1,254 research outputs found

    County Road 622 at San Francisco Perez Creek Medina County, San Antonio District

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    On October 11, 2017, archeologists James T. Abbott and Eric R. Oksanen of TxDOT’s Archeological Studies Branch conducted an archeological survey of the proposed 0.45 acre Area of Potential Effect (APE) as part of the environmental review process in support of the replacement of the existing bridge on County Road 622 at San Francisco Perez Creek in Medina County. Previously documented archeological site 41ME103 is shown in the Texas Archeological Sites Atlas to extend into the APE. Investigations examined the APE for evidence of the site and a single shovel test was excavated and encountered a lens of cobble and larger gravels at 40 cm below surface. No evidence of site 41ME103 was observed in the APE and no archeological historic property was observed in the APE. The existing right of way is unlikely to contained preserved archeological deposits because of previous impacts from construction and maintenance. No artifacts were observed or collected, therefore, nothing was curated. Records are retained at TxDOT under terms of the MOU between TxDOT and the THC

    Synfuel Production As An Economic Farm Enterprise

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    The Effects of Nutrient Availability on Pseudomonas aeruginosa Mono and Co-culture Biofilms

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    Cystic Fibrosis (CF) is a genetic disorder characterized by faulty ion channels and result in thick mucus accumulation, especially in lungs. Mucus buildup provides ideal conditions for bacterial infections. Pseudomonas aeruginosa (PA) is the second most prevalent bacterium isolated from people with CF and has a high clinical importance. Most CF pathogens form biofilms which make treatment of infections difficult. Biofilms are clusters of cells attached to a surface enclosed in a structured matrix. These structures are a means to provide shelter for bacteria from the environment, especially antibiotics and the immune system. PA alone can form these biofilms, but communities of different bacterial species can also form biofilms together. Multispecies biofilms can form beneficial or antagonistic relationships with PA. In this study, we investigated the interaction between PA and two other important CF pathogens, Staphylococcus aureus (SA) and Burkholderia cenocepacia (BC). SA is the most prevalent CF pathogen and BC is arguably the most fatal. We tested the survival of these species in groups or alone in various nutrient conditions and in differing tobramycin concentrations. We chose tobramycin because it is an antibiotic commonly prescribed to treat PA infections. Our results show that nutrient composition, antibiotic concentration, and time all had a significant effect on the interactions between PA mono-culture and co-cultured biofilms. Understanding these interactions may set the stage for a better understanding of the clinical course of infection and how treatments can be altered for multi-species infections.https://ir.library.louisville.edu/uars/1017/thumbnail.jp

    Proxima Centauri b is not a transiting exoplanet

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    We report Spitzer Space Telescope observations during predicted transits of the exoplanet Proxima Centauri b. As the nearest terrestrial habitable-zone planet we will ever discover, any potential transit of Proxima b would place strong constraints on its radius, bulk density, and atmosphere. Subsequent transmission spectroscopy and secondary-eclipse measurements could then probe the atmospheric chemistry, physical processes, and orbit, including a search for biosignatures. However, our photometric results rule out planetary transits at the 200~ppm level at 4.5 μm~{\mu}m, yielding a 3σ\sigma upper radius limit of 0.4~R_\rm{\oplus} (Earth radii). Previous claims of possible transits from optical ground- and space-based photometry were likely correlated noise in the data from Proxima Centauri's frequent flaring. Follow-up observations should focus on planetary radio emission, phase curves, and direct imaging. Our study indicates dramatically reduced stellar activity at near-to-mid infrared wavelengths, compared to the optical. Proxima b is an ideal target for space-based infrared telescopes, if their instruments can be configured to handle Proxima's brightness.Comment: 8 pages, 3 figures, 2 tables, accepted for publication in MNRA

    Megakaryocytes: Regulators of Bone Mass and Hematopoiesis

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    poster abstractEmerging evidence demonstrates that megakaryocytes (MK) play a key role in regulating skeletal homeostasis and hematopoiesis. Recent reports show that MK reside in close proximity to hematopoietic stem cells (HSC). Genetic depletion of MK resulted in mitotic activation of HSC suggesting that MK maintain HSC quiescence. Other studies demonstrated that following irradiation, surviving MK migrate to endosteal surfaces where osteoblast (OB) lineage cells dramatically increase and promote engraftment of transplanted HSC. Here we investigated if MK directly impact hematopoiesis or whether they indirectly support HSC function through their interaction with OB-lineage cells. Our data suggests that LSK (Lin-Sca+CD117+, an enriched HSC population) co-cultured with MK and OB generate significantly higher numbers of colony forming cells (HSC function) compared to LSK cocultured with either MK or OB alone. The functionality of this in vitro data was confirmed in vivo with transplantation studies which showed increased engraftment in mice transplanted with LSK cells co-cultured with OB and MK compared to LSK cells co-cultured with OB alone. To test if loss of MK negatively impacts osteoblastogenesis, we generated conditional knockout mice where cMpl, the receptor for the main MK growth factor, thrombopoietin (TPO), was deleted in MK (cMplfl/fl x PF4Cre). Unexpectedly, these mice exhibited a 10-fold increase in platelet numbers, megakaryocytosis, a dramatic expansion of phenotypically defined hematopoietic precursors, and a remarkable 20-fold increase in the bone volume fraction. Collectively, these data indicate that while MK modulate HSC function, this activity is in part mediated through interactions with OB and suggest a complex role for TPO and MK in HSC regulation. While work is needed to further elucidate mechanisms, understanding the coordinated interaction between MK, OB, HSC, and TPO/Mpl should inform the development of novel treatments to enhance HSC recovery following myelosuppressive injuries, as well as bone loss diseases, such as osteoporosis

    Grid-Based Atmospheric Retrievals for Reflected-Light Spectra of Exoplanets using PSGnest

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    Techniques to retrieve the atmospheric properties of exoplanets via direct observation of their reflected light have often been limited in scope due to computational constraints imposed by the forward-model calculations. We have developed a new set of techniques which significantly decreases the time required to perform a retrieval while maintaining accurate results. We constructed a grid of 1.4 million pre-computed geometric albedo spectra valued at discrete sets of parameter points. Spectra from this grid are used to produce models for a fast and efficient nested sampling routine called PSGnest. Beyond the upfront time to construct a spectral grid, the amount of time to complete a full retrieval using PSGnest is on the order of seconds to minutes using a personal computer. An extensive evaluation of the error induced from interpolating intermediate spectra from the grid indicates that this bias is insignificant compared to other retrieval error sources, with an average coefficient of determination between interpolated and true spectra of 0.998. We apply these new retrieval techniques to help constrain the optimal bandpass centers for retrieving various atmospheric and bulk parameters from a LuvEx-type mission observing several planetary archetypes. We show that spectral observations made using a 20\% bandpass centered at 0.73 microns can be used alongside our new techniques to make detections of H2OH_2O and O2O_2 without the need to increase observing time beyond what is necessary for a signal-to-noise ratio of 10. The methods introduced here will enable robust studies of the capabilities of future observatories to characterize exoplanets.Comment: 32 pages, 17 figures. Accepted for publication in The Astronomical Journa

    Winter Movements of Louisiana Pine Snakes (Pituophis ruthveni) in Texas and Louisiana

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    Despite concerns that the Louisiana Pine Snake (Pituophis ruthveni) has been extirpated from large portions of its historic range, only a limited number of studies on their movement patterns have been published. Winter movement patterns are of particular interest since it has been hypothesized that impacts of management practices would be reduced during the winter. Using radiotelemetry, we determined winter movement patterns of Louisiana Pine Snakes (11 males, 8 females) in 5 study areas (2 in Louisiana and 3 in Texas). Movements during winter (November–February) were greatly curtailed compared to the remainder of the year; however, snakes occasionally undertook substantial movements. Relocations were typically within the snake’s previous active-season home range, and movements were more frequent in the early portion of winter. All hibernation sites were within Baird’s Pocket Gopher (Geomys breviceps) burrow systems at depths ranging from 13–25 cm. Louisiana Pine Snakes did not use communal hibernacula, nor did individual snakes return to previously used sites in successive years
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