Informacja

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

English (EN)·Polski (PL)·Yкраїнський (UK)
Przejdź do strony domowej biblioteki Pedagogiczna Biblioteka Wojewódzka im. Komisji Edukacji Narodowej w Lublinie Link otwiera się w nowym oknie Logo biblioteki Prolib Integro - strona głównaPedagogiczna Biblioteka Wojewódzka im. Komisji Edukacji Narodowej w Lublinie
Zmień bibliotekę

Wyszukujesz frazę "Bi, J.-X." wg kryterium: Autor

  Lista filtrów
Wyrównaj
    Wyświetlanie 1-6 z 6
    Tytuł:
    Research on Double Collision Avoidance Mechanism of Ships at Sea
    Autorzy:
    Bi, X.
    Liu, X. J.
    Tematy:
    safety of navigation
    collision avoidance
    collision avoidance mechanism
    close quarter situation
    immediate danger
    mathematical model
    collision risk
    double collision avoidance
    Pokaż więcej
    Wydawca:
    Uniwersytet Morski w Gdyni. Wydział Nawigacyjny
    Powiązania:
    https://bibliotekanauki.pl/articles/117085.pdf  Link otwiera się w nowym oknie
    Opis:
    When power driven vessels encounter at sea, they need to avoid collision. The definition of right vessel may mislead ships officers think his or her direct navigating has absolute power with this special ship. This paper will define DCPA symbols; give the cause and the method of double collision avoidance mechanism of ships at sea.
    Dostawca treści:
    Biblioteka Nauki
    Artykuł
    Tytuł:
    An Early Miocene microtoid cricetid rodent from the Junggar Basin of Xinjiang, China
    Autorzy:
    Maridet, O.
    Wu, W.
    Ye, J.
    Meng, J.
    Bi, S.
    Ni, X.
    Wydawca:
    Polska Akademia Nauk. Instytut Paleobiologii PAN
    Powiązania:
    https://bibliotekanauki.pl/articles/21577.pdf  Link otwiera się w nowym oknie
    Opis:
    Microtoid cricetids are widely considered to be the ancestral form of arvicoline rodents, a successful rodent group includ− ing voles, lemmings and muskrats. The oldest previously known microtoid cricetid is Microtocricetus molassicus from the Late Miocene (MN9, ca. 10–11 Ma) of Europe. Here, we report a new microtoid cricetid, Primoprismus fejfari gen. et sp. nov., from the Junggar Basin of Xinjiang, northwestern China. The rodent assemblage found in association with this specimen indicates a late Early Miocene age, roughly estimated at 18–17 Ma, and thus more than 6 million years older than M. molassicus. While morphological comparisons suggest that the new taxon is most closely related to M. molas− sicus, it differs from the latter in a striking combination of primitive characters, including a lower crown, smaller size, a differentiated posterolophid and hypolophid, a faint anterolophid, the absence of an ectolophid, and the presence of a stylid on the labial border of the tooth. Arid conditions prevailing across the mid−latitude interior of Eurasia during the Early Miocene, enhanced by the combined effects of the Tibetan uplift and the gradual retreat of the Tethys Ocean, likely played a role in the appearance of grasslands, which in turn triggered the evolution of microtoid cricetids and, ultimately, the origin of arvicoline rodents.
    Dostawca treści:
    Biblioteka Nauki
    Artykuł
    Tytuł:
    Generation and characterization of a monoclonal antibody against duck Tembusu virus envelope protein
    Autorzy:
    Han, K.
    Zhao, D.
    Liu, Y.
    Liu, Q.
    Huang, X.
    Yang, J.
    Bi, K.
    Xu, T.
    Li, Y.
    Wydawca:
    Polska Akademia Nauk. Czytelnia Czasopism PAN
    Powiązania:
    https://bibliotekanauki.pl/articles/31495.pdf  Link otwiera się w nowym oknie
    Opis:
    Duck Tembusu virus (DTMUV) is a newly emerging pathogenic flavivirus that has caused massive economic losses to the duck industry in China. Envelope (E) protein of DTMUV is an important structural protein, which is able to induce protective immune response in target animals and can be used as specific serological diagnosis tool. In this study, a novel monoclonal antibody, designated mAb 3E9, was generated against DTMUV E protein. It is positive in indirect ELISA against both His-E protein and the purified whole viral antigen. Also, this mAb showed positive reaction with DTMUV in Western blot and indirect immunofluorescence assay, and the isotype was IgG1. End-point neutralizing assay performed in BHK-21 cells revealed that the neutralization titer of 3E9 against DTMUV JS804 strain reached 1:50. Furthermore, functional studies revealed that 3E9 blocks infection of DTMUV at a step on viral attachment. The anti-E mAbs produced in the present work may be valuable in developing an antigen-capture ELISA test for antigen detection or a competitive ELISA test for antibody detection or therapeutic medicine for DTMUV in poultry.
    Dostawca treści:
    Biblioteka Nauki
    Artykuł
    Tytuł:
    Combined dark matter searches towards dwarf spheroidal galaxies with Fermi-LAT, HAWC, H.E.S.S., MAGIC, and VERITAS
    Autorzy:
    van der Walt, J.
    Giacinti, G.
    Hueyotl-Zahuantitla, F.
    McGrath, C.
    Joshi, V.
    Pueschel, E.
    Ostrowski, Michał
    Le Stum, S.
    Roache, E.
    Hawc
    Huber, D.
    Fegan, S.
    Reville, B.
    Berley, D.
    Senniappan, M.
    Ribeiro, D.
    Mares, A.
    Tollefson, K.
    Reynolds, P.
    Schutte, H.
    Cotzomi, J.
    Davids, H.
    Baghmanyan, V.
    Noel, Angel
    Moore, C.
    Holler, M.
    Kieda, D.
    Taylor, A.
    Lemoine-Goumard, M.
    Garfias, F.
    DuVernois, M.
    Smith, A. J.
    Herzog, I.
    Rudak, B.
    Nellen, L.
    Nisa, M. U.
    Feng, Q.
    Salesa Greus, F.
    Thiersen, H.
    Cotter, G.
    Naurois (de), M.
    O'Brien, P.
    Brun, F.
    Werner, F.
    Martinez Castellanos, I.
    Frans, L.
    Kleiner, T.
    Barbosa Martins, V.
    Springer, W. R.
    Barnard, M.
    Foote, G.
    Aharonian, F.
    Moriarty, P.
    Gallant, Y.
    Terrier, R.
    Tsuji, N.
    Steenkamp, R.
    Moderski, R.
    Hüntemeyer, P.
    Giuri, C.
    Thorpe-Morgan, C.
    Zacharias, M.
    Alfaro, R.
    Nayerhoda, A.
    Wood, J.
    Peron, G.
    Harding, J. P.
    Schaefer, J.
    Fuessling, M.
    Surajbali, P.
    Buckley, J.
    Archer, A.
    Turner, R.
    Kostunin, D.
    Lypova, I.
    Sailer, S.
    Steinmassl, S.
    Goodman, J. A.
    Chromey, A.
    Diaz Hernandez, R.
    Kasai, E.
    Catalano, J.
    Espinoza Hernández, M. C.
    Arteaga Velazquez, J. C.
    Khangulyan, D.
    Morales Soto, J. A.
    Salzmann, H.
    Alvarez, C.
    Murach, T.
    Benbow, W.
    Newbold, M.
    Rosa-Gonzalez, D.
    Moreno Barbosa, E.
    Garcia Aguilar, D.
    Pérez Pérez, E. G.
    Kertzman, M.
    Majumdar, J.
    Katarzynski, K.
    Curlo, M.
    Gueta, O.
    Matthews, J.
    Torres Escobedo, R.
    Rowell, G.
    Mostafa, M.
    Marx, R.
    Vargas, H. Leon
    Villaseñor, L.
    Meyer, M.
    Damascene Mbarubucyeye, J.
    Weinstein, A.
    Leuschner, F.
    Tavernier, T.
    Zmija, A.
    Mackey, J.
    Williamson, T.
    Holder, J.
    Anguener, O.
    Reichherzer, P.
    Patel, S.
    Schoorlemmer, H.
    Lennarz, D.
    Malone, K.
    Poireau, V.
    Caroff, S.
    Avila Rojas, D. O.
    Tsirou, M.
    Takahashi, T.
    Batzofin, R.
    Engel, K.
    Brill, A.
    Santangelo, A.
    Mukherjee, R.
    Jankowsky, F.
    Belmont-Moreno, E.
    Camacho, J. R. Angeles
    Davids, I. D.
    Chambery, P.
    Lenain, J. P.
    Einecke, S.
    Ayala Solares, H. A.
    Fan, J.
    Devin, J.
    Panny, S.
    Wagner, S.
    Steppa, C.
    Ashkar, H.
    Kaaret, P.
    Haupt, M.
    van Rensburg, C.
    Yodh, G.
    Armstrong, T.
    Glawion, D.
    Lee, W. H.
    Kukec Mezek, G.
    Lundy, M.
    Shiningayamwe, K.
    Simoni, R.
    Fang, K.
    Grondin, M. H.
    Remy, Q.
    Linnemann, J.
    Zouari, S.
    Brisbois, C.
    Rho, C. D.
    Veritas
    Huang, Z.
    Bernloehr, K.
    Noriega-Papaqui, R.
    Gabici, S.
    Taboada, I.
    Marcowith, A.
    Bony (de), M.
    Lara, A.
    Schwanke, U.
    Otte, A.
    Gent, A. E.
    Ait-Benkhali, F.
    Seyffert, A.
    Lemiere, A.
    Quinn, J.
    Punch, M.
    Goksu, H.
    Nievas-Rosillo, M.
    Mohrmann, L.
    Oberholzer, L. L.
    Sun, L.
    Huang, D.
    Puehlhofer, G.
    Marti'i-Devesa, G.
    Schneider, M.
    Christiansen, J.
    Hoischen, C.
    Chaparro-Amaro, O.
    Dreyer, L.
    Zanin, R.
    Salazar, H. I.
    Hanna, D.
    Kundu, A.
    Glicenstein, J. F.
    Żywucka, N.
    Yusafzai, A.
    Durocher, M.
    Nakashima, K.
    Jamrozy, Marek
    Adams, C.
    Falcone, A.
    Tomankova, L.
    Capistrán Rojas, T.
    Humensky, T. B.
    Pita, S.
    Vasileiadis, G.
    Sembroski, G.
    Hinton, J.
    Luis-Raya, G.
    White, R.
    Lee, J.
    Carramiñana, A.
    Giunti, L.
    Wang, X.
    Mitchell, A.
    Reimer, A.
    Miranda-Romagnoli, P.
    Zhou, H.
    Giavitto, G.
    McEnery, J.
    de la Fuente, E.
    Ernenwein, J. P.
    Serna-Franco, J.
    Reimer, O.
    Ryan, J.
    Funk, S.
    Flores, J. L.
    Caballero Mora, K. S.
    Jhee, H.
    Sahakian, V.
    Kunwar, S.
    Egberts, K.
    Pohl, M.
    Yassin, H.
    Lamanna, G.
    Feijen, K.
    Gillanders, G.
    Kunde, G. J.
    Rueda Ricarte, H.
    Jin, W.
    BenZvi, S.
    Sanchez, D.
    Konno, R.
    van Soelen, B.
    Tuffs, R.
    Barber, A. S.
    Patel, S. R.
    Davies, J.
    Boisson, C.
    Pfrang, K.
    González, M. M.
    Doroshenko, V.
    O'Brien, S.
    Kreter, M.
    Katz, U.
    Díaz Vélez, J. C.
    Dmytriiev, A.
    Rieger, F.
    Dingus, B.
    Wierzcholska, Alicja
    Coutiño de Leon, S.
    Ona-Wilhelmi (de), E.
    Sandoval, A.
    Sasaki, M.
    Willox, E.
    Maier, G.
    Niemiec, J.
    Backes, M.
    Berge, D.
    Cotti, U.
    Fleischhack, H.
    Watson, I. J.
    Kluzniak, W.
    Fortson, L.
    Chen, A.
    Becherini, Y.
    Stegmann, C.
    Tak, D.
    Marandon, V.
    Tluczykont, M.
    Fichet de Clairfontaine, G.
    Vassiliev, V.
    Ragan, K.
    Djannati-Ataï, A.
    Moulin, E.
    Prokoph, H.
    Pérez Araujo, Y.
    Ohm, S.
    Martinez, O.
    Santander, M.
    Chand, T. B.
    Uchiyama, Y.
    Watson, J. J.
    Marchegiani, P.
    Barnacka, Anna
    López-Coto, R.
    Meintjes, P.
    Sinnis, G.
    Quirrenbach, A.
    Kumar, S.
    Weisgarber, T.
    Klepser, S.
    Levy, C.
    Montanari, A.
    Shang, R. Y.
    Völk, H. J.
    Nieto, D.
    Lang, M.
    Torres, I.
    Abeysekara, A. U.
    Fick, B.
    Böttcher, M.
    Duffy, C.
    Hörbe, M.
    Wong, Y. W.
    Hernández Cadena, S.
    Renaud, M.
    Muller, J.
    Dalgleish, H.
    Ellsworth, R.
    Zdziarski, A.
    Peisker, A.
    Morris, P.
    Jung, I.
    Tanner, M.
    García-Torales, G.
    Bulik, T.
    Álvarez Romero, J. d. D.
    Horns, D.
    Casanova, S.
    Brose, R.
    Hofmann, W.
    Tanaka, T.
    Martínez Huerta, H.
    Schüssler, F.
    Ruiz-Velasco, E.
    Prokhorov, D.
    Vincent, P.
    Becerra González, J.
    Hui, M.
    Kosack, K.
    Romoli, C.
    Longinotti, A. L.
    Shapopi, J. N. S.
    Luashvili, A.
    Omodei, N.
    de León, C. L.
    Sadeh, I.
    Specovius, A.
    Spir-Jacob, M.
    Ruiz Velasco, E.
    Williams, D.
    Spencer, S. T.
    Cangemi, F.
    Martínez-Castro, J.
    Hervet, O.
    Jardin-Blicq, A.
    Stawarz, Łukasz
    Zargaryan, D.
    Farrell, K.
    Bolmont, J.
    Sinha, A.
    Lohse, T.
    Ong, R.
    Furniss, A.
    Venter, C.
    Khelifi, B.
    Zhu, S.
    Malyshev, D.
    Spackman, H.
    Breuhaus, M.
    Albert, A.
    Diaz, L.
    Zepeda, A.
    Komin, N.
    Veh, J.
    Abdalla, H.
    Holch, T.
    Iriarte, A.
    Fiasson, A.
    Kollamparambil, A. B.
    García-Luna, J. L.
    Vink, J.
    Capasso, M.
    van Eldik, C.
    Fraija, N. I.
    Parsons, D.
    Hona, B.
    Olivera-Nieto, L.
    Bylund, T.
    Zech, A.
    Hattingh, S.
    Fernandez Alonso, M.
    Arcaro, C.
    Rivière, C.
    Bi, B.
    Du Plessis, L.
    Ureña-Mena, F.
    Armand, C.
    Donath, A.
    Babu, R.
    Garcia-Gonzalez, J. A.
    Maurin, G.
    Fontaine, G.
    Hermann, G.
    Humensky, B.
    Prado, R.
    Errando, M.
    Sol, H.
    Lundeen, J.
    Panter, M.
    Opis:
    Cosmological and astrophysical observations suggest that 85% of the total matter of the Universe is made of Dark Matter (DM). However, its nature remains one of the most challenging and fundamental open questions of particle physics. Assuming particle DM, this exotic form of matter cannot consist of Standard Model (SM) particles. Many models have been developed to attempt unraveling the nature of DM such as Weakly Interacting Massive Particles (WIMPs), the most favored particle candidates. WIMP annihilations and decay could produce SM particles which in turn hadronize and decay to give SM secondaries such as high energy 𝛾 rays. In the framework of indirect DM search, observations of promising targets are used to search for signatures of DM annihilation. Among these, the dwarf spheroidal galaxies (dSphs) are commonly favored owing to their expected high DM content and negligible astrophysical background. In this work, we present the very first combination of 20 dSph observations, performed by the Fermi-LAT, HAWC, H.E.S.S., MAGIC, and VERITAS collaborations in order to maximize the sensitivity of DM searches and improve the current results. We use a joint maximum likelihood approach combining each experiment’s individual analysis to derive more constraining upper limits on the WIMP DM self-annihilation cross-section as a function of DM particle mass. We present new DM constraints over the widest mass range ever reported, extending from 5 GeV to 100 TeV thanks to the combination of these five different 𝛾-ray instruments.
    Dostawca treści:
    Repozytorium Uniwersytetu Jagiellońskiego
    Inne
      Wyświetlanie 1-6 z 6

      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