Paper
19 December 2002 Spatial Clustering of Galaxies in Large Datasets
Alexander Szalay, Tamas Budavari, Andrew Connolly, Jim Gray, Takahiko Matsubara, Adrian Pope, Istvan Szapudi
Author Affiliations +
Abstract
Datasets with tens of millions of galaxies present new challenges for the analysis of spatial clustering. We have built a framework, that integrates a database of object catalogs, tools for creating masks of bad regions, and a fast (NlogN) correlation code. This system has enabled unprecedented efficiency in carrying out the analysis of galaxy clustering in the SDSS catalog. A similar approach is used to compute the three-dimensional spatial clustering of galaxies on very large scales. We describe our strategy to estimate the effect of photometric errors using a database. We discuss our efforts as an early example of data-intensive science. While it would have been possible to get these results without the framework we describe, it will be infeasible to perform these computations on the future huge datasets without using this framework.
© (2002) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alexander Szalay, Tamas Budavari, Andrew Connolly, Jim Gray, Takahiko Matsubara, Adrian Pope, and Istvan Szapudi "Spatial Clustering of Galaxies in Large Datasets", Proc. SPIE 4847, Astronomical Data Analysis II, (19 December 2002); https://doi.org/10.1117/12.476761
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Cited by 5 scholarly publications.
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KEYWORDS
Galactic astronomy

Databases

Statistical analysis

Error analysis

Correlation function

Astronomy

Modulation

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