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Data · dataset · 2025

SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC V1.0

Listed in Open NASA

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.

Description

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].

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Related

Provenance · 1 source records, 6 field assertions
SourceKeyLast seenRaw
Open NASA7a2ecb70-6e6e-41ff-b4ec-d3369e7cc3ef16 h agoJSON v1
FieldAssertionExtractorEvidence
created_datesource · open nasa govconnector:open_nasa_gov@1.0.0
descriptionsource · open nasa govconnector:open_nasa_gov@1.0.0/notes
license_textsource · open nasa govconnector:open_nasa_gov@1.0.0
publication_datesource · open nasa govconnector:open_nasa_gov@1.0.0
titlesource · open nasa govconnector:open_nasa_gov@1.0.0/title
updated_datesource · open nasa govconnector:open_nasa_gov@1.0.0