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Telescope observations, star catalogs, exoplanet surveys, galaxy morphology, gravitational waves, spectroscopy
3,259 datasets
ROSETTA-ORBITER PRELANDING OSIWAC 3 RDR MTP007 V2.0 contains images from the Rosetta mission's OSIRIS Wide Angle Camera. The dataset covers the prelanding phase at comet 67P/Churyumov-Gerasimenko from September 2 to September 23, 2014. This version, V2.0, merges two previous dataset deliveries and is provided by the National Aeronautics and Space Administration.
A global map of iron concentration within the regolith of asteroid 1 Ceres, provided on twenty-degree quasi-equal-area pixels. Iron concentrations were determined from gamma ray data acquired by NASA's Dawn spacecraft in a low altitude mapping orbit about 385 km from the surface. The methods used to determine iron concentration are described by PRETTYMANETAL2017.
Raw magnetometer data from the ROSETTA orbiter's RPCMAG instrument, collected during the EXTENDED MISSION PHASE 2 near comet 67P/Churyumov-Gerasimenko. The dataset covers observations from April 6 to June 29, 2016 and is provided by the National Aeronautics and Space Administration. This version, V9.0, includes updates to documentation and quality flagging for consistency with other data releases.
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.
The Rosetta mission's OSIRIS Narrow Angle Camera captured images of comet 67P/Churyumov–Gerasimenko during its prelanding phase. This dataset contains those images from September 2 to September 23, 2014, and is version 2.0, which merges two previous dataset deliveries. The data was provided by the National Aeronautics and Space Administration (NASA).
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).
OSIRIS Narrow Angle Camera images were acquired during the Rosetta mission's prelanding phase at comet 67P/Churyumov–Gerasimenko. The dataset covers the period from 2014-06-04 to 2014-07-02 and is version V2.0, which merges two previous dataset deliveries. The data originates from the National Aeronautics and Space Administration.
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.
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.
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.