cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.7783173
title: CoUDlabs_WP8_T812_UDC_001. Identifying sediment deposits from temperature signals

description: This dataset contains the results of the experimental campaign and how data were collected on the research activity “Identifying sediment deposits from temperature signals” performed under Joint Research Activity “JRA 3- Improving Resilience and Sustainability in Urban Drainage solutions” of Co-UDlabs project, funded under the European Union’s Horizon 2020 research and innovation programme under grant agreement No 101008626. The experiments introduce a new approach which uses high-resolution temperature data to identify sediment bed deposits by analysing time series. Water (wastewater or drainage water in UDS) and sediments show different thermal properties and heat transfer dynamics. Thus, the aim of the dataset is to estimate or at least evidenced the presence of sediments by analyzing the differences between the temperature timeseries measured in the water phase and at the bottom of bed deposits. Results from this experimental campaign will help to understand heat transfer processes between water and saturated sediment mixtures and, therefore, develop new methodologies to estimate accumulation in UDS. The data are described so that others can use them.
DOI: 10.5281/zenodo.7827667
title: CoUDlabs_WP8_T812_UDC_001. Identifying sediment deposits from temperature signals

description: This dataset contains the results of the experimental campaign and how data were collected on the research activity “Identifying sediment deposits from temperature signals” performed under Joint Research Activity “JRA 3- Improving Resilience and Sustainability in Urban Drainage solutions” of Co-UDlabs project, funded under the European Union’s Horizon 2020 research and innovation programme under grant agreement No 101008626. The experiments introduce a new approach which uses high-resolution temperature data to identify sediment bed deposits by analysing time series. Water (wastewater or drainage water in UDS) and sediments show different thermal properties and heat transfer dynamics. Thus, the aim of the dataset is to estimate or at least evidenced the presence of sediments by analyzing the differences between the temperature timeseries measured in the water phase and at the bottom of bed deposits. Results from this experimental campaign will help to understand heat transfer processes between water and saturated sediment mixtures and, therefore, develop new methodologies to estimate accumulation in UDS. The data are described so that others can use them.
DOI: 10.35003/ycukox
title: Replication Data for: Origin of 182W anomalies in ocean island basalts

description: • 182W deficits in ocean island basalts are confirmed using a new method • Correlated 182W-183W anomalies that are present in prior datasets are not confirmed, ruling out a nucleosynthetic origin for 182W deficits • 182W deficits may reflect either core-mantle interaction or an overabundance of late-accreted materials • Mo isotope data do not reveal resolved nucleosynthetic anomalies • Combined W-Mo data rule out significant contribution of CC-like material to Earth’s core or late accretion
DOI: 10.35003/ycukox/hutdig
title: Table3.tab

description: Molybdenum isotopic compositions of ocean island basalts
DOI: 10.35003/ycukox/hxrfom
title: Table1.tab

description: Tungsten isotopic compositions of geological reference materials and doped MORB PS66-261
DOI: 10.35003/ycukox/ceyo9w
title: Table2.tab

description: Tungsten isotopic compositions of ocean island basalts
DOI: 10.35003/ycukox/j1dgif
title: Table3.tab

description: :unav
DOI: 10.35003/sya4dc/nwm0t5
title: fig1_basin_table.xls

description: :unav
DOI: 10.35003/sya4dc/pcsynz
title: fig3c.xls

description: :unav
DOI: 10.35003/sya4dc/0lzncz
title: fig3b.xls

description: :unav
DOI: 10.35003/sya4dc/k2dqfx
title: fig4.xls

description: :unav
DOI: 10.35003/sya4dc/a87eti
title: fig2c.xls

description: :unav
DOI: 10.35003/sya4dc/yv14jf
title: fig2b.xls

description: :unav
DOI: 10.34740/kaggle/dsv/5402150
title: Sainfoin Seeds
DOI: 10.15151/esrf-es-1120060906
title: Cryo-electron microscopy EPN BAG

description: At the EPN campus level structural biology work is carried out in all the 4 institutes (IBS, ESRF, ILL and EMBL). Today all structural biology groups are turning to cryo-EM. The EM demand is therefore extremely high and present in the 4 Institutes. In a nutshell, there are more than 45 PIs that could benefit from Krios time on the EPN campus (more than 90 different samples). Around 20 % of the sample are ready for high resolution data collection with already prepared grids that have been pre-screened on Glacios microscopes. Whereas some work could be carried out on Glacios microscopes, for difficult samples the use of a krios is indispensable (heterogeneous sample or limited concentration requiring a large number of images; small protein etc). Only these samples will be selected for Krios time at the BAG level
DOI: 10.35003/v9afaz/pdujwg
title: CRATER_South_Ray.zip

description: :unav
DOI: 10.35003/v9afaz/3qjz7f
title: AREA_North_Ray.zip

description: :unav
DOI: 10.35003/v9afaz/yj5agm
title: CRATER_Giordano_Bruno_Moore_F.zip

description: :unav
DOI: 10.35003/v9afaz/p6i3kr
title: AREA_Giordano_Bruno_Moore_F.zip

description: :unav
DOI: 10.35003/v9afaz/gspwlz
title: CRATER_North_Ray.zip

description: :unav
DOI: 10.35003/v9afaz/jeijfx
title: AREA_South_Ray.zip

description: :unav
DOI: 10.6084/m9.figshare.22632850
title: Meta_analysis_examplar_data

description: This data is linked to the publication: Shayan, S. J., Nazari, R., & Kiwanuka, F. (2021). Prevalence of HIV and HCV among injecting drug users in three selected WHO-EMRO countries: a meta-analysis. <em>Harm Reduction Journal</em>, <em>18</em>(1), 59. 10.6084/m9.figshare.22632850
DOI: 10.6084/m9.figshare.22632850.v1
title: Meta_analysis_examplar_data

description: This data is linked to the publication: Shayan, S. J., Nazari, R., & Kiwanuka, F. (2021). Prevalence of HIV and HCV among injecting drug users in three selected WHO-EMRO countries: a meta-analysis. <em>Harm Reduction Journal</em>, <em>18</em>(1), 59. 10.6084/m9.figshare.22632850
DOI: 10.35003/5ttozg
title: Replication Data for: Low volcanic outgassing rates for a stagnant lid Archean earth with graphite-saturated magmas

description: • Stagnant lid C-O-H outgassing rates predicted across mantle oxidation states. • Fully-coupled convection model reveals limiting effect of mantle volatile budget. • Early Archean CO2 outgassing was not necessarily stronger than the modern rate.
DOI: 10.35003/5ttozg/h4dslc
title: supplementary_data_figures_tables.xlsx

description: :unav
DOI: 10.35003/5ttozg/e7a4g1
title: References.docx

description: :unav
DOI: 10.5281/zenodo.7806376
title: Dynamically coupled kinetic chemistry in brown dwarf atmospheres I. Performing global scale kinetic modelling

description: Gifs and Exo-FMS GCM output from the 3D brown dwarf atmospheric simulations in Lee, Tan and Tsai (2023). Animated gifs for each effective temperature (Teff - first number in filename) of the brown dwarf (OLR and CH4 VMR). The gifs frames are every hour of simulation for 4 simulated days. Exo-FMS GCM output in netCDF format containing the 3D T-p structure and chemical results from the coupled mini-chem and GCM model for each Teff simulation (number in filename). `average' is the averaged output of the last 100 days. `daily' is the snapshot at the end of the simulation.
DOI: 10.5281/zenodo.7806375
title: Dynamically coupled kinetic chemistry in brown dwarf atmospheres I. Performing global scale kinetic modelling

description: Gifs and Exo-FMS GCM output from the 3D brown dwarf atmospheric simulations in Lee, Tan and Tsai (2023). Animated gifs for each effective temperature (Teff - first number in filename) of the brown dwarf (OLR and CH4 VMR). The gifs frames are every hour of simulation for 4 simulated days. Exo-FMS GCM output in netCDF format containing the 3D T-p structure and chemical results from the coupled mini-chem and GCM model for each Teff simulation (number in filename). `average' is the averaged output of the last 100 days. `daily' is the snapshot at the end of the simulation.
DOI: 10.6084/m9.figshare.22616587
title: asv_table_fungi.txt

description: ASV table
DOI: 10.6084/m9.figshare.22616587.v1
title: asv_table_fungi.txt

description: ASV table
DOI: 10.21227/zz78-4461
title: Ground Grid Resistance Synthetic Data

description: 我们提出了一种用于地网阻抗快速成像的优化微分-多重网格-同伦算法。设置了数值模拟和实验模拟来验证该算法的性能。该数据集包含我们的实验数据和实验结果
DOI: 10.35003/kdwjuk
title: Replication Data for: Late accretionary history of Earth and Moon preserved in lunar impactites.

description: Abstract: Late accretion describes the final addition of Earth’s mass following Moon formation and includes a period of Late Heavy Bombardment (LHB), which occurred either as a short-lived cataclysm triggered by a late giant planet orbital instability or a declining bombardment during late accretion. Using genetically characteristic ruthenium and molybdenum isotope compositions of lunar impact–derived rocks, we show that the impactors during the LHB and the entire period of late accretion were the same type of bodies and that they originated in the terrestrial planet region. Because a cataclysmic LHB would have, in part, resulted in compositionally distinct projectiles, we conclude that the LHB reflects the tail end of accretion. This implies that the giant planet orbital instability occurred during the main phase of planet formation. Last, because of their inner solar system origin, late-accreted bodies cannot be the primary source of Earth’s water.
DOI: 10.35003/kdwjuk/y7gb0c
title: Figure3.pptx

description: :unav
DOI: 10.35003/kdwjuk/w2wemk
title: Figure 1-3 Captions.docx

description: :unav
DOI: 10.35003/kdwjuk/aogqtr
title: Figure2.pptx

description: :unav
DOI: 10.35003/kdwjuk/pxef6g
title: Figure1.pptx

description: :unav
DOI: 10.35003/kdwjuk/gogwyb
title: Supplementary Materials.docx

description: :unav
DOI: 10.35003/kdwjuk/antnew
title: Table_1.tab

description: :unav
DOI: 10.35003/vhxr9w
title: Replication Data for: No 182W evidence for early Moon formation

description: Abstract: The Moon-forming giant impact was probably the last major event in Earth’s accretion, so dating this event is critical to determine the timeline of terrestrial planet formation. Recently, Thiemens et al. ( https://doi.org/10.1038/s41561-019-0398-3) used the short-lived 182Hf–182W system to argue that the Moon formed within the first 60 Myr of Solar System history. Here we demonstrate, however, that mixing processes during and after the giant impact modified the 182W compositions of the Earth and Moon, which hampers the use of the Hf–W system to date the Moon. Our results show that the lunar 182W record is fully consistent with a recently determined, younger age of the Moon of 142 ± 25 Myr after Solar System formation (Maurice et al., Adv. 6, eaba8949, 2020)
DOI: 10.35003/vhxr9w/0ba6nm
title: Figures and captions.tab

description: :unav
DOI: 10.34740/kaggle/dsv/5402341
title: Health Workforce Shortage Areas
DOI: 10.34740/kaggle/dsv/5402355
title: AutoXGB
DOI: 10.4121/eaa8ceb3-77cc-452b-b2f2-2796ba33e5ab
title: FE models related to report "Deciding where to verify the fatigue resistance of an orthotropic steel bridge deck"

description: FE models related to the master thesis with the name: Deciding where to verify the fatigue resistance of an orthotropic steel bridge deck<br>This contains a total of 11 different FE model which all model the behaviour of a single bridge.4 models are made of 2D elements and do not contain any weld details. The difference is the mesh refinement applied at the welds at the connection between the trough webs and the deck plate4 models are made of 2D elements and do contain weld details according to the Dutch regulations (ROK 2.0). The weld details are at the point for which the model is made. At this point the maximum stress interval is determined. The different points are point: A, B, 1, 2. The locations of this point can be found in the master thesis these model were generated for. Or, by opening the models and observing the location of the mesh refinement.2 models are made of 1D ellements. They are used to research the difference between the choice of modelling of the cross section of the stiffeners. Either "open" or "closed"1 1D models is used the research the response of the main girders due to the loads applied on them by the cross beams<br>
DOI: 10.4121/eaa8ceb3-77cc-452b-b2f2-2796ba33e5ab.v1
title: FE models related to report "Deciding where to verify the fatigue resistance of an orthotropic steel bridge deck"

description: FE models related to the master thesis with the name: Deciding where to verify the fatigue resistance of an orthotropic steel bridge deck<br>This contains a total of 11 different FE model which all model the behaviour of a single bridge.4 models are made of 2D elements and do not contain any weld details. The difference is the mesh refinement applied at the welds at the connection between the trough webs and the deck plate4 models are made of 2D elements and do contain weld details according to the Dutch regulations (ROK 2.0). The weld details are at the point for which the model is made. At this point the maximum stress interval is determined. The different points are point: A, B, 1, 2. The locations of this point can be found in the master thesis these model were generated for. Or, by opening the models and observing the location of the mesh refinement.2 models are made of 1D ellements. They are used to research the difference between the choice of modelling of the cross section of the stiffeners. Either "open" or "closed"1 1D models is used the research the response of the main girders due to the loads applied on them by the cross beams<br>
DOI: 10.35003/vsf2hg
title: Replication Data for: Nd isotope variation between the Earth–Moon system and enstatite chondrites

description: Abstract: Reconstructing the building blocks that made Earth and the Moon is critical to constrain their formation and compositional evolution to the present. Neodymium (Nd) isotopes identify these building blocks by fingerprinting nucleosynthetic components. In addition, the 146Sm–142Nd and 147Sm–143Nd decay systems, with half-lives of 103 million years and 108 billion years, respectively, track potential differences in their samarium (Sm)/Nd ratios. The difference in Earth’s present-day 142Nd/144Nd ratio compared with chondrites (Burkhardt et al., Nature, 2016; Bouvier et al., Nature, 2016), and in particular enstatite chondrites, is interpreted as nucleosynthetic isotope variation in the protoplanetary disk. This necessitates that chondrite parent bodies have the same Sm/Nd ratio as Earth’s precursor materials (Bouvier et al., Nature, 2016). Here we show that Earth and the Moon instead had a Sm/Nd ratio approximately 2.4 ± 0.5 per cent higher than the average for chondrites and that the initial 142Nd/144Nd ratio of Earth’s precursor materials is more similar to that of enstatite chondrites than previously proposed (Burkhardt et al., Nature, 2016; Bouvier et al., Nature, 2016). The difference in the Sm/Nd ratio between Earth and chondrites probably reflects the mineralogical distribution owing to mixing processes within the inner protoplanetary disk. This observation simplifies lunar differentiation to a single stage from formation to solidification of a lunar magma ocean (McLeod, et al., Earth Planet. Sci. Lett., 2014). This also indicates that no Sm/Nd fractionation occurred between the materials that made Earth and the Moon in the Moon-forming giant impact.
DOI: 10.35003/vsf2hg/ccawka
title: Supplementary Table 5.tab

description: Compilation of Nd isotope data used to calculate group averages for Allende CAIs and Allende.
DOI: 10.35003/vsf2hg/3nqzud
title: Supplementary Table 1.tab

description: Compilation of measured and calculated Nd isotope compositions for bulk chondrites and CAI's.
DOI: 10.35003/vsf2hg/i5urok
title: Supplementary Table 2.xlsx

description: Nd isotope ratios and values for samples and standards analyzed in this study.
DOI: 10.35003/vsf2hg/xrpcnv
title: Supplementary Table 6.tab

description: Values used for collisional erosion models in Figure 2.
DOI: 10.35003/vsf2hg/7ffzcx
title: Supplementary Table 7.tab

description: Values used for mixing models in Figure 3.
DOI: 10.35003/vsf2hg/g7kj7l
title: Source Data Table_1.tab

description: Nd isotope compositions of chondrite samples
DOI: 10.35003/vsf2hg/yqwqkh
title: Supplementary Table 4.tab

description: Average Nd isotope compositions for chondritic and terrestrial sample groups.
DOI: 10.35003/vsf2hg/kacr1p
title: Extended Data Fig_1.docx

description: Nucleosynthetic anomaly patterns for Nd.
DOI: 10.35003/vsf2hg/vaugl9
title: Fig_3.docx

description: Mixing models for enstatite chondrites with oldhamite and olivine.
DOI: 10.35003/vsf2hg/4az7ji
title: Fig_2.docx

description: μ142Nd versus ε143Nd for a single-stage collisional erosion model coincident with the Moon-forming giant impact.
DOI: 10.35003/vsf2hg/t7cxco
title: Supplementary Table 3.tab

description: Measured and corrected 142Nd values
DOI: 10.35003/vsf2hg/00jksz
title: Extended Data Fig_2.docx

description: Nd isotope compositions of chondrite groups and CAIs.
DOI: 10.35003/vsf2hg/7jrghq
title: Extended Data Fig_3.docx

description: Nd isotope variations in chondrites, CAI’s and accessible Earth.
DOI: 10.35003/vsf2hg/bponlq
title: Fig_1.docx

description: Neodymium isotope variations of chondrites, CAIs and Earth.
DOI: 10.35003/vsf2hg/w2sl1m
title: Data ReferencesList.docx

description: :unav
DOI: 10.35003/6d0kzx
title: Replication Data for: Collisional mixing between inner and outer solar system planetesimals inferred from the Nedagolla iron meteorite

description: Abstract: The ungrouped iron meteorite Nedagolla is the first meteorite with bulk Mo, Ru, and Ni isotopic compositions that are intermediate between those of the non-carbonaceous (NC) and carbonaceous (CC) meteorite reservoirs. The Hf-W chronology of Nedagolla indicates that this mixed NC-CC isotopic composition was established relatively late, more than 7 million years after Solar System formation. The mixed NC-CC isotopic composition is consistent with the chemical composition of Nedagolla, which combines signatures of metal segregation under more oxidizing conditions (relative depletions in Mo and W), characteristic for CC bodies, and more reducing conditions (high Si and Cr contents), characteristic for some NC bodies, in a single sample. These data combined suggest that Nedagolla formed as the result of collisional mixing of NC and CC core material, which partially re-equilibrated with silicate mantle material that predominantly derives from the NC body. These mixing processes might have occurred during a hit-and-run collision between two differentiated bodies, which also provides a possible pathway for Nedagolla's extreme volatile element depletion. As such, Nedagolla provides the first isotopic evidence for early collisional mixing of NC and CC bodies that is expected as a result of Jupiter's growth.
DOI: 10.35003/6d0kzx/hrcdx6
title: 10.1111-maps.13744_tables.tab

description: Tables 1-6
DOI: 10.35003/6d0kzx/2mt2sk
title: 10.1111-maps.13744Figure137440006.pptx

description: :unav
DOI: 10.35003/6d0kzx/pnvz52
title: 10.1111-maps.13744Figure137440003.pptx

description: :unav
DOI: 10.35003/6d0kzx/typhw5
title: 10.1111-maps.13744Figure137440004.pptx

description: :unav
DOI: 10.35003/6d0kzx/igtttq
title: 10.1111-maps.13744Figure137440002.pptx

description: :unav
DOI: 10.35003/6d0kzx/bs7hbx
title: 10.1111-maps.13744Figure137440001.pptx

description: :unav
DOI: 10.35003/6d0kzx/w5tgrd
title: 10.1111-maps.13744Figure137440005.pptx

description: :unav
DOI: 10.35003/6d0kzx/0wfhrm
title: 10.1111-maps.13744Figure137440007.pptx

description: :unav
DOI: 10.35003/wlb2eq
title: Replication Data for: The storage capacity of fluorine in olivine and pyroxene under upper mantle conditions.

description: Abstract: We present new experimental results on the fluorine storage capacity of olivine and orthopyroxene in the Earth’s mantle. Experiments were performed in the system MgO-SiO2 + MgF2 at temperatures between 1350 °C and 1700 °C and pressures up to 17 GPa. Electron microprobe measurements show that fluorine concentrations in olivine reach up to 5100 µg/g. The storage capacity of fluorine in olivine shows only a small pressure dependence but a strong temperature dependence with a positive correlation between increasing temperature and fluorine storage capacity. Fluorine concentrations found in enstatite are one order of magnitude smaller and reach up to 670 µg/g. Our data show that concentrations of fluorine in fluorine-saturated olivine are in the same range as water concentrations in olivine. Nevertheless, fluorine and water solubility in olivine show opposing behavior with increasing pressure and temperature. The fluorine solubility in olivine increases with increasing temperature but is not much affected by pressure. In contrast, water solubility in olivine has previously been shown to decrease with increasing temperature and increase with increasing pressure. Our experiments show that nominally fluorine-free minerals like forsterite and enstatite are capable of storing the entire fluorine budget of the upper mantle, without the need to invoke accessory phases such as apatite or amphibole. TRR 170 no. 19
DOI: 10.35003/wlb2eq/9sclmr
title: 1-s2.0-S0016703717302041-mmc1.docx

description: supplement
DOI: 10.35003/wlb2eq/k53pw9
title: Fig._3.jpg

description: F solubility in forsterite with increasing T and constant P.
DOI: 10.35003/wlb2eq/o9edn3
title: Tables 1-4.tab

description: Table 1. Starting material compositions Table 2. Experiments. Table 3. Representative major element composition of olivines and orthopyroxenes. Table 4. Representative olivine/melt or fluid and opx/melt or fluid partition coefficients in different experimental systems. ol = olivine.
DOI: 10.35003/wlb2eq/g1aqhv
title: Fig._1.jpg

description: Backscattered electron images of experimental runs.
DOI: 10.35003/wlb2eq/4d2fln
title: Fig._2.jpg

description: F solubility in forsterite olivine at 1500 °C and different P.
DOI: 10.35003/wlb2eq/vjvba4
title: Full captions figures 1-3.docx

description: Full captions of figures 1-3.
DOI: 10.5281/zenodo.7778703
title: Optimized OPEP Force Field for Simulation of Crowded Protein Solutions

description: Initial structures (in the PDB format) and LBMD trajectories (in the GROMACS XTC format) of crowded protein solutions simulated using the OPEPv7 force field and presented in the article entitled <em>Optimized OPEP Force Field for Simulation of Crowded Protein Solutions </em>(https://doi.org/10.1021/acs.jpcb.3c00253).
DOI: 10.5281/zenodo.7778702
title: Optimized OPEP Force Field for Simulation of Crowded Protein Solutions

description: Initial structures (in the PDB format) and LBMD trajectories (in the GROMACS XTC format) of crowded protein solutions simulated using the OPEPv7 force field and presented in the article entitled <em>Optimized OPEP Force Field for Simulation of Crowded Protein Solutions </em>(https://doi.org/10.1021/acs.jpcb.3c00253).
DOI: 10.35003/ty6mkx
title: Replication Data for: Nucleosynthetic zinc isotope anomalies reveal a dual origin of terrestrial volatiles

description: • Nucleosynthetic isotope anomalies for volatile element zinc. • Same nucleosynthetic NC-CC dichotomy as for non-volatile elements. • Terrestrial zinc mixture of ~70% NC and ~ 30% CC. • Same mixing proportions for hydrogen and nitrogen. • Terrestrial volatiles predominantly from inner and not outer Solar System.
DOI: 10.35003/ty6mkx/oywugo
title: Fig._2.jpg

description: :unav
DOI: 10.35003/ty6mkx/d1uled
title: Fig._3.jpg

description: :unav
DOI: 10.35003/ty6mkx/znuznx
title: Fig._1.jpg

description: :unav
DOI: 10.35003/ty6mkx/qrm0ev
title: Tbl_1.xlsx

description: Mass-independent Zn isotope compositions of meteorites and terrestrial samples.
DOI: 10.35003/ty6mkx/w3upgn
title: 1-s2.0-S0019103522002731-mmc1.docx

description: Supplementary materials_Nucleosynthetic zinc isotope anomalies reveal a dual origin of terrestrial volatiles.