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Batch is back: CasJobs, serving multi-TB data on the Web

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arxiv cs/0502072 v1 pith:LBVKTPYU submitted 2005-02-17 cs.DC cs.DB

classification cs.DCcs.DB
keywords dataqueriestheybecausecasjobsmydbsdsssystem
verification ladder T0 review T1 audit T2 compute T3 formal
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The Sloan Digital Sky Survey (SDSS) science database describes over 140 million objects and is over 1.5 TB in size. The SDSS Catalog Archive Server (CAS) provides several levels of query interface to the SDSS data via the SkyServer website. Most queries execute in seconds or minutes. However, some queries can take hours or days, either because they require non-index scans of the largest tables, or because they request very large result sets, or because they represent very complex aggregations of the data. These "monster queries" not only take a long time, they also affect response times for everyone else - one or more of them can clog the entire system. To ameliorate this problem, we developed a multi-server multi-queue batch job submission and tracking system for the CAS called CasJobs. The transfer of very large result sets from queries over the network is another serious problem. Statistics suggested that much of this data transfer is unnecessary; users would prefer to store results locally in order to allow further joins and filtering. To allow local analysis, a system was developed that gives users their own personal databases (MyDB) at the server side. Users may transfer data to their MyDB, and then perform further analysis before extracting it to their own machine. MyDB tables also provide a convenient way to share results of queries with collaborators without downloading them. CasJobs is built using SOAP XML Web services and has been in operation since May 2004.

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Cited by 1 Pith paper

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  1. Fast Luminous Extragalactic Transients in the VLA Sky Survey: Implications for the rates of Accretion-Induced Collapse Events, Fast Blue Optical Transients and Gamma Ray Burst Afterglows

    astro-ph.HE 2025-06 conditional novelty 6.0 of 10

    Six fast luminous radio transients from VLASS yield new upper limits on the rates of accretion-induced collapse, radio-bright luminous fast blue optical transients, and off-axis gamma-ray burst afterglows.

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