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BIOL2017ORTEGARODRIGUEZ29751 BIOL

Mercury contamination of eight taxa of shoreline spiders and possible risk to arachnivorous songbirds

Type: Graduate
Author(s): Celeste Ortega-Rodriguez Biology MacGregor Hall Biology James Kennedy Biology Kyle Lauck Biology Kirkland Polk Biology Edward Williams Biology
Advisor(s): Matt Chumchal Biology Ray Drenner Biology

Mercury (Hg) is a hazardous contaminant that can be transferred from aquatic to terrestrial environments by emerging aquatic insects. Terrestrial predators, such as spiders, that live along shorelines of water bodies may consume emerging aquatic insects and become contaminated with Hg. Mercury-contaminated spiders may pose a risk to arachnivorous songbirds. The degree to which most families of spiders are contaminated with Hg and the risk they pose to songbirds is not well understood. The objectives of this study were to determine 1) Hg concentrations in seven families of shoreline spiders, 2) if each family was connected to the aquatic food web via the consumption of emergent insects and 3) determine the risk these spiders pose to arachnivorous birds. We collected representatives from seven families of spiders along with a variety of aquatic and terrestrial plant, invertebrate, and fish samples from 10 ponds located in north Texas, USA. We used methylmercury (MeHg) concentrations in combination with stable isotopes of nitrogen (δ15N) to determine if each family of shoreline spider was connected to the aquatic food web. All spider taxa in the present study were contaminated with Hg and connected to the aquatic food chain. We calculated wildlife values for various songbirds to determine health risks that Hg-contaminated spiders may pose to songbirds. Spider based wildlife values revealed that six of the seven families of shoreline spiders examined had concentrations of MeHg high enough that they may pose a risk to arachnivorous songbirds that forage for spiders along shorelines of ponds.

(Presentation is private)

BIOL2017ROUSH11987 BIOL

Pilot study on the transport and effect of hormonally-active compounds in Texas watersheds

Type: Graduate
Author(s): Kyle Roush Biology
Advisor(s): Marlo Jeffries Biology

Globally, there is demand for increased meat production. Texas, a leader in cattle production in the United States, has met this demand utilizing confined animal feeding operations (CAFOs) containing hundreds to thousands of cattle. To increase production efficiency, cattle receive growth-promoting hormone treatments to enhance growth and increase cattle mass. These hormonally-active compounds (HACs) have been found in cattle waste, feedlot runoff, and surface waters. The ultimate goal of this project was to identify watershed characteristics that promote the transport of cattle-associated HACs to surface waters. Therefore, the objectives of this pilot study were to: 1) identify and define a study area for evaluating HACs in Texas watersheds and 2) begin preliminary assessments of HAC activity in watersheds downstream of cattle feedlots. A suitable study site was identified using satellite imagery, elevation data and the ArcGIS hydrology tool pack. Sample sites were selected within this area based on geographical features and position to CAFOs. Caged fish studies, followed by analysis of estrogen-responsive gene expression, were utilized to assess the presence and activity of HACs. Though no statistically significant alterations in estrogen-responsive gene expression metrics were observed, females from three of the four sites downstream of CAFOs experienced 2.9 to 3.7-fold and 1.9 to 5.3-fold decreases in the expression of estrogen receptor alpha and vitellogenin, respectively. This could have larger implications as previous research by Miller et al. 2007 forecasted that a 50% reduction in vitellogenin plasma concentration could result in a 41.8% decrease in average population size after one year.

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CHEM2017BODIFORD28560 CHEM

Controlled drug delivery from composites of nanostructured porous silicon and polycaprolactone

Type: Graduate
Author(s): Nelli Bodiford Chemistry & Biochemistry Steven McInnes Chemistry & Biochemistry Nico Voelcker Chemistry & Biochemistry
Advisor(s): Jeffery Coffer Chemistry & Biochemistry

The combination of inorganic porous silicon (pSi) and flexible biocompatible polymers has been shown to yield more beneficial hybrid scaffolds for tissue engineering (i.e. use of synthetic materials to facilitate healing). PSi has a variety of tunable properties, including pore size, pore volume and non-toxic degradation; the addition of a flexible polymer component provides the benefit that such a construct can easily conform to any shape of the actual site of an injury/disease, suggesting that pSi/polymer composites can be suitable candidates for localized drug delivery.
In this work, composite materials consisting of oxidized porous silicon (ox-pSi) with particle size of ~ 30 μm and pore size of 40-100 nm and thin polycaprolactone (PCL) films. PCL solid films were fabricated from an initial fibrous structure that was exposed to a temperature of 65-80 oC causing fusion of these fibers into a solid film. Ox-pSi particles were then physically embedded into PCL films, resulting in ~30-40% loading of ox-pSi (ox-pSi/PCL film). Ox-pSi particles of the composite were loaded with a model cytotoxic (anticancer) drug-camptothecin (CPT). Drug release from the ox-pSi particles alone and ox-pSi/PCL film composites was monitored fluorometrically, showing distinct release profiles for each material.
Ox-pSi/PCL film composites release a CPT payload in accordance with the Higuchi release model and showed a significant decrease in burst effect compared to ox-pSi particles only. In addition, composite evolution after 5 weeks in a given solution was examined by determining weight loss and surface morphology/composition (FESEM). Overall weight loss of the composites was less then 10% mainly attributed to pSi particles detachment and dissolution.

(Presentation is private)

CHEM2017BREWER4655 CHEM

Catalytic and Mechanistic Investigation of Three Tetra-aza Macrocyclic Iron(III) Complexes

Type: Graduate
Author(s): Samantha Brewer Chemistry & Biochemistry
Advisor(s): Kayla Green Chemistry & Biochemistry

Iron plays a pivotal role in metabolism and transport processes in nature but can also be used to accomplish important chemical transformations on the bench top; recently, iron(II) salts have been shown to catalyze direct Suzuki – Miyaura coupling of N-heterocyclic compounds and arylboronic acid derivatives in the presence of oxygen. Presented herein are three tetra-aza macrocyclic iron(III) complexes [L1Fe(III)(Cl)2]+ (L1Fe), [L2Fe(III)(Cl)2]+ (L2Fe), and [L3Fe(III)(Cl)2]+ (L3Fe) [L1 (Pyclen)=1,4,7,10-tetra-aza-2,6-pyridinophane; L2 =3,6,9,15-tetraazabicyclo[9.3.1]penta-deca-1(15),11,13-trien-13-ol; L3 =3,6,9,15-tetra-azabicyclo[9.3.1]penta-deca-1(15),11,13-trien-12-ol] that catalyze the coupling of pyrrole and phenylboronic acid. Following the synthesis and reactivity studies, investigation into the oxidation state of the iron center throughout the catalytic cycle was explored. The results of this work to date will be presented and will facilitate the understanding of challenging chemical reactions catalyzed using inexpensive earth abundant metals such as iron.

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CHEM2017DACHILLE1815 CHEM

Suppression of Melanin Synthesis by Europium Doped Cerium Oxide Nanomaterials

Type: Graduate
Author(s): Anne D'Achille Chemistry & Biochemistry
Advisor(s): Jeffery Coffer Chemistry & Biochemistry

Nanomaterials based on cerium (IV) oxide, CeO2, have been extensively investigated due to interesting chemistry from a readily available transition between Ce3+ and Ce4+. Oxygen vacancies present in the oxide lattice combined with the available redox transition gives CeO2 materials antioxidant and enzyme mimetic behavior. The addition of tri-valent, fluorescent ions such as Eu3+ further increase the oxygen vacancy concentration, may allow control over the Ce3+/Ce4+ ratio, and may add fluorescence to the doped material. These properties give europium doped cerium oxide (EuCeO¬2) potential applications within biological systems.
Eumelanin is a complex dark brown pigment originating from the oxidation and oligomerization of tyrosine. The pigment can also be synthesized through the auto-oxidation of L-3,4-dihydroxyphenylalanine (L-DOPA). While its structure has not been fully determined, eumelanin has shown antioxidant and free-radical scavenging behavior, strong UV-VIS absorption, and conductive properties. The pigment has been researched for its radiation damage protection, and for activity against amyloids associated with Parkinson’s and Alzheimer’s disease.
Our research thus far has focused on the controlled synthesis of various EuCeO2 nanomaterials, and their interaction with the auto-oxidation of L-DOPA to eumelanin as measured through the observation of eumelanin fluorescence at 471 nm. Nanorods, nanowires, and nanocubes of EuCeO2 were each synthesized with a range of dimensions and europium content. EuCeO2 nanorods and nanocubes were synthesized through precipitation of EuCe(OH)3 and a subsequent hydrothermal reaction between 100°C and 180°C. Nanowires were synthesized using electrospinning and annealing techniques. All materials were analyzed using transmission electron microscopy (TEM), energy dispersive x-ray analysis (EDX), and powder x-ray diffraction (XRD).
The presence of CeO2 or EuCeO2 materials in L-DOPA containing solutions consistently suppressed the eumelanin-associated fluorescence intensity. Various parameters, including temperature, pH, nanomaterial concentration and morphology, and europium doping concentration have been evaluated for their potential impact on the evolution of eumelanin from L-DOPA in the presence of these EuCeO2 nanomaterials.

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CHEM2017KALLURI41876 CHEM

Plant based nanotechnology for drug delivery and anti-inflammatory therapy

Type: Graduate
Author(s): Jhansi Kalluri Chemistry & Biochemistry Giridhar Akkaraju Biology Jeffery Coffer Chemistry & Biochemistry Julianna West Biology
Advisor(s): Jeffery Coffer Chemistry & Biochemistry

Plant based nanotechnology for drug delivery and anti-inflammatory therapy
Jhansi Kalluri, Julianna West, Giridhar Akkaraju, Leigh Canhm and Jeffery L. Coffer*
Abstract:
Chronic inflammation is one of the characteristics of Alzheimer’s, cancer, and selected auto inflammatory diseases. Medicinal plant extracts rich in polyphenols have shown the ability to aid in the prevention of degenerative diseases such as Alzheimer’s due to their anti-inflammatory and anti-oxidant properties. One of the problems of using polyphenols to treat these diseases is their potentially low bioavailability and short half-life in vivo. An alternative to using free compound is to use plant polyphenol-loaded nano/micro particles to increase their bioavailability and half-life.
Equisetum arvense is a silicon accumulator plant serving as a source for a viable eco-friendly route for fabricating nanostructured porous silicon (pSi) drug delivery carriers; at the same time, if selected plant components contain medicinally-active species as well, then the single substance can provide not only the nanoscale high surface area drug delivery carrier (pSi), but the drug itself. With this idea in mind, porous silicon was fabricated from stems/fronds of the silicon accumulator plant Equisetum arvense and the anti-inflammatory activity of the leaf components (aqueous ethanol extract) of Equisetum arvense was tested using a luciferase assay. We evaluated the dose dependent activity of the extract to inhibit TNF-induced NF- kB activation. Our long-term goal is to measure the anti-inflammatory activity of extract-loaded porous silicon particles in a sustained manner.

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CHEM2017LE35834 CHEM

Silicon Nanotubes as Drug Delivery Vectors

Type: Graduate
Author(s): Nguyen Le Chemistry & Biochemistry
Advisor(s): Jeffery Coffer Chemistry & Biochemistry

Semiconducting silicon (Si) is a promising element that has been extensively studied in various fields ranging from microelectronics to bio-relevant applications.1 In fact, nanostructured porous silicon has received widespread attention due to its unique chemical and physical characteristics.1 Another relatively more well-defined example of nanostructured silicon is Si nanotubes (SiNTs) with well-characterized sidewalls, inner void space and lengths, allowing opportunities to study its potential properties in diverse fields, such as Li ion batteries, solar cells.2,3 In particular, SiNTs are potential vectors in drug delivery systems. The available interior free space of the NTs offer the material the ability of confining a desired amount of payload of therapeutic agents. Moreover, the available silanol groups on the surface of the NTs also enable attachment to a linker, whose other end is subsequently attached to a drug molecule of interests. Within a biological environment, therapeutic molecules of interest can be released in a sustained manner into targeted sites through either dissolution of the SiNT carriers or their detachment from the linkers.
In terms of therapeutic candidates, cisplatin has been renowned for its ability to treat a variety of cancers including lymphomas, carcinomas, etc. Due to low chloride ions concentrations (4-12mM) in the intracellular environment of cancer cells, chloride ligands on cisplatin are readily displaced by water, producing either cis-[PtCl(NH3)2(H2O)]+ or cis-[Pt(NH3)2(H2O)2]2+ aquo complexes, which actively target DNA and trigger apoptosis.4 However, since drug resistance is developed in cancer cells and undesirable interactions between cisplatin and other biological molecules occur, the therapeutic effects become diminished and negative side effects are also observed.5,6 In order to enhance the therapeutic efficiency of cisplatin, in this project, SiNTs are employed as carriers that can be loaded with cisplatin and potentially deliver the drugs to the desired sites. For the purpose of controlling the release of cisplatin from SiNTs, 3-aminopropyltriethoxysilane (APTES) is employed as the linker, which can covalently bind to the nanotubes through the available silanol groups on the surface, and the amino group on the other end of APTES can subsequently coordinate cisplatin.
In this study, SiNTs with lengths less than 1 µm are used (for optimal cellular uptake), and a sidewall thickness ~ 10 nm for desirable dissolution within a biological environment. Moreover, the distinct porous morphology of the nanotubes permits infiltration of the molecules of interest. By varying solvents (acetone and toluene) of APTES solution and functionalization time, the amount of cisplatin loaded into SiNTs can be modulated ranging from 20-40 weight %, thereby suggesting the ability of SiNTs to carry therapeutic agents.
References
1. Canham, L.T. Hanbook of Porous Silicon. Switzerland: Springer International Publishing AG, 2014.
2. Tesfaye A, Gonzalez R., Coffer J., Djenizian T. Porous Silicon Nanotube Arrays as Anode Material for Li-Ion Batteries, ACS Appl Mater. Inter. 2015, 7, 20495−20498.
3. Gonzalez-Rodriguez R., Arad-Vosk N., Rozenfeld N, Sa’ar A, Coffer JL (2016) Control of CH3NH3 PbI3 Perovskite Nanostructure Formation through the Use of Silicon Nanotube Templates, Small 2016, 12, 4477–4480.
4. Ma P., Xiao H., Li C., Dai Y., Cheng Z., Hou Z., Lin J. Inorganic nanocarriers for platinum drug delivery, Materials Today 2015, 18(10), 554-564.
5. Martin L.P., Hamilton T.C., Schilder R.J. Platinum Resistance: The Role of DNA Repair Pathways, Clin Cancer Res. 2008, 14(5):1291-1295.
6. Xue X., You S., Zhang Q., Wu Y., Zou G., Wang P. C., Zhao Y., Xu Y., Jia L., Zhang X., Liang X. Mitaplatin Increases Sensitivity of Tumor Cells to Cisplatin by Inducing Mitochondrial Dysfunction, Mol. Pharmaceutics, 2012, 9 (3), 634–644.

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CHEM2017OCHOA7485 CHEM

Intramolecular deMayo photocyclization: The total synthesis of hippadine and pratosine

Type: Graduate
Author(s): Charles Ochoa Chemistry & Biochemistry
Advisor(s): David Minter Chemistry & Biochemistry

Various total syntheses of the Lycorine-type pharmacologically active alkaloids hippadine and pratosine have been developed. However, most of these synthetic routes require prohibitively expensive materials and/or achieve yields that are subpar, making these schemes unlikely to be used in an industrial setting. Current research involves developing better synthetic methods for these two alkaloids starting with a 6,7-disubstituted isoquinoline. These syntheses are appealing since they utilize readily available starting materials and avoid expensive catalysts. The key step in the synthetic scheme centers around an intramolecular de Mayo photocyclization which involves a reaction between an alkene moiety in the isocarbostyril system and a 1,3-diketone (a functionalized tether on nitrogen), which forms a third ring in the structure of the molecule. Research on a model system (an isocarbostyril without the substituents at positions 6 and 7) for these natural products has been done in order to elucidate the optimal conditions for each step on the synthetic strategy. Initial attempts were made in order to synthesize the 6,7-disubstituted isocarbostyril with the 1,3-diketone tether so that the deMayo photocyclization could be performed. However, the established synthetic strategy led to compounds along the synthetic route that had very undesirable solubility properties. To resolve this issue, the substituents were replaced with bulkier, more non-polar moieties in order to increase the solubility of the compound in ethyl ether.

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GEOL2017ANDREWS23076 GEOL

Intermixed Hawaiian, Strombolian and phreatomagmatic pyroclastic deposits in a Mesoproterozoic volcanic arc sequence (Barby Formation), southwest Namibia

Type: Graduate
Author(s): Virginia Andrews Geological Sciences
Advisor(s): Richard Hanson Geological Sciences

The Barby Formation makes up part of the Konkiep Terrane, which is a major Mesoproterozoic arc complex along the Kalahari craton margin in southwest Namibia. Previous mapping indicates that the Barby Formation contains a laterally and vertically complex series of basaltic to rhyolitic lavas, rhyolitic ignimbrites, and associated hypabyssal intrusions. Our new work shows that significant basaltic to andesitic pyroclastic successions are also present within the unit and record a wide variation in eruption styles.

Detailed mapping reveals the presence of Hawaiian, Strombolian and phreatomagmatic pyroclastic deposits forming successions up to X m thick emplaced close to source vents and intercalated with fine-grained lacustrine strata in an area ~20 km2. The most abundant deposits consist of basaltic to andesitic spatter accumulations formed from vigorous lava fountains during Hawaiian-style eruptions. These sequences show random vertical transitions on the scale of a few meters from moderately agglutinated to densely welded spatter, which reflect variations in pyroclast accumulation rates. Individual spatter pieces are up to x cm long. The densely welded spatter forms lava-like units, but we see no evidence of clastogenic lava flows. Sequences of basaltic lapillistone with dispersed ribbon and fusiform bombs up to 50 cm across record Strombolian eruptions during episodes of lower magma flux without involvement of external water. The spatter accumulations typically grade upward into phreatomagmatic deposits containing minor amounts of spatter and cauliflower bombs mixed with poorly vesicular lapilli tuff, in which particle shapes are controlled mostly by fracture surfaces rather than broken bubble walls; up to 30% lacustrine sediment is intermixed with juvenile lapilli and ash in these deposits. We infer that changes in eruptive style in this part of the arc sequence were controlled at least partly by variations in magma ascent rates at shallow depths, as documented in numerous other volcanic provinces. Transitions from Hawaiian to phreatomagmatic eruptions may at least partly reflect a decrease in magma flux in the presence of external water, lowering the magma-to-water mass ratio so that hydrovolcanic explosions became possible.

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GEOL2017GOMEZ40480 GEOL

PROVENANCE OF CENOZOIC CLASTIC SEDIMENTS IN THE TACHIRA SADDLE, WESTERN VENEZUELA, AND IMPLICATIONS OF SEDIMENT DISPERSAL PATTERNS IN THE NORTHERN ANDES

Type: Graduate
Author(s): Ali Ricardo Gomez Geological Sciences
Advisor(s): Xiangyang Xie Geological Sciences

Northwestern South America is highly deformed due to the transpressive boundary with complex interactions among the Caribbean plate, the South American plate, the Nazca plate and the Panama arc. Previous studies suggest that the Cenozoic uplifting of the Mérida Andes and Eastern Cordillera of Colombia affected sediment dispersal patterns in the region, shifting from a Paleocene foreland basin configuration with an axial major fluvial system, to the modern configuration of isolated basins with distinctive sediment dispersal patterns. Well-exposed Cretaceous to Pliocene strata in the Táchira saddle between the Easter Cordillera and Merida Andes provide a unique opportunity to test proposed sediment dispersal patterns in the region. U-Pb detrital zircon geochronology and supplementary XRD heavy mineral identification were used together to document provenance of Cretaceous to Pliocene clastic rocks collected from the area of La Alquitrana. Results from the U-Pb detrital zircon geochronology show that there are six age groups recorded in this samples. Two groups related with Precambrian Guyana shield Terranes and Putumayo basement in the Eastern Cordillera, and four groups related to different magmatic episodes during the Andean Orogenic process. Three major paleogeography changes were also recorded in these detrital signatures, including a transition between the Cretaceous passive margin and the Paleocene foreland basin, the initial uplifting of the Eastern Cordillera with the isolation the Llanos Basin and Táchira Saddle from the Central Cordillera and the Magdalena Valley in the Early Oligocene, and the uplifting of the Mérida Andes by the Early Miocene. The outcomes of this study emphasize the importance of the Mérida Andes and Eastern Cordillera Uplift in controlling the evolution of the sediment dispersal patterns in northern South America and represent a contribution in the understanding of the paleogeographic evolution in the region.

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GEOL2017HOWE26318 GEOL

The Architecture and Connective Potential of Blowout Wings in Fluvio-Deltaic Environments

Type: Graduate
Author(s): Tyler Howe Geological Sciences
Advisor(s): John Holbrook Geological Sciences

Fluvio-lacustrine systems are prone to experiencing significant flood events separated by longer low energy periods. During low flow, sediment is stored upstream of the lake as mid-channel and side-attached bars. During high-discharge events, water level rises above the topographically low delta front levees, the turbulent jet of the river is positioned upstream of the levee terminus where levees are less confining, and the previously stored sediment is flushed from the channel into the lake basin laterally as sheets. This process forms a laterally extensive, well sorted wedge shaped deposit of fine grained sand called a blowout wing (after Tomanka, 2013). These wings are documented in the ancient within the Kayenta Formation, UT, where the sand wings demonstrated a significant increase in connectivity between statistically clustered fluvio-lacustrine channel belts. In this research, we document two examples of blowout wings forming in the modern. The first example is a lake sourced by a mud dominated river (Denton Creek, Lake Grapevine, TX), and the second is a lake sourced by a sandy, bedload dominated river (Red River, Lake Texoma, TX). Wings are composed of fine to medium grained, well sorted, and clean sand. The deposits are thin and laterally continuous, with measured thicknesses of 5-10 cm that thin away from channel axis. Wings have an aerial extent up several hundred meters, scaling to 4-6 times the channel width. The Red River at Lake Texoma has a channel width of 125m and deposits wings with an aerial extent of 250-350m long along the levee of the delta channel and 300-500m laterally. As the Red River has prograded into the basin, 5-6 individual blowout wings form a wing complex 1500m long and 500-600m laterally from the channel. Denton Creek at Lake Grapevine has a channel width of 25m and deposits wings on the order of 50-125m along the levee of the delta channel and 60-150m laterally. Three wings at Lake Grapevine form a wing complex 300m long and 100-150m laterally. The amalgamation and statistical clustering of fluvio-deltaic channel belts is increased by the presence of blowout wings, resulting in higher total reservoir size and connectivity. Blowout wings should be, and are, found in modern systems and subsequently the rock record recording fluvio-lacustrine environments of deposition.

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GEOL2017MCGREGOR60725 GEOL

Humid terminal splays as sand-sheet reservoirs: A first look at the modern, Andean foreland, and a new look at the ancient, Raton Basin

Type: Graduate
Author(s): Graham McGregor Geological Sciences
Advisor(s): John Holbrook Geological Sciences

Thin sand sheets presumed to be terminal splay bodies have potential to serve as hydrocarbon reservoirs. The few studies of terminal splays managed from arid systems has provided insight, but ground study of the humid equivalent is lacking. Deposited in the distal zone of a distributary fluvial system (DFS), the splay bodies are formed as rivers terminate from loss of slope into unconfined dispersive flow and deposit bed load as splays and advect mud to more distal floodplains. The splay sheets and floodplain together provide potential for both reservoir and seal. We examined terminal splay deposits in a modern humid terminal splay system, Andean foreland of northern Argentina, and in ancient foreland deposits, Paleocene Raton Formation of the Colorado Raton Basin. I am going to compare the two locations in terms of grain-size, sedimentary structures, geometry, and scale and see how they relate. I hypothesize that the two are going to have similar grain sizes, and that the sedimentary structures and geometries will also be analogous but expect them to be scaled down in the Raton Basin.
The modern splay in Argentina is nearly 1.3 km wide and 1.9 km long and was deposited during a single large flood in 2012. Cross sections generated by hand augers show a maximum thickness of 0.8 m, an average of 0.5 m, and a consistently very fine-grained to lower medium-grained sand texture throughout. Total sand deposited in the flood event is ~ 1.2 million cubic meters (~2.0 million cubic meter maximum), and accumulates over earlier splay deposits separated by weakly developed soils that are locally removed by splay incision. Subsequent dissection of the splay permits examination of sedimentary structures, which are dominantly climbing ripples, planar laminations, and cross sets, but climbing antidunes are locally found near the splay apex. Ancient terminal splays of the Raton Formation are made of thinner sand sheets (~0.25 m) and tend to have thicker muddy floodplain deposits between. Grain-size distribution, sheet geometry, and sedimentary structures however are consistent between the modern and ancient examples. Both the Argentina and Raton examples reflect the distal end of a humid Distributive Fluvial System, however, the Raton system appears to have been of smaller scale. This is consistent with the comparatively smaller scale of the Raton vs. Andean tectonic system.

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GEOL2017MCGUIRE35162 GEOL

U-Pb Detrital Zircon Signature of the Ouachita Orogenic Belt

Type: Graduate
Author(s): Preston McGuire Geological Sciences
Advisor(s): Xaingyang Xie Geological Sciences

The Late Paleozoic Ouachita fold-and-thrust belt extends from the southern terminus of the Appalachian thrust belt in eastern Mississippi up through central Arkansas, southeastern Oklahoma, and Texas terminating in northeastern Mexico. A series of Carboniferous foreland basins were formed sequentially to the thrust front. The interaction between the Laurentian craton and the Appalachian-Ouachita orogenic belts controlled sedimentation in the southern midcontinent region throughout the Paleozoic. In contrast to the Appalachian orogenic belt to the east, the Ouachita orogenic belt and associated sediments remain poorly documented and less constrained.
In this study, seven Ordovician to Mississippian aged clastic units from the Ouachita Mountain in central Arkansas were sampled and tested using U-Pb detrital zircon geochronology. Three major age peaks are prominent, including the Grenville Province (~0.95-1.2 Ga), the Granite-Rhyolite Province (~1.3-1.5 Ga), and the Superior Province (>~2.5 Ga) in Ordovician to Silurian aged rocks. A change in this signature becomes clear at the beginning of the Carboniferous from Early Mississippian Stanley Group samples showing the additional Paleozoic age peak (~490-520 Ma) potentially derived from the Appalachian orogenic belt to the east, and/or from peri-Gondwanan terranes accreted to Laurentia just before the collision with Gondwana. This stratigraphic variation of detrital zircon age signature suggests that the transition from a passive to an active margin in the Ouachita trough started, at the latest, in early Mississippian times. Results of this study is the first systematic study of the U-Pb detrital zircon signature of the Ouachita orogenic belt and have important implications in sediment dispersal, provenance interpretations, and paleogeography reconstructions in North America, especially in the southern mid-continent and surrounding areas.

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GEOL2017WILLIAMS23742 GEOL

FRACTURE ANALYSIS AND MAPPING OF THE CRETACEOUS BOQUILLAS FORMATION, BLACK GAP WILDLIFE MANANGEMENT AREA, BREWSTER COUNTY, TX

Type: Graduate
Author(s): John Williams Geological Sciences
Advisor(s): Helge Alsleben Geological Sciences

The Eagle Ford Shale in south Texas is one of the most prolific unconventional hydrocarbon plays in the world (Breyer, 2016). In 2015, natural gas and oil from this field hit peak production numbers at 5,539 MMcf (million cubic feet) and 1,118,648 Bbl (barrels) per day, respectively (Texas RRC, 2016).  In order for this low-permeability formation to produce, companies are using hydraulic fracturing, a stimulation treatment used in low-permeability rock whereby fluids are pumped at high pressures into reservoirs, causing new fractures to form and possibly reactivating existing fractures (Schlumberger, 2016).  The aim of this study is to identify any geomechanical and geochemical properties that optimize fracture connectivity within the Boquillas Formation, the West Texas Eagle Ford equivalent.  Energy-dispersive x-ray fluorescence (ED-XRF) and strength/hardness data from this study suggests that fracture frequency and length are affected by the clay and calcium carbonate content, and, by inference, the strength of the rock.

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MATH2017HELLERMAN41492 MATH

Winding Numbers and Toeplitz Operators

Type: Graduate
Author(s): Nathanael Hellerman Mathematics
Advisor(s): Efton Park Mathematics

The winding number of a continuous function on the unit circle counts how many times a graph of the function loops around the origin. It is homotopy invariant and has applications to several areas of Mathematics.
Toeplitz operators with continuous symbol are bounded linear operators on the Hardy Space involving multiplication by a continuous function. The index of such a Toeplitz operator is closely connected to the winding number of its symbol.
This connection is examined and then extended for Toeplitz operators with crossed product symbols.

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MATH2017SMITH36813 MATH

Indices of Algebraic Integers in Cubic Fields

Type: Graduate
Author(s): Jeremy Smith Mathematics
Advisor(s): George Gilbert Mathematics

An algebraic integer is a complex number that is a root of a monic polynomial with integer coefficients. It is well-known that there is not always a single algebraic integer that can generate the ring of algebraic integers contained in a field extension of the rational numbers. The index of an algebraic integer is a natural number that measures how far a ring of integers is from having such a "primitive element." We investigate these indices in cubic fields and determine which natural numbers occur as indices in given families.

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PHYS2017CIAMPA7324 PHYS

Supernovae in Large Magellanic Cloud Drive Massive Winds Toward Milky Way Galaxy

Type: Graduate
Author(s): Drew Ciampa Physics & Astronomy
Advisor(s): Kat Barger Physics & Astronomy

Located inside the Large Magellanic Cloud, fierce explosions called supernovae have thrown out massive amounts of gas in every direction. A portion of this gas is aimed toward the Milky Way and is on a crash course with our galaxy. We are observing this gas with the Wisconsin H-Alpha Mapper, which provides a window into how the gas is distributed. These observations show two periods of supernovae explosions that created two distinct gas winds. One of these winds is currently active while the other was produced roughly 300 Million years old. Studying these gas clouds will provide information on how massive these winds are and the rate at which they are produced. The ejected gas is headed toward the Milky Way could supply our galaxy with additional gas to form stars in the future.

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PHYS2017HASAN32286 PHYS

Tuning the Optical Band Gap of Graphene Oxide by Ozone Treatment

Type: Graduate
Author(s): Md Tanvir Hasan Physics & Astronomy Roberto Gonzalez-Rodriguez Chemistry & Biochemistry Anton Naumov Physics & Astronomy Conor Ryan Physics & Astronomy Brian Senger Physics & Astronomy
Advisor(s): Anton Naumov Physics & Astronomy

Graphene oxide (GO) inherits high transparency, substantial conductivity, high tensile strength from its parent materials graphene. Apart from these properties, it emits fluorescence which makes it a potential material to use in optoelectronics and bio-sensing applications. In this work, we have utilized systematic ozone treatment to alter the optical band gap of single-layered graphene oxide in aqueous suspensions. Due to controlled ozonation, additional functionalization takes place in GO graphitic sheet which changes GO electronic structure. This is confirmed by the increase in vibrational transitions of a number of oxygen-containing functional groups with treatment and the appearance of the prominent carboxylic group feature at c.a. 1700 1/cm. Albeit, timed ozone induction introduces only slight change in color and absorption spectra of GO samples, the emission spectra show a gradual increase in intensity with a significant blue shift up to 100 nm from deep red to green. This large blue shift suggests an increase in optical band gap with additional functionalization introduced by ozone treatment. We utilize a semi-empirical theoretical approach to describe the effects of functionalization-induced changes. This model attributes the origins of fluorescence emission to the quantum confined sp² carbon islands in GO encircled by the functional groups. As we decrease the graphitic carbon cluster size on the GO sheet, the optical bandgap calculated via HyperChem molecular modeling increases, which supports the experimentally observed blue shifts in emission. This theoretical result is further supported by the TEM measurement of ozone-treated samples, which shows a decreasing trend of average ordered graphitic carbon cluster size on GO sheets with treatment time. Theoretical modeling, as well as the experimental results, indicate that the optical bandgap and emission intensity of GO are alterable with controlled ozone treatment, which allows tailoring the optical properties of GO for specific applications in optoelectronics and bio-sensing.

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PHYS2017MELENDEZ16706 PHYS

The Open Cluster Chemical Abundances and Mapping (OCCAM) Survey: Optical Extension for Neutron Capture Elements

Type: Graduate
Author(s): Matthew Melendez Physics & Astronomy John Donor Physics & Astronomy Peter Frinchaboy Physics & Astronomy Julia O'Connell Physics & Astronomy
Advisor(s): Peter Frinchaboy Physics & Astronomy

The Open Cluster Chemical Abundances and Mapping (OCCAM) survey is a systematic survey of Galactic open clusters using data primarily from the SDSS-III/APOGEE-1 survey. However, neutron capture elements are limited in the IR region covered by APOGEE. In an effort to fully study detailed Galactic chemical evolution, we are conducting a high resolution (R~60,000) spectroscopic abundance analysis of neutron capture elements for OCCAM clusters in the optical regime to complement the APOGEE results. As part of this effort, we present Ba II, La II, Ce II and Eu II results for a few open clusters without previous abundance measurements using data obtained at McDonald Observatory with the 2.1 m Otto Struve telescope and Sandiford Echelle Spectrograph.

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PHYS2017RAY20657 PHYS

A Survey of Nearby M-dwarfs with Robo-AO

Type: Graduate
Author(s): Amy Ray Physics & Astronomy Angelle Tanner Physics & Astronomy
Advisor(s): Peter Frinchaboy Physics & Astronomy

The goal of this study was to conduct a survey of 913 M-dwarf stars from the Lepine and Shara Proper Motion(LSPM) catalog within 33 parsecs. This research was conducted to improve upon the statistics of nearby multiple M-dwarf star systems. Identifying and confirming multiple systems at both wide and small separations will expand understanding of M-dwarf formation by comparing these results to existing star formation models. Data for these targets was collected with the Robo-AO camera on the Palomar 60in telescope. Separation and position angles were determined and compared for two epochs of the images containing multiple stars, one taken in 2012 and the other taken in 2014, to look for changes in these values. Stars with little change in position with respect to one another suggest they are common proper motion pairs. The Washington Double Star(WDS) catalog and other resources were used to further determine binarity. There were 50 multiple star system candidates found with a multiplicity fraction of 28.6±3.0 and a companion star fraction of 34.7±2.1.

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PHYS2017SUN7458 PHYS

Star formation in galaxies

Type: Graduate
Author(s): Jing Sun Physics & Astronomy
Advisor(s): Kat Barger Physics & Astronomy

A galaxy environment influences its internal properties. All galaxies start out small and grow bigger after merging with other galaxies. We are conducting a statistical study on isolated and interacting galaxies to determine how their environment impacts on their star-formation ability. We are using observations from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, which has already observed more than 3000 galaxies. We are examining the differences and similarities of the gas and stars in isolated and interacting galaxies to explore their past and current star formation activity. From these comparisons, we will identify which conditions promote and hinder star formation to learn how different types of galaxies evolved. An example of an isolated galaxy is shown here.

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