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Spectroscopy of the nova-like system UX UMa and three classical novae : V603 Aql, BT Mon and V1425 AqlArenas Villarroel, Jose L. January 2000 (has links)
No description available.
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New Methods in Finding Binary Constant Weight CodesTaub, David January 2007 (has links)
<p>This thesis presents new methods for finding optimal and near-optimal constant weight binary codes with distance d and weight w such that d=2(w-1). These methods have led to the discovery of a number of new codes which are being submitted for publication. Improvements in methods for generating lexicographic codes are also discussed, with suggestions for further research in this area.</p>
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Spectroscopic studies of Hercules X-1Quaintrell, Hannah January 1999 (has links)
No description available.
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Predicting the phase equilibria of associating and reacting systemsGrice, Sarah Jane January 1999 (has links)
No description available.
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Influence of variables in Bayesian predictionBhattacharjee, Sushanta Kumar January 1987 (has links)
No description available.
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Internal representation and biological plausibility in an artificial neural networkBrady, Patrick January 1995 (has links)
No description available.
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Optical and X-ray studies of interacting binariesMcGowan, Katherine Elizabeth January 2000 (has links)
No description available.
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Labour supply and absenteeismBarmby, Timothy Alan January 1998 (has links)
No description available.
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Optical observations of the supersoft sourcesSouthwell, Karen Anne January 1997 (has links)
No description available.
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Infrared Speckle Observations of Binary Ross 614 AB: Combined Shift-and-Add and Zero-and-Add AnalysisDavey, B. L. K., Cocke, W. J., Bates, R. H. T., McCarthy, D. W., jr., Christou, J. C., Cobb, M. L. 12 1900 (has links)
One -dimensional infrared speckle scans of Ross 614 AB were recorded at a wavelength
of 2.2μm. For each scan an estimate of the instantaneous quality of the seeing was
calculated and the scan was binned accordingly. The three bins corresponding to the three
best seeing conditions were further processed by applying the shift -and -add algorithm to
the set of images contained within each bin, thereby generating three shift- and -add images
with differing shift -and -add point -spread- functions. After windowing the shift -and -add
images (using edge -extension) to reduce the effect of contamination, we have obtained
parameters corresponding to the separation and brightness ratio of a two component
model of the double star Ross 614 AB by deconvolving the three shift -and -add images
with the aid of the zero-and -add technique. Least squares analysis on the positions
of the clusters of zeros found from zero- and -add yields a separation of 1.04 arcseconds
and a brightness ratio of 4.3 for the binary system at this wavelength. An extension
of the processing, which takes explicit account of the nonlinear motion of the scanning
mechanism gives improved estimates of 1.04 arcseconds and 3.9 for the separation and
brightness ratio, respectively.
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