Xu Teng, Adam Corpstein, Joel Holm, Willis Knox, Becker Mathie, Philip R. O. Payne, Ethan Vander Wiel, Prabin Giri, Goce Trajcevski, A. Dotter, J. Andrews, S. Coughlin, Y. Qin, J. G. Serra-Perez, N. Tran, Jaime Roman-Garja, K. Kovlakas, E. Zapartas, S. Bavera, D. Misra, T. Fragos
{"title":"CACSE: Context Aware Clustering of Stellar Evolution","authors":"Xu Teng, Adam Corpstein, Joel Holm, Willis Knox, Becker Mathie, Philip R. O. Payne, Ethan Vander Wiel, Prabin Giri, Goce Trajcevski, A. Dotter, J. Andrews, S. Coughlin, Y. Qin, J. G. Serra-Perez, N. Tran, Jaime Roman-Garja, K. Kovlakas, E. Zapartas, S. Bavera, D. Misra, T. Fragos","doi":"10.1145/3469830.3470916","DOIUrl":null,"url":null,"abstract":"We present CACSE – a system for Context Aware Clustering of Stellar Evolution – for datasets corresponding to temporal evolution of stars, which are multivariate time series, usually with a large number of attributes (e.g., ≥ 40). Typically, the datasets are obtained by simulation and are relatively large in size (5 ∼ 10 GB per certain interval of values for various initial conditions). Investigating common evolutionary trends in these datasets often depends on the context – i.e., not all the attributes are always of interest, and among the subset of the context-relevant attributes, some may have more impact than others. To enable such context-aware clustering, our CACSE system provides functionalities allowing the domain experts to dynamically select attributes that matter, and assign desired weights/priorities. Our system consists of a PostgreSQL database, Python-based middleware with RESTful and Django framework, and a web-based user interface as frontend. The user interface provides multiple interactive options, including selection of datasets and preferred attributes along with the corresponding weights. Subsequently, the users can select a time instant or a time range to visualize the formed clusters. Thus, CACSE enables a detection of changes in the the set of clusters (i.e., convoys) of stellar evolution tracks. Current version provides two of the most popular clustering algorithms – k-means and DBSCAN.","PeriodicalId":206910,"journal":{"name":"17th International Symposium on Spatial and Temporal Databases","volume":"22 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2021-08-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"17th International Symposium on Spatial and Temporal Databases","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1145/3469830.3470916","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
Abstract
We present CACSE – a system for Context Aware Clustering of Stellar Evolution – for datasets corresponding to temporal evolution of stars, which are multivariate time series, usually with a large number of attributes (e.g., ≥ 40). Typically, the datasets are obtained by simulation and are relatively large in size (5 ∼ 10 GB per certain interval of values for various initial conditions). Investigating common evolutionary trends in these datasets often depends on the context – i.e., not all the attributes are always of interest, and among the subset of the context-relevant attributes, some may have more impact than others. To enable such context-aware clustering, our CACSE system provides functionalities allowing the domain experts to dynamically select attributes that matter, and assign desired weights/priorities. Our system consists of a PostgreSQL database, Python-based middleware with RESTful and Django framework, and a web-based user interface as frontend. The user interface provides multiple interactive options, including selection of datasets and preferred attributes along with the corresponding weights. Subsequently, the users can select a time instant or a time range to visualize the formed clusters. Thus, CACSE enables a detection of changes in the the set of clusters (i.e., convoys) of stellar evolution tracks. Current version provides two of the most popular clustering algorithms – k-means and DBSCAN.