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Telescope observations, star catalogs, exoplanet surveys, galaxy morphology, gravitational waves, spectroscopy
2,943 datasets
16,259 spurious examples and 1,639 real pulsar examples collected during the HTRU survey. The dataset describes pulsar candidates for binary classification, with all examples checked by human annotators. It was created by Dr Robert Lyon from the University of Manchester using the PulsarFeatureLab tool.
Monte Carlo generated data simulating the registration of high-energy gamma particles in a ground-based atmospheric Cherenkov telescope. The dataset was created for a classification benchmark on numerical features, using the Corsika simulation program. It was donated by P. Savicky from the Institute of Computer Science, AS of CR, Czech Republic, and originates from the UCI repository.
MagicTelescope is a dataset used in a tabular data benchmark, originally from the UCI repository. The data are Monte Carlo generated to simulate the registration of high-energy gamma particles in a ground-based atmospheric Cherenkov gamma telescope using the imaging technique. It was created by the MAGIC project and donated by P. Savicky of the Institute of Computer Science, AS of CR, Czech Republic.
Monte Carlo-generated data simulates the registration of high-energy gamma particles in a ground-based atmospheric Cherenkov telescope. The dataset belongs to a benchmark for regression on numerical features and was originally sourced from the UCI Machine Learning Repository. It contains parameters derived from shower image patterns, known as Hillas parameters, used to discriminate gamma-ray signals from cosmic-ray background.
Monte Carlo generated data simulating the registration of high-energy gamma particles in a ground-based atmospheric Cherenkov gamma telescope. The dataset was created using the Corsika simulation program and belongs to a benchmark for regression on numerical features. It was donated by P. Savicky from the Institute of Computer Science, AS of CR, Czech Republic, and originates from the MAGIC telescope project.
Monte Carlo generated data simulating the registration of high-energy gamma particles in a ground-based atmospheric Cherenkov telescope. The dataset was created using the Corsika simulation program and is part of a benchmark for regression on numerical features. It was donated by P. Savicky from the Institute of Computer Science, AS of CR, Czech Republic, and the original source is the UCI Machine Learning Repository.
MagicTelescope is a dataset for classification on numerical features, used in a tabular data benchmark. The data were generated by a Monte Carlo program (Corsika) to simulate the registration of high-energy gamma particles in a ground-based atmospheric Cherenkov gamma telescope. The dataset was donated by P. Savicky from the Institute of Computer Science, AS of CR, Czech Republic, and originates from the MAGIC (Major Atmospheric Gamma Imaging Cherenkov) Telescope project.
Titled MagicTelescope and is sourced from the OpenML platform. No information is available regarding its contents, size, authorship, or temporal coverage.
Ulysses spacecraft's High Energy Telescope recorded instantaneous housekeeping parameters like voltages and temperatures every 256 seconds to monitor instrument health. Data files are listed readout-by-readout with timestamps in fractional year, day of year, and milliseconds of day. The National Aeronautics and Space Administration provides these raw, unprocessed measurements with no noise removal or averaging applied.
Ulysses GAS experiment data provides pixel map data and image files for sky maps generated from measurements of neutral helium atoms flowing into the heliosphere. The dataset includes accumulated counts and Ecliptic angle coordinates in ASCII files, with full images provided in GIF and PostScript formats. It was produced by the National Aeronautics and Space Administration, with key methods described in publications from 1992 and 1996.
Vega 1 spacecraft magnetic field data averaged over 2.5-minute intervals from December 1984 to March 1986. The dataset includes measurements from the cruise phase to Venus and after its flyby, presented in spacecraft coordinates and solar ecliptic coordinates. Data was provided by the National Aeronautics and Space Administration.
Daily files contain readout-by-readout listings of counts accumulated in 18 spin-averaged counting rates (H10-H27) from the Ulysses spacecraft's High Energy Telescope. The data includes heavy ion counts in four energy ranges (26-36, 44-127, 127-173, and >173 MeV/n) and single detector health counts, with each line representing a readout interval averaging 128 seconds. The dataset is provided by the National Aeronautics and Space Administration (NASA) and was last updated in March 2026.
Vega 2 Magnetic Field Data provides 2.5-minute averaged magnetic field measurements from the Vega 2 spacecraft mission. The data, provided by the National Aeronautics and Space Administration, covers the cruise phase from Earth to Venus (December 1984 to June 1985) and the period after the Venus flybys up to the encounter with Comet Halley in March 1986. Measurements are presented in different coordinate systems depending on the spacecraft's orientation phase.
180 unique winegrape leaves with measured trait values and untransformed reflectance spectroscopy data. The dataset supports the 2025 manuscript "Predicting leaf traits in wine grapes with reflectance spectroscopy". It was authored by Rachel Mariani and harvested from the Borealis Dataverse platform.
Harvey's 2009 PhD thesis contributed this spectral library of marine benthic habitats to the Australian National Spectral Database. Data was collected from Rottnest, Marmion, and Shoalwater sites during 2006-2007. The library is hosted by the Australian Ocean Data Network.
Spectral data records for marine benthic habitats are hosted in the National Spectral Database. The library was developed from research by Murdoch University for classifying habitats in oligotrophic, temperate waters. The underlying data was collected during field campaigns in 2006 and 2007.
Derived radial profiles of Saturn's rings were created from stellar occultations observed by the Cassini spacecraft's VIMS instrument. The data originates from the Cassini nominal mission, managed by the National Aeronautics and Space Administration. This dataset captures ring structure details from observations made between 2005 and 2009.
24467 bytes of data accompany a paper addressing a stabilization problem for a coupled string-beam system with damping of indefinite sign. The dataset likely contains results from detailed spectral analysis, including eigenvalue distributions, used to determine stability conditions. It provides a mathematical model for studying the spectrum of a partial differential equation system.
NASA's Rosetta spacecraft OSIRIS Narrow Angle Camera data set contains radiometric calibrated and geometric distortion corrected image data in W/m^2/sr/nm. The data covers the PRELANDING mission phase from 2014-05 07 to 2014-06-04, with the prime target being comet 67P/Churyumov-Gerasimenko. This version V2.0 includes corrections from an external peer review, updated documentation, and improved handling of images with missing packets.
79 ks of combined archival Chandra X-Ray Observatory observations of the starburst galaxy NGC 4214, conducted in 2001 and 2004. The catalog contains 116 high-significance X-ray point sources down to a limiting luminosity of ~5e35 erg/s, produced by NASA HEASARC in September 2015. It includes hardness ratios, spectral analysis, and cross-correlations with Hubble Space Telescope data for preliminary source classification.