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Structure in the 3D Galaxy Distribution: I. Methods and Example Results
M. J. Way, P. R. Gazis, Jeffrey D. Scargle
Three methods for detecting and characterizing structure in point data, such as that generated by redshift surveys, are described: classification using self-organizing maps, segmen…
Viewpoints: A high-performance high-dimensional exploratory data analysis tool
P. R. Gazis, C. Levit, M. J. Way
Scientific data sets continue to increase in both size and complexity. In the past, dedicated graphics systems at supercomputing centers were required to visualize large data sets,…
Kepler Mission Design, Realized Photometric Performance, and Early Science
David G. Koch, William J. Borucki, Gibor Basri +44
The Kepler Mission, launched on Mar 6, 2009 was designed with the explicit capability to detect Earth-size planets in the habitable zone of solar-like stars using the transit photo…
Instrument Performance in Kepler's First Months
Douglas A. Caldwell, Jeffery J. Kolodziejczak, Jeffrey E. Van Cleve +16
The Kepler Mission relies on precise differential photometry to detect the 80 parts per million (ppm) signal from an Earth-Sun equivalent transit. Such precision requires superb in…