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4500 square degrees of the Southern sky are imaged in five optical filters (U, V, R, I, Z) to depths comparable to the Sloan Digital Sky Survey (SDSS). This dataset, provided by NASA via the MAST archive, is designed to study baryon wiggles in galaxy power spectra and examine luminous red galaxies to constrain dark energy. The survey also serves as an imaging base for spectroscopic follow-up by the Very Large Telescope (VLT).
License is listed as 'other-license-specified'; users should verify terms before use. Data is accessed via Cone Search endpoints (BIN, HTML formats).