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Small Main-Belt Asteroid Spectroscopic Survey (SMASS) V1.0
The Small Main-Belt Asteroid Spectroscopic Survey (SMASS) was a wide wavelength-coverage visible spectroscopic survey of asteroids carried out primarily at the Michagan-... -
24-COLOR ASTEROID SURVEY
This bundle is comprised of asteroid flux data measured in 26 filters using the McCord dual beam photometer, and covering the range 0.32 - 1.08 microns for 285 numbered... -
24-COLOR ASTEROID SURVEY
This dataset is comprised of asteroid flux data measured in 26 filters using the McCord dual beam photometer, and covering the range 0.32 - 1.08 microns for 285 numbered... -
EIGHT COLOR ASTEROID SURVEY V3.0
Reflectance spectra and associated data for 589 numbered asteroids. -
24-COLOR ASTEROID SURVEY
This dataset is comprised of asteroid flux data measured in 26 filters using the McCord dual beam photometer, and covering the range 0.32 - 1.08 microns for 285 numbered... -
SMASS ASTEROID SURVEY V2.1
Small Main-Belt Asteroid Spectrographic Survey over the visual range. -
ASTEROID PHOTOMETRIC CATALOG V1.1
The Asteroid Photometric Catalog (3rd update), Lagerkvist, et.al., 1993 [LAGERKVISTETAL1993], is a compilation of all asteroid lightcurve photometry published up to and... -
ASTEROID PHOTOMETRIC CATALOG V1.1
The Asteroid Photometric Catalog (3rd update), Lagerkvist, et.al., 1993 [LAGERKVISTETAL1993], is a compilation of all asteroid lightcurve photometry published up to and... -
EARTH ASTEROID DBP 24COLOR SURVEY V2.0
Photometric spectra covering the range 0.32 - 1.08 micrometers for 285 numbered asteroids, as published in Chapman & Gaffey (1979b) and McFadden, et al. (1984). -
EARTH ASTEROID DBP 24COLOR SURVEY V2.0
Photometric spectra covering the range 0.32 - 1.08 micrometers for 285 numbered asteroids, as published in Chapman & Gaffey (1979b) and McFadden, et al. (1984). -
EIGHT COLOR ASTEROID SURVEY V3.0
Reflectance spectra and associated data for 589 numbered asteroids. -
SMASS ASTEROID SURVEY V2.1
Small Main-Belt Asteroid Spectrographic Survey over the visual range.