5,856 research outputs found

    The Most Exciting Time to Be a Catholic Art Critic

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    Laggards No More: The Changed Socioeconomic Status of Francophones in Quebec

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    The economic returns to knowing French in the Quebec labour market have increased steadily since 1970, while the returns to knowing English have decreased. The ability to speak both English and French has increased the earnings of anglophone men since 1980 and anglophone women since 1990, while the returns to bilingualism for francophone men and women remain positive. The health state of the French language in Quebec is also evident in the impressive growth in ownership of Quebec's economy by francophone firms, from 47 percent to 67 percent since the early 1960s.social policy, francophone socioeconomic status

    Polarized Emission from Interstellar Dust

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    Observations of far-infrared (FIR) and submillimeter (SMM) polarized emission are used to study magnetic fields and dust grains in dense regions of the interstellar medium (ISM). These observations place constraints on models of molecular clouds, star-formation, grain alignment mechanisms, and grain size, shape, and composition. The FIR/SMM polarization is strongly dependent on wavelength. We have attributed this wavelength dependence to sampling different grain populations at different temperatures. To date, most observations of polarized emission have been in the densest regions of the ISM. Extending these observations to regions of the diffuse ISM, and to microwave frequencies, will provide additional tests of grain and alignment models. An understanding of polarized microwave emission from dust is key to an accurate measurement of the polarization of the cosmic microwave background. The microwave polarization spectrum will put limits on the contributions to polarized emission from spinning dust and vibrating magnetic dust.Comment: 19 pages; LaTeX2e uses eas.cls; embeds 10 eps files into 7 Figures in document. To appear in "Sky Polarisation at Far-infrared to Radio Wavelengths: The Galactic Screen before the Cosmic Microwave Background," eds. M.-A. Miville-Deschenes and F. Boulanger. EAS Publications Series, Paris. Proceedings of a conference held at IAS, University of Paris-Sud, September 200

    Combining losing games into a winning game

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    Parrondo's paradox is extended to regime switching random walks in random environments. The paradoxical behavior of the resulting random walk is explained by the effect of the random environment. Full characterization of the asymptotic behavior is achieved in terms of the dimensions of some random subspaces occurring in Oseledec's theorem. The regime switching mechanism gives our models a richer and more complex asymptotic behavior than the simple random walks in random environments appearing in the literature, in terms of transience and recurrence

    Astronomical Image Processing with Array Detectors

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    We address the question of astronomical image processing from data obtained with array detectors. We define and analyze the cases of evenly, regularly, and irregularly sampled maps for idealized (i.e., infinite) and realistic (i.e., finite) detectors. We concentrate on the effect of interpolation on the maps, and the choice of the kernel used to accomplish this task. We show how the normalization intrinsic to the interpolation process must be carefully accounted for when dealing with irregularly sampled grids. We also analyze the effect of missing or dead pixels in the array, and their consequences for the Nyquist sampling criterion.Comment: 31 pages, 5 figures, accepted for publication in the PAS
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