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datasets available to search
ShareScore release 0.9.0
Dataset results
31 results for “image cube”
Mock Image Cube
<p>A mock image cube made from the ALMA logo, for testing purposes with radio interferometers. Total flux is comparable to a bright protoplanetary disk in 12CO J=2-1.</p>
Cube with evangelical images
Cube from the exposition of the Museum of Ancient Belarusian Culture of the National Academy of Sciences of Belarus. Excavated by Georgy Stychau in 1986. Material: horn Date: the beginning of the 17 century Location: Belarus, Minsk, сultural layer of the lower market Cube face length: about 4 cm Source: Objaverse 1.0 / Sketchfab
Chemical imaging data collected on small wood cubes after impregnation-treatment with phenol formaldehyde resin
<p>This dataset contains UV microspectrophotometry (UMSP) and near infrared (NIR) imaging data from the following publication: Altgen M., Awais M. Altgen D., Klüppel A., Koch G., Mäkelä M., Olbrich A., Rautkari L. (2022) Chemical imaging to reveal the resin distribution in impregnation-treated wood at different spatial scales. Materials & Design, DOI: <a href="https://doi.org/10.1016/j.matdes.2022.111481">https://doi.org/10.1016/j.matdes.2022.111481</a>.</p> <p>The data was measured on small beech wood cubes (15x15x15 mm<sup>3</sup>) that were impregnation-treated with a low molecular weight phenol formaldehyde resin. Experimental details can be found in the publication.</p> <p>The file “NIR sample IDs with weight and dimensional changes.csv” contains the sample IDs as well as the weight percent gains and dimensional changes caused by the resin treatment of each sample in the dataset. To generate the NIR image files, a region of interest of 881 x 384 pixels was selected from the raw image files to produce an image that contains the sample surrounded by background. The spectral data was corrected using the calibration reflectance target values and then converted to absorbance. Each NIR image is stored in a separate MATLAB file (.mat) with the sample ID as the file name.</p> <p>The file "UMSP sample IDs.csv" contains the sample IDs of the UMSP images. The folder "UMSP image profiles.zip" contains the corresponding UMSP image profiles, which are stored as excel files (.xlsx) with the sample IDs as file names. The files contain the absorbance at 278 nm per pixel with a pixel resolution of 0.25 x 0.25 µm<sup>2</sup>.</p>
ALMA Titan image cubes for CH3CN, HC3N and HNC observed August 2016 and May 2017
<p>These 3D FITS files contain spectral line emission flux from Titan (in Janskys per beam) as a function of RA, dec. and frequency, observed using Atacama Large Millimeter/submillimeter Array (ALMA).</p> <p>ALMA observations of Titan were obtained on 2017-05-08 and 2017-05-16 (as part of ALMA program 2016.A.00014.S; PI: Cordiner) and on 2016-08-18 and 2016-08-19 (as part of ALMA program 2015.1.01023.S; PI: Gurwell). The HNC (J=4-3), HC3N (J=40-39) and CH3CN (J=19-18) transitions were observed in 2017, whereas the HNC (J=4-3), HC3N (J=39-38) and CH3CN (J=19-18) were observed in 2016.</p> <p>The raw observations were calibrated using standard scripts supplied by the observatory. The resulting measurement sets were continuum-subtracted using low-order polynomial fits to the line-free spectral regions adjacent to our lines of interest. The data were then imaged and cleaned (deconvolved) using the tclean algorithm in CASA 5.6. This routine implicitly corrects for the time-variability of Titan's position and radial velocity with respect to the observer, so the resulting image cubes are in the rest frame of Titan's center-of-mass. To facilitate meaningful intercomparisons, accounting for Titan's varying Geocentric distance, the 2016 and 2017 datasets were convolved to common circular beam dimensions, as projected in the plane of the sky. The image cubes were then cropped to isolate the emission lines of interest.</p>
G0.412+0.052 continuum image & data cubes (ALMA project 2016.1.00949.S)
<p>This dataset contains data from the ALMA project 2016.1.00949.S for G0.412+0.052 as presented in Williams et al. (2022). These data include the dust continuum, and data cubes for SiO (5-4), 13CO (2-1), and three transitions of H2CO. Both primary beam- and non primary beam-corrected data are included.</p>
CASSINI ORBITER SATURN UVIS SPATIAL SPECTRAL IMAGE CUBE V1.4
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
HIRES NIMS IDA SPECTRAL IMAGE CUBES
This data volume contains 17 channel spectral image cubes of asteroid 243 Ida ranging from 0.7 to 5.2 micrometers in wavelength in cgs units of radiance. These data were obtained by the Galileo spacecraft Near Infrared Mapping Spectrometer on August 28, 1993. They were radiometrically calibrated using calibration measurements obtained by the Near Infrared Mapping Spectrometer during its observations of Europa on June 28, 1996.
HIRES NIMS GASPRA SPECTRAL IMAGE CUBE
This data volume contains a 17 channel spectral image cube of asteroid 951 Gaspra ranging from 0.7 to 5.2 micrometers in wavelength in cgs units of radiance. The spatial resolution of this data is 1.28 km/pixel. This data set was obtained by the Galileo spacecraft Near Infrared Mapping Spectrometer on October 29, 1991. It was radiometrically calibrated using calibration measurements obtained by the Near Infrared Mapping Spectrometer during its observations of Earth on December 9, 1990.
CASSINI ORBITER SATURN UVIS SPATIAL SPECTRAL IMAGE CUBE 1.0
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
CASSINI ORBITER SATURN UVIS SPATIAL SPECTRAL IMAGE CUBE V1.3
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
CASSINI ORBITER SATURN UVIS SPATIAL SPECTRAL IMAGE CUBE 1.1
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
CASSINI ORBITER SATURN UVIS SPATIAL SPECTRAL IMAGE CUBE 1.2
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
GALILEO NIMS SPECTRAL IMAGE CUBES: JUPITER OPERATIONS
The natural form of imaging spectrometer data is the spectral image cube. It is normally in band sequential format, but has a dual nature. It is a series of 'images' of the target, each in a different wavelength, in ascending order. It is also a set of spectra, each at a particular line and sample, over the target area. Each spectrum describes a small portion of the area. When transformed into cubes, the data may be analyzed spatially, an image at a time, or spectrally, a spectrum at a time, or in more complex spatial-spectral fashion.
CASSINI ORBITER N/A UVIS SPATIAL SPECTRAL IMAGE CUBE 1.0
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
CASSINI ORBITER JUPITER UVIS SPATIAL SPECTRAL IMAGE CUBE 1.0
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
NIMS SPECTRAL IMAGE CUBES OF THE EARTH: E1 & E2 ENCOUNTERS
Unknown
NIMS SPECTRAL IMAGE CUBES OF VENUS
Unknown
NIMS SPECTRAL IMAGE CUBES OF THE EARTH: E1 & E2 ENCOUNTERS
Unknown
CASSINI ORBITER SATURN UVIS SPATIAL SPECTRAL IMAGE CUBE 1.2
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
GALILEO NIMS SPECTRAL IMAGE CUBES: JUPITER OPERATIONS
The natural form of imaging spectrometer data is the spectral image cube. It is normally in band sequential format, but has a dual nature. It is a series of 'images' of the target, each in a different wavelength, in ascending order. It is also a set of spectra, each at a particular line and sample, over the target area. Each spectrum describes a small portion of the area. When transformed into cubes, the data may be analyzed spatially, an image at a time, or spectrally, a spectrum at a time, or in more complex spatial-spectral fashion.
ScienceDex guides
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Allen Brain Atlas
Allen Brain Atlas is an Allen Institute collection of brain map atlases, datasets, APIs, and analysis tools covering mouse, human, and non-human primate brain resources.
Annotated Behaviour and Observability Dataset (ABODe)
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DANDI Archive for NWB datasets
DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.
International Brain Laboratory public data
The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.
OpenNeuro
OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.