385 research outputs found

    Multilingual Museums: A Proposal to Increase Linguistic Diversity in Contemporary Art Museums

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    The U.S. population is becoming more ethnically, racially, and linguistically diverse. It is estimated that by the year 2050, the U.S. will shift to a majority-minority population, meaning that the total minority population will become the majority of the U.S. population. But while the U.S. is diversifying, the current museum visitorship demographic is not representative of or on track to measure up to these changes in the future. If museums are valuable civic spaces with several associated health, social, and educational benefits, and a large percentage of the population have low-English proficiency and cannot access the information, then there is a large percentage of potential museum visitors that are being denied the opportunity to a significant cultural activity. One way museums can break down linguistic barriers is to provide bilingual and multilingual exhibitions. The creation of these translated exhibitions not only give low-English proficiency individuals the opportunity to create meaningful experiences in a museum, it also purposefully welcomes them into a space that has been historically inaccessible to them. While research and evaluation are currently being conducted in many science and children’s museums, little is being done in art museums. This capstone proposes the creation of a set of guidelines to be utilized by contemporary art museums in the United States in order to increase linguistic diversity by creating bilingual and multilingual exhibitions

    ArsRS-Dependent Regulation of homB Contributes to Helicobacter pylori Biofilm Formation

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    One elusive area in the Helicobacter pylori field is an understanding of why some infections result in gastric cancer, yet others persist asymptomatically for the life-span of the individual. Even before the genomic era, the high level of intraspecies diversity of H. pylori was well recognized and became an intriguing area of investigation with respect to disease progression. Of interest in this regard is the unique repertoire of over 60 outer membrane proteins (OMPs), several of which have been associated with disease outcome. Of these OMPs, the association between HomB and disease outcome varies based on the population being studied. While the molecular roles for some of the disease-associated OMPs have been evaluated, little is known about the role that HomB plays in the H. pylori lifecycle. Thus, herein we investigated homB expression, regulation, and contribution to biofilm formation. We found that in H. pylori strain G27, homB was expressed at a relatively low level until stationary phase. Furthermore, homB expression was suppressed at low pH in an ArsRS-dependent manner; mutation of arsRS resulted in increased homB transcript at all tested time-points. ArsRS regulation of homB appeared to be direct as purified ArsR was able to specifically bind to the homB promoter. This regulation, combined with our previous finding that ArsRS mutations lead to enhanced biofilm formation, led us to test the hypothesis that homB contributes to biofilm formation by H. pylori. Indeed, subsequent biofilm analysis using a crystal-violet quantification assay and scanning electron microscopy (SEM) revealed that loss of homB from hyper-biofilm forming strains resulted in reversion to a biofilm phenotype that mimicked wild-type. Furthermore, expression of homB in trans from a promoter that negated ArsRS regulation led to enhanced biofilm formation even in strains in which the chromosomal copy of homB had been deleted. Thus, homB is necessary for hyper-biofilm formation of ArsRS mutant strains and aberrant regulation of this gene is sufficient to induce a hyper-biofilm phenotype. In summary, these data suggest that the ArsRS-dependent regulation of OMPs such as HomB may be one mechanism by which ArsRS dictates biofilm development in a pH responsive manner

    KMT-2016-BLG-1107: A New Hollywood-Planet Close/Wide Degeneracy

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    We show that microlensing event KMT-2016-BLG-1107 displays a new type of degeneracy between wide-binary and close-binary Hollywood events in which a giant-star source envelops the planetary caustic. The planetary anomaly takes the form of a smooth, two-day "bump" far out on the falling wing of the light curve, which can be interpreted either as the source completely enveloping a minor-image caustic due to a close companion with mass ratio q=0.036q=0.036, or partially enveloping a major-image caustic due to a wide companion with q=0.004q=0.004. The best estimates of the companion masses are both in the planetary regime (3.3−1.8+3.5 Mjup3.3^{+3.5}_{-1.8}\,M_{\rm jup} and 0.090−0.037+0.096 Mjup0.090^{+0.096}_{-0.037}\,M_{\rm jup}) but differ by an even larger factor than the mass ratios due to different inferred host masses. We show that the two solutions can be distinguished by high-resolution imaging at first light on next-generation ("30m") telescopes. We provide analytic guidance to understand the conditions under which this new type of degeneracy can appear.Comment: 23 pages, 7 figures, accepted for publication in A

    KMT-2018-BLG-1990Lb: A Nearby Jovian Planet From A Low-Cadence Microlensing Field

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    We report the discovery and characterization of KMT-2018-BLG-1990Lb, a Jovian planet (mp=0.57−0.25+0.79 MJ)(m_p=0.57_{-0.25}^{+0.79}\,M_J) orbiting a late M dwarf (M=0.14−0.06+0.20 M⊙)(M=0.14_{-0.06}^{+0.20}\,M_\odot), at a distance (D_L=1.23_{-0.43}^{+1.06}\,\kpc), and projected at 2.6±0.62.6\pm 0.6 times the snow line distance, i.e., a_{\rm snow}\equiv 2.7\,\au (M/M_\odot), This is the second Jovian planet discovered by KMTNet in its low cadence (0.4 hr−10.4\,{\rm hr}^{-1}) fields, demonstrating that this population will be well characterized based on survey-only microlensing data.Comment: 24 pages, 7 figures, 4 table

    Highly ordered tailored three-dimensional hierarchical nano/microporous gold–carbon architectures

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    The preparation and characterization of three-dimensional hierarchical architectures, consisting of monolithic nanoporous gold or silver films formed on highly ordered 3D microporous carbon supports, are described. The formation of these nano/microporous structures involves the electrodeposition or sputtering of metal alloys onto the lithographically patterned multi-layered microporous carbon, followed by preferential chemical dealloying of the less noble component. The resulting hierarchical structure displays a highly developed 3D interconnected network of micropores with a nanoporous metal coating. Tailoring the nanoporosity of the metal films and the diameter of the large micropores has been accomplished by systematically changing the alloy compositions via control of the deposition potential, plating solution and coarsening time. SEM imaging illustrates the formation of unique biomimetic nanocoral- or nanocauliflower-like self-supporting structures, depending on the specific preparation conditions. The new 3D hierarchical nano/microporous architectures allow for enhanced mass transport and catalytic activity compared to common nanoporous films prepared on planar substrates. The functionality of this new carbon–gold hierarchical structure is illustrated for the greatly enhanced performance of enzymatic biofuel cells where a substantially higher power output is observed compared to the bare microporous carbon substrate

    KMT-2018-BLG-1292: A Super-Jovian Microlens Planet in the Galactic Plane

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    We report the discovery of KMT-2018-BLG-1292Lb, a super-Jovian Mplanet=4.5±1.3 MJM_{\rm planet} = 4.5\pm 1.3\,M_J planet orbiting an F or G dwarf Mhost=1.5±0.4 M⊙M_{\rm host} = 1.5\pm 0.4\,M_\odot, which lies physically within {\cal O}(10\,\pc) of the Galactic plane. The source star is a heavily extincted AI∼5.2A_I\sim 5.2 luminous giant that has the lowest Galactic latitude, b=−0.28∘b=-0.28^\circ, of any planetary microlensing event. The relatively blue blended light is almost certainly either the host or its binary companion, with the first explanation being substantially more likely. This blend dominates the light at II band and completely dominates at RR and VV bands. Hence, the lens system can be probed by follow-up observations immediately, i.e., long before the lens system and the source separate due to their relative proper motion. The system is well characterized despite the low cadence Γ=0.15\Gamma=0.15--0.20 hr−10.20\,{\rm hr^{-1}} of observations and short viewing windows near the end of the bulge season. This suggests that optical microlensing planet searches can be extended to the Galactic plane at relatively modest cost.Comment: 35 pages, 3 Tables, 8 figure
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