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Telescope observations, star catalogs, exoplanet surveys, galaxy morphology, gravitational waves, spectroscopy
2,945 datasets
SOHO LASCO C2 Level 1.0 FITS Data contains calibrated solar corona images from the Large Angle Spectroscopic Coronagraph. The C2 instrument images the corona from 1.5 to 6 solar radii with a spatial resolution of ~23 arcsec using a 1024 x 1024 pixel CCD. Data is provided by the National Aeronautics and Space Administration.
Raw FITS image data from the LASCO C2 coronagraph aboard the SOHO spacecraft, capturing the solar corona from 1.5 to 6 solar radii. The data is produced by NASA's National Aeronautics and Space Administration and was last updated on 2026-03-13. The instrument uses a 1024 x 1024 pixel CCD with a spatial resolution of approximately 23 arcseconds.
1024 x 1024 pixel images of the solar corona captured by the LASCO C3 coronagraph aboard the SOHO spacecraft, covering a field from 3 to 30 solar radii. The data is provided in FITS format by the National Aeronautics and Space Administration (NASA) and was last updated in March 2026. The instrument uses a passively cooled CCD with a spatial resolution of 112 arcseconds and can be scheduled for various observation programs.
NASA's Interface Region Imaging Spectrograph (IRIS) provides calibrated ultraviolet images and spectra of the Sun. Images capture features as small as 240 km every 5-10 seconds at temperatures from 5,000 K to 120,000 K (up to 10 million K during flares). Spectra are obtained every 2-30 seconds along a slit, providing data on material velocity, temperature, and density in the solar atmosphere.
Geoscience Australia data details significant revisions in the age classification of marine Tertiary deposits in Australia. The description notes the recognition of Eocene deposits over a wide area in south-eastern Australia, supported by detailed mapping and the discovery of the foraminiferal genus Hantkenina. At least 4,000 feet of Middle Eocene beds have been proven in bores, and the dataset discusses reclassifications from Oligocene/Miocene to Eocene and from Oligocene to Miocene.
NASA's SOHO mission provides raw FITS data from the LASCO C1 coronagraph, which images the solar corona from 1.1 to 3 solar radii. The instrument uses a 1024 x 1024 pixel CCD and a Fabry-Perot interferometer to capture monochromatic images with a spectral resolution of 0.07 nm, enabling the derivation of line profiles and Doppler shifts. This dataset is based on the instrument described in the 1992 paper by G. E. Brueckner et al.
LASCO C2 coronagraph images capture polarized brightness of the solar corona from 1.5 to 6 solar radii. The instrument uses a 1024 x 1024 pixel CCD with a spatial resolution of ~23 arcsec and can be scheduled for observation programs. This data originates from NASA's SOHO mission, with a last update recorded in March 2026.
Percent Polarized data from the LASCO C2 coronagraph on the SOHO spacecraft. The dataset likely contains images of the solar corona from 1.5 to 6 solar radii, with a spatial resolution of approximately 23 arcseconds. The data is produced by NASA and was last updated in March 2026.
SOHO LASCO C3 Level 0.5 FITS Data provides raw images of the solar corona captured by the Large Angle Spectroscopic Coronagraph's outer instrument. The LASCO C3 coronagraph images the corona from 3 to 30 solar radii with a spatial resolution of 112 arcsec, using a 1024 x 1024 pixel CCD. This dataset is produced by the National Aeronautics and Space Administration.
Percent Polarized data from the LASCO C3 coronagraph on the SOHO spacecraft. The LASCO instrument images the solar corona from 3 to 30 solar radii using a 1024 x 1024 pixel CCD. This dataset is provided by the National Aeronautics and Space Administration (NASA) and was last updated on March 13, 2026.
Polarized Brightness data from the LASCO C3 coronagraph on the SOHO spacecraft. The instrument images the solar corona from 3 to 30 solar radii with a spatial resolution of 112 arcsec, using a 1024 x 1024 pixel CCD. The dataset is produced by the National Aeronautics and Space Administration (NASA) and was last updated in March 2026.
76 participants (40 with ASD, 36 typically developing) were assessed for autistic traits, parenting attitudes, and self-esteem. The data, authored by Kazuhiko Yamamuro and last updated in March 2026, shows children with ASD had significantly lower self-esteem than their peers. Higher autistic trait scores were independently associated with lower self-esteem, while parenting attitudes were more closely related to self-esteem than clinician-rated symptom severity.
Global annual average planetary boundary layer (PBL) height climatology derived from GPS radio occultation measurements. The National Aeronautics and Space Administration produced this dataset using data from the COSMIC/FORMOSAT-3 and TerraSAR-X satellites between June 2006 and December 2015. Data are binned into 2-degree latitude/longitude grids, providing mean and standard deviation values.
Global seasonal averages of planetary boundary layer (PBL) height derived from GPS radio occultation measurements. The data spans from June 2006 to December 2015, produced by NASA using instruments aboard the COSMIC/FORMOSAT-3 and TerraSAR-X satellites. PBL heights are calculated from refractivity profiles and binned into 2-degree latitude/longitude grids.
1,066 publications on Stereotactic Ablative Radiotherapy for oligometastatic cancer were analyzed from 2006 to 2025. The bibliometric analysis by Yupeng Di maps publication trends, key contributors, and research hotspots. It identifies the United States, Italy, and Canada as leading countries and highlights influential clinical trials like SABR-COMET and ORIOLE.
2006-2007 spectral data from the National Spectral Database's Aquatic Library, focusing on marine benthic habitats in oligotrophic, temperate waters off Western Australia. The dataset was developed by M.J. Harvey for a PhD thesis at Murdoch University and is hosted by Geoscience Australia. It is part of the Australian National Spectral Database.
209 X-ray-detected active galactic nuclei (AGNs) at redshifts greater than 3, comprising the largest high-z X-ray-selected sample to date. The catalog includes rest-frame 2-10 keV luminosities and X-ray hardness ratios, with analysis confirming a decreasing comoving space density of AGNs with increasing redshift up to z ~ 7. It was created by NASA HEASARC in March 2016 based on data from the Chandra Cosmological Evolution Survey and Chandra Multi-wavelength Project.
Over the last decade, the GLIMPSE Proper project re-imaged about 43 square degrees of the Galactic center to measure the proper motions of millions of sources within 5 degrees of the Galactic center. The dataset is provided by the National Aeronautics and Space Administration and was last updated in March 2026.
The Bulge Radial Velocity Assay (BRAVA) consists of spectra for approximately 8500 red giants in the Galactic bulge. The dataset was published by the National Aeronautics and Space Administration and was last updated in March 2026.
The GLIMPSE Proper project re-images about 43 square degrees of the Galactic center. It measures the proper motions of millions of sources within 5 degrees of the Galactic center over the last decade. The dataset is provided by the National Aeronautics and Space Administration and was last updated in March 2026.