Found 30 datasets matching "354-eleonora".
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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: 25.77 | 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: 21.32 | 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: 21.04 | Views last month: 0 -
Compilation of published polarimetry for 123 numbered asteroids.
Search relevance: 16.13 | 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: 15.78 | 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: 15.69 | Views last month: 0 -
Compilation of published polarimetry for 123 numbered asteroids.
Search relevance: 15.54 | Views last month: 0 -
52-color IR Spectra of Numbered Asteroids.
Search relevance: 15.54 | Views last month: 0 -
52-color IR Spectra of Numbered Asteroids.
Search relevance: 15.54 | 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: 15.54 | 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: 12.45 | 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: 11.81 | 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: 11.81 | 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: 8.10 | 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: 7.94 | 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: 7.94 | 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: 7.94 | 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: 7.80 | Views last month: 0 -
Small Main-Belt Asteroid Spectrographic Survey over the visual range.
Search relevance: 7.33 | Views last month: 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-Dartmouth-MIT (McGraw Hill)...
Search relevance: 7.33 | Views last month: 0
