The economic geography of the tourist industry by U.S. metropolitan area: a supply-side analysis

The research in this dissertation articulates the economic geography of the tourist industry in the United States by metropolitan statistical area (MSA) from a supply-side perspective. It examines the complex economic mix of the tourism production system by employment patterns, number of establishments, and wages. One of the key purposes of this dissertation is to analyze the intense geographical concentration that underlies the tourist industry and to identify the typologies of metropolitan-based economies that explain much of the clusters. A key hypothesis is that, although the tourism direct providers (e.g. hotels, airlines, etc.) attract more attention in the tourism geography literature than tourism supply service industries (e.g. food and drinking services, performing arts, etc.), that a broad economic equivalence exists between these macro-sectors in terms of number of jobs and establishments by MSA. Overall, it is hypothesized that the tourism production system is largely shaped by the logic of agglomeration theory and that metropolitan area economies that experience high levels of specialization as expressed by elevated tourism-related market shares in terms of jobs and establishments, will also generate a higher overall tourism average wage. Another purpose of this dissertation was to examine the overall impact of tourism specialization on quality of life scores as indicated by per capita income, percent of population with college degrees, and population growth rates. Furthermore, the dissertation examined whether metropolitan area economies that attract disproportionately high levels of tourism market share in terms of employment also attract disproportionate creative class employment based on Florida's (2002) definition. The overall analysis revealed that a broad economic equivalency in terms of number of jobs and number of establishments exists between tourism direct providers (e.g., air transportation and hotels) and the tourism supporting services (e.g., restaurants, performing arts, and sports). Additionally, the findings highlighted an acute geographic concentration of the tourism production system. The top ten MSAs in terms of employment market share accounted for 40% of all tourism jobs. The analysis also revealed that four major tourism MSA typologies existed including casino-based, coastal resort, retirement resorts, and natural resource gateway metropolitan areas. The findings further revealed that tourism average wages varied by MSA and they were highly influenced by the level of tourism concentration and specialization partly due to an economies of scale and agglomeration effect. The analysis supported the notion that the tourism industry's overall impact on various quality of life indicators was largely random, suggesting that the general notion that tourism can be a panacea for an urban economies' ill needs to be re-evaluated and questioned. The analysis also showed that a random relationship existed between tourism employment levels and the percent creative class employment contrary to much of the literature. Additionally, the analysis also suggested that a statistically significant correlation existed between percent creative class employment and cultural tourism employment (e.g., performing arts, spectator sports etc.) Suggesting that targeting culturally-oriented tourism amenities may be a more effective strategy to attract the creative class. Data sets for the dissertation came from different sources including: The Bureau of Economic Analysis (BEA), The Bureau of Labor Statistics (BLS), and The Census Bureau. The North American Industrial Classification System (NAICS) methodology was used to quantify the tourist industry from a supply side perspective

Traditional Underground Grain Storage in Clay Soils in Sudan Improved by Recent Innovations

In the central clay plain of the Sudan, traditional subsistence farmers and small farmers that also produce for local markets want to keep the region near food self-sufficiency. They combine annual production of sorghum with underground pit storage of part of the harvest. With increasing climate variability this food security is coming more and more under pressure. Farmers recently experimented with pit innovations that would allow storage for more than one season. These innovations were quantified and further improvements were suggested. It was found that in the most abundantly occurring cracking clay soils, wide shallow pits, using thick chaff linings, with wider above ground soil caps, are most suitable for longer term storage

Hypercalcemia in a patient with disseminated paracoccidioidomycosis: a case report

<p>Abstract</p> <p>Introduction</p> <p>Hypercalcemia is well described in various granulomatous disorders, such as sarcoidosis, tuberculosis, berylliosis, leprosy and fungal infections. However, the association of <it>Paracoccidioides brasiliensis </it>and hypercalcemia is rare: to the best of our knowledge, only two cases have previously been reported, and neither had a clear documentation of the etiology of the hypercalcemia.</p> <p>Case presentation</p> <p>We report the case of a 22-year-old man in whom disseminated infection with paracoccidioidomycosis was associated with hypercalcemia. The patient had a high normal serum level of 1,25-dihydroxyvitamin D and a suppressed parathyroid hormone value, an indication that the hypercalcemia was not mediated by parathyroid hormone and might be associated with 1,25-dihydroxyvitamin D.</p> <p>Conclusion</p> <p>The episode resolved readily with administration of corticosteroids, an outcome suggesting that this is an effective treatment of hypercalcemia of this origin. On follow-up, while receiving antifungal therapy for <it>P. brasiliensis </it>the patient's calcium values remained normal.</p

Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions

We perform a joint analysis of the auto and cross-correlations between three cosmic fields: the galaxy density field, the galaxy weak lensing shear field, and the cosmic microwave background (CMB) weak lensing convergence field. These three fields are measured using roughly 1300 sq. deg. of overlapping optical imaging data from first year observations of the Dark Energy Survey and millimeter-wave observations of the CMB from both the South Pole Telescope Sunyaev-Zel'dovich survey and Planck. We present cosmological constraints from the joint analysis of the two-point correlation functions between galaxy density and galaxy shear with CMB lensing. We test for consistency between these measurements and the DES-only two-point function measurements, finding no evidence for inconsistency in the context of flat $\Lambda$CDM cosmological models. Performing a joint analysis of five of the possible correlation functions between these fields (excluding only the CMB lensing autospectrum) yields $S_{8}\equiv \sigma_8\sqrt{\Omega_{\rm m}/0.3} = 0.782^{+0.019}_{-0.025}$ and $\Omega_{\rm m}=0.260^{+0.029}_{-0.019}$. We test for consistency between these five correlation function measurements and the Planck-only measurement of the CMB lensing autospectrum, again finding no evidence for inconsistency in the context of flat $\Lambda$CDM models. Combining constraints from all six two-point functions yields $S_{8}=0.776^{+0.014}_{-0.021}$ and $\Omega_{\rm m}= 0.271^{+0.022}_{-0.016}$. These results provide a powerful test and confirmation of the results from the first year DES joint-probes analysis

Dark Energy Survey Year 1 Results: Cross-correlation between Dark Energy Survey Y1 galaxy weak lensing and South Pole Telescope +Planck CMB weak lensing

We cross-correlate galaxy weak lensing measurements from the Dark Energy Survey (DES) year-one data with a cosmic microwave background (CMB) weak lensing map derived from South Pole Telescope (SPT) and Planck data, with an effective overlapping area of 1289 deg2. With the combined measurements from four source galaxy redshift bins, we obtain a detection significance of 5.8σ. We fit the amplitude of the correlation functions while fixing the cosmological parameters to a fiducial ΛCDM model, finding A=0.99±0.17. We additionally use the correlation function measurements to constrain shear calibration bias, obtaining constraints that are consistent with previous DES analyses. Finally, when performing a cosmological analysis under the ΛCDM model, we obtain the marginalized constraints of ωm=0.261-0.051+0.070 and S8σ8ωm/0.3=0.660-0.100+0.085. These measurements are used in a companion work that presents cosmological constraints from the joint analysis of two-point functions among galaxies, galaxy shears, and CMB lensing using DES, SPT, and Planck data

Cosmological lensing ratios with des Y1, SPT, and Planck

Correlations between tracers of the matter density field and gravitational lensing are sensitive to the evolution of the matter power spectrum and the expansion rate across cosmic time. Appropriately defined ratios of such correlation functions, on the other hand, depend only on the angular diameter distances to the tracer objects and to the gravitational lensing source planes. Because of their simple cosmological dependence, such ratios can exploit available signal-to-noise ratio down to small angular scales, even where directly modelling the correlation functions is difficult. We present a measurement of lensing ratios using galaxy position and lensing data from the Dark Energy Survey, and CMB lensing data from the South Pole Telescope and Planck, obtaining the highest precision lensing ratio measurements to date. Relative to the concordance CDM model, we find a best-fitting lensing ratio amplitude of A = 1.1 ± 0.1. We use the ratio measurements to generate cosmological constraints, focusing on the curvature parameter. We demonstrate that photometrically selected galaxies can be used to measure lensing ratios, and argue that future lensing ratio measurements with data from a combination of LSST and Stage-4 CMB experiments can be used to place interesting cosmological constraints, even after considering the systematic uncertainties associated with photometric redshift and galaxy shear estimation

Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole Telescope+Planck

We measure the cross-correlation between redMaGiC galaxies selected from the Dark Energy Survey (DES) year 1 data and gravitational lensing of the cosmic microwave background (CMB) reconstructed from South Pole Telescope (SPT) and Planck data over 1289 deg2. When combining measurements across multiple galaxy redshift bins spanning the redshift range of 0.1

Significance of Elevated Blood Metal Ion Levels in Patients with Metal-on-Metal Prostheses: An Evaluation of Oxidative Stress Markers

It is widely known that cobalt and chromium ions can enhance the production of reactive oxygen species, known to be damaging to cells by disturbing their redox status and then generating oxidative stress. The aim of the present study was to determine if increased metal ion levels induce a state of oxidative stress in patients with metal-on-metal (MM) hip arthroplasty. Results indicated that there was no significant difference in the concentration of oxidative stress markers (total antioxidants, peroxides, and nitrated proteins) in the patients with MM bearings compared to patients without prostheses. The activity antioxidant enzymes was stable (catalase and glutathione peroxidase) or slightly decreased (superoxide dismutase and heme oxygenase-1) over time. This work is the first to determine the biological effects of metal ions released from MM hip implants with regards to mid-term systemic oxidative stress and showed that the increased levels of Co and Cr ions are not associated with significant oxidative stress damage in the plasma of patients with these implants