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  • 1
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    In:  Bull. Seism. Soc. Am., Tokyo, Conseil de l'Europe, vol. 63, no. 12, pp. 2091-2104, pp. L01306, (ISSN: 1340-4202)
    Publication Date: 1973
    Keywords: Seismology ; Corner frequency ; Body waves ; Source ; Source parameters ; SModelling ; BSSA
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  • 2
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    Kluwer
    In:  Dordrecht, xvii+329 pp., Kluwer, vol. 271, no. ALEX(01)-FR-77-01, AFTAC Contract F08606-76-C-0025, pp. 329, (ISBN: 0-08-043649-8)
    Publication Date: 1993
    Keywords: Earthquake hazard ; Earthquake risk ; Turkey ; Earthquake engineering, engineering seismology ; Armenia ; Japan ; Vancouver ; Lisbon ; Patras ; Quito
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  • 3
    Publication Date: 2015-05-23
    Description: Type Ia supernovae are thought to be the result of a thermonuclear runaway in carbon/oxygen white dwarfs, but it is uncertain whether the explosion is triggered by accretion from a non-degenerate companion star or by a merger with another white dwarf. Observations of a supernova immediately following the explosion provide unique information on the distribution of ejected material and the progenitor system. Models predict that the interaction of supernova ejecta with a companion star or circumstellar debris lead to a sudden brightening lasting from hours to days. Here we present data for three supernovae that are likely to be type Ia observed during the Kepler mission with a time resolution of 30 minutes. We find no signatures of the supernova ejecta interacting with nearby companions. The lack of observable interaction signatures is consistent with the idea that these three supernovae resulted from the merger of binary white dwarfs or other compact stars such as helium stars.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Olling, Rob P -- Mushotzky, Richard -- Shaya, Edward J -- Rest, Armin -- Garnavich, Peter M -- Tucker, Brad E -- Kasen, Daniel -- Margheim, Steve -- Filippenko, Alexei V -- England -- Nature. 2015 May 21;521(7552):332-5. doi: 10.1038/nature14455.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Astronomy Department, University of Maryland, College Park, Maryland 20742-2421, USA. ; Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA. ; Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA. ; 1] Mt Stromlo Observatory, The Australian National University, via Cotter Road, Weston Creek, Australian Capital Territory 2611, Australia [2] Department of Astronomy, University of California, Berkeley, California 94720-3411, USA. ; 1] Department of Astronomy, University of California, Berkeley, California 94720-3411, USA [2] Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720, USA. ; Gemini Observatory, Southern Operations Center, c/o AURA, Casilla 603, La Serena, Chile. ; Department of Astronomy, University of California, Berkeley, California 94720-3411, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25993963" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 4
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2013-09-07
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Tucker, Brian E -- New York, N.Y. -- Science. 2013 Sep 6;341(6150):1070-2. doi: 10.1126/science.1239236.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉GeoHazards International, 687 Bay Road, Menlo Park, CA 94025, USA. tucker@geohaz.org〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/24009380" target="_blank"〉PubMed〈/a〉
    Keywords: Asia, Central ; Caribbean Region ; Chile ; Disaster Planning/*methods ; Earthquakes/*statistics & numerical data ; Humans ; Public Health ; Risk ; Safety Management/*methods ; Tokyo ; Turkey
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 5
    Publication Date: 2015-03-07
    Description: In 1964, Refsdal hypothesized that a supernova whose light traversed multiple paths around a strong gravitational lens could be used to measure the rate of cosmic expansion. We report the discovery of such a system. In Hubble Space Telescope imaging, we have found four images of a single supernova forming an Einstein cross configuration around a redshift z = 0.54 elliptical galaxy in the MACS J1149.6+2223 cluster. The cluster's gravitational potential also creates multiple images of the z = 1.49 spiral supernova host galaxy, and a future appearance of the supernova elsewhere in the cluster field is expected. The magnifications and staggered arrivals of the supernova images probe the cosmic expansion rate, as well as the distribution of matter in the galaxy and cluster lenses.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Kelly, Patrick L -- Rodney, Steven A -- Treu, Tommaso -- Foley, Ryan J -- Brammer, Gabriel -- Schmidt, Kasper B -- Zitrin, Adi -- Sonnenfeld, Alessandro -- Strolger, Louis-Gregory -- Graur, Or -- Filippenko, Alexei V -- Jha, Saurabh W -- Riess, Adam G -- Bradac, Marusa -- Weiner, Benjamin J -- Scolnic, Daniel -- Malkan, Matthew A -- von der Linden, Anja -- Trenti, Michele -- Hjorth, Jens -- Gavazzi, Raphael -- Fontana, Adriano -- Merten, Julian C -- McCully, Curtis -- Jones, Tucker -- Postman, Marc -- Dressler, Alan -- Patel, Brandon -- Cenko, S Bradley -- Graham, Melissa L -- Tucker, Bradley E -- New York, N.Y. -- Science. 2015 Mar 6;347(6226):1123-6. doi: 10.1126/science.aaa3350.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA. pkelly@astro.berkeley.edu. ; Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218, USA. ; Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA. ; University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801, USA. Department of Physics, University of Illinois at Urbana-Champaign, 1110 West Green Street, Urbana, IL 61801, USA. ; Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA. ; Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA. Western Kentucky University, 1906 College Heights Boulevard, Bowling Green, KY 42101, USA. ; Center for Cosmological and Particle Physics, New York University, 4 Washington Place, New York, NY 10003, USA. Department of Astrophysics, American Museum of Natural History, Central Park West and 79th Street, New York, NY 10024, USA. ; Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA. ; Department of Physics and Astronomy, Rutgers, the State University of New Jersey, Piscataway, NJ 08854, USA. ; Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218, USA. Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA. ; Department of Physics, University of California, Davis, CA 95616, USA. ; Steward Observatory, University of Arizona, Tucson, AZ 85721, USA. ; Department of Physics, University of Chicago, 5720 South Ellis Avenue, Chicago, IL 60637, USA. Kavli Institute for Cosmological Physics, University of Chicago, 5720 South Ellis Avenue, Chicago, IL 60637, USA. ; Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Demark. Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA. ; School of Physics, University of Melbourne, VIC 3010, Australia. ; Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Demark. ; Institut d'Astrophysique de Paris, 98 bis Boulevard Arago, F-75014 Paris, France. ; INAF-OAR, Via Frascati 33, 00040 Monte Porzio, Rome, Italy. ; Las Cumbres Observatory Global Telescope Network, 6740 Cortona Drive Suite 102, Goleta, CA 93117, USA. ; Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101, USA. ; Astrophysics Science Division, NASA Goddard Space Flight Center, MC 661, Greenbelt, MD 20771, USA. Joint Space-Science Institute, University of Maryland, College Park, MD 20742, USA. ; Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA. The Research School of Astronomy and Astrophysics, Australian National University, Mount Stromlo Observatory, via Cotter Road, Weston Creek, Australian Capital Territory 2611, Australia.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25745167" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 6
    Publication Date: 2015-06-25
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Olling, Rob P -- Mushotzky, Richard -- Shaya, Edward J -- Rest, Armin -- Garnavich, Peter M -- Tucker, Brad E -- Kasen, Daniel -- Margheim, Steve -- Filippenko, Alexei V -- England -- Nature. 2015 Aug 27;524(7566):502. doi: 10.1038/nature14572. Epub 2015 Jun 24.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/26106862" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 7
    ISSN: 1615-6102
    Keywords: Uromyces ; Differentiation ; Cytoskeleton ; Actin ; Cytochalasin E ; Phalloidin
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology
    Notes: Summary The role of F-actin in cell differentiation ofUromyces appendiculatus (bean rust fungus) germlings was examined by treating differentiating and nondifferentiating germlings with the actin-binding drugs cytochalasin E (CE) and phalloidin. Prolonged exposure of urediospores to 5×10−3–5 × 10−5 M CE induced nuclear division in up to 28–45% of the resulting germlings, whereas the rate of mitosis in established germlings exposed to these concentrations of CE was significantly lower (4–11%). Germlings treated with CE shifted from polarized apical growth to spherical expansion, cytoplasmic microfilaments were depolymerized, and nuclear inclusions became enlarged. Differentiating germlings exposed to a 10 minute pulse of 5×10−6M CE before the initiation of septum formation prevented the establishment of the F-actin septal ring and growth of the crosswall delimiting the appressorium. Although these CE treatments resulted in morphological and nuclear events similar to those occurring during normal appressorium formation, transient microfilament depolymerization was not sufficient to induce differentiation. Phalloidin stabilized cytoplasmic microfilaments, especially posteriorly-located microfilaments, but did not affect differentiation, nor did it significantly inhibit the effects of CE.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Hoboken, NJ : Wiley-Blackwell
    Journal of Biomedical Materials Research 29 (1995), S. 1499-1505 
    ISSN: 0021-9304
    Keywords: Chemistry ; Polymer and Materials Science
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Medicine , Technology
    Notes: The purpose of this study was to develop an analytical method for evaluating the dissolution behavior of plasmasprayed hydroxyapatite (HAP) coatings. Six commercially available and clinically used coatings applied to nonporous titanium coupons according to their respective specifications for orthopedic devices were used in this study. Dissolution behavior was monitored by first preconditioning the implant in 0.15 mol L-1 sodium chloride solution at 37°C until either equilibrium or the desired change in solution hydrogen and calcium ion concentrations had been reached. In the second step, the implants were subjected to dual constant composition (DCC) dissolution under conditions of controlled undersaturation. Results indicate that the dissolution rates of the HAP coatings may differ by as much as a factor of 5 despite the fact that analytical techniques, including X-ray diffraction and FTIR, indicate no change in crystallinity or composition of the coatings before and after the solution treatment. These results indicate that HAP coatings from different sources react very differently when placed in the same local aqueous environment. However, more work will be necessary before these in vitro results can be used to predict in vivo behavior. © 1995 John Wiley & Sons, Inc.
    Additional Material: 7 Ill.
    Type of Medium: Electronic Resource
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  • 9
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    Unknown
    Kluwer
    In:  Dordrecht, 276 pp., Kluwer, vol. 13, no. XVI:, pp. 227-235, (ISBN 0-7923-5587-3)
    Publication Date: 1999
    Keywords: Earthquake hazard ; Earthquake engineering, engineering seismology ; Handbook of geophysics
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  • 10
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