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Telescope observations, star catalogs, exoplanet surveys, galaxy morphology, gravitational waves, spectroscopy
2,947 datasets
NASA's ROSETTA-ORBITER 67P RPCICA 4 PRL CORR-CTS V1.0 dataset contains corrected and resampled raw data from the RPCICA instrument during the mission's pre-landing phase. The data has been corrected for cross-talk and treated for noise, resulting in measurements in counts, which may include negative values. It captures measurements of the undisturbed solar wind and its interaction with the atmosphere of comet 67P.
Raw data from the RPCICA instrument on the ROSETTA mission during its flyby of asteroid Lutetia. The dataset is version 2.0, which expanded data to a uniform resolution and added new quality flags. The data was produced by the National Aeronautics and Space Administration and last updated in March 2026.
Three infrared thermal scans of comet 9P/Tempel 1's surface were acquired by the Deep Impact spacecraft's High Resolution Infrared Spectrometer on 4 July 2005, approximately 19, 12, and 5 minutes before impact. The data set includes derived temperature maps ranging from 272K to 336K with an uncertainty of +/- 7K, a high-resolution 120 m/pixel composite map, and associated incidence and emission angle maps. It was produced by the National Aeronautics and Space Administration (NASA).
Corrected and resampled raw data from the RPCICA instrument aboard the ROSETTA spacecraft during its flyby of asteroid Lutetia. The dataset has been processed for cross-talk and noise, resulting in values in counts that may include negative numbers. NASA produced this data, which was last updated on March 13, 2026.
NASA's ROSETTA orbiter magnetometer data collected in the vicinity of comet 67P/Churyumov-Gerasimenko. The dataset contains calibrated observations from the Extended Mission Phase 1, spanning from January 13 to April 6, 2016. This version (V9.0) features an improved sensor temperature model and quality flagging system.
ROSETTA-ORBITER 67P RPCMAG 2 EXT1 RAW V9.0 contains edited raw magnetometer data from the Rosetta orbiter's extended mission phase 1. The data was collected from January 13 to April 6, 2016, in the vicinity of comet 67P/Churyumov-Gerasimenko. This version 9.0 dataset is provided by the National Aeronautics and Space Administration and includes updates to documentation and quality flagging.
OSIRIS Wide Angle Camera images captured by the Rosetta spacecraft during its approach to comet 67P/Churyumov–Gerasimenko. The dataset covers a specific prelanding phase from June 4 to July 2, 2014, and is a consolidated V2.0 release from NASA that merges two previous deliveries.
NASA's Deep Impact mission acquired calibrated images of comet 9P/Tempel 1 using the Impactor Targeting Sensor Visible CCD on 03 July 2005. The dataset, processed by the EPOXI mission pipeline in Version 3.0, includes corrected observation times and adjustments for radiance product conversion. It contains images from the period after the impactor was released from the flyby spacecraft.
54-second resolution measurements of electron density and temperature from the ISEE-3/ICE spacecraft's radio mapping experiment. The data covers the two-hour interval from 10:00 to 12:00 UT on September 11, 1985, during the tail crossing of comet Giacobini-Zinner. It was provided to NASA's National Space Science Data Center by Dr. Jean-Louis Steinberg of the Observatoire de Paris.
NASA's RPCICA instrument on the ROSETTA mission collected raw data of the undisturbed solar wind and its interaction with comet 67P's atmosphere during the prelanding phase. Version 3.0 of this dataset expands data to a uniform resolution and includes new quality flags and variables. The dataset was last updated on March 13, 2026.
Geoscience Australia Data provides airborne magnetic and radiometric survey data from the Cobar, Nymagee, and Cargelligo (Euabalong) regions of New South Wales, collected between 1957 and 1958. The dataset is a legacy product, and no abstract is available. It was last updated on 2026-05-14 04:33:06.035831.
IllustrisTNG SKIRT SDSS provides preprocessed synthetic galaxy images derived from the IllustrisTNG cosmological simulations. Raw multi-band FITS images were produced with the SKIRT Monte Carlo radiative transfer code in SDSS photometric bands and processed into 128 × 128 RGB images. The dataset, created by HITS-AIN and last updated on 2026-05-07, is designed as training data for the Spherinator/HiPSter framework but is suitable for general-purpose galaxy-morphology tasks.
Charles H. Ross created this dataset to test cosmological models using Pantheon+ supernovae observations. The data includes Excel files for parameterized calculations and TIF files for generated plots, supporting the manuscript 'Testing an expanding-spacetime cosmology with Pantheon+ supernovae and early-Universe constraints'. The dataset is 2.1 MB in size and was last updated on April 14, 2026.
Carrington Maps summarize short-term and long-term coronal evolution from the STEREO mission. The maps illustrate the corona's transition from a simple two-sectored structure to a complex multi-sectored one, with distortions linked to active regions and coronal mass ejections. National Aeronautics and Space Administration provides these maps for each Carrington Rotation since the mission's start.
Synoptic maps summarize short-term and long-term coronal evolution from the STEREO mission. East and West limb maps from the Cor1 and Cor2 coronagraphs, HI1/2 imagers, and central meridian maps from the EUVI telescope are available for each Carrington Rotation since the mission's start. The maps illustrate the corona's evolution from a simple two-sectored structure to a complex multi-sectored one.
Calibrated magnetometer data from the ROSETTA orbiter's RPCMAG instrument during the EXTENDED MISSION PHASE 2, spanning from April 6 until June 29, 2016. Observations were made in the vicinity of comet 67P/Churyumov-Gerasimenko. The dataset is version 9.0 and was provided by the National Aeronautics and Space Administration.
Daily averaged intensities and counts for 24 cosmic ray elements from boron to nickel, measured by the ACE spacecraft's Cosmic Ray Isotope Spectrometer. The data covers seven energy bins per element, with energy ranges from 49-172 MeV/n for boron to 130-496 MeV/n for nickel. Calibrated science quality data is provided by NASA and accessible via FTP in HDF, CDF, and ASCII formats.
MESSENGER MASCS VIRS derived observations are spectral data from the Mercury Atmospheric and Surface Composition Spectrometer's Visible and Infrared Spectrograph. The data set, version 2.0, is produced by the National Aeronautics and Space Administration and was last updated in March 2026. It contains derived data records covering visible and near-infrared wavelengths from the MESSENGER spacecraft mission to Mercury.
Voyager 1 Planetary Radio Astronomy (PRA) data from the Jupiter encounter phase between 1979-01-06 and 1979 04-13. The dataset provides high-resolution, 6-second mean power measurements from the lowband receiver across 70 instrument channels covering 1.2 to 1326.0 kHz. Data was collected by NASA's Voyager-1 spacecraft and is calibrated in units of millibels.
NASA's STEREO mission provides synoptic maps summarizing short-term and long-term coronal evolution. The resource contains East and West limb maps from Cor1 and Cor2 coronagraphs, HI1/2-A and HI1/2-B imagers, and central meridian maps from the EUVI telescope. Maps are available for each Carrington Rotation since the mission's beginning.