129 research outputs found

    The Philosophy of the Western

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    The western is arguably the most iconic and influential genre in American cinema. The solitude of the lone rider, the loyalty of his horse, and the unspoken code of the West render the genre popular yet lead it to offer a view of America’s history that is sometimes inaccurate. For many, the western embodies America and its values. In recent years, scholars had declared the western genre dead, but a steady resurgence of western themes in literature, film, and television has reestablished the genre as one of the most important. In The Philosophy of the Western, editors Jennifer L. McMahon and B. Steve Csaki examine philosophical themes in the western genre. Investigating subjects of nature, ethics, identity, gender, environmentalism, and animal rights, the essays draw from a wide range of westerns including the recent popular and critical successes Unforgiven (1992), All the Pretty Horses (2000), 3:10 to Yuma (2007), and No Country for Old Men (2007), as well as literature and television serials such as Deadwood. The Philosophy of the Western reveals the influence of the western on the American psyche, filling a void in the current scholarship of the genre. Jennifer L. McMahon, associate professor and chair of the English and Languages Department at East Central University, is a contributor to The Philosophy of TV Noir, The Philosophy of Martin Scorsese, and The Simpsons and Philosophy. B. Steve Csaki was most recently a visiting professor at Centre College, where he taught courses in philosophy, the humanities, and Japanese. The writing is accessible to nonspecialists and should be of interest to general readers who enjoy thinking about philosophy, film, or westerns. --Karen D. Hoffman, Hood College A delightful collection, one that goes a long way toward bridging the fields of philosophy and film studies. At once erudite and readable, many of its essays offer solid summaries of philosophic concepts and movements. . . .those familiar with the classic westerns will find the book a painless way to pick up some philosophy. --American Studies The authors examine the rise and recent resurgence of the iconic genre of American cinema—its popularity, its claims on encapsulating American values, and its historical inaccuracies. --Moving Image Archives These essays, and others, connect rewardingly to ongoing discussions of Westerns in a broad context --Choice Magazine The collection is evenly divided between classic and contemporary Westerns, providing a comprehensive overview of the history of the genre -- Western American Literature For Western film fams and American scholars alike, The Philosophy of the Western is both enjoyable and enlightening. It will leave you longing to dust off the covers of your favorite Western films and rewatch them with a deeper sense of significance adn newfound appreciation. --Journal of American Studies Association of Texas These essays make compelling cases --Western Historical Quarterly Anyone interested in the mythic grip that Westerns have had and continue to have on the American imaginary will no doubt find something of interest in this collection. --Great Plains Quarterlyhttps://uknowledge.uky.edu/upk_american_popular_culture/1010/thumbnail.jp

    DAzLE: The Dark Ages z (redshift) Lyman-alpha Explorer

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    DAzLE is an near infrared narrowband differential imager being built by the Institute of Astronomy, Cambridge, in collaboration with the Anglo-Australian observatory. It is a special purpose instrument designed with a sole aim; the detection of redshifted Lyman-alpha emission from star forming galaxies at z>7. DAzLE will use pairs of high resolution (R=1000) narrowband filters to exploit low background `windows' in the near infrared sky emission spectrum. This will enable it to reach sensitivities of ~2E-21 W/m^2, thereby allowing the detection of z>7 galaxies with star formation rates as low as a few solar masses per year. The design of the instrument, and in particular the crucial narrowband filters, are presented. The predicted performance of DAzLE, including the sensitivity, volume coverage and expected number counts, is discussed. The current status of the DAzLE project, and its projected timeline, are also presented.Comment: 11 pages, 7 figures, to appear in Proceedings of SPIE Vol. 5492, Ground-based Instrumentation for Astronom

    The retinoblastoma tumor suppressor modulates DNA repair and radioresponsiveness.

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    PURPOSE: Perturbations in the retinoblastoma pathway are over-represented in advanced prostate cancer; retinoblastoma loss promotes bypass of first-line hormone therapy. Conversely, preliminary studies suggested that retinoblastoma-deficient tumors may become sensitized to a subset of DNA-damaging agents. Here, the molecular and in vivo consequence of retinoblastoma status was analyzed in models of clinical relevance. EXPERIMENTAL DESIGN: Experimental work was performed with multiple isogenic prostate cancer cell lines (hormone sensitive: LNCaP and LAPC4 cells and hormone resistant C42, 22Rv1 cells; stable knockdown of retinoblastoma using shRNA). Multiple mechanisms were interrogated including cell cycle, apoptosis, and DNA damage repair. Transcriptome analysis was performed, validated, and mechanisms discerned. Cell survival was measured using clonogenic cell survival assay and in vivo analysis was performed in nude mice with human derived tumor xenografts. RESULTS: Loss of retinoblastoma enhanced the radioresponsiveness of both hormone-sensitive and castrate-resistant prostate cancer. Hypersensitivity to ionizing radiation was not mediated by cell cycle or p53. Retinoblastoma loss led to alteration in DNA damage repair and activation of the NF-ÎșB pathway and subsequent cellular apoptosis through PLK3. In vivo xenografts of retinoblastoma-deficient tumors exhibited diminished tumor mass, lower PSA kinetics, and decreased tumor growth after treatment with ionizing radiation (P \u3c 0.05). CONCLUSIONS: Loss of retinoblastoma confers increased radiosensitivity in prostate cancer. This hypersensitization was mediated by alterations in apoptotic signaling. Combined, these not only provide insight into the molecular consequence of retinoblastoma loss, but also credential retinoblastoma status as a putative biomarker for predicting response to radiotherapy

    The Fungicide Chlorothalonil Is Nonlinearly Associated with Corticosterone Levels, Immunity, and Mortality in Amphibians

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    Background: Contaminants have been implicated in declines of amphibians, a taxon with vital systems similar to those of humans. However, many chemicals have not been thoroughly tested on amphibians or do not directly kill them

    The Atacama Cosmology Telescope: Detection of mm-wave transient sources

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    We report on the serendipitous discovery of three transient mm-wave sources using data from the Atacama Cosmology Telescope. The first, detected at RA = 273.8138, dec = -49.4628 at ∌50σ{\sim}50\sigma total, brightened from less than 5 mJy to at least 1100 mJy at 150 GHz with an unknown rise time shorter than thirteen days, during which the increase from 250 mJy to 1100 mJy took only 8 minutes. Maximum flux was observed on 2019-11-8. The source's spectral index in flux between 90 and 150 GHz was positive, α=1.5±0.2\alpha = 1.5\pm0.2. The second, detected at RA = 105.1584, dec = -11.2434 at ∌20σ{\sim}20\sigma total, brightened from less than 20 mJy to at least 300 mJy at 150 GHz with an unknown rise time shorter than eight days. Maximum flux was observed on 2019-12-15. Its spectral index was also positive, α=1.8±0.2\alpha = 1.8\pm0.2. The third, detected at RA = 301.9952, dec = 16.1652 at ∌40σ{\sim}40\sigma total, brightened from less than 8 mJy to at least 300 mJy at 150 GHz over a day or less but decayed over a few days. Maximum flux was observed on 2018-9-11. Its spectrum was approximately flat, with a spectral index of α=−0.2±0.1\alpha = -0.2\pm0.1. None of the sources were polarized to the limits of these measurements. The two rising-spectrum sources are coincident in position with M and K stars, while the third is coincident with a G star.Comment: 8 pages, 4 figures, 1 tabl

    The Atacama Cosmology Telescope: Microwave Intensity and Polarization Maps of the Galactic Center

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    We present arcminute-resolution intensity and polarization maps of the Galactic center made with the Atacama Cosmology Telescope (ACT). The maps cover a 32 deg2^2 field at 98, 150, and 224 GHz with ∣lâˆŁâ‰€4∘\vert l\vert\le4^\circ, ∣bâˆŁâ‰€2∘\vert b\vert\le2^\circ. We combine these data with Planck observations at similar frequencies to create coadded maps with increased sensitivity at large angular scales. With the coadded maps, we are able to resolve many known features of the Central Molecular Zone (CMZ) in both total intensity and polarization. We map the orientation of the plane-of-sky component of the Galactic magnetic field inferred from the polarization angle in the CMZ, finding significant changes in morphology in the three frequency bands as the underlying dominant emission mechanism changes from synchrotron to dust emission. Selected Galactic center sources, including Sgr A*, the Brick molecular cloud (G0.253+0.016), the Mouse pulsar wind nebula (G359.23-0.82), and the Tornado supernova remnant candidate (G357.7-0.1), are examined in detail. These data illustrate the potential for leveraging ground-based Cosmic Microwave Background polarization experiments for Galactic science.Comment: 26 pages, 14 figures, accepted for publication in Ap

    The Simons Observatory microwave SQUID multiplexing detector module design

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    Advances in cosmic microwave background (CMB) science depend on increasing the number of sensitive detectors observing the sky. New instruments deploy large arrays of superconducting transition-edge sensor (TES) bolometers tiled densely into ever larger focal planes. High multiplexing factors reduce the thermal loading on the cryogenic receivers and simplify their design. We present the design of focal-plane modules with an order of magnitude higher multiplexing factor than has previously been achieved with TES bolometers. We focus on the novel cold readout component, which employs microwave SQUID multiplexing (Ό\mumux). Simons Observatory will use 49 modules containing 60,000 bolometers to make exquisitely sensitive measurements of the CMB. We validate the focal-plane module design, presenting measurements of the readout component with and without a prototype detector array of 1728 polarization-sensitive bolometers coupled to feedhorns. The readout component achieves a 95%95\% yield and a 910 multiplexing factor. The median white noise of each readout channel is 65 pA/Hz\mathrm{pA/\sqrt{Hz}}. This impacts the projected SO mapping speed by <8%< 8\%, which is less than is assumed in the sensitivity projections. The results validate the full functionality of the module. We discuss the measured performance in the context of SO science requirements, which are exceeded.Comment: Accepted to The Astrophysical Journa

    The Atacama Cosmology Telescope: Modeling the Gas Thermodynamics in BOSS CMASS galaxies from Kinematic and Thermal Sunyaev-Zel'dovich Measurements

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    The thermal and kinematic Sunyaev-Zel'dovich effects (tSZ, kSZ) probe the thermodynamic properties of the circumgalactic and intracluster medium (CGM and ICM) of galaxies, groups, and clusters, since they are proportional, respectively, to the integrated electron pressure and momentum along the line-of-sight. We present constraints on the gas thermodynamics of CMASS galaxies in the Baryon Oscillation Spectroscopic Survey (BOSS) using new measurements of the kSZ and tSZ signals obtained in a companion paper. Combining kSZ and tSZ measurements, we measure within our model the amplitude of energy injection Ï”M⋆c2\epsilon M_\star c^2, where M⋆M_\star is the stellar mass, to be Ï”=(40±9)×10−6\epsilon=(40\pm9)\times10^{-6}, and the amplitude of the non-thermal pressure profile to be αNth<0.2\alpha_{\rm Nth}<0.2 (2σ\sigma), indicating that less than 20% of the total pressure within the virial radius is due to a non-thermal component. We estimate the effects of including baryons in the modeling of weak-lensing galaxy cross-correlation measurements using the best fit density profile from the kSZ measurement. Our estimate reduces the difference between the original theoretical model and the weak-lensing galaxy cross-correlation measurements in arXiv:1611.08606 by half, but does not fully reconcile it. Comparing the kSZ and tSZ measurements to cosmological simulations, we find that they under predict the CGM pressure and to a lesser extent the CGM density at larger radii. This suggests that the energy injected via feedback models in the simulations that we compared against does not sufficiently heat the gas at these radii. We do not find significant disagreement at smaller radii. These measurements provide novel tests of current and future simulations. This work demonstrates the power of joint, high signal-to-noise kSZ and tSZ observations, upon which future cross-correlation studies will improve.Comment: Accepted for publication in Physical Review D. Editors' Suggestion. New Fig. 1-2, Tab.

    Breeding progress and preparedness for mass‐scale deployment of perennial lignocellulosic biomass crops switchgrass, miscanthus, willow and poplar

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    UK: The UK‐led miscanthus research and breeding was mainly supported by the Biotechnology and Biological Sciences Research Council (BBSRC), Department for Environment, Food and Rural Affairs (Defra), the BBSRC CSP strategic funding grant BB/CSP1730/1, Innovate UK/BBSRC “MUST” BB/N016149/1, CERES Inc. and Terravesta Ltd. through the GIANT‐LINK project (LK0863). Genomic selection and genomewide association study activities were supported by BBSRC grant BB/K01711X/1, the BBSRC strategic programme grant on Energy Grasses & Bio‐refining BBS/E/W/10963A01. The UK‐led willow R&D work reported here was supported by BBSRC (BBS/E/C/00005199, BBS/E/C/00005201, BB/G016216/1, BB/E006833/1, BB/G00580X/1 and BBS/E/C/000I0410), Defra (NF0424) and the Department of Trade and Industry (DTI) (B/W6/00599/00/00). IT: The Brain Gain Program (Rientro dei cervelli) of the Italian Ministry of Education, University, and Research supports Antoine Harfouche. US: Contributions by Gerald Tuskan to this manuscript were supported by the Center for Bioenergy Innovation, a US Department of Energy Bioenergy Research Center supported by the Office of Biological and Environmental Research in the DOE Office of Science, under contract number DE‐AC05‐00OR22725. Willow breeding efforts at Cornell University have been supported by grants from the US Department of Agriculture National Institute of Food and Agriculture. Contributions by the University of Illinois were supported primarily by the DOE Office of Science; Office of Biological and Environmental Research (BER); grant nos. DE‐SC0006634, DE‐SC0012379 and DE‐SC0018420 (Center for Advanced Bioenergy and Bioproducts Innovation); and the Energy Biosciences Institute. EU: We would like to further acknowledge contributions from the EU projects “OPTIMISC” FP7‐289159 on miscanthus and “WATBIO” FP7‐311929 on poplar and miscanthus as well as “GRACE” H2020‐EU.3.2.6. Bio‐based Industries Joint Technology Initiative (BBI‐JTI) Project ID 745012 on miscanthus.Peer reviewedPostprintPublisher PD
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