Search Results
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data set:
SMALL MAIN-BELT ASTEROID SPECTROSCOPIC SURVEY, PHASE II
Visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999.
SUPPORT ARCHIVES - EAR-A-I0028-4-SBN0001/SMASSII-V1.0 - starting 1993-08-21T10:48:51Z -
data set:
SMASS ASTEROID SURVEY V1.0
Visual spectra from the Small Main-Belt Asteroid Survey (SMAS), 1990-1994
SUPPORT ARCHIVES - EAR-A-M3SPEC-3-RDR-SMASS-V1.0 - starting 1990-01-01T00:00:00Z -
data set:
SMASS ASTEROID SURVEY V2.1
Small Main-Belt Asteroid Spectrographic Survey over the visual range.
SUPPORT ARCHIVES - EAR-A-M3SPEC-3-RDR-SMASS-V2.1 - starting 1990-01-01T00:00:00Z -
instrument:
MARK III SPECTROGRAPH for MDM
Information about the MARK III SPECTROGRAPH for MDM instrument -
instrument:
MARK III SPECTROGRAPH for OBS325T1
Information about the MARK III SPECTROGRAPH for OBS325T1 instrument -
instrument:
MARK III SPECTROGRAPH for OBS325T2
Information about the MARK III SPECTROGRAPH for OBS325T2 instrument -
telescope:
1.3-m Tinsley Cassegrain/Coude reflector
Information about the telescope 1.3-m Tinsley Cassegrain/Coude reflector -
telescope:
2.4-m Hiltner Ritchey-Chretien equatorial reflector
Information about the telescope 2.4-m Hiltner Ritchey-Chretien equatorial reflector -
instrument:
Mark III Spectrograph
Information about the Mark III Spectrograph instrument -
collection:
Small Main-Belt Asteroid Spectroscopic Survey, Phase II V1.0
This data set contains visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999. The purpose of the SMASSII survey was to provide a new basis for studying the compositional diversity and structure of the asteroid belt. Based on experiences gained from the earlier SMASS survey, SMASSII focused on producing an even larger, internally consistent set of CCD spectra for small (D < 20 km) main-belt asteroids. The observing strategies and procedures used during SMASSII roughly parallel those used in the first survey (Xu et al. Icarus 115 1-35, 1995), though several minor changes were made in instrumentation and in portions of the data reduction process. -
bundle:
Small Main-Belt Asteroid Spectroscopic Survey, Phase II V1.0
This data set contains visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999. The purpose of the SMASSII survey was to provide a new basis for studying the compositional diversity and structure of the asteroid belt. Based on experiences gained from the earlier SMASS survey, SMASSII focused on producing an even larger, internally consistent set of CCD spectra for small (D < 20 km) main-belt asteroids. The observing strategies and procedures used during SMASSII roughly parallel those used in the first survey (Xu et al. Icarus 115 1-35, 1995), though several minor changes were made in instrumentation and in portions of the data reduction process. -
collection:
Small Main-Belt Asteroid Spectroscopic Survey, Phase II V1.0
This data set contains visible-wavelength (0.435-0.925 micron) spectra for 1341 main-belt asteroids observed during the second phase of the Small Main-belt Asteroid Spectroscopic Survey (SMASSII) between August 1993 and March 1999. The purpose of the SMASSII survey was to provide a new basis for studying the compositional diversity and structure of the asteroid belt. Based on experiences gained from the earlier SMASS survey, SMASSII focused on producing an even larger, internally consistent set of CCD spectra for small (D < 20 km) main-belt asteroids. The observing strategies and procedures used during SMASSII roughly parallel those used in the first survey (Xu et al. Icarus 115 1-35, 1995), though several minor changes were made in instrumentation and in portions of the data reduction process.
Data Sets and Information