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TOPCAT: Desktop Exploration of Tabular Data for Astronomy and Beyond

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arxiv 1707.02160 v1 pith:56THF3MQ submitted 2017-07-07 astro-ph.IM

classification astro-ph.IM
keywords desktopinteractiveothertopcatastronomydataexplorationfeatures
verification ladder T0 review T1 audit T2 compute T3 formal
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TOPCAT, the Tool for OPerations on Catalogues And Tables, is an interactive desktop application for retrieval, analysis and manipulation of tabular data, offering a powerful and flexible range of interactive visualization options amongst other features. Its visualization capabilities focus on enabling interactive exploration of large static local tables - millions of rows and hundreds of columns can easily be handled on a standard desktop or laptop machine, and various options are provided for meaningful graphical representation of such large datasets. TOPCAT has been developed in the context of astronomy, but many of its features are equally applicable to other domains. The software, which is free and open source, is written in Java, and the underlying high-performance visualisation library is suitable for re-use in other applications.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Visual analytics for cosmological simulation results

    astro-ph.IM 2026-07 conditional novelty 6.0 of 10

    A browser-native visual-analytics tool lets astronomers interactively explore millions of simulated particles and drill down from galaxy catalogues to per-pixel image dashboards.

  2. SRG/eROSITA X-ray selected cataclysmic variable candidates observed in SDSS-V DR20

    astro-ph.SR 2026-07 conditional novelty 6.0 of 10

    eROSITA-selected SDSS-V DR20 spectroscopy yields 587 cataclysmic variables (274 known), including new nearby systems, AM CVns, and a low-accretion-rate polar.

  3. The Role of Stellar Mass and Star Formation in Shaping X-ray Emission of Radio-Loud and Radio-Quiet AGN

    astro-ph.GA 2025-08 reject novelty 3.0 of 10

    Claims radio-loud AGN show a strong Lx-SFR correlation without a stellar-mass link, while radio-quiet AGN correlate across all three, but the radio-loud result rests on just 7 sources.

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