46 research outputs found

    Revisiting the design intent concept in the context of mechanical CAD education

    Get PDF
    [EN] Design intent is generally understood simply as a CAD modelÂżs anticipated behavior when altered. However, this representation provides a simplified view of the modelÂżs construction and purpose, which may hinder its general understanding and future reusability. Our vision is that design intent communication may be improved by recognizing the multifaceted nature of design intent, and by instructing users to convey each facet of design intent through the better-fitted CAD resource. This paper reviews the current understanding of design intent and its relationship to design rationale and builds on the idea that communication of design intent conveyed via CAD models can be satisfied at three levels provided that specialized instruction is used to instruct users in selection of the most suitable level for each intent.Otey, J.; Company, P.; Contero, M.; Camba, J. (2018). Revisiting the design intent concept in the context of mechanical CAD education. Computer-Aided Design and Applications. 15(1):47-60. https://doi.org/10.1080/16864360.2017.1353733S476015

    Suzaku Observations of Luminous Quasars: Revealing the Nature of High-Energy Blazar Emission in Quiescent States

    Full text link
    We present the results from the Suzaku X-ray observations of five flat-spectrum radio quasars (FSRQs), namely PKS0208-512, Q0827+243, PKS1127-145, PKS1510-089 and 3C 454.3. All these sources were additionally monitored simultaneously or quasi-simultaneously by the Fermi satellite in gamma-rays and the Swift UVOT in the UV and optical bands, respectively. We constructed their broad-band spectra covering the frequency range from 10^14 Hz up to 10^25 Hz, and those reveal the nature of high-energy emission of luminous blazars in their low-activity states. The analyzed X-ray spectra are well fitted by a power-law model with photoelectric absorption. In the case of PKS0208-512, PKS1127-145, and 3C 454.3, the X-ray continuum showed indication of hard-ening at low-energies. Moreover, when compared with the previous X-ray observations, we see a significantly increasing contribution of low-energy photons to the total X-ray fluxes when the sources are getting fainter. The same behavior can be noted in the Suzaku data alone. A likely explanation involves a variable, flat-spectrum component produced via inverse-Compton (IC) emission, plus an additional, possibly steady soft X-ray component prominent when the source gets fainter. This soft X-ray excess is represented either by a steep powerlaw (photon indices Gamma ~ 3 - 5) or a blackbody-type emission with temperatures kT ~ 0.1-0.2 keV. We model the broad-band spectra spectra of the five observed FSRQs using synchrotron self-Compton (SSC) and/or external-Compton radiation (ECR) models. Our modeling suggests that the difference between the low and high-activity states in luminous blazars is due to the different total kinetic power of the jet, most likely related to varying bulk Lorentz factor of the outflow within the blazar emission zone.Comment: 36 pages, 8 figures, 11 tables. Accepted for publication in the Astrophysical Journal

    Fermi/LAT discovery of gamma-ray emission from the flat-spectrum radio quasar PKS 1454-354

    Full text link
    We report the discovery by the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope of high-energy gamma-ray (GeV) emission from the flat-spectrum radio quasar PKS 1454-354 (z=1.424). On 4 September 2008 the source rose to a peak flux of (3.5 +/- 0.7)x 10^-6 ph cm^-2 s^-1 (E > 100 MeV) on a time scale of hours and then slowly dropped over the following two days. No significant spectral changes occurred during the flare. Fermi/LAT observations also showed that PKS 1454-354 is the most probable counterpart of the unidentified EGRET source 3EG J1500-3509. Multiwavelength measurements performed during the following days (7 September with Swift; 6-7 September with the ground-based optical telescope ATOM; 13 September with the Australia Telescope Compact Array) resulted in radio, optical, UV and X-ray fluxes greater than archival data, confirming the activity of PKS 1454-354.Comment: 8 pages, 5 figures, 2 tables. Accepted for publication on ApJ Main Journa

    City for sale: the transformation of San Francisco

    No full text
    San Francisco is perhaps the most exhilarating of all American cities--its beauty, cultural and political avant-gardism, and history are legendary, while its idiosyncrasies make front-page news. In this revised edition of his highly regarded study of San Francisco's economic and political development since the mid-1950s, Chester Hartman gives a detailed account of how the city has been transformed by the expansion--outward and upward--of its downtown. His story is fueled by a wide range of players and an astonishing array of events, from police storming the International Hotel to citizens forcing the midair termination of a freeway. Throughout, Hartman raises a troubling question: can San Francisco's unique qualities survive the changes that have altered the city's skyline, neighborhoods, and economy? Hartman was directly involved in many of the events he chronicles and thus had access to sources that might otherwise have been unavailable. A former activist with the National Housing Law Project, San Franciscans for Affordable Housing, and other neighborhood organizations, he explains how corporate San Francisco obtained the necessary cooperation of city and federal governments in undertaking massive redevelopment. He illustrates the rationale that produced BART, a subway system that serves upper-income suburbs but few of the city's poor neighborhoods, and cites the environmental effects of unrestrained highrise development, such as powerful wind tunnels and lack of sunshine. In describing the struggle to keep housing affordable in San Francisco and the seemingly intractable problem of homelessness, Hartman reveals the human face of the city's economic transformation

    Sweet charity gone sour

    No full text

    Feedback

    No full text
    corecore