Text and context : an examination of the way in which John's prologue has been interpreted by selected writers : Origen, Luther and Bultmann

In chapter one of this work, as a preliminary to the formulation of the question that this thesis will attempt to answer, the changing understanding of the part played by the interpreter in the process of interpretation is discussed. This outline begins with the understanding of the role of the interpreter in liberal theology - where he is thought of as one who applies critical methods to the text in a detached and scientific way. After this the hermeneutic spiral is discussed - the formation of this model acknowledges to a greater degree the individual and human part played by the interpreter. This is followed by a brief examination of the most recent theories of interpretation in which meaning is regarded as residing not in the text but in the interpreter himself. The task of this thesis is to determine whether, as these recent theorists suggest, the reader creates meaning instead of reading out what somehow lies in the text itself. The task of this thesis is to ascertain, by studying the interpretationsof John's Prologue by Origen, Luther and Bultmann, whether the text does in fact operate as a series of sign-posts that pOint the interpreter to a destination within his own semantic universe. This may be determined by noting whether or not the contexts, i n the broadest sense, of these interpreters have played a formative part in their interpretations. contextual influences are regarded as existing wherever there is a procedure or meaning in the interpreter's commentary which one expe cts to find there as a result of one's knowledge of the interpreter's life and previous writings. Our research reveals that Orige n, Luther and Bultmann have produced three very different commentaries in which the common denominator is the formative influence of the interpreter's context. Each of these writers has produced an interpretation that is consistent, in both approach and theology, with their previous exegetical and theological thought. This indicates that contextual factors have played a significant part in determining their interpr etations of John 1 :1-18. It would appear that these interpreters have been led to find the meaning of John's Prologue not with reference to any new, unprecedented set of symbols, but with reference to their own, well-worn semantic universes. In the conclusion it is noted that this research appears to support what many modern theorists have said as to the locus of meaning in interpretation. In the conclusion it is also noted that many of the fears raised by these findings - that readers and writers, or speakers and hearers, may become so isolated and trapped in their own thought worlds that any real contact with the outside is impossible - may be groundless. These findings also point to a certain consistency between the interpreters and their communities. This refutes the fears as to the isolation and solitary development of the individual in that it points to a certain community or corporate aspect which plays a part in the development of the indivi dual's semantic universe .KMBT_363Adobe Acrobat 9.53 Paper Capture Plug-i

Between freedom and givenness: (a study of the hermeneutical consequences of the concept of canon for the authority of scripture)

The aim of this thesis is to arrive at an understanding of the authority of scripture that is able to accommodate both a faith perspective and the fruits of the historical-critical approach to the New Testament. Put differently, the aim of this thesis is the pursuit of a specifically christian, faith-promoting, reading of the New Testament whilst still enjoying the benefit, in an as uncompromised a form as possible, of the historical- critical approach. In a sense it may be said that this task, given that the roots of both the historical-critical approach and modern Western culture are deeply imbedded in Rationalism, is equivalent to the basic hermeneutical question of whether it is possible to interpret scripture relevantly from within a cultural web of meaning that does not readily accommodate that embodied in the New Testament. In section one of this dissertation we present a characteristic depiction, based on the historical-critical theory of literature, of the authority of the New Testament. This is followed by a brief assessment that makes explicit why the historical- critical approach is not conducive to the adoption of a faith perspective on these writings. In section two, still and inevitably based on critical foundations, we adopt a perspective that is more sympathetic to faith and that seeks to discover in the concerns evidenced in the canonical process, when traditions about Jesus gradually took on more complex and stable forms, culminating in the canon of the New Testament, guidelines in helping us to deal with the problem with which this study is concerned . In the specific example of the rather ordinary concerns underlying the unusual history of the pericope de adultera (John 7:53-8:11), examined against the background of the interests underlying the canonical process, it becomes clear that christians from the very beginning faced a dilemma not unlike that with which the historical-critical approach confronts us. They had to interpret afresh, and faithfully, the traditions in order to meet the demands of situations that had never been foreseen by earlier tradents. In this respect, therefore, the history of the pericope de adultera presents us with an ongoing struggle to hold in tension the demands of new contexts with the imperative of strict continuity with Jesus. In section three, on the basis of the foundation of the authority of scripture in strict continuity with Jesus combined with the contextual reinterpretation of the tradition, the social sciences are employed. Using the social sciences, it is discovered that the two contradictory approaches that we wish to reconcile form part of two different models for interpreting reality. It is on this basis, and made possible by the common culture underlying these opposing models and by the common contact with an unspecified common core of concrete reality, that a solution is proposed in terms of a complex 'fusion of horizons', promoted by a 'precipitative environment'. In the conclusion our solution is decisively aligned with the concerns evidenced in the canonical proces

The Mutational Consequences of Plant Transformation

Plant transformation is a genetic engineering tool for introducing transgenes into plant genomes. It is now being used for the breeding of commercial crops. A central feature of transformation is insertion of the transgene into plant chromosomal DNA. Transgene insertion is infrequently, if ever, a precise event. Mutations found at transgene insertion sites include deletions and rearrangements of host chromosomal DNA and introduction of superfluous DNA. Insertion sites introduced using Agrobacterium tumefaciens tend to have simpler structures but can be associated with extensive chromosomal rearrangements, while those of particle bombardment appear invariably to be associated with deletion and extensive scrambling of inserted and chromosomal DNA. Ancillary procedures associated with plant transformation, including tissue culture and infection with A tumefaciens, can also introduce mutations. These genome-wide mutations can number from hundreds to many thousands per diploid genome. Despite the fact that confidence in the safety and dependability of crop species rests significantly on their genetic integrity, the frequency of transformation-induced mutations and their importance as potential biosafety hazards are poorly understood

Targeted and all-sky search for nanosecond optical pulses at Harvard-Smithsonian

We have built a system to detect nanosecond pulsed optical signals from a target list of some 10,000 sun-like stars, and have made some 20,000 observations during its two years of operation. A beamsplitter feeds a pair of hybrid avalanche photodetectors at the focal plane of the 1.5m Cassegrain at the Harvard/Smithsonian Oak Ridge Observatory (Agassiz Station), with a coincidence triggering measurement of pulse width and intensity at sub-nanosecond resolution. A flexible web-enabled database, combined with mercifully low background coincidence rates (approximately 1 event per night), makes it easy to sort through far-flung data in search of repeated events from any candidate star. An identical system will soon begin observations, synchronized with ours, at the 0.9m Cassegrain at Princeton University. These will permit unambiguous identification of even a solitary pulse. We are planning an all-sky search for optical pulses, using a dedicated 1.8m f/2.4 spherical glass light bucket and an array of pixelated photomultipliers deployed in a pair of matched focal planes. The sky pixels, 1.5 arcmin square, tessellate a 1.6 by 0.2 degree patch of sky in transit mode, covering the Northern sky in approximately 150 clear nights. Fast custom IC electronics will monitor corresponding pixels for coincident optical pulses of nanosecond timescale, triggering storage of a digitized waveform of the light flash

Discovery and Precise Characterization by the MEarth Project of LP 661-13, an Eclipsing Binary Consisting of Two Fully Convective Low-mass Stars

We report the detection of stellar eclipses in the LP 661-13 system. We present the discovery and characterization of this system, including high resolution spectroscopic radial velocities and a photometric solution spanning two observing seasons. LP 661-13 is a low mass binary system with an orbital period of $4.7043512^{+0.0000013}_{-0.0000010}$ days at a distance of $24.9 \pm 1.3$ parsecs. LP 661-13A is a $0.30795 \pm 0.00084$ $M_\odot$ star while LP 661-13B is a $0.19400 \pm 0.00034$ $M_\odot$ star. The radius of each component is $0.3226 \pm 0.0033$ $R_\odot$ and $0.2174 \pm 0.0023$ $R_\odot$, respectively. We detect out of eclipse modulations at a period slightly shorter than the orbital period, implying that at least one of the components is not rotating synchronously. We find that each component is slightly inflated compared to stellar models, and that this cannot be reconciled through age or metallicity effects. As a nearby eclipsing binary system where both components are near or below the full-convection limit, LP 661-13 will be a valuable test of models for the structure of cool dwarf stars.Comment: 24 pages, 8 tables, 6 figures. Submitted to ApJ, comments welcom

Traffic of p24 Proteins and COPII Coat Composition Mutually Influence Membrane Scaffolding

SummaryEukaryotic protein secretion requires efficient and accurate delivery of diverse secretory and membrane proteins. This process initiates in the ER, where vesicles are sculpted by the essential COPII coat. The Sec13p subunit of the COPII coat contributes to membrane scaffolding, which enforces curvature on the nascent vesicle. A requirement for Sec13p can be bypassed when traffic of lumenally oriented membrane proteins is abrogated. Here we sought to further explore the impact of cargo proteins on vesicle formation. We show that efficient ER export of the p24 family of proteins is a major driver of the requirement for Sec13p. The scaffolding burden presented by the p24 complex is met in part by the cargo adaptor Lst1p, which binds to a subset of cargo, including the p24 proteins. We propose that the scaffolding function of Lst1p is required to generate vesicles that can accommodate difficult cargo proteins that include large oligomeric assemblies and asymmetrically distributed membrane proteins. Vesicles that contain such cargoes are also more dependent on scaffolding by Sec13p, and may serve as a model for large carrier formation in other systems

The atmospheres of the hot-Jupiters Kepler-5b and Kepler-6b observed during occultations with Warm-Spitzer and Kepler

This paper reports the detection and the measurements of occultations of the two transiting hot giant exoplanets Kepler-5b and Kepler-6b by their parent stars. The observations are obtained in the near infrared with Spitzer Space Telescope and at optical wavelengths by combining more than a year of Kepler photometry. The investigation consists of constraining the eccentricities of these systems and of obtaining broad band emergent spectra for individual planets. For both targets, the occultations are detected at 3 sigma level at each wavelength with mid-occultation times consistent with circular orbits. The brightness temperatures of these planets are deduced from the infrared observations and reach T=1930+/-100K and T=1660+/-120K for Kepler-5b and Kepler-6b respectively. We measure optical geometric albedos A_g in the Kepler bandpass and find A_g=0.12+/-0.04 for Kepler-5b and A_g=0.11+/-0.04 for Kepler-6b leading to an upper limit for the Bond albedo of A_B < 0.17 in both cases. The observations for both planets are best described by models for which most of the incident energy is redistributed on the dayside, with only less than 10% of the absorbed stellar flux redistributed to the night side of these planets. The data for Kepler-5b favor a model without a temperature inversion, whereas for Kepler-6b they do not allow distinguishing between models with and without inversion.Comment: 26 pages, 18 figures, 3 tables, submitted to Ap

Low False-Positive Rate of Kepler Candidates Estimated From A Combination Of Spitzer And Follow-Up Observations

(Abridged) NASA's Kepler mission has provided several thousand transiting planet candidates, yet only a small subset have been confirmed as true planets. Therefore, the most fundamental question about these candidates is the fraction of bona fide planets. Estimating the rate of false positives of the overall Kepler sample is necessary to derive the planet occurrence rate. We present the results from two large observational campaigns that were conducted with the Spitzer telescope during the the Kepler mission. These observations are dedicated to estimating the false positive rate (FPR) amongst the Kepler candidates. We select a sub-sample of 51 candidates, spanning wide ranges in stellar, orbital and planetary parameter space, and we observe their transits with Spitzer at 4.5 microns. We use these observations to measures the candidate's transit depths and infrared magnitudes. A bandpass-dependent depth alerts us to the potential presence of a blending star that could be the source of the observed eclipse: a false-positive scenario. For most of the candidates (85%), the transit depths measured with Kepler are consistent with the depths measured with Spitzer as expected for planetary objects, while we find that the most discrepant measurements are due to the presence of unresolved stars that dilute the photometry. The Spitzer constraints on their own yield FPRs between 5-40%, depending on the KOIs. By considering the population of the Kepler field stars, and by combining follow-up observations (imaging) when available, we find that the overall FPR of our sample is low. The measured upper limit on the FPR of our sample is 8.8% at a confidence level of 3 sigma. This observational result, which uses the achromatic property of planetary transit signals that is not investigated by the Kepler observations, provides an independent indication that Kepler's false positive rate is low.Comment: 33 pages, 16 figures, 3 tables; accepted for publication in ApJ on February 7, 201

Visual Search Behavior in Individuals With Retinitis Pigmentosa During Level Walking and Obstacle Crossing

Purpose: Investigate the visual search strategy of individuals with retinitis pigmentosa (RP) when negotiating a floor-based obstacle compared with level walking, and compared with those with normal vision. Methods: Wearing a mobile eye tracker, individuals with RP and normal vision walked along a level walkway or walked along the walkway negotiating a floor-based obstacle. In the level walking condition, tape was placed on the floor to act as an object attracting visual attention. Analysis compared where individuals looked within the environment. Results: In the obstacle compared with level walking condition: (1) the RP group reduced the length of time and the number of times they looked Ahead, and increased the time and how often they looked at features on the ground (Object and Down, P < 0.05); and (2) the visual normal group reduced the time (by 19%) they looked Ahead (P = 0.076), and increased the time and how often they looked at the Object (P < 0.05). Compared with the normal vision group, in both level walking and obstacle conditions, the RP group reduced the time looking Ahead and looked for longer and more often Down (P < 0.05). Conclusions: The RP group demonstrated a more active visual search pattern, looking at more areas on the ground in both level walking and obstacle crossing compared with visual normals. This gaze strategy was invariant across conditions. This is most likely due to the constricted visual field and inability to rely on inferior peripheral vision to acquire information from the floor within the environment when walking