Informacja

Drogi użytkowniku, aplikacja do prawidłowego działania wymaga obsługi JavaScript. Proszę włącz obsługę JavaScript w Twojej przeglądarce.

Wyszukujesz frazę "Sengupta, A. K." wg kryterium: Autor


Wyświetlanie 1-3 z 3
Tytuł:
Evaluation of Low Back Pain Risks in a Beef Skinning Operation
Autorzy:
Das, B.
Sengupta, A. K.
Tematy:
low back pain
biomechanical analysis
ergonomic analysis
posture analysis
meat processing
ból pleców
analiza biomechaniczna
analiza ergonomiczna
postawa
Pokaż więcej
Wydawca:
Centralny Instytut Ochrony Pracy
Powiązania:
https://bibliotekanauki.pl/articles/89837.pdf  Link otwiera się w nowym oknie
Opis:
The low back pain risks in a beef skinning operation at a high stand kill floor workstation was evaluated. The increases in compressive forces at lower back (L5/S1) between normal slump (back angle 25°, measured in the sagittal plane) and severe (45°) and between normal slump and very severe (70°) bent back postures were 387 N or 28% and 616 N or 45%, respectively. The high spine load coupled with high level of repetition can have a high probability of fatigue failure in the spine structural members. Non-neutral back posture for a large portion of the total work time can be a low back pain risk factor. The videotape analysis showed that the times involved during the task performance for the bent back (more than 25°) and severe bent back (more than 45°) were 48.4 and 33.5% of the total cycle time, respectively. The upper limit from OWAS (Ovako Working Posture Analysis System) for bent back posture is 30% of the total cycle time. The bent and twisted back posture (both more than 25°) time was 10.4% compared to OWAS limit of 5%. This indicated that actions are needed in the near future to alleviate the risk of low back pain. Ergonomics redesign of the workstation was recommended for the operation.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Validation of the Polish version of the Anderson and Dedrick Trust in Physician scale
Autorzy:
Krajewska-Kułak, E.
Kułak, W.
Łukaszuk, C.
Lewko, J.
Sengupta, P.
Cybulski, M.
Guzowski, A.
Kowalczuk, K.
Jankowiak, B.
Kowalewska, B.
Kondzior, D.
Rolka, H.
Baranowska, A.
Lankau, A.
Klimaszewska, K.
Sierakowska, M.
Krajewska-Ferishah, K.
Szyszko-Perłowska, A.
Tematy:
Trust in Physician Scale
validation
Polish version
Pokaż więcej
Wydawca:
Uniwersytet Medyczny w Białymstoku
Powiązania:
https://bibliotekanauki.pl/articles/1918629.pdf  Link otwiera się w nowym oknie
Opis:
Purpose: The aim of this study was to validate the Trust in Physician Scale (TPS) for Polish patients. Materials and Methods: The validation of a Polish-language version of Anderson and Dedrick’s TPS was performed with a group of 849 patients. Validation consisted of the translation and evaluation of the psychometric properties of the Polish TPS and its application among Polish-speaking patients. We also explored the TPS with the patient’s sex, age, education, income, marital status, and number of physician visits. Results: The internal consistency of the Polish TPS was high (Cronbach’s alpha = .891). In our study, the TPS is positively associated with age, education, income, marital status, and number of physician visits. Also, we have found that the TPS is negatively associated with sex and place of residence. Conclusions: The Polish-language scale fulfills all the criteria of psychometric and functional validation with the original version of the Trust in Physician Scale.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory
Autorzy:
Pandey, A.
Cristofari, P.
Siejkowski, H.
Karas, V.
Cicciari, G. M.
Saturni, F. G.
Jarnot, C.
Chadwick, P. M.
Kubo, H.
Roache, E.
Meyer, D. M.-A.
Burmistrov, L.
Nosek, D.
Simongini, A.
Lindfors, E.
Escarate, P.
Komin, N.
de Gouveia Dal Pino, E. M.
Gallozzi, S.
Leone, F.
Hadasch, D.
Yao, Y.
Zhang, W.
Mereghetti, S.
Pech, M.
Bottacini, E.
Kluźniak, W.
Hara, S.
Okumura, A.
Laadim, F. De Frondat
García-Lago, F. Frías
Biland, A.
Galanti, G.
Ponti, G.
Abhishek, A.
Green, D.
Silvestri, G.
Takahashi, M.
Zech, A.
Stamerra, A.
Živec, M.
Zavrtanik, M.
Paredes, J. M.
Vigorito, C F.
Lombardi, S.
Nieto, D.
Nishijima, K.
Stuani, L. Augusto
Romano, P.
Sáez, J. Buces
Bosnjak, Z.
Gradetzke, T.
Rando, R.
Ferrarotto, F.
Sano, H.
Brose, R.
Doro, M.
Zamanillo, V. Moya
Chiavassa, A.
Balazs, C.
Chen, Y.
Bringmann, T.
Sánchez-Conde, M.
Spinello, S.
Antonelli, L. A.
Giordano, F.
Vandenbroucke, J.
Gianotti, F.
Rodríguez-Fernández, G.
Tanaka, S. J.
Berge, D.
Vacula, M.
Goldoni, P.
Ricci, C.
Miener, T.
Bahilo, J. Lozano
Aguasca-Cabot, A.
Batista, P. I.
Caraveo, P.
Barrio, J. A.
Contreras, J. L.
Burton, M.
Cotter, G.
Fedorova, E.
Prouza, M.
Voutsinas, G.
Berti, A.
Mackey, J.
Calisse, P. G.
Germani, S.
Cascone, E.
Cerasole, D.
Kowal, G.
Lamastra, A.
Rowell, G.
Travnicek, P.
Kushida, J.
Hussain, S.
Vercellone, S.
Romeo, G.
Dazzi, F.
Amans, J.-P.
Del Burgo, R.
Paoletti, R.
Tejedor, L. A.
Larriva, A. Baquero
Torres, D. F.
Blanch, O.
Djuvsland, J.
Testa, V.
Linhoff, M.
Chernyakova, M.
Eckner, C.
Chon, G.
Xotta, F.
Pantaleo, F. R.
Leonora, E.
Majumdar, P.
Otero-Santos, J.
Orito, R.
Falceta-Goncalves, D.
Gaug, M.
Castro-Tirado, A. J.
Alfaro, R.
Kaufmann, S.
Cerruti, M.
Hnatyk, R.
Beck, G.
Mello, A. J. T. S.
Jaroschewski, I.
Martínez, I. Jiménez
Pirola, G.
Paiva, J. G. Giesbrecht Formiga
Ducci, L.
Pintore, F.
Sergijenko, O.
Tothill, N.
Kerszberg, D.
Beshley, V.
Persic, M.
Sapienza, V.
Ruina, A.
Depaoli, D.
Gasbarra, C.
Viaux, N.
Tutone, A.
Glicenstein, J.-F.
Malyshev, D.
Pumo, M. L.
Furniss, A.
Elsässer, D.
Parmiggiani, N.
Sangiorgi, P.
Stanič, S.
Esposito, P.
Fukui, Y.
Castignani, G.
Yamazaki, R.
Kazanas, D.
Mariotti, M.
Bonollo, A.
Kataoka, J.
Girolamo, T. Di
Wierzcholska, A.
Principe, G.
Batzofin, R.
Fiasson, A.
Longo, F.
Aguirre-Santaella, A.
Ramos, A. Moreno
Murach, T.
Emery, G.
Schiavone, F.
Novotny, V.
de Leon, A. Rosales
Gasparrini, D.
de Souza, V.
Dwarkadas, V. V.
Martínez, M.
Fukazawa, Y.
Acero, F.
Verna, G.
Reis, I.
Zuriaga-Puig, J.
Lacave, B.
Viana, A.
Morselli, A.
Podobnik, F.
Pagliaro, A.
de Lavergne, M. de Bony
Recchia, S.
Barrios-Jiménez, L.
Cornejo, B.
Coelho, J. Goulart
Hoffmann, D.
Mitchell, A.
Salzmann, H.
Pfeifle, F.
Rodríguez-Vázquez, J. J.
Fegan, S.
Gammaldi, V.
Hofmann, W.
Olive, J.-F.
Hassan, T.
D’Amico, G.
Piano, A. Di
Keita, T.
Savchenko, V.
Perrotta, F.
Pecimotika, M.
López-Moya, M.
Mazin, D.
Molfese, C.
Carosi, R.
Gallego, J. Méndez
Panebianco, G.
Takeishi, R.
Volpe, D. della
Fiandrini, E.
Torradeflot, F.
Kieda, D. B.
Neto, J. P.
Galaz, G.
López-Coto, R.
Hanlon, W.
Oya, I.
Incardona, F.
Janecek, P.
Martínez, G. A.
Dinesh, A.
Siqueira, C.
Montaruli, T.
Arcaro, C.
Grolleron, G.
Queiroz, F. S.
Luciani, H.
Heckmann, L.
Caroff, S.
Inada, T.
Lazarević, S.
Sol, H.
Acosta, M. Vázquez
Kornecki, P.
Tibaldo, L.
Hayashi, K.
Garczarczyk, M.
Heller, M.
Orlando, E.
Capasso, G.
Hrupec, D.
Tonev, D.
Starecki, T.
Brunelli, G.
Carquin, E.
Vassiliev, V.
Blazek, J.
Palatiello, M.
De Angelis, A.
Horvath, P.
Moralejo, A.
Yoshikoshi, T.
Batković, I.
Fontaine, G.
Alfaro, J.
Rhode, W.
Costantini, H.
Gréaux, L.
de Naurois, M.
Lenain, J.-P.
Pinchbeck, L.
Orlando, S.
Moulin, E.
Sarkar, S.
Marsella, G.
Inoue, Y.
Miranda, J. M.
Abe, S.
Bunse, M.
Barbera, A. La
Aguilera, A. Pérez
Böttcher, M.
Ong, R. A.
Rizi, V.
Meyer, M.
Pierro, F. Di
Amato, E.
Miceli, M.
Inoue, S.
Cortina, J.
Pohl, M.
Prandini, E.
Macias, O.
Nemmen, R.
Truzzi, S.
Orlandini, M.
Molina, E.
Abhir, J.
Pietropaolo, E.
Roy, A.
White, M.
del Peral, L.
Tjus, J. Becker
Lyard, E.
Sadeh, I.
Menon, S.
Curtis-Ginsberg, Z.
Donini, A.
Ambrosino, D.
Kolar, D.
Márquez, I.
Cifuentes, A.
Green, J. G.
Diebold, S.
Niemiec, J.
Bonnoli, G.
González, C. Pozo
Tian, W. W.
Vorobiov, S.
Granot, J.
Peresano, M.
Feng, Q.
Chai, Y.
De Palma, G.
Sofia, I.
Delgado, C.
Duangchan, C.
Paneque, D.
Jahanvi, -
Saha, L.
Tramacere, A.
Acharyya, A.
Hnatyk, B.
Stolarczyk, T.
Reimer, O.
Voitsekhovskyi, V.
Guedes, L. M. V.
Mandat, D.
Bigongiari, C.
Pollet, V.
Dörner, J.
Vecchi, M.
Visentin, E.
Ríos, C.
Nikołajuk, M.
Quirrenbach, A.
Schipani, P.
Foffano, L.
Domínguez, D. Martín
Backes, M.
Miceli, D.
Conforti, V.
Soto, S. García
Marchetti, A.
Campoy-Ordaz, A.
Fioretti, V.
Araujo, C. H. Coimbra
Giglietto, N.
Muraishi, H.
Cuevas, O.
D’Ammando, F.
Walter, R.
Richtler, T.
Martinez, O.
Teshima, M.
Sengupta, D.
Agudo, I.
Batista, R. Alves
Capuzzo-Dolcetta, R.
Rosillo, M. Nievas
Balbo, M.
Tingay, S. J.
Loporchio, S.
Ruiz-Velasco, E.
Ambrosino, F.
Molero, M.
Bernardini, E.
Bissaldi, E.
Ebr, J.
Noda, K.
Zhdanov, V. I.
Reimer, A.
Vigliano, A.
Adam, R.
Egberts, K.
Wechakama, M.
Ferrand, G.
Bronzini, E.
Tajima, H.
Manicò, G.
González, J. M.
Alispach, C.
Asano, K.
Chudoba, J.
del Valle, M. V.
Tibolla, O.
Viale, I.
Glombitza, J.
Munari, K.
Nakamori, T.
Rico, J.
Hiroshima, N.
Frías, M. D. Rodríguez
Savarese, S.
Jean, P.
Petruk, O.
Reisenegger, A.
Pittori, C.
Giuffrida, R.
Cantlay, B. K.
Kohri, K.
Jamrozy, Marek
Iocco, F.
Pueschel, E.
Michailidis, M.
Ambrosi, G.
Iarlori, M.
Jin, W.
Ventura, S.
Moghadam, M. Ozlati
Iuliano, A.
Harvey, V. M.
Carrasco, M.-S.
Sguera, V.
Ghalumyan, A.
Heß, B.
Regeard, M.
Ascasibar, Y.
Tria, R. Di
Scherer, A.
Pérez-Romero, J.
van Eldik, C.
Bhattacharyya, S.
Rainò, S.
Jurysek, J.
Cortínez, A. Cerviño
De Lotto, B.
Nozaki, S.
Peron, G.
Luque-Escamilla, P. L.
Lapington, J.
Mangano, S.
Schussler, F.
Ribó, M.
Benbow, W.
Li, Y.
Delicado, M. Molina
Wohlleben, F.
Santos-Lima, R.
Kissmann, R.
Láinez, M.
Riitano, L.
Trois, A.
Rudak, B.
David, L.
Zavrtanik, D.
Starling, R.
Hamal, P.
Filipovic, M.
Costa, A.
Palombara, N. La
Gueta, O.
Sliusar, V.
González, J. Becerra
Abe, K.
Godoy, M. Escobar
Venere, L. Di
Aramo, C.
Martins, V. Barbosa
Kalekin, O.
Bernete, J.
Spiga, D.
Bhattacharjee, P.
Patricelli, B.
Chen, A. W.
Pühlhofer, G.
Nieves, C. Escañuela
Colapietro, M.
Vitale, V.
Vignatti, J.
López-Oramas, A.
Ettori, S.
Jankowsky, F.
Bartolini, C.
Horan, D.
Chaty, S.
Muraczewski, A.
Suda, Y.
Rieger, F.
Angel, L.
Tombesi, F.
Bertucci, B.
Caproni, A.
Poireau, V.
Rosado, J.
Opis:
The dwarf spheroidal galaxies (dSphs) orbiting the Milky Way are widely regarded as systems supported by velocity dispersion against self-gravity, and as prime targets for the search for indirect dark matter (DM) signatures in the GeV-to-TeV $\gamma$-ray range owing to their lack of astrophysical $\gamma$-ray background. We present forecasts of the sensitivity of the forthcoming Cherenkov Telescope Array Observatory (CTAO) to annihilating or decaying DM signals in these targets. An original selection of candidates is performed from the current catalogue of known objects, including both classical and ultrafaint dSphs. For each, the expected DM content is derived using the most comprehensive photometric and spectroscopic data available, within a consistent framework of analysis. This approach enables the derivation of novel astrophysical factor profiles for indirect DM searches, which are compared with results from the literature. From an initial sample of 64 dSphs, eight promising targets are identified – Draco I, Coma Berenices, Ursa Major II, Ursa Minor, and Willman 1 in the North, Reticulum II, Sculptor, and Sagittarius II in the South – for which different DM density models yield consistent expectations, leading to robust predictions. CTAO is expected to provide the strongest limits above ∼ 10 TeV, reaching velocity-averaged annihilation cross sections of $\sim 5 \times 10^{-25} cm^{3} s^{-1}$ and decay lifetimes up to $\sim 10^{26}$ s for combined limits. The dominant uncertainties arise from the imprecise determination of the DM content, particularly for ultrafaint dSphs. Observation strategies are proposed that optimize either deep exposures of the best candidates or diversified target selections.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
    Wyświetlanie 1-3 z 3

    Ta witryna wykorzystuje pliki cookies do przechowywania informacji na Twoim komputerze. Pliki cookies stosujemy w celu świadczenia usług na najwyższym poziomie, w tym w sposób dostosowany do indywidualnych potrzeb. Korzystanie z witryny bez zmiany ustawień dotyczących cookies oznacza, że będą one zamieszczane w Twoim komputerze. W każdym momencie możesz dokonać zmiany ustawień dotyczących cookies