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Dataset results
587 results for “asteroids”
SAWYER ASTEROID SPECTRA
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.
SDSS-BASED ASTEROID TAXONOMY V1.1
The Sloan Digital Sky Survey Moving Object Catalog (SDSS-MOC) is a large data set that provides five-filter magnitudes and astrometric information for all moving objects identified in the SDSS images (Izevic et al., 2010). The photometric observations were classified by Carvano et al. (2010) into nine taxonomic classes: Vp, Op, Qp, Sp, Ap, Lp, Dp, Xp and Cp, which are related to the classes and complexes of Bus Taxonomy (Bus & Binzel, 2002b). This data set is contains the taxonomic classification of each SDSS detections and its compilation for each observed asteroid.
EIGHT COLOR ASTEROID SURVEY MEAN DATA V1.0
The eight color asteroid survey provides reflection spectra for minor planets using eight filter passbands. This dataset includes mean data averaged for each of 589 minor planets. The primary data for these minor planets, the response curves for the filters, and the values determined for standard stars, are included in other related datasets. The wavelength range covered is .33 to 1.04 micrometers.
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).
Gazetteer of Planetary Nomenclature: Asteroids: Steins
These images display asteriods documented and approved by the International Astronomical Union (IAU).
ASTEROID MASSES V1.0
This collection of asteroid masses and densities was compiled from the published literature by Jim Baer, Steve Chesley, and Dan Britt. This is the version of the compilation as of January 7, 2009.
ASTEROID PROPER ELEMENTS V1.0
Proper elements of asteroids are derived from the osculating orbital elements by correcting for the perturbations of the major planets to arrive at elements which are stable over time periods comparable to the age of the solar system. The purpose of computing proper elements is twofold, to detect asteroid 'families', which are dynamically related groupings of asteroids potentially of common origin, and to understand the dynamical structure of the asteroid belt.
ASTEROID RADAR V3.0
This dataset is intended to include all groundbased asteroid radar detections. These data were collected from the published literature by Dr. Steven J. Ostro. Observations which have not yet been published, or which have been reported only in an abstract, are included in the dataset as an entry with blank data fields, for the purpose of informing the dataset users of the existence of these detections. As the data from these detections are published, the data are added to this dataset in yearly updates.
ASTEROID ABSOLUTE MAGNITUDES V8.0
Absolute magnitudes and slopes, mostly IAU-adopted with exceptions noted, for all asteroids numbered as of the 2004 April 15 batch of Minor Planet Circulars
SUBMILLIMETER LIGHTCURVES OF ASTEROIDS V1.0
Submillimeter lightcurves of large asteroids Ceres, Davida, Io, Juno, Pallas, Vesta, and Victoria, observed at the Heinrich-Hertz Submillimeter Telescope from January 2003 through May 2004.
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 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.
ASTEROID SPIN VECTORS V4.0
This is a tabulation of determinations of asteroid pole orientations gathered from the literature from 1932 through 1995. It is an updated (Dec. 1995) version of the tabulation given in Magnusson (1989) [MAGNUSSON1989] in the Asteroids II book. For more information about the Uppsala Asteroid Database, of which this collection is a part, see Magnusson et al. 1993 [MAGNUSSONETAL1993].
EIGHT COLOR ASTEROID SURVEY V4.0
This data set contains the reflectance spectra and associated data of the Eight Color Asteroid Survey (ECAS), including results for 589 asteroids.
SDSS-BASED ASTEROID TAXONOMY V1.0
This data set contains Sloan Digital Sky Survey (SDSS) asteroid photometric observations classified according to the SDSS-based Asteroid Taxonomy, as developed by Carvano et al. (2010).
MOTHE-DINIZ ASTEROID DYNAMICAL FAMILIES V1.0
This dataset contains an updated compilation of asteroid families and clusters, resulting from the application of the Hierarchical Clustering Method (HCM) on a set of around 120,000 asteroids with available proper elements. Whenever available, the classification in the Bus taxonomy is provided for family members, based on spectra from the SMASS, SMASS2 and S3OS2 spectroscopic surveys.
ASTEROID RADAR V17.0
This data set is intended to include all published groundbased asteroid radar detections. The file is based on the collection of asteroid radar detections established by Steven J. Ostro and currently maintained by Lance A.M. Benner. The file includes disc-integrated radar properties extracted from the published papers.
RIVKIN THREE MICRON ASTEROID DATA V1.0
This data set includes 3-micron spectra of asteroids taken by Andy Rivkin (1995) [RIVKINETAL1995]. The spectra include both measured reflectance and error bars at six points in the range 1.25-3.35 microns. 17 spectra of 16 different asteroids are included.
ASTEROID POLARIMETRIC DATABASE V7.0
The Asteroid Polarimetric Database (APD) is a collection of asteroid polarimetry results compiled by D.F. Lupishko and S.V. Vasiliev of Karazin Kharkiv National University, Ukraine. It is intended to include most asteroid polarimetry available through March 7, 2012.
Asteroids - NeoWs API
NeoWs (Near Earth Object Web Service) is a RESTful web service for near earth Asteroid information. With NeoWs a user can: search for Asteroids based on their closest approach date to Earth, lookup a specific Asteroid with its NASA JPL small body id, as well as browse the overall data-set.
ASTEROID RADAR V14.0
This data set is intended to include all published groundbased asteroid radar detections. The entries were collected by Steven J. Ostro, and selected data have been collected from the published literature.
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Allen Brain Atlas
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DANDI Archive for NWB datasets
DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.
International Brain Laboratory public data
The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.
OpenNeuro
OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.