cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.10797730
title: Longyearbyen CO2 Lab - Core Photos - DH5

description: Includes drill core photographs (whole boxes) for the Longyearbyen CO2 Lab borehole DH5.

Missing Intervals:

DH5 (Boxes): 0.0-74.0 m; 75.0-105.0 m; 222.0-226.0 m; 590.0-599.0 m; 701.0-702 m DH5 (HighRes): 0.0-105.0 m; 210.0-702 m
DOI: 10.5281/zenodo.10818002
title: Tear film

description: Tear film surface from patiens before and after cataract surgery
DOI: 10.5281/zenodo.10818001
title: Tear film

description: Tear film surface from patiens before and after cataract surgery
DOI: 10.5281/zenodo.10813549
title: Example of reverse Monte Carlo simulation for fcc high-entropy alloy CrMnFeCoNi

description: The data set contains the example of reverse Monte Carlo (RMC) simulation of EXAFS spectra collected for fcc high-entropy alloy CrMnFeCoNi.

The simulation was performed by the EvAX code freely available from http://www.dragon.lv/evax/.
DOI: 10.5281/zenodo.10813548
title: Example of reverse Monte Carlo simulation for fcc high-entropy alloy CrMnFeCoNi

description: The data set contains the example of reverse Monte Carlo (RMC) simulation of EXAFS spectra collected for fcc high-entropy alloy CrMnFeCoNi.

The simulation was performed by the EvAX code freely available from http://www.dragon.lv/evax/.
DOI: 10.5281/zenodo.10797745
title: Longyearbyen CO2 Lab - Core Photos - DH6

description: Includes drill core photographs (whole boxes) for the Longyearbyen CO2 Lab borehole DH6.

Missing interval:

DH6 (Boxes): 0.0-164.0 m DH6 (HighRes): 0.0-108.0 m
DOI: 10.5281/zenodo.10797746
title: Longyearbyen CO2 Lab - Core Photos - DH6

description: Includes drill core photographs (whole boxes) for the Longyearbyen CO2 Lab borehole DH6.

Missing interval:

DH6 (Boxes): 0.0-164.0 m DH6 (HighRes): 0.0-108.0 m
DOI: 10.5281/zenodo.10800928
title: Spherical harmonic models of the shape of asteroid (4) Vesta [DLR SPG]

description: This archive contains four spherical harmonic models of the shape of asteroid 4 Vesta, truncated at different maximum spherical harmonic degrees. The highest resolution model has a maximum spherical harmonic degree of 5759, which was generated from a shape model sampled at 64 pixels per degree.

The data used to generate these models are from a DLR stereo photogrammetric shape model based on Dawn high altitude mapping orbit framing camera images, as found in the file VE_HAMO_G_00N_330E_EQU_DTM.IMG on NASA's PDS website. This image file was first converted to netcdf format using the generic-mapping-tools function xyz2grd, and it was then converted to a gridline registration using the function grdsample. The grid was then shifted such that the frist column corresponded to 0 E longitude using the function grdedit, and the resulting netcdf file was read into the pyshtools software and expanded into spherical harmonics using the function SHCoeffs.expand(). The spherical harmonic functions were chosen to be "4pi" normalized and to exclude the Condon-Shortley phase factor of (-1)m. The units of the coefficients are meters.

The four files in this archive are



Vesta_DLR_SPG_shape_5759.bshc.gz

Vesta_DLR_SPG_shape_2879.bshc.gz

Vesta_DLR_SPG_shape_1439.bshc.gz

Vesta_DLR_SPG_shape_719.bshc.gz


The numbers 5759, 2879, 1439, and 719 in the filename refer to the maximum spherical harmonic degree of file, which corresponds to effective spatial resolutions of 64, 32, 16, and 8 pixels per degree, respectively. The files are stored in the binary "bshc" format as described in the pyshtools documentation and are furthermore compressed using gzip. The lower resolution models were generated by truncating the spherical harmonic coefficients of the highest resolution model.
DOI: 10.5281/zenodo.10800929
title: Spherical harmonic models of the shape of asteroid (4) Vesta [DLR SPG]

description: This archive contains four spherical harmonic models of the shape of asteroid 4 Vesta, truncated at different maximum spherical harmonic degrees. The highest resolution model has a maximum spherical harmonic degree of 5759, which was generated from a shape model sampled at 64 pixels per degree.

The data used to generate these models are from a DLR stereo photogrammetric shape model based on Dawn high altitude mapping orbit framing camera images, as found in the file VE_HAMO_G_00N_330E_EQU_DTM.IMG on NASA's PDS website. This image file was first converted to netcdf format using the generic-mapping-tools function xyz2grd, and it was then converted to a gridline registration using the function grdsample. The grid was then shifted such that the frist column corresponded to 0 E longitude using the function grdedit, and the resulting netcdf file was read into the pyshtools software and expanded into spherical harmonics using the function SHCoeffs.expand(). The spherical harmonic functions were chosen to be "4pi" normalized and to exclude the Condon-Shortley phase factor of (-1)m. The units of the coefficients are meters.

The four files in this archive are



Vesta_shape_5759.sh.gz

Vesta_shape_2879.sh.gz

Vesta_shape_1439.sh.gz

Vesta_shape_719.sh.gz


The numbers 5759, 2879, 1439, and 719 in the filename refer to the maximum spherical harmonic degree of file, which corresponds to effective spatial resolutions of 64, 32, 16, and 8 pixels per degree, respectively. The files are stored in the binary "bshc" format as described in the pyshtools documentation and are furthermore compressed using gzip. The lower resolution models were generated by truncating the spherical harmonic coefficients of the highest resolution model.
DOI: 10.5281/zenodo.10820643
title: Spherical harmonic models of the shape of asteroid (4) Vesta [DLR SPG]

description: This archive contains four spherical harmonic models of the shape of asteroid 4 Vesta, truncated at different maximum spherical harmonic degrees. The highest resolution model has a maximum spherical harmonic degree of 5759, which was generated from a shape model sampled at 64 pixels per degree.

The data used to generate these models are from a DLR stereo photogrammetric shape model based on Dawn high altitude mapping orbit framing camera images, as found in the file VE_HAMO_G_00N_330E_EQU_DTM.IMG on NASA's PDS website. This image file was first converted to netcdf format using the generic-mapping-tools function xyz2grd, and it was then converted to a gridline registration using the function grdsample. The grid was then shifted such that the frist column corresponded to 0 E longitude using the function grdedit, and the resulting netcdf file was read into the pyshtools software and expanded into spherical harmonics using the function SHCoeffs.expand(). The spherical harmonic functions were chosen to be "4pi" normalized and to exclude the Condon-Shortley phase factor of (-1)m. The units of the coefficients are meters.

The four files in this archive are



Vesta_DLR_SPG_shape_5759.bshc.gz

Vesta_DLR_SPG_shape_2879.bshc.gz

Vesta_DLR_SPG_shape_1439.bshc.gz

Vesta_DLR_SPG_shape_719.bshc.gz


The numbers 5759, 2879, 1439, and 719 in the filename refer to the maximum spherical harmonic degree of file, which corresponds to effective spatial resolutions of 64, 32, 16, and 8 pixels per degree, respectively. The files are stored in the binary "bshc" format as described in the pyshtools documentation and are furthermore compressed using gzip. The lower resolution models were generated by truncating the spherical harmonic coefficients of the highest resolution model.
DOI: 10.5281/zenodo.10820681
title: Spherical harmonic models of the shape of asteroid (4) Vesta [DLR SPG]

description: This archive contains four spherical harmonic models of the shape of asteroid 4 Vesta, truncated at different maximum spherical harmonic degrees. The highest resolution model has a maximum spherical harmonic degree of 5759, which was generated from a shape model sampled at 64 pixels per degree.

The data used to generate these models are from a DLR stereo photogrammetric shape model based on Dawn high altitude mapping orbit framing camera images, as found in the file VE_HAMO_G_00N_330E_EQU_DTM.IMG on NASA's PDS website. This image file was first converted to netcdf format using the generic-mapping-tools function xyz2grd, and it was then converted to a gridline registration using the function grdsample. The grid was then shifted such that the frist column corresponded to 0 E longitude using the function grdedit, and the resulting netcdf file was read into the pyshtools software and expanded into spherical harmonics using the function SHCoeffs.expand(). The spherical harmonic functions were chosen to be "4pi" normalized and to exclude the Condon-Shortley phase factor of (-1)m. The units of the coefficients are meters.

The four files in this archive are



Vesta_DLR_SPG_shape_5759.bshc.gz

Vesta_DLR_SPG_shape_2879.bshc.gz

Vesta_DLR_SPG_shape_1439.bshc.gz

Vesta_DLR_SPG_shape_719.bshc.gz


The numbers 5759, 2879, 1439, and 719 in the filename refer to the maximum spherical harmonic degree of file, which corresponds to effective spatial resolutions of 64, 32, 16, and 8 pixels per degree, respectively. The files are stored in the binary "bshc" format as described in the pyshtools documentation and are furthermore compressed using gzip. The lower resolution models were generated by truncating the spherical harmonic coefficients of the highest resolution model.
DOI: 10.5281/zenodo.10820539
title: THE DEVELOPMENT OF LEGAL NORMS ON LIABILITY FOR CRIMES IN THE CUSTOMS SPHERE IN THE REPUBLIC OF UZBEKISTAN
DOI: 10.5281/zenodo.10820538
title: THE DEVELOPMENT OF LEGAL NORMS ON LIABILITY FOR CRIMES IN THE CUSTOMS SPHERE IN THE REPUBLIC OF UZBEKISTAN
DOI: 10.5519/qd.3p5l80ld
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (61 records)
DOI: 10.5281/zenodo.10797699
title: Longyearbyen CO2 Lab - Core Photos - DH4

description: Includes drill core photographs (whole boxes) for the Longyearbyen CO2 Lab borehole DH4.

Missing intervals:

DH4 (Boxes): 0.0-65.0 m; 612.0-616.0 m DH4 (HighRes): 0.0-969.72 m
DOI: 10.5281/zenodo.10797700
title: Longyearbyen CO2 Lab - Core Photos - DH4

description: Includes drill core photographs (whole boxes) for the Longyearbyen CO2 Lab borehole DH4.

Missing intervals:

DH4 (Boxes): 0.0-65.0 m; 612.0-616.0 m DH4 (HighRes): 0.0-969.72 m
DOI: 10.5281/zenodo.10797684
title: Longyearbyen CO2 Lab - Core Photos - DH3

description: Includes drill core photographs (whole boxes) for the Longyearbyen CO2 Lab borehole DH3.

Missing intervals:

DH3 (Boxes): 0.0-65.0 m; 217.0-221.0 m; 225.0-233.0 m DH3 (HighRes): 0.0-402 m
DOI: 10.5281/zenodo.10797683
title: Longyearbyen CO2 Lab - Core Photos - DH3

description: Includes drill core photographs (whole boxes) for the Longyearbyen CO2 Lab borehole DH3.

Missing intervals:

DH3 (Boxes): 0.0-65.0 m; 217.0-221.0 m; 225.0-233.0 m DH3 (HighRes): 0.0-402 m
DOI: 10.5281/zenodo.10818475
title: Tear film - DED group CG2

description: Tear film surface from control group 2 - CG2 with Dry Eye Disease (DED) - Data collected with the research project founded by SONATA BIS (NCN)
DOI: 10.5281/zenodo.10818476
title: Tear film - DED group CG2

description: Tear film surface from control group 2 - CG2 with Dry Eye Disease (DED) - Data collected with the research project founded by SONATA BIS (NCN)
DOI: 10.6084/m9.figshare.24464203
title: Figure 2_2d plot by JMP

description: The dataset for the article "The current utilization status of wearable devices in clinical research".Analyses were performed by utilizing the JMP Pro 16.10.The file extension "jrp" is a file of the statistical analysis software JMP, which contains both the analysis code and the data set.In case JMP is not available, a "csv" file as a data set and JMP script, the analysis code, are prepared in "rtf" format.JMP repot files used to create the figures（Figure 2. 2D scatterplot of relationships between annual enrollment and trial number over time）,including the csv dataset of JMP repot files and JMP scripts.Figure 2. 2D scatterplot of relationships between annual enrollment and trial number over time2d plot.jrp2d plot(JMP script).rftdataset_2d.csv<br><br>
DOI: 10.5281/zenodo.8340252
title: Data associated with global-bird-detection-paper

description: Data for repository located at https://github.com/sarabsethi/global-bird-detection-paper Unzip the file to the directory and follow the instructions in the repository to run the code.
DOI: 10.5281/zenodo.10566339
title: Example environment and files for the ATS evaluation

description: Example of an working environment for ATS. Included are the workflows and manual evaluation scripts, the target lists  for LC-ESIpos and GC-EI, the minified raw data in .mzML as well as the results after ATS evaluation.
DOI: 10.5281/zenodo.10047378
title: Example environment and files for the ATS evaluation

description: Example of an working environment for ATS. Included are the workflows and manual evaluation scripts, the target lists  for LC-ESIpos and GC-EI, the minified raw data in .mzML as well as the results after ATS evaluation.
DOI: 10.5281/zenodo.10777244
title: Example environment and files for the ATS evaluation

description: Example of an working environment for ATS. Included are the workflows and manual evaluation scripts, the target lists  for LC-ESIpos and GC-EI, the minified raw data in .mzML as well as the results after ATS evaluation.
DOI: 10.5281/zenodo.10797667
title: Longyearbyen CO2 Lab - Core Photos - DH2

description: Includes drill core photographs (whole boxes) for the Longyearbyen CO2 Lab borehole DH2.

Missing interval (boxes): 0 - 10 m
DOI: 10.5281/zenodo.10797668
title: Longyearbyen CO2 Lab - Core Photos - DH2

description: Includes drill core photographs (whole boxes) for the Longyearbyen CO2 Lab borehole DH2.

Missing interval (boxes): 0 - 10 m
DOI: 10.5281/zenodo.10814780
title: Does Diglossia impact brain structure? Data from Swiss Ger-man early diglossic speakers

description: This repository contrains the raw MRI images and the analysis files used in the following paper : Berger Lea, Mouthon Michael, Jost Lea, Schwab Sandra, Aybek Selma and Annoni Jean-Marie (2024), Does Diglossia impact brain structure? Data from Swiss Ger-man early diglossic speakersBain Sciences

Note: The raw MRI images include in this repository are partially publish in two other dataset (https://doi.org/10.5281/zenodo.4761370, https://doi.org/10.5281/zenodo.7031880)
DOI: 10.5281/zenodo.10814781
title: Does Diglossia impact brain structure? Data from Swiss Ger-man early diglossic speakers

description: This repository contrains the raw MRI images and the analysis files used in the following paper : Berger Lea, Mouthon Michael, Jost Lea, Schwab Sandra, Aybek Selma and Annoni Jean-Marie (2024), Does Diglossia impact brain structure? Data from Swiss Ger-man early diglossic speakersBain Sciences

Note: The raw MRI images include in this repository are partially publish in two other dataset (https://doi.org/10.5281/zenodo.4761370, https://doi.org/10.5281/zenodo.7031880)
DOI: 10.5281/zenodo.10820608
title: Spherical harmonic models of the shape of asteroid (1) Ceres [DLR SPG]

description: This archive contains four spherical harmonic models of the shape of asteroid (1) Ceres, truncated at different maximum spherical harmonic degrees. The highest resolution model has a maximum spherical harmonic degree of 5399, which was generated from a shape model sampled at 60 pixels per degree.

The data used to generate these models are from a DLR stereo photogrammetric shape model based on Dawn high altitude mapping orbit framing camera images, as found in the file CE_HAMO_G_00N_180E_EQU_DTM.IMG on NASA's PDS website. This image file was first converted to netcdf format using the generic-mapping-tools function xyz2grd, it was then converted to a gridline registration using the function grdsample, and the resulting netcdf file was read into the pyshtools software and expanded into spherical harmonics using the function SHCoeffs.expand(). The spherical harmonic functions were chosen to be "4pi" normalized and to exclude the Condon-Shortley phase factor of (-1)m. The units of the coefficients are meters.

The four files in this archive are



Ceres_DLR_SPG_shape_5399.bshc.gz

Ceres_DLR_SPG_shape_2879.bshc.gz

Ceres_DLR_SPG_shape_1439.bshc.gz

Ceres_DLR_SPG_shape_719.bshc.gz


The numbers 5399, 2879, 1439, and 719 in the filename refer to the maximum spherical harmonic degree of file, which corresponds to effective spatial resolutions of 60, 32, 16, and 8 pixels per degree, respectively. The files are stored in the binary "bshc" format as described in the pyshtools documentation and are furthermore compressed using gzip. The lower resolution models were generated by truncating the spherical harmonic coefficients of the highest resolution model.
DOI: 10.5281/zenodo.10804156
title: Spherical harmonic models of the shape of asteroid (1) Ceres [DLR SPG]

description: This archive contains four spherical harmonic models of the shape of asteroid (1) Ceres, truncated at different maximum spherical harmonic degrees. The highest resolution model has a maximum spherical harmonic degree of 5399, which was generated from a shape model sampled at 60 pixels per degree.

The data used to generate these models are from a DLR stereo photogrammetric shape model based on Dawn high altitude mapping orbit framing camera images, as found in the file CE_HAMO_G_00N_180E_EQU_DTM.IMG on NASA's PDS website. This image file was first converted to netcdf format using the generic-mapping-tools function xyz2grd, it was then converted to a gridline registration using the function grdsample, and the resulting netcdf file was read into the pyshtools software and expanded into spherical harmonics using the function SHCoeffs.expand(). The spherical harmonic functions were chosen to be "4pi" normalized and to exclude the Condon-Shortley phase factor of (-1)m. The units of the coefficients are meters.

The four files in this archive are



Ceres_DLR_SPG_shape_5399.bshc.gz

Ceres_DLR_SPG_shape_2879.bshc.gz

Ceres_DLR_SPG_shape_1439.bshc.gz

Ceres_DLR_SPG_shape_719.bshc.gz


The numbers 5399, 2879, 1439, and 719 in the filename refer to the maximum spherical harmonic degree of file, which corresponds to effective spatial resolutions of 60, 32, 16, and 8 pixels per degree, respectively. The files are stored in the binary "bshc" format as described in the pyshtools documentation and are furthermore compressed using gzip. The lower resolution models were generated by truncating the spherical harmonic coefficients of the highest resolution model.
DOI: 10.5281/zenodo.10820437
title: KupferDigital mechanical testing datasets: Stress relaxation and low-cycle fatigue (LCF) tests

description: The KupferDigital project deals with the development of a data ecosystem for digital materials research on the basis of ontology-based digital representations of copper and copper alloys. This document provides exemplary mechanical testing datasets for training the developed KupferDigital infrastructures. Different types of cast copper alloys were provided for this research and their mechanical testing (stress relaxation and low-cycle fatigue) was performed in the accredited materials testing laboratory, while the test results were reported according to the DIN/ISO standards and attached with the maximum possible metadata about the sample history, equipment, and calibration. The attached content file consisted of the obtained primary raw testing data as well as the secondary datasets of these tests containing the detailed metadata of mechanical testing methods. Such test data files are processed by the KupferDigital digital tools to be converted to standardized machine-readable data files.
DOI: 10.5281/zenodo.10820562
title: Multi-scale soil moisture data and process-based modeling reveal the importance of lateral groundwater flow in a subarctic catchment

description: Hydrological data measured in Lompolonjängänoja (LJO) catchment and used in Nousu et al.

 

ET_fluxes.csv- Eddy-covariance based, daily evapotranspiration (ET) fluxes [mm/d] at Kenttärova (NFOR) and Lompolojänkkä (NWET) stations

GW_levels.csv- Observed groundwater levels [m] relative to the ground surface measured around the LJO catchment

Q_runoff.csv- Observed specific discharge [mm/d] at the LJO catchment outlet

THETA_kenttarova.csv- Automatically measured soil moisture (i.e. volumetric water content [m3/m3]) around Kenttärova stations

THETA_spatial.csv- Manually measured soil moisture (i.e. volumetric water content [m3/m3]) around the LJO catchment
DOI: 10.5281/zenodo.10813218
title: TF Cytology

description: Data from research grant funded by the National Science Centre of Poland (SONATA BIS)
DOI: 10.5281/zenodo.10813217
title: TF Cytology

description: Data from research grant funded by the National Science Centre of Poland (SONATA BIS)
DOI: 10.5281/zenodo.10796823
title: Spherical harmonic models of the shape of the Moon [LOLA]

description: This archive contains four spherical harmonic models of the shape of the Moon truncated at different maximum spherical harmonic degrees. The highest resolution model has a maximum spherical harmonic degree of 5759, which was generated from a lunar shape model sampled at 64 pixels per degree in the DE421 mean Earth/polar axis coordinate frame.

The data used to generate these models are from the LOLA instrument on the Lunar Reconaissance Orbiter, as found in the file ldem_64_float.img on NASA's PDS website. This image file was first converted to netcdf format using the generic-mapping-tools function xyz2grd, and the resulting pixel registed map was then converted to a gridline registration using the function grdsample. Following this, the resulting netcdf file was read into the pyshtools software and expanded into spherical harmonics using the function SHCoeffs.expand(). The spherical harmonic functions were chosen to be "4pi" normalized and to exclude the Condon-Shortley phase factor of (-1)m. The units of the coefficients are meters.

The four files in this archive are



Moon_shape_5759.sh.gz

Moon_shape_2879.sh.gz

Moon_shape_1439.sh.gz

Moon_shape_719.sh.gz


The numbers 5759, 2879, 1439, and 719 in the filename refer to the maximum spherical harmonic degree of file, which corresponds to effective spatial resolutions of 64, 32, 16, and 8 pixels per degree, respectively. The files are stored in the binary "bshc" format as described in the pyshtools documentation and are furthermore compressed using gzip. The lower resolution models were generated by truncating the spherical harmonic coefficients of the highest resolution model.

Note that this shape model should not be used in conjunction with most gravity models of the Moon. The gravity models use a principal axis coordinate system that differs from the mean Earth/polar axis frame by about 1 km at the equator. For a principal axis coordinate system model, use Spherical harmonic models of the shape of the Moon (principal axis coordinate system).
DOI: 10.25345/c5wm14502
title: MassIVE MSV000094329 - Affinity Purification Mass Spectrometry of protein protein interactors with alternatively-spliced Uromodulin
title: We identified an alternatively spliced UMOD which is uniquely localized intracellularly. This intracellular isoform enhanced mitochondrial function. To understand its molecular mechanism, we performed affinity-purification coupled to mass spectrometry using MDCK cell lysate expressing UMOD variant. We prepared MDCK cells which express mock (negative control), wild-type human UMOD or alternatively spliced human UMOD. UMOD was isolated by Immunoprecipitation and interacting proteins were identified by mass spectrometry proteomics analysis.