Rubin Science Platform APIs
Integrate Rubin data into your analysis tools with APIs.
To access APIs you need an access token. See our guide Creating user tokens to learn how to create tokens and use them in VO clients.
API endpoints
Data Preview 1
Data Preview 1 contains image and catalog products from the Rubin Science Pipelines v29 processing of observations obtained with the LSST Commissioning Camera of seven ~1 square degree fields, over seven weeks in late 2024. Read the documentation
https://rsp-test.lsst.ac.uk/auth/gmshttps://rsp-test.lsst.ac.uk/api/taphttps://rsp-test.lsst.ac.uk/api/hips/v2/dp1/list
macauff_gaiadr3xcatwise
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. docsUrl: "https://dp1.lsst.io/"
https://rsp-test.lsst.ac.uk/auth/gms
Documentation
Learn more about the APIs in the Rubin Science Platform API Aspect guide.