Open Access
Multivariate statistical analysis software technologies for astrophysical research involving large data bases
S. George Djorgovski
- 01 Jan 1993
TL;DR: A package to process and analyze the data from the digital version of the Second Palomar Sky Survey, which incorporates the latest in machine learning and expert systems software technology, in order to classify the detected objects objectively and uniformly, and facilitate handling of the enormous data sets from digital sky surveys and other sources.
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Abstract: We developed a package to process and analyze the data from the digital version of the Second Palomar Sky Survey. This system, called SKICAT, incorporates the latest in machine learning and expert systems software technology, in order to classify the detected objects objectively and uniformly, and facilitate handling of the enormous data sets from digital sky surveys and other sources. The system provides a powerful, integrated environment for the manipulation and scientific investigation of catalogs from virtually any source. It serves three principal functions: image catalog construction, catalog management, and catalog analysis. Through use of the GID3* Decision Tree artificial induction software, SKICAT automates the process of classifying objects within CCD and digitized plate images. To exploit these catalogs, the system also provides tools to merge them into a large, complex database which may be easily queried and modified when new data or better methods of calibrating or classifying become available. The most innovative feature of SKICAT is the facility it provides to experiment with and apply the latest in machine learning technology to the tasks of catalog construction and analysis. SKICAT provides a unique environment for implementing these tools for any number of future scientific purposes. Initial scientific verification and performance tests have been made using galaxy counts and measurements of galaxy clustering from small subsets of the survey data, and a search for very high redshift quasars. All of the tests were successful and produced new and interesting scientific results. Attachments to this report give detailed accounts of the technical aspects of the SKICAT system, and of some of the scientific results achieved to date. We also developed a user-friendly package for multivariate statistical analysis of small and moderate-size data sets, called STATPROG. The package was tested extensively on a number of real scientific applications and has produced real, published results.
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Citations
Clustering on very small scales from a large sample of confirmed quasar pairs: does quasar clustering track from Mpc to kpc scales?
Sarah Eftekharzadeh,Adam D. Myers,Joseph F. Hennawi,S. G. Djorgovski,Gordon T. Richards,A. A. Mahabal,Matthew J. Graham +6 more
TL;DR: In this paper, the authors present the most precise estimate to date of the clustering of quasars on very small scales, based on a sample of 47 binary quasar pairs with magnitudes of g < 20.85 and proper transverse separations of ∼25 h^(−1) kpc.
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References
Clustering on very small scales from a large sample of confirmed quasar pairs: does quasar clustering track from Mpc to kpc scales?
Sarah Eftekharzadeh,Adam D. Myers,Joseph F. Hennawi,S. G. Djorgovski,Gordon T. Richards,A. A. Mahabal,Matthew J. Graham +6 more
TL;DR: In this paper, the authors present the most precise estimate to date of the clustering of quasars on very small scales, based on a sample of 47 binary quasar pairs with magnitudes of g < 20.85 and proper transverse separations of ∼25 h^(−1) kpc.
Depression among older people in rural Thailand : Knowledge of population, experiences and perceptions of patients, families, and psychiatric nurses
Duangkaew Kleebthong
- 01 Jan 2018
TL;DR: This data indicates that the number of older persons (defined as age 60 and over) in Thailand has grown rapidly, and will be projected to increase to over 20 million by 2035.
4
Ideal observational cosmology
TL;DR: In this paper, it is shown that if ideal observations are available, they are insufficient to determine the space-time structure on the past light cone of the observer; however, in the cosmological case they are precisely necessary and sufficient to determine a spacetime geometry on the light cone and in its causal past (down to where caustics or curps first occur).