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VOStat: A Statistical Web Service for Astronomers

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arxiv 1302.0387 v1 pith:YEUMJ4GQ submitted 2013-02-02 astro-ph.IM

classification astro-ph.IM
keywords analysisstatisticalvostatcrandataserviceacquiredadd-on
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

VOStat is a Web service providing interactive statistical analysis of astronomical tabular datasets. It is integrated into the suite of analysis and visualization tools associated with the international Virtual Observatory (VO) through the SAMP communication system. A user supplies VOStat with a dataset extracted from the VO, or otherwise acquired, and chooses among $\sim 60$ statistical functions. These include data transformations, plots and summaries, density estimation, one- and two-sample hypothesis tests, global and local regressions, multivariate analysis and clustering, spatial analysis, directional statistics, survival analysis (for censored data like upper limits), and time series analysis. The statistical operations are performed using the public domain {\bf R} statistical software environment, including a small fraction of its $>4000$ {\bf CRAN} add-on packages. The purpose of VOStat is to facilitate a wider range of statistical analyses than are commonly used in astronomy, and to promote use of more advanced methodology in {\bf R} and {\bf CRAN}.

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Cited by 3 Pith papers

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

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    astro-ph.GA 2026-06 unverdicted novelty 6.0 of 10

    A beta-VAE analysis of pop-cosmos models finds that five latent dimensions capture the rest-frame optical SED, corresponding to stellar mass, recent star formation, dust, and two gas ionization states.

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    astro-ph.GA 2026-06 conditional novelty 6.0 of 10

    Rest-frame optical galaxy SEDs from a 16-parameter SPS model are captured by five disentangled VAE latents (mass, young stars, dust, soft/hard ionization); metallicity and age are not independent drivers.

  3. pop-cosmos: Galaxy size evolution across structural and star-formation classifications in COSMOS-Web

    astro-ph.GA 2026-06 unverdicted novelty 5.0 of 10

    Galaxy size-mass relations exhibit double power-law breaks at different pivot masses for quiescent versus bulge-dominated samples, coinciding with AGN activity scales.

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