Search Results
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collection:
document collection for the "REDDY MAIN BELT ASTEROID SPECTRA" bundle
This is the document collection for the gbo.ast-mb.reddy.spectra bundle. This data set contains low-resolution (R~150) near-infrared (0.7-2.5 microns) spectra of 90 main belt asteroids observed with the SpeX instrument on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i. This data set archives reduced, calibrated spectra of targets of opportunity observed from 2001 to 2012. -
collection:
data collection for the "VILAS ASTEROID SPECTRA" bundle
This is the data collection for the gbo.ast.vilas.spectra bundle. This data set contains 81 published spectra of asteroids obtained by Faith Vilas during the years 1982 - 1992. -
bundle:
Gartrelle et al. IRTF Asteroid Spectra V1.0
This data set is comprised of the VNIR (0.69-2.5 micron) spectra of twenty-five D-type asteroids from varying Solar System locations. The spectra were obtained from NASA/IRTF on Mauna Kea between 2016-2019 using the SpeX instrument in Low-Resolution Prism mode and the 0.8 x 15" slit. Guiding was performed using spillover light from the slit (GuideDog) for targets with apparent magnitude > 15.5. For targets fainter than magnitude 15.5, guiding was accomplished using the MORIS CCD imager. -
bundle:
REDDY NEAR-EARTH AND MARS-CROSSING ASTEROIDS
This data set contains low-resolution (R~150) near-infrared (0.7-2.5 microns) spectra of 27 asteroids, 5 Mars-crossing and 22 near-Earth asteroids, observed with the SpeX instrument on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i. This data set archives reduced, calibrated spectra of targets of opportunity observed from 2001 to 2008. -
bundle:
REDDY VESTA ROTATIONALLY RESOLVED NEAR-INFRARED SPECTRA
This data set contains low-resolution near-infrared (~0.7-2.5 microns) spectra of main belt asteroid (4) Vesta observed with the SpeX instrument on NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i, and reported in Reddy et al. (2011). This data set archives reduced, calibrated spectra that were obtained as part of ground-based characterization of Vesta prior to the arrival of Dawn spacecraft. They have been used for detailed rotationally-resolved mineralogical/compositional analysis. -
bundle:
Fieber-Beyer IRTF Mainbelt Asteroid Spectra V2.0
The data set contains observations obtained with the NASA IRTF SpeX instrument covering the 0.7 to 2.5 micron near-infrared portion of the spectrum. The data set archives reduced, calibrated spectra which were obtained by Sherry Fieber-Beyer. -
collection:
Gaffey Meteorite Spectra V1.0
This data set contains 166 laboratory spectra of 108 meteorite samples, as reported by M. J. Gaffey in Gaffey (1976) [GAFFEY1976]. This in turn was based on his PhD thesis work (Gaffey 1974 [GAFFEY1974]). -
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. -
collection:
data collection for the "REDDY NEAR-EARTH AND MARS-CROSSING ASTEROIDS" bundle
This is the data collection for the ast_spectra_reddy_neos_marscrossers bundle. This data set contains low-resolution (R~150) near-infrared (0.7-2.5 microns) spectra of 27 asteroids, 5 Mars-crossing and 22 near-Earth asteroids, observed with the SpeX instrument on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i. This data set archives reduced, calibrated spectra of targets of opportunity observed from 2001 to 2008. -
collection:
document collection for the "REDDY VESTA ROTATIONALLY RESOLVED NEAR-INFRARED SPECTRA" bundle
This is the document collection for the gbo.ast-vesta.reddy.spectra bundle. This data set contains low-resolution near-infrared (~0.7-2.5 microns) spectra of main belt asteroid (4) Vesta observed with the SpeX instrument on NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i, and reported in Reddy et al. (2011). This data set archives reduced, calibrated spectra that were obtained as part of ground-based characterization of Vesta prior to the arrival of Dawn spacecraft. They have been used for detailed rotationally-resolved mineralogical/compositional analysis. -
collection:
document collection for the "REDDY NEAR-EARTH AND MARS-CROSSING ASTEROIDS" bundle
This is the document collection for the ast_spectra_reddy_neos_marscrossers bundle. This data set contains low-resolution (R~150) near-infrared (0.7-2.5 microns) spectra of 27 asteroids, 5 Mars-crossing and 22 near-Earth asteroids, observed with the SpeX instrument on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i. This data set archives reduced, calibrated spectra of targets of opportunity observed from 2001 to 2008. -
bundle:
Gaffey Meteorite Spectra V1.0
This data set contains 166 laboratory spectra of 108 meteorite samples, as reported by M. J. Gaffey in Gaffey (1976) [GAFFEY1976]. This in turn was based on his PhD thesis work (Gaffey 1974 [GAFFEY1974]). -
bundle:
FIEBER-BEYER IRTF MAINBELT ASTEROID SPECTRA
The data set contains observations obtained with the NASA IRTF SpeX instrument covering the 0.7 to 2.5 micron near-infrared portion of the spectrum. The data set archives reduced, calibrated spectra which were obtained and used in Sherry Fieber-Beyer's Ph.D. dissertation at the University of North Dakota and archives reduced, calibrated spectra subsequent 2010. The research focused on asteroids in a zone centered on the 3:1 resonance. These spectra were used to mineralogically characterize asteroids in this zone in an attempt to identify their meteorite analogs. -
bundle:
IRTF NEAR-IR SPECTROSCOPY OF ASTEROIDS
This data set contains low-resolution, near-infrared (0.8 - 2.5 micron) spectra of asteroids obtained with SpeX at the NASA Infrared Telescope Facility (IRTF) on Mauna Kea. Since it was commissioned in June 2000, SpeX has been the premier instrument for producing high quality near-IR spectra of asteroids. These spectra have been used for both taxonomic studies of asteroids, and for more detailed mineralogical and compositional investigations. This data set archives the reduced, calibrated spectra that have been published in the peer-reviewed literature, and will be regularly updated as more data become publicly available. -
bundle:
VILAS ASTEROID SPECTRA
This data set contains 81 published spectra of asteroids obtained by Faith Vilas during the years 1982 - 1992. -
bundle:
FORNASIER SPECTRA OF M ASTEROIDS
This data set contains reduced composite visual and near-infrared spectra of thirty M-type asteroids, observed over the years 2004-2008 and presented in Fornasier et al. (2010). The spectra were taken with the Dolores and NICS instruments at the Telescopio Nationale Galileo (TNG) in La Palma, with the EMMI and SOFI instruments at the ESO New Technology Telescope (NTT) in Chile, and with the SPeX instrument at the Infrared Telescope Facility (IRTF) in Hawaii. The individual spectra from the various instruments used to produce the composite spectra are also included. -
bundle:
REDDY MAIN BELT ASTEROID SPECTRA
This data set contains low-resolution (R~150) near-infrared (0.7-2.5 microns) spectra of 90 main belt asteroids observed with the SpeX instrument on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i. This data set archives reduced, calibrated spectra of targets of opportunity observed from 2001 to 2012. -
bundle:
Sawyer Asteroid Spectra V1.0
This data set contains 94 optical asteroid spectra obtained by Scott Sawyer as part of his Ph.D. dissertation at the University of Texas at Austin. Observational circumstances and processing level are also provided. -
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:
Sawyer Asteroid Spectra V1.0
This data set contains 94 optical asteroid spectra obtained by Scott Sawyer as part of his Ph.D. dissertation at the University of Texas at Austin. Observational circumstances and processing level are also provided. -
collection:
Gaffey Meteorite Spectra V1.0
This data set contains 166 laboratory spectra of 108 meteorite samples, as reported by M. J. Gaffey in Gaffey (1976) [GAFFEY1976]. This in turn was based on his PhD thesis work (Gaffey 1974 [GAFFEY1974]). -
collection:
data collection for the "REDDY MAIN BELT ASTEROID SPECTRA" bundle
This is the data collection for the gbo.ast-mb.reddy.spectra bundle. This data set contains low-resolution (R~150) near-infrared (0.7-2.5 microns) spectra of 90 main belt asteroids observed with the SpeX instrument on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i. This data set archives reduced, calibrated spectra of targets of opportunity observed from 2001 to 2012. -
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. -
collection:
document collection for the "FORNASIER SPECTRA OF M ASTEROIDS" bundle
This is the document collection for the gbo.ast-m-type.fornasier.spectra bundle. This data set contains reduced composite visual and near-infrared spectra of thirty M-type asteroids, observed over the years 2004-2008 and presented in Fornasier et al. (2010). The spectra were taken with the Dolores and NICS instruments at the Telescopio Nationale Galileo (TNG) in La Palma, with the EMMI and SOFI instruments at the ESO New Technology Telescope (NTT) in Chile, and with the SPeX instrument at the Infrared Telescope Facility (IRTF) in Hawaii. The individual spectra from the various instruments used to produce the composite spectra are also included. -
collection:
Fieber-Beyer IRTF Mainbelt Asteroid Spectra V2.0
The data set contains observations obtained with the NASA IRTF SpeX instrument covering the 0.7 to 2.5 micron near-infrared portion of the spectrum. The data set archives reduced, calibrated spectra which were obtained by Sherry Fieber-Beyer and archives reduced, calibrated spectra. -
collection:
Gartrelle et al. IRTF Asteroid Spectra V1.0
This data set is comprised of the VNIR (0.69-2.5 micron) spectra of twenty-five D-type asteroids from varying Solar System locations. The spectra were obtained from NASA/IRTF on Mauna Kea between 2016-2019 using the SpeX instrument in Low-Resolution Prism mode and the 0.8 x 15" slit. Guiding was performed using spillover light from the slit (GuideDog) for targets with apparent magnitude > 15.5. For targets fainter than magnitude 15.5, guiding was accomplished using the MORIS CCD imager. -
collection:
document collection for the "FIEBER-BEYER IRTF MAINBELT ASTEROID SPECTRA" bundle
This is the document collection for the gbo.ast.fieber-beyer.spectra bundle. The data set contains observations obtained with the NASA IRTF SpeX instrument covering the 0.7 to 2.5 micron near-infrared portion of the spectrum. The data set archives reduced, calibrated spectra which were obtained and used in Sherry Fieber-Beyer's Ph.D. dissertation at the University of North Dakota and archives reduced, calibrated spectra subsequent 2010. The research focused on asteroids in a zone centered on the 3:1 resonance. These spectra were used to mineralogically characterize asteroids in this zone in an attempt to identify their meteorite analogs. -
collection:
Sawyer Asteroid Spectra V1.0
This data set contains 94 optical asteroid spectra obtained by Scott Sawyer as part of his Ph.D. dissertation at the University of Texas at Austin. Observational circumstances and processing level are also provided. -
collection:
IRTF Near-IR Imaging of Comet 9P/Tempel 1 during Deep Impact Encounter
Near-IR images of Comet 9P/Tempel 1 were obtained at the NASA IRTF during the period from June 24 through July 17, 2005 UT. These observations were taken as part of a campaign designed to support the science objectives of the Deep Impact spacecraft around the time of its encounter with Tempel 1. This data set contains all raw images, including those required for reduction and photometric calibration of the comet observations. These data were migrated from the PDS3 dataset DI/EAR-C-I0046-2-IRTF-NIRIMG-TMPL1-V1.0. -
collection:
data collection for the "FORNASIER SPECTRA OF M ASTEROIDS" bundle
This is the data collection for the gbo.ast-m-type.fornasier.spectra bundle. This data set contains reduced composite visual and near-infrared spectra of thirty M-type asteroids, observed over the years 2004-2008 and presented in Fornasier et al. (2010). The spectra were taken with the Dolores and NICS instruments at the Telescopio Nationale Galileo (TNG) in La Palma, with the EMMI and SOFI instruments at the ESO New Technology Telescope (NTT) in Chile, and with the SPeX instrument at the Infrared Telescope Facility (IRTF) in Hawaii. The individual spectra from the various instruments used to produce the composite spectra are also included. -
collection:
Fieber-Beyer IRTF Mainbelt Asteroid Spectra V2.0
The data set contains observations obtained with the NASA IRTF SpeX instrument covering the 0.7 to 2.5 micron near-infrared portion of the spectrum. The data set archives reduced, calibrated spectra which were obtained by Sherry Fieber-Beyer and archives reduced, calibrated spectra. -
collection:
Gartrelle et al. IRTF Asteroid Spectra V1.0
This data set is comprised of the VNIR (0.69-2.5 micron) spectra of twenty-five D-type asteroids from varying Solar System locations. The spectra were obtained from NASA/IRTF on Mauna Kea between 2016-2019 using the SpeX instrument in Low-Resolution Prism mode and the 0.8 x 15" slit. Guiding was performed using spillover light from the slit (GuideDog) for targets with apparent magnitude > 15.5. For targets fainter than magnitude 15.5, guiding was accomplished using the MORIS CCD imager. -
collection:
data collection for the "REDDY VESTA ROTATIONALLY RESOLVED NEAR-INFRARED SPECTRA" bundle
This is the data collection for the gbo.ast-vesta.reddy.spectra bundle. This data set contains low-resolution near-infrared (~0.7-2.5 microns) spectra of main belt asteroid (4) Vesta observed with the SpeX instrument on NASA Infrared Telescope Facility (IRTF) on Mauna Kea, Hawai'i, and reported in Reddy et al. (2011). This data set archives reduced, calibrated spectra that were obtained as part of ground-based characterization of Vesta prior to the arrival of Dawn spacecraft. They have been used for detailed rotationally-resolved mineralogical/compositional analysis. -
collection:
data collection for the "FIEBER-BEYER IRTF MAINBELT ASTEROID SPECTRA" bundle
This is the data collection for the gbo.ast.fieber-beyer.spectra bundle. The data set contains observations obtained with the NASA IRTF SpeX instrument covering the 0.7 to 2.5 micron near-infrared portion of the spectrum. The data set archives reduced, calibrated spectra which were obtained and used in Sherry Fieber-Beyer's Ph.D. dissertation at the University of North Dakota and archives reduced, calibrated spectra subsequent 2010. The research focused on asteroids in a zone centered on the 3:1 resonance. These spectra were used to mineralogically characterize asteroids in this zone in an attempt to identify their meteorite analogs. -
collection:
data collection for the "IRTF NEAR-IR SPECTROSCOPY OF ASTEROIDS " bundle
This is the data collection for the gbo.ast.irtf-spex-collection.spectra bundle. This data set contains low-resolution, near-infrared (0.8 - 2.5 micron) spectra of asteroids obtained with SpeX at the NASA Infrared Telescope Facility (IRTF) on Mauna Kea. Since it was commissioned in June 2000, SpeX has been the premier instrument for producing high quality near-IR spectra of asteroids. These spectra have been used for both taxonomic studies of asteroids, and for more detailed mineralogical and compositional investigations. This data set archives the reduced, calibrated spectra that have been published in the peer-reviewed literature, and will be regularly updated as more data become publicly available. -
collection:
document collection for the "VILAS ASTEROID SPECTRA" bundle
This is the document collection for the gbo.ast.vilas.spectra bundle. This data set contains 81 published spectra of asteroids obtained by Faith Vilas during the years 1982 - 1992. -
collection:
document collection for the "IRTF NEAR-IR SPECTROSCOPY OF ASTEROIDS " bundle
This is the document collection for the gbo.ast.irtf-spex-collection.spectra bundle. This data set contains low-resolution, near-infrared (0.8 - 2.5 micron) spectra of asteroids obtained with SpeX at the NASA Infrared Telescope Facility (IRTF) on Mauna Kea. Since it was commissioned in June 2000, SpeX has been the premier instrument for producing high quality near-IR spectra of asteroids. These spectra have been used for both taxonomic studies of asteroids, and for more detailed mineralogical and compositional investigations. This data set archives the reduced, calibrated spectra that have been published in the peer-reviewed literature, and will be regularly updated as more data become publicly available.
Data Sets and Information