SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC V1.0
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].
Resources
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Tags
- asteroid-44447
- 7558-yurlov
- 9147-kourakuen
- asteroid-134455
- asteroid-26886
- 5498-gustafsson
- 9481-menchu
- asteroid-24941
- asteroid-56570
- asteroid-36840
- asteroid-12543
- asteroid-56026
- asteroid-53143
- support-archives
- 9553-colas
- asteroid-113844
- asteroid-38070
- asteroid-94005
- asteroid-131010
- asteroid-28517
- asteroid-114544
- 9254-shunkai
- asteroid-111515
- 2000-up66
- asteroid-122357
- asteroid-37304
- asteroid-28034
- asteroid-10537
- asteroid-60669
- asteroid-46690