Faro: A framework for measuring the scientific performance of petascale Rubin Observatory data products
Leanne P. Guy, Keith Bechtol, Jeffrey L. Carlin, Erik Dennihy, Peter, S. Ferguson, K. Simon Krughoff, Robert H. Lupton, Colin T. Slater, Krzysztof, Findeisen, Arun Kannawadi, Lee S. Kelvin, Nate B. Lust, Lauren A. MacArthur,, Michael N. Martinez, Sophie L. Reed, Dan S. Taranu

TL;DR
Faro is a framework designed to automatically evaluate the scientific performance of LSST data products, ensuring they meet quality standards and support transformative astronomical research.
Contribution
This paper introduces Faro, a novel automated framework for measuring and monitoring the scientific performance of petascale LSST data products across multiple data granularities.
Findings
Faro effectively characterizes data product performance on simulated datasets.
It enables trend analysis and regression testing during development.
Initial results demonstrate Faro's capability to verify LSST data quality.
Abstract
The Vera C. Rubin Observatory will advance many areas of astronomy over the next decade with its unique wide-fast-deep multi-color imaging survey, the Legacy Survey of Space and Time (LSST). The LSST will produce approximately 20TB of raw data per night, which will be automatically processed by the LSST Science Pipelines to generate science-ready data products -- processed images, catalogs and alerts. To ensure that these data products enable transformative science with LSST, stringent requirements have been placed on their quality and scientific fidelity, for example on image quality and depth, astrometric and photometric performance, and object recovery completeness. In this paper we introduce faro, a framework for automatically and efficiently computing scientific performance metrics on the LSST data products for units of data of varying granularity, ranging from single-detector to…
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Taxonomy
TopicsAstronomy and Astrophysical Research
