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I discuss th eu se of Type Ia supernovae (SNe Ia) for cosmo f logica ld istance deter- minations. Low-redshift SNe Ia (z < 0.1) demonstrate that the Hubble expan- sion is linear with H0 H0 =7 2±8 km s −1 Mpc −1 , and that the properties o fd ust in other galaxies are generally similar to those of dust in the Milky Way. The light curves o fh igh -redshif t( f z = 0.3-1) SNe Ia are stretche di n a manner consis- ten tw ith the expansion of space; similarly, their spectra exhibi ts lower temporal evolution (by a factor o f f 1 + z )t han those of nearby r SNe Ia. The measured luminosity distances of SNe Ia as a function of redshift have shown that the ex- pansion of the Universe is currently accelerating, probably due to the presence of repulsive dark energy such as Einstein's cosmological constant (Λ). From about 200 SNe Ia, we find that H0 H0t0 = 0.96 ± 0.04, and ΩΛ − 1.4ΩM = 0.35 ± 0.14. Combining our data with th er esu lts o fl arge-scale structure surveys ,w e fin da best fit for ΩM and ΩΛ of 0.28 and 0.72, respectively — essentially identical to the recent WM
T cells expressing the gd receptor are the major lymphocyte type represented in intraepithelial layers of various organs in the mouse. The gd cells found in distinct anatomical locations express distinct restricted subsets of Vg and Vd genes. Cells in each site are probably derived from progressive intrathymic waves of gd cells expressing these restricted V gene subsets. These features of the cells suggest a role in monitoring epithelial layers for distinctive ligands, and recent studies implicate mycobacterial "stress proteins' as antigens for g/d T cells. Thus gd T cells may represent an arm of the immune system devoted to elimination of infected, transformed or otherwise stressed autologous epithelial cells, based on recognition of induced stress proteins. They may also be devoted to mycobacterial immunity by virtue of specificity for mycobacterial stress proteins and other antigens.
We characterize the problem of pose estimation for rigid objects in terms of determining viewpoint to explain coarse pose and keypoint prediction to capture the finer details. We address both these tasks in two different settings - the constrained setting with known bounding boxes and the more challenging detection setting where the aim is to simultaneously detect and correctly estimate pose of objects. We present Convolutional Neural Network based architectures for these and demonstrate that leveraging viewpoint estimates can substantially improve local appearance based keypoint predictions. In addition to achieving significant improvements over state-of-the-art in the above tasks, we analyze the error modes and effect of object characteristics on performance to guide future efforts towards this goal.
Abstract : We have used a shockfront, produced in a small, electrothermal shocktube filled with 40-60 torr D2, as a model target for studies of the interaction of intense laser light with hot, dense, inhomogeneous plasmas. The CO2 laser pulse (lambda = 10.6 micrometer; 100-500 psec FWHM; typical energy 100 mJ) is tightly focussed, at an oblique angle, onto the shockfront axis, and a laser-Schlieren shockfront detection system fires the laser at the instant the Mach-5 shockfront passes into focus. The shockfront, whose motion is negligible on the time scale of the laser pulse is ionized by optical breakdown. When the laser pulse and the shockfront are properly synchronized, we observe energetic electrons (40-140 keV) to be emitted in a narrow cone centered on the shocktube axis. Our measurements of the angular distribution and energy spectrum of these electrons are in agreement with the predictions of the theory of resonance absorption of laser light by plasmas.