., additional, Imazawa, R., additional, Inada, T., additional, Inome, Y., additional, Ioka, K., additional, Iori, M., additional, Iotov, R., additional, Ishio, K., additional, Jacquemont, M., additional, Jiménez Martínez, I., additional, Jobst, E., additional, Jormanainen, J., additional, Jurysek, J., additional, Kagaya, M., additional, Karas, V., additional, Katagiri, H., additional, Kataoka, J., additional, Kerszberg, D., additional, Kluge, G. W., additional, Kobayashi, Y., additional, Kohri, K., additional, Kong, A., additional, Kouch, P. M., additional, Kubo, H., additional, Kushida, J., additional, Lainez, M., additional, Lamanna, G., additional, Lamastra, A., additional, Le Flour, T., additional, Leone, F., additional, Lindfors, E., additional, Linhoff, L., additional, Linhoff, M., additional, Lombardi, S., additional, Longo, F., additional, Loporchio, S., additional, Lorini, A., additional, Lozano Bahilo, J., additional, Luque-Escamilla, P. L., additional, Lyard, E., additional, Láinez Lezáun, M., additional, López-Coto, R., additional, López-Moya, M., additional, López-Oramas, A., additional, Machado de Oliveira Fraga, B., additional, Majumdar, P., additional, Makariev, M., additional, Mandat, D., additional, Maneva, G., additional, Manganaro, M., additional, Mangano, S., additional, Mang, N., additional, Manicò, G., additional, Mannheim, K., additional, Mariotti, M., additional, Marquez, P., additional, Marsella, G., additional, Martinez, O., additional, Martínez, G., additional, Martínez, M., additional, Martí, J., additional, Mas-Aguilar, A., additional, Maurin, G., additional, Mazin, D., additional, Menchiari, S., additional, Mender, S., additional, Mestre Guillen, E., additional, Micanovic, S., additional, Miceli, D., additional, Miener, T., additional, Miranda, J. M., additional, Mirzoyan, R., additional, Mizuno, T., additional, Mićanović, S., additional, Molero González, M., additional, Molina, E., additional, Mondal, H. A., additional, Montaruli, T., additional, Monteiro, I., additional, Moralejo, A., additional, Morcuende, D., additional, Morselli, A., additional, Moya, V., additional, Muraishi, H., additional, Murase, K., additional, Nagataki, S., additional, Nakamori, T., additional, Nanci, C., additional, Neronov, A., additional, Neustroev, V., additional, Nickel, L., additional, Nievas Rosillo, M., additional, Nigro, C., additional, Nikolić, L., additional, Nilsson, K., additional, Nishijima, K., additional, Njoh Ekoume, T., additional, Noda, K., additional, Nosek, D., additional, Nozaki, S., additional, Ohishi, M., additional, Ohtani, Y., additional, Oka, T., additional, Okumura, A., additional, Orito, R., additional, Otero-Santos, J., additional, Paiano, S., additional, Palatiello, M., additional, Paneque, D., additional, Pantaleo, F. R., additional, Paoletti, R., additional, Paredes, J. M., additional, Pavletić, L., additional, Pech, M., additional, Pecimotika, M., additional, Peresano, M., additional, Persic, M., additional, Pfeiffle, F., additional, Pietropaolo, E., additional, Pihet, M., additional, Pirola, G., additional, Plard, C., additional, Podobnik, F., additional, Poireau, V., additional, Polo, M., additional, Pons, E., additional, Prada Moroni, P. G., additional, Prandini, E., additional, Prast, J., additional, Principe, G., additional, Priyadarshi, C., additional, Prouza, M., additional, Rando, R., additional, Rhode, W., additional, Ribó, M., additional, Rico, J., additional, Righi, C., additional, Rizi, V., additional, Rodriguez Fernandez, G., additional, Rodríguez Frías, M. D., additional, Sahakyan, N., additional, Saito, T., additional, Sakurai, S., additional, Sanchez, D. A., additional, Satalecka, K., additional, Sato, M., additional, Sato, Y., additional, Saturni, F. G., additional, Savchenko, V., additional, Schleicher, B., additional, Schmidt, K., additional, Schmuckermaier, F., additional, Schubert, J. L., additional, Schussler, F., additional, Schweizer, T., additional, Sciaccaluga, A., additional, Siegert, T., additional, Silvia, R., additional, Sitarek, J., additional, Sliusar, V., additional, Sobczynska, D., additional, Spolon, A., additional, Stamerra, A., additional, Strišković, J., additional, Strom, D., additional, Strzys, M., additional, Suda, Y., additional, Suutarinen, S., additional, Šarić, T., additional, Tajima, H., additional, Takahashi, H., additional, Takahashi, M., additional, Takata, J., additional, Takeishi, R., additional, Tam, P. H. T., additional, Tanaka, S. J., additional, Tateishi, D., additional, Tavecchio, F., additional, Temnikov, P., additional, Terada, Y., additional, Terauchi, K., additional, Terzić, T., additional, Teshima, M., additional, Tluczykont, M., additional, Tokanai, F., additional, Torres, D. F., additional, Tosti, L., additional, Travnicek, P., additional, Truzzi, S., additional, Tutone, A., additional, Ubach, S., additional, Vacula, M., additional, Vallania, P., additional, van Scherpenberg, J., additional, Vazquez Acosta, M., additional, Ventura, S., additional, Verguilov, V., additional, Viale, I., additional, Vigliano, A., additional, Vigorito, C. F., additional, Visentin, E., additional, Vitale, V., additional, Voutsinas, G., additional, Vovk, I., additional, Vuillaume, T., additional, Vázquez Acosta, M., additional, Walter, R., additional, Wei, Z., additional, Will, M., additional, Yamamoto, T., additional, Yamazaki, R., additional, Yoshida, T., additional, Yoshikoshi, T., additional, and Zywucka, N., additional
Published: 2023
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