Optical Design for Extremely Large Telescope Adaptive Optics Systems (open access)

Optical Design for Extremely Large Telescope Adaptive Optics Systems

Designing an adaptive optics (AO) system for extremely large telescopes (ELT's) will present new optical engineering challenges. Several of these challenges are addressed in this work, including first-order design of multi-conjugate adaptive optics (MCAO) systems, pyramid wavefront sensors (PWFS's), and laser guide star (LGS) spot elongation. MCAO systems need to be designed in consideration of various constraints, including deformable mirror size and correction height. The y,{bar y} method of first-order optical design is a graphical technique that uses a plot with marginal and chief ray heights as coordinates; the optical system is represented as a segmented line. This method is shown to be a powerful tool in designing MCAO systems. From these analyses, important conclusions about configurations are derived. PWFS's, which offer an alternative to Shack-Hartmann (SH) wavefront sensors (WFS's), are envisioned as the workhorse of layer-oriented adaptive optics. Current approaches use a 4-faceted glass pyramid to create a WFS analogous to a quad-cell SH WFS. PWFS's and SH WFS's are compared and some newly-considered similarities and PWFS advantages are presented. Techniques to extend PWFS's are offered: First, PWFS's can be extended to more pixels in the image by tiling pyramids contiguously. Second, pyramids, which are difficult to manufacture, can …
Date: November 26, 2003
Creator: Bauman, B J
System: The UNT Digital Library
Analysis of Hypothetical Promoter Domains of DKFZp564A1164, NPHS1 and HSPOX1 Genes (open access)

Analysis of Hypothetical Promoter Domains of DKFZp564A1164, NPHS1 and HSPOX1 Genes

For this study, a high throughput method for identifying and testing regulatory elements was examined. In addition, the validity of promoters predicted by FirstEF was tested. It was found that by combining computer based promoter and first exon predictions from FirstEF (Davuluri et al., 2001) with PCR-based cloning to generate luciferase reporter constructs, and by testing reporter activity in cultured mammalian cells plated in a 96 well format one could identify promoter activity in a relatively high throughput manner. The data generated in this study suggest that FirstEF predictions are sometimes incorrect. Therefore, having a strategy for defining which FirstEF predicted promoters to test first may accelerate the process. Initially testing promoters that are at a confirmed transcription start site for a gene, at a possible alternate transcription start site or in a region of conserved sequence would be the best candidates, while promoters predicted in gene desert regions may not be as easy to confirm. The luciferase assay lent itself very well to the high throughput search, however the subcloning did not always go smoothly. The numerous steps that this traditional subcloning method requires were time consuming and increased the opportunities for errors. A faster method that skips many …
Date: November 29, 2003
Creator: Hammond, S S
System: The UNT Digital Library
Measurement of the Top Quark Mass at CDF II (open access)

Measurement of the Top Quark Mass at CDF II

The authors describe a measurement of the top quark mass using events with two charged leptons collected by the CDF II Detector from p{bar p} collisions with {radical}s = 1.96 TeV at the Fermilab Tevatron. The posterior probability distribution of the top quark pole mass is calculated using the differential cross-section for the t{bar t} production and decay expressed with respect to observed leptons and jets momenta. The presence of background events in the collected sample is modeled using calculations of the differential cross-sections for major background processes. This measurement represents the first application of this method to events with two charged leptons. In a data sample with integrated luminosity of 340 pb{sup -1}, they observe 33 candidate events and measure M{sub top} = 165.2 {+-} 61.{sub stat} {+-} 3.4{sub syst} GeV/c{sup 2}.
Date: November 1, 2003
Creator: Kovalev, Andrew N.
System: The UNT Digital Library