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Telescope observations, star catalogs, exoplanet surveys, galaxy morphology, gravitational waves, spectroscopy
2,951 datasets
NASA's Rosetta spacecraft acquired this radiometric calibrated image data of comet 67P/Churyumov-Gerasimenko using the OSIRIS Narrow Angle Camera. The dataset covers the period from 2014-09 02 to 2014-09-23 during the PRELANDING mission phase. Version 3.0 includes corrections from peer reviews, updated documentation, and improved handling of image quality issues.
V3.0 radiometric calibrated image data in W/m^2/sr/nm, acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the ROSETTA EXTENSION 2 mission phase from 2016-05 31 to 2016-06-28. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This CODMAC level 3 dataset from NASA supersedes previous versions with corrections from 2018 peer reviews and improvements to calibration and documentation.
Uncalibrated image data in DN units acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the PRELANDING mission phase. The data covers the period from 2014-09 02T10:00:00.000 to 2014-09-23T09:59:59.000, with the prime target being comet 67P/Churyumov-Gerasimenko. This version V3.0 dataset from NASA supersedes previous deliveries with updated documentation, ancillary files, and improved handling of image quality issues.
Uncalibrated image data acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the ROSETTA EXTENSION 2 mission phase. The dataset covers the period from 2016-04-05T23:25:00.000 to 2016-05-03T23:25:00.000, targeting comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V3.0 supersedes previous deliveries with corrections and updates following external peer reviews.
Posterior samples and metadata for 44 gravitational-wave candidates from the first half of the LIGO-Virgo-KAGRA third observing run (O3a) and 10 binary-black-hole candidates from GWTC-1. The data release includes cosmologically reweighted and non-reweighted samples, skymaps, and analysis configuration files. The LIGO Scientific Collaboration and Virgo Collaboration produced this data using inference software like Bilby, Parallel Bilby, and RIFT.
Temperature-depth profiles collected using expendable bathythermograph (XBT) instruments across multiple oceans and seas between October 1974 and May 1976. Data was gathered from over 50 vessels, including research ships and naval vessels, and processed by the National Oceanographic Data Center (NODC) into the standard C116 format. The dataset captures ocean thermal structure at non-uniform depth intervals, focusing on inflection points to define the temperature curve.
NASA's Rosetta spacecraft OSIRIS Wide Angle Camera captured radiometric calibrated image data of comet 67P/Churyumov-Gerasimenko. The dataset covers the period from September 2 to September 26, 2016, and contains images calibrated in units of W/m^2/sr/nm. This version 3.0 includes corrections from external reviews and improvements to calibration and documentation.
Radiometric calibrated image data in W/m^2/sr/nm, acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft. The dataset covers the period from 2016-03 08T23:25:00.000 to 2016-04-05T23:24:59.000, targeting comet 67P/Churyumov-Gerasimenko. This version V3.0, delivered by the National Aeronautics and Space Administration, includes corrections from 2018 peer reviews and improved calibration for ballistic mode images.
Australia's AUSTopo series provides 516 digital topographic maps covering the continent at a 1:250,000 scale. Each standard map depicts an area of approximately 150 by 110 kilometers. The series includes natural and constructed features like road infrastructure, vegetation, hydrography, and 50-meter contours.
Radiometric calibrated image data in W/m^2/sr/nm acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the ROSETTA EXTENSION 3 mission phase. The dataset covers the period from 2016-07 26 to 2016-08-09, with the prime target being comet 67P/Churyumov-Gerasimenko. This version V3.0 data set was produced by the National Aeronautics and Space Administration and includes corrections and documentation updates from 2018 peer reviews.
Uncalibrated image data acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during its ROSETTA EXTENSION 1 mission phase. The data covers the period from 2016-02-09 to 2016-03-08, with the prime target being comet 67P/Churyumov-Gerasimenko. This version V3.0 dataset was delivered by the National Aeronautics and Space Administration and includes corrections and documentation updates following external peer reviews.
Uncalibrated image data acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft. The data covers the period from 2016-03-08 to 2016-04-05, with the prime target being comet 67P/Churyumov-Gerasimenko. This version 3.0 dataset was delivered by NASA and includes updates to documentation, file handling, and data quality keywords.
Numerical modeling analysis investigates topographic controls on post-Oligocene ice-sheet dynamics in the Prydz Bay region of East Antarctica. The study uses geological data and ice-sheet modeling to link bed morphology, bathymetric volume, and sedimentation history to changes from ice-cliff to ice-stream dynamics.
Seasonal integrated surface albedo values are derived from global vegetation and cultivation intensity maps for snow-free conditions. The data comprises four files representing winter, spring, summer, and autumn, each with a spatial resolution of one degree latitude/longitude. It was compiled by Matthews at the Goddard Institute for Space Studies and published in 1983.
A 115 square degree survey of the Equatorial SDSS Stripe 82 field conducted by the Spitzer Space Telescope. The catalog contains 5.4 million sources detected in both the 3.6 and 4.5 micron infrared bands, with additional single-band catalogs for 6.1 million and 6.4 million sources. It was produced by the National Aeronautics and Space Administration and last updated in March 2026.
The Hubble Source Catalog (HSC) is a master catalog combining tens of thousands of visit-based source lists from the Hubble Legacy Archive. It provides a single row entry for each cross-matched astronomical object, with averaged values for magnitudes and other parameters. The catalog currently contains over 16 million entries and is maintained by the National Aeronautics and Space Administration, last updated in March 2026.
The YSOVAR program obtained the first extensive mid-infrared time series photometry of the Orion Nebula Cluster and 11 other star-forming cores using the Spitzer Space Telescope. It contains light curves for approximately 29,000 unique objects in the 3.6 and 4.5 micron IRAC channels. The data is from NASA, with initial results described in 2011 and project details published in 2014.
The Kepler Target Search interface provides access to a 12.5 million row table created by the Mikulski Archive for Space Telescopes (MAST). It merges entries from the Kepler Input Catalog with the Kepler Characteristics table and associated data from multiple ground-based surveys. This dataset is intended for guest observers to locate potential targets for the Kepler space telescope.
The YSOVAR (Young Stellar Object VARiability) Spitzer Space Telescope program obtained the first extensive mid-infrared time series photometry for the Orion Nebula Cluster and 11 other star-forming cores. It contains light curves for approximately 29,000 unique objects in the 3.6 and 4.5 micron IRAC channels. The data is from NASA, with initial results described in 2011 and conventions detailed in 2014.
Over 100 million entries combine tens of thousands of visit-based source lists from the Hubble Legacy Archive into a single master catalog. The Hubble Source Catalog (HSC) is designed to optimize science from the Hubble Space Telescope, maintained by the National Aeronautics and Space Administration. The detailed search displays an entry for each separate detection or nondetection using all relevant Hubble observations for a given object.