{"@type": "dcat:Dataset", "accessLevel": "public", "bureauCode": ["026:00"], "contactPoint": {"@type": "vcard:Contact", "fn": "Planetary Data System", "hasEmail": "mailto:pds-operator@jpl.nasa.gov"}, "description": "These data are the results of a spectroscopic survey designed to target and detect asteroids whose photometric colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. The colors of these candidates were measured as part of the 3rd release of the Sloan Digital Sky Survey Moving Object Catalog (Ivezic et al. 2001) [IVEZICETAL2001]. These spectra were obtained with two visible wavelength instruments: the Echellete Spectrograph and Imager (ESI, Sheinis et al. 2002) [SHEINISETAL2002] on Keck II and the Supernova Integral Field Spectrograph (SNIFS, Lantz et al. 2004) [LANTZETAL2004] at the University of Hawaii 2.2m telescope. A subset of these data were published in Moskovitz et al. (2008a, 2008b) [MOSKOVITZETAL2008, MOSKOVITZETAL2008B].", "identifier": "urn:nasa:pds:context_pds3:data_set:data_set.ear-a-i0039-i0576-4-sdssmocvspec-v1.0;urn:nasa:pds:context_pds3:data_set:data_set.ear-a-i0039-i0576-4-sdssmocvspec-v1.0::1.0", "keyword": ["__"], "license": "https://www.usa.gov/government-works", "modified": "2026-08-17", "programCode": ["026:000"], "publisher": {"@type": "org:Organization", "name": "Small Bodies"}, "theme": ["Planetary Science"], "title": "SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC V1.0"}