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Telescope observations, star catalogs, exoplanet surveys, galaxy morphology, gravitational waves, spectroscopy
2,973 datasets
This dataset supports research on human presence detection using Wi-Fi range-filtered Doppler spectrum, as presented in a 2026 IEEE PerCom workshop paper by Jessica Bartholdy Sanson, Rahul C. Shah, and Valerio Frascolla. It contains time series data tagged for Wi-Fi, Doppler Spectrum, and Wireless Sensing.
Kaggle hosts a dataset titled 'Stellar Dataset'. The dataset's content likely pertains to stars or astronomical objects. The author, organization, and specific details about its creation are unknown.
A NASA mission led by the California Institute of Technology, the Galaxy Evolution Explorer Satellite (GALEX) collected ultraviolet data to investigate star formation evolution. The data likely contains direct images in near-UV (NUV) and far-UV (FUV) bands, as well as low-resolution spectroscopy. The dataset is hosted by the Space Telescope Science Institute and is available in S3 format.
The Transiting Exoplanet Survey Satellite (TESS) is a multi-year NASA mission that has discovered exoplanets orbiting bright stars across the entire sky using high-precision photometry. The data is hosted on AWS Open Data and originates from the Space Telescope Science Institute. The survey also enables studies in stellar astrophysics, solar system science, and extragalactic variability.
A decision model dataset supporting a manuscript on applying Value-Focused Thinking to evaluate outer solar system destinations for human exploration. The data was shared by author Fan Bu via Harvard Dataverse to accompany the academic publication. It was last updated in March 2026.
Two experiments from Cape Evans investigated the effects of UV-B radiation on sea ice algal growth and productivity. A 15-day in-situ study measured biomass under four light treatments, while a lab experiment subjected cores to varying UV-B and PAR irradiances. The data was collected by SCIOPS and published in November 1997.
Seasonal Integrated Albedo data provides modeled percentages of incoming radiation reflected into space for snow-free land conditions. The dataset includes four files representing winter, spring, summer, and autumn seasons, derived from vegetation and cultivation intensity maps. It was produced by CEOS_EXTRA and last updated in 1991.
Martian radii and elevations relative to the 6 millibar reference surface, measured against the JPL DE_118 ephemeris. The data were obtained by the Goldstone Solar System Radar during the oppositions spanning 1971 to 1982. The table's present form was generated by R. Mehlman at UCLA/IGPP.
Derived data products from the Rosetta spacecraft's RPC-LAP instrument during the pre-landing phase at comet 67P/Churyumov-Gerasimenko. The dataset contains high-level measurements in physical units, including electron density, electron temperature, and spacecraft potential. It was produced by the National Aeronautics and Space Administration and last updated in March 2026.
The Rosetta spacecraft OSIRIS Wide Angle Camera captured this data during the STEINS FLY-BY mission phase from August 4 to October 5, 2008. It contains solar stray light corrected, radiometric calibrated, and geometric distortion corrected image data in units of W/m^2/sr/nm. This V1.0 dataset was produced by the National Aeronautics and Space Administration.
Asteroid 21 Lutetia was imaged by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft between 2010-05 17 and 2010-09-03. This CODMAC level 4 dataset contains radiometric calibrated and geometric distortion corrected image data in reflectance units. The data was produced by the National Aeronautics and Space Administration and represents the first version (V1.0) of this dataset.
From 2008-08-04 to 2008-10-05, this dataset contains solar stray light corrected, radiometric calibrated, and geometric distortion corrected image data in reflectance units. It was acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the STEINS fly-by mission phase, targeting asteroid 2867 Steins. The data is provided by the National Aeronautics and Space Administration and is version V1.0.
OSIRIS Narrow Angle Camera images of asteroid 2867 Steins, corrected for solar stray light and radiometrically calibrated. The dataset covers the fly-by period from August 4 to October 5, 2008, and is the first version (V1.0) of this processed data. It was produced by the National Aeronautics and Space Administration.
Solar stray light corrected, radiometric calibrated, and geometric distortion corrected image data in W/m^2/sr/nm acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft. The dataset covers the Lutetia fly-by mission phase from 2010-05-17 to 2010-09-03, with the prime target being asteroid 21 Lutetia. This V1.0 dataset is the first version of this data product from NASA.
From 2010-05-17 to 2010-09-03, the Rosetta spacecraft's OSIRIS Narrow Angle Camera captured uncalibrated image data of asteroid 21 Lutetia. This dataset contains the raw digital number (DN) unit images from that fly-by mission phase. The data was produced by the National Aeronautics and Space Administration and reprocessed after an October 2018 external review.
A collection of far-infrared polarization maps from the SOFIA/HAWC+ instrument, covering nearby galactic star-forming regions. The data includes FITS files containing Stokes I, Q, and U parameters, their errors, and derived percent polarization and angle. The collection is associated with the paper 'Far-infrared Polarization Properties of Nearby Star-Forming Regions: A New Compendium of SOFIA/HAWC+ Observations' by Karpovich et al., and was last updated on March 17, III.
Radiometric calibrated and geometric distortion corrected image data in reflectance units from the OSIRIS Wide Angle Camera on the Rosetta spacecraft. The dataset covers the LUTETIA FLY-BY mission phase from 2010-05 17 to 2010-09-03, with the prime target being asteroid 21 Lutetia. This V1.0 dataset was produced by the National Aeronautics and Space Administration.
Derived data from the Rosetta spacecraft's RPC-LAP instrument, acquired during the ROSETTA EXTENSION 2 mission phase targeting comet 67P/Churyumov-Gerasimenko. The dataset contains high-level data products in physical units, such as electron density, electron temperature, and spacecraft potential. It was published by the National Aeronautics and Space Administration and last updated on March 13, -2026.
The DWE dataset contains sky frequencies measured at the Green Bank and Parkes telescopes and retrieved zonal wind speed along the descent path of the Huygens probe. It was produced by the National Aeronautics and Space Administration and last updated in March 2026. The dataset includes geometrical parameters used to separate the Huygens velocity components and associated documentation.
From 2010-05-17 to 2010-09-03, the Rosetta spacecraft's OSIRIS Narrow Angle Camera captured images of asteroid 21 Lutetia. This dataset contains processed, calibrated, and corrected image data in reflectance units, representing the first version (V1.0) of this collection. The data was produced by the National Aeronautics and Space Administration (NASA).