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Data · dataset · 2025

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

Listed in NASA Data Portal

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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Inferred from text
Astronomical sciences 74%

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Provenance · 1 source records, 7 field assertions
SourceKeyLast seenRaw
NASA Data Portal7a2ecb70-6e6e-41ff-b4ec-d3369e7cc3ef10 d agoJSON v1
FieldAssertionExtractorEvidence
concepts[field].anzsrc:group:5101enrichment · data nasa govtaxonomy-embedding@1.1.0title+keywords+description (74%)
created_datesource · data nasa govconnector:data_nasa_gov@1.0.0
descriptionsource · data nasa govconnector:data_nasa_gov@1.0.0/notes
license_textsource · data nasa govconnector:data_nasa_gov@1.0.0
publication_datesource · data nasa govconnector:data_nasa_gov@1.0.0
titlesource · data nasa govconnector:data_nasa_gov@1.0.0/title
updated_datesource · data nasa govconnector:data_nasa_gov@1.0.0