Found 28 datasets matching "46-hestia".
-
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,...
Search relevance: 24.36 | Views last month: 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,...
Search relevance: 24.26 | Views last month: 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,...
Search relevance: 24.22 | Views last month: 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...
Search relevance: 21.38 | Views last month: 0 -
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...
Search relevance: 19.21 | Views last month: 0 -
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...
Search relevance: 18.73 | Views last month: 0 -
This data set contains 52-color IR data of asteroids, taken using a double circularly variable filter. The short wavelength portion of the CVF covered the octave from 0.8 to 1.6 microns with...
Search relevance: 14.21 | Views last month: 0 -
This data set contains 52-color IR data of asteroids, taken using a double circularly variable filter. The short wavelength portion of the CVF covered the octave from 0.8 to 1.6 microns with 3...
Search relevance: 14.21 | Views last month: 0 -
Compilation of published polarimetry for 123 numbered asteroids.
Search relevance: 14.11 | Views last month: 0 -
Compilation of published polarimetry for 123 numbered asteroids.
Search relevance: 13.84 | Views last month: 0 -
52-color IR Spectra of Numbered Asteroids.
Search relevance: 13.84 | Views last month: 0 -
52-color IR Spectra of Numbered Asteroids.
Search relevance: 13.84 | Views last month: 0 -
This data set contains 52-color IR data of asteroids, taken using a double circularly variable filter. The short wavelength portion of the CVF covered the octave from 0.8 to 1.6 microns with 3...
Search relevance: 13.84 | Views last month: 0 -
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...
Search relevance: 10.34 | Views last month: 0 -
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...
Search relevance: 10.34 | Views last month: 0 -
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...
Search relevance: 10.33 | Views last month: 0 -
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 asteroids, as published in...
Search relevance: 7.15 | Views last month: 1 -
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).
Search relevance: 7.15 | Views last month: 0 -
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...
Search relevance: 7.15 | Views last month: 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).
Search relevance: 7.09 | Views last month: 0
