SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC
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
- 111515-2001-yc91
- 114544-2003-bn28
- 7558-yurlov
- 9147-kourakuen
- none
- 5498-gustafsson
- 113844-2002-tv237
- 9481-menchu
- 134455-1998-st116
- 12543-1998-qm5
- 131010-2000-xq9
- 38070-redwine
- 36840-2000-sh112
- 28517-2000-dd7
- 9553-colas
- 94005-2000-xo25
- 56026-1998-vn52
- 44447-1998-um21
- 53143-1999-bb9
- 37304-2001-ew23
- 9254-shunkai
- 24941-1997-jm14
- 334008-2000-up66
- 10537-1991-ry16
- 26886-1994-tj2
- 122357-2000-qh49
- 56570-2000-ja21
- 28034-1998-eu13
- 46690-1997-an23
- 60669-2000-ge4