Table of counterpart associations between Gaia DR3 and CatWISE2020. Uses probabilistic cross-match algorithms as described by Wilson & Naylor (MNRAS, 2017, 2018a,b) and Wilson (RNAAS, 2022). Sources are returned either as a pairing, in which the Gaia and WISE objects are the same astrophysical source detected twice, or as non-matches, with that particular object in one of the catalogues having a corresponding flux upper limits in the opposing catalogue, and entries include various pieces of metadata such as the probability of the match/non-match, likelihood of match on purely position or brightness grounds, and information on the level to which objects suffer contamination due to hidden and unresolved background sources.
Rubin Science Platform documentation
Find documentation for Rubin Observatory data, science platform services, and software.
Data documentation
GaiaXCatwise
VISTA-HSC
Platform and software documentation
Phalanx
The configuration repository for Rubin's Kubernetes deployments.
Rubin Science Platform
The Notebook aspect is a powerful data analysis environment with Jupyter Notebooks and terminals in the browser. Documentation for the Rubin Science Platform, including account set up, portal, notebooks, and API aspects.
Portal
The Portal enables you to explore LSST image and table data in your browser.
LSST Science Pipelines
The Science Pipelines include the Butler for accessing LSST data and a pipeline framework for processing data. The LSST Science Pipelines Python package is preinstalled in the Notebook aspect.
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