10,718 research outputs found

    Refitting successful daily wear GP patients into thirty day continuous wear gas permeable lenses: A case series

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    Current rigid gas permeable lens wearers were refit into the thirty day continuous wear Menicon Z gas permeable lens. The purpose of the study was to evaluate how the subjects transitioned to the new Menicon Z lenses and the thirty day wearing schedule. Subjects were monitored for two months for an ocular health changes by assessing visual acuity, performing biomicroscopy and lens fit evaluation, and corneal topography

    Extending Bauer's corollary to fractional derivatives

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    We comment on the method of Dreisigmeyer and Young [D. W. Dreisigmeyer and P. M. Young, J. Phys. A \textbf{36}, 8297, (2003)] to model nonconservative systems with fractional derivatives. It was previously hoped that using fractional derivatives in an action would allow us to derive a single retarded equation of motion using a variational principle. It is proven that, under certain reasonable assumptions, the method of Dreisigmeyer and Young fails.Comment: Accepted Journal of Physics A at www.iop.org/EJ/journal/JPhys

    The QUEST-La Silla AGN Variability Survey

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    We present the characterization and initial results from the QUEST-La Silla AGN variability survey. This is an effort to obtain well sampled optical light curves in extragalactic fields with unique multi-wavelength observations. We present photometry obtained from 2010 to 2012 in the XMM-COSMOS field, which was observed over 150 nights using the QUEST camera on the ESO-Schmidt telescope. The survey uses a broadband filter, the QQ-band, similar to the union of the gg and the rr filters, achieving an intrinsic photometric dispersion of 0.050.05 mag, and a systematic error of 0.050.05 mag in the zero-point. Since some detectors of the camera show significant non-linearity, we use a linear correlation to fit the zero-points as a function of the instrumental magnitudes, thus obtaining a good correction to the non-linear behavior of these detectors. We obtain good photometry to an equivalent limiting magnitude of r∌20.5r\sim 20.5. Studying the optical variability of X-ray detected sources in the XMM-COSMOS field, we find that the survey is ∌75−80\sim75-80% complete to magnitudes r∌20r\sim20, and ∌67\sim67% complete to a magnitude r∌21r\sim21. The determination and parameterization of the structure function (SFnorm(τ)=AÏ„Îł{SF}_{norm}(\tau) = A \tau^{\gamma}) of the variable sources shows that most BL AGN are characterized by A>0.1A > 0.1 and Îł>0.025\gamma > 0.025. It is further shown that variable NL AGN and GAL sources occupying the same parameter space in AA and Îł\gamma are very likely to correspond to obscured or low luminosity AGN. Our samples are, however, small, and we expect to revisit these results using larger samples with longer light curves obtained as part of our ongoing survey.Comment: Accepted for publication in Ap

    Dust in the reionization era: ALMA observations of a zz=8.38 Galaxy

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    We report on the detailed analysis of a gravitationally-lensed Y-band dropout, A2744_YD4, selected from deep Hubble Space Telescope imaging in the Frontier Field cluster Abell 2744. Band 7 observations with the Atacama Large Millimeter Array (ALMA) indicate the proximate detection of a significant 1mm continuum flux suggesting the presence of dust for a star-forming galaxy with a photometric redshift of z≃8z\simeq8. Deep X-SHOOTER spectra confirms the high redshift identity of A2744_YD4 via the detection of Lyman α\alpha emission at a redshift zz=8.38. The association with the ALMA detection is confirmed by the presence of [OIII] 88ÎŒ\mum emission at the same redshift. Although both emission features are only significant at the 4 σ\sigma level, we argue their joint detection and the positional coincidence with a high redshift dropout in the HST images confirms the physical association. Analysis of the available photometric data and the modest gravitational magnification (Ό≃2\mu\simeq2) indicates A2744_YD4 has a stellar mass of ∌\sim 2×\times109^9 M⊙_{\odot}, a star formation rate of ∌20\sim20 M⊙_{\odot}/yr and a dust mass of ∌\sim6×\times106^{6} M⊙_{\odot}. We discuss the implications of the formation of such a dust mass only ≃\simeq200 Myr after the onset of cosmic reionisation.Comment: Accepted for publication in ApJ

    High Time for Conservation: Adding the Environment to the Debate on Marijuana Liberalization

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    The liberalization of marijuana policies, including the legalization of medical and recreational marijuana, is sweeping the United States and other countries. Marijuana cultivation can have significant negative collateral effects on the environment that are often unknown or overlooked. Focusing on the state of California, where by some estimates 60% -- 70% of the marijuana consumed in the United States is grown, we argue that (a) the environmental harm caused by marijuana cultivation merits a direct policy response, (b) current approaches to governing the environmental effects are inadequate, and (c) neglecting discussion of the environmental impacts of cultivation when shaping future marijuana use and possession policies represents a missed opportunity to reduce, regulate, and mitigate environmental harm

    Nonconservative Lagrangian mechanics II: purely causal equations of motion

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    This work builds on the Volterra series formalism presented in [D. W. Dreisigmeyer and P. M. Young, J. Phys. A \textbf{36}, 8297, (2003)] to model nonconservative systems. Here we treat Lagrangians and actions as `time dependent' Volterra series. We present a new family of kernels to be used in these Volterra series that allow us to derive a single retarded equation of motion using a variational principle
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