cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.17632/bnfzdtbmzf.2
title: Open dataset for: "Delta-beta cross-frequency coupling as an index of stress regulation during social-evaluative threat"

description: Open data and R analysis scripts for the paper as submitted for publication: "Poppelaars, E. S., Klackl, J., Pletzer, B., & Jonas, E. (2019). Delta-beta cross-frequency coupling as an index of stress regulation during social-evaluative threat." Hypotheses and analyses were preregistered: Poppelaars, E. S., Klackl, J., Pletzer, B., & Jonas, E. (2018). Delta-beta cross-frequency coupling as an index of stress regulation during social-evaluative threat. Open Science Framework. https://osf.io/8gchf/register/565fb3678c5e4a66b5582f67. Description of the dataset: A dataset of 37 men and 30 women (tested in the luteal phase of their menstrual cycle) participated in a public speaking task to induce social-evaluative threat. Responses of multiple stress systems were measured (sympathetic and parasympathetic nervous system activity, self-reported affect, and hypothalamic–pituitary–adrenal axis activity), as well as personality traits (e.g. trait social anxiety), and EEG delta-beta cross-frequency coupling (e.g., frontal and parietal amplitude-amplitude correlation and phase-amplitude coupling). Description of analyses files: - File 'README.txt' contains the description of the files (metadata). - File 'SET_CFC_MatlabOutput.xlsx' contains the delta-beta coupling data, calculated using MATLAB scripts from https://github.com/ESPoppelaars/Cross-frequency-coupling. - File 'SETData.sav' contains the raw stress and personality data, taken from https://doi.org/10.17632/7vj8r76s6f. - Files 'SET_CFC.outl.del.RData' contains the complete dataset with missing values and outliers deleted. - File 'Codebook_SET_CFC.outl.del.csv' contains a description of all variables in the 'SET_CFC.outl.del.RData' file (metadata). - Files 'SET_CFC.outl.del.imp.RData' and 'SET_CFC.outl.del.imp.extra.RData' contain multiple imputed datasets (without missing values) that can be used to reproduce results from the paper. - File 'LSA_HSA_brief.RData' contains data to use as informed priors for the Bayesian analyses, calculated from data published at https://doi.org/10.3758/s13415-018-0603-7. - File 'Codebook_LSA_HSA_brief.csv' contains a description of all variables in the 'LSA_HSA_brief.RData' file (metadata). - File '01_CalculationOfData.R' is an R analysis script that imports the raw data, calculates new variables, and imputes missing data via multiple imputation using the 'predictorMatrixAdj.xlsx' file. - File '02_AnalysisOfImputedData.R' is an R analysis script that calculates descriptive statistics, creates plots, and tests hypotheses using t-tests, Bayesian statistics, and multiple lineair regressions. Also uses the custom functions: 'BF.evidence.R', 'cohen.d.magnitude.R' and 'p.value.sig.R', as well as the 'BF_t.R' file as taken from https://doi.org/10.17045/sthlmuni.4981154.v3.
DOI: 10.21227/8ydn-a311
title: Improving the Performance of Low Voltage Networks by an Optimized Unbalance Operation of Three-Phase Distributed Generators

description: This work focuses on using the full potential of PV inverters in order to improve the efficiency of low voltage networks. More specifically, the independent per-phase control capability of PV three-phase four-wire inverters, which are able to inject different active and reactive powers in each phase, in order to reduce the system phase unbalance is considered. This new operational procedure is analyzed by raising an optimization problem which uses a very accurate modelling of European low voltage networks. The paper includes a comprehensive quantitative comparison of the proposed strategy with two state-of-the-art methodologies to highlight the obtained benefits. The achieved results evidence that the proposed independent per-phase control of three-phase PV inverters improves considerably the network performance contributing to increase the penetration of renewable energy sources.
DOI: 10.5281/zenodo.3541148
title: Extended Data for Publication "Testing the Spectroscopic Extraction of Suppression of Convective Blueshift"

description: Efforts to detect low-mass exoplanets using stellar radial velocities (RVs) are currently limited by magnetic photospheric activity. Suppression of convective blueshift is the dominant magnetic contribution to RV variability in low-activity Sun-like stars. Due to convective plasma motions, the magnitude of RV contributions from the suppression of convective blueshift is roughly correlated with the depth of formation of photospheric spectral lines used to compute the RV time series. Meunier et al. (2017), used this relation to demonstrate a method for spectroscopic extraction of the suppression of convective blueshift in order to isolate RV contributions, including planetary RVs, that contribute equally to the timeseries for each spectral line. In this publication, we extract disk-integrated solar RVs from observations over a 2.5 year time span made with the solar telescope integrated with the HARPS-N spectrograph at the Telescopio Nazionale Galileo (La Palma, Canary Islands, Spain). We apply the methods outlined by Meunier et al. (2017) - as part of this analysis, we fit Gaussian line profiles to 765 iron lines measured over 457 exposures. Here, we provide the complete line list (Table 1; Table1_LineList.csv) used in our analysis, and the resulting RVs time series in their entirety (Table 3; Table3_TimeSeries.csv). Wavelengths are given in Angstroms, and RVs in m/s. We also include 4 CSV files with the line fit parameters of each line profile: Each row corresponds to a single exposure time (corresponding to the JDs in Table 3) and each column corresponds to a specific spectral line (with wavelength specified in Table 1). We fit each spectral line to a Gaussian of the form: \(f(\lambda) = p_1 - p_2 \exp \left[- {1 \over 2} \left({{\lambda - p_3} \over p_4}\right)^2 \right]\) p<sub>1</sub> is the continuum level in arbitrary units (LineProfiles_Continuum.csv)<br> p<sub>2</sub> is the line strength in arbitrary units (LineProfiles_Amplitude.csv)<br> p<sub>3</sub> is the line shift in Angstroms (LineProfiles_Shift.csv)<br> p<sub>4</sub> is the line width in Angstroms (LineProfiles_Width.csv)
DOI: 10.5281/zenodo.3541149
title: Extended Data for Publication "Testing the Spectroscopic Extraction of Suppression of Convective Blueshift"

description: Efforts to detect low-mass exoplanets using stellar radial velocities (RVs) are currently limited by magnetic photospheric activity. Suppression of convective blueshift is the dominant magnetic contribution to RV variability in low-activity Sun-like stars. Due to convective plasma motions, the magnitude of RV contributions from the suppression of convective blueshift is roughly correlated with the depth of formation of photospheric spectral lines used to compute the RV time series. Meunier et al. (2017), used this relation to demonstrate a method for spectroscopic extraction of the suppression of convective blueshift in order to isolate RV contributions, including planetary RVs, that contribute equally to the timeseries for each spectral line. In this publication, we extract disk-integrated solar RVs from observations over a 2.5 year time span made with the solar telescope integrated with the HARPS-N spectrograph at the Telescopio Nazionale Galileo (La Palma, Canary Islands, Spain). We apply the methods outlined by Meunier et al. (2017) - as part of this analysis, we fit Gaussian line profiles to 765 iron lines measured over 457 exposures. Here, we provide the complete line list (Table 1; Table1_LineList.csv) used in our analysis, and the resulting RVs time series in their entirety (Table 3; Table3_TimeSeries.csv). Wavelengths are given in Angstroms, and RVs in m/s. We also include 4 CSV files with the line fit parameters of each line profile: Each row corresponds to a single exposure time (corresponding to the JDs in Table 3) and each column corresponds to a specific spectral line (with wavelength specified in Table 1). We fit each spectral line to a Gaussian of the form: \(f(\lambda) = p_1 - p_2 \exp \left[- {1 \over 2} \left({{\lambda - p_3} \over p_4}\right)^2 \right]\) p<sub>1</sub> is the continuum level in arbitrary units (LineProfiles_Continuum.csv)<br> p<sub>2</sub> is the line strength in arbitrary units (LineProfiles_Amplitude.csv)<br> p<sub>3</sub> is the line shift in Angstroms (LineProfiles_Shift.csv)<br> p<sub>4</sub> is the line width in Angstroms (LineProfiles_Width.csv)
DOI: 10.5285/c8ed5d039558446bbcd12b695389abb1
title: HadUK-Grid Gridded Climate Observations on a 25km grid over the UK, v1.0.0.0 (1862-2017)

description: HadUK-Grid is a collection of gridded climate variables derived from the network of UK land surface observations. The data have been interpolated from meteorological station data onto a uniform grid to provide complete and consistent coverage across the UK. The data set at 25 km resolution is derived from the associated 1km x 1km resolution to allow for comparison to data from UKCP18 climate projections. The dataset spans the period from 1862 to 2017, but the start time is dependent on climate variable and temporal resolution. The grids are produced for daily, monthly, seasonal and annual timescales, as well as long term averages for a set of climatological reference periods. Variables include air temperature (maximum, minimum and mean), precipitation, sunshine, mean sea level pressure, wind speed, relative humidity, vapour pressure, days of snow lying, and days of ground frost. This data set supersedes the UKCP09 gridded observations. Subsequent versions may be released in due course and will follow the version numbering as outlined by Hollis et al. (2018, see linked documentation). The primary purpose of these data are to facilitate monitoring of UK climate and research into climate change, impacts and adaptation. The datasets have been created by the Met Office with financial support from the Department for Business, Energy and Industrial Strategy (BEIS) and Department for Environment, Food and Rural Affairs (DEFRA) in order to support the Public Weather Service Customer Group (PWSCG), the Hadley Centre Climate Programme, and the UK Climate Projections (UKCP18) project. The data recovery activity to supplement 19th and early 20th Century data availability has also been funded by the Natural Environment Research Council (NERC grant ref: NE/L01016X/1) project "Analysis of historic drought and water scarcity in the UK". The dataset is provided under Open Government Licence.
DOI: 10.5286/isis.e.rb1920227
title: Metal Ion Solubility in Deep Eutectic Solvents

description: Recent work on deep eutectic solvents (DES) has demonstrated that these novel H-bonded liquids can be used to modify nanomaterial morphologies under mild conditions in solvothermal syntheses. In addition to being inexpensive, non-flammable and having low volatility, it has been shown that DES can be excellent solvents for a variety of transition metal species. However the solubility of, for instance, metal oxides varies dramatically with the solvent type and molar ratio of the components. Here we wish to better understand how metal ions are solvated in DES using the example of p-toluenesulfonic acid:choline chloride DES, which dissolves substantial amounts of many transition metal oxides. The solubility of ZnO in this DES is much higher when a molar ratio of 2:1 is used than at a ratio of 1:2. We will probe the DES structure at these ratios and how addition of Zn2+ perturbs the structure
DOI: 10.5286/isis.e.rb1920227-1
title: Metal Ion Solubility in Deep Eutectic Solvents

description: Recent work on deep eutectic solvents (DES) has demonstrated that these novel H-bonded liquids can be used to modify nanomaterial morphologies under mild conditions in solvothermal syntheses. In addition to being inexpensive, non-flammable and having low volatility, it has been shown that DES can be excellent solvents for a variety of transition metal species. However the solubility of, for instance, metal oxides varies dramatically with the solvent type and molar ratio of the components. Here we wish to better understand how metal ions are solvated in DES using the example of p-toluenesulfonic acid:choline chloride DES, which dissolves substantial amounts of many transition metal oxides. The solubility of ZnO in this DES is much higher when a molar ratio of 2:1 is used than at a ratio of 1:2. We will probe the DES structure at these ratios and how addition of Zn2+ perturbs the structure
DOI: 10.5286/isis.e.rb1920250
title: Vibrational behaviour of confined water molecules in NaX faujasite as function of the hydration levels

description: We propose to investigate the vibrational spectra of NaX faujasite as a function of hydration using simultaneous INS and Raman spectroscopy on TOSCA. Prior to the beamtime we will prepare 3 NaX faujasite samples with a different hydration level (10%, 15% and 30% in mass). The ability of TOSCA to capture the entire vibrational energy range in one measurement is key to the experiment. The use of neutron spectroscopy will allow more direct access to the boson peak information than other techniques would afford. Measuring the Raman spectra simultaneously with the INS is vital in ensuring that the samples measured have identical moisture content and will mean that the full energy range can be measured for each sample
DOI: 10.5286/isis.e.rb1920250-1
title: Vibrational behaviour of confined water molecules in NaX faujasite as function of the hydration levels

description: We propose to investigate the vibrational spectra of NaX faujasite as a function of hydration using simultaneous INS and Raman spectroscopy on TOSCA. Prior to the beamtime we will prepare 3 NaX faujasite samples with a different hydration level (10%, 15% and 30% in mass). The ability of TOSCA to capture the entire vibrational energy range in one measurement is key to the experiment. The use of neutron spectroscopy will allow more direct access to the boson peak information than other techniques would afford. Measuring the Raman spectra simultaneously with the INS is vital in ensuring that the samples measured have identical moisture content and will mean that the full energy range can be measured for each sample
DOI: 10.5286/isis.e.rb1920608-1
title: OH- and water dynamics in Anionic Exchange Membranes (AEMs)

description: Over the past few decades, fuel cell research has grown exponentially with the continued development of new materials and systems for automotive and stationary applications. Most interest has focused on polymer electrolyte (both cation -CEM- and anion -AEM- exchange membranes) membrane fuel cells because of their power densities, lower cost and wider applications. Albeit intensive efforts have been made to develop and improve AEMs membranes, they still display poor ionic conductivity. This is also because, to date, very little is known on the relation between OH- transport and water dynamics. In this proposal, we want to investigate the OH- and water dynamics in a commercial AEM membrane by QENS in function of hydration and temperature with the final aim to unravel the transport basic mechanisms and with a view to advancing towardshelp designing advanced higher performance AEMs.
DOI: 10.7910/dvn/piokqz/cvwjm2
title: 02_36_Fodder_Poultry_Livestock_Which_Used_Labor_After_Fodder.tab

description: :unav
DOI: 10.7910/dvn/piokqz/dtrtyg
title: 02_31_Fodder_Poultry_Livestock_Inputs_After_Fodder.tab

description: :unav
DOI: 10.7910/dvn/piokqz/esm7f2
title: 01_14_Active_Restoration_Livestock_Products_before_restoration.tab

description: :unav
DOI: 10.7910/dvn/piokqz/gubekt
title: 01_10_Active_Restoration_Livestock_kept_after_restoration.tab

description: :unav
DOI: 10.7910/dvn/piokqz/mb96jb
title: 02_13_Fodder_Poultry_Crop_Inputs_After_Fodde_Supp.tab

description: :unav
DOI: 10.7910/dvn/piokqz/pcsotz
title: 02_05_Fodder_Poultry_Crops_Yr4before_Fodder.tab

description: :unav
DOI: 10.7910/dvn/piokqz/qpm4qv
title: 02_33_Fodder_Poultry_Livestock_Labor_After_Fodder.tab

description: :unav
DOI: 10.7910/dvn/piokqz/reuwif
title: 02_17_Fodder_Poultry_Crop_Inputs_Yr4before_Fodde_Supp.tab

description: :unav
DOI: 10.7910/dvn/piokqz/s1sphl
title: 01_05_Active_Restoration_Inputs_used_for_livestock_production_after.tab

description: :unav
DOI: 10.7910/dvn/piokqz/yqq1ui
title: 02_01_Fodder_Poultry_Main_File.tab

description: :unav
DOI: 10.5281/zenodo.3541733
title: A semi-analytical interpretation model of pulse decay measurement on ultra-tight rocks

description: This contribution presents a new semi-analytical model for the evaluation of the initial (early time) stage of pulse decay permeability tests, i.e. before reaching quasi-steady state flow conditions and prior to a significant pressure increase in the downstream reservoir. The analytical model considers gas compressibility and slippage effects. In order to validate the proposed method, measurements were performed on a core sample of the Cretaceous Eagle Ford shale, Texas, USA, under different pore and confining pressures. Helium was used as the test fluid to minimize effects from adsorption. Permeability coefficients obtained from this new approach agree well with those from the classical pulse decay evaluation while the duration of tests was reduced from hours to minutes. The present model is a good supplement for the pulse decay method and suitable for measurements of ultra-low-permeability rocks.
DOI: 10.5281/zenodo.3541734
title: A semi-analytical interpretation model of pulse decay measurement on ultra-tight rocks

description: This contribution presents a new semi-analytical model for the evaluation of the initial (early time) stage of pulse decay permeability tests, i.e. before reaching quasi-steady state flow conditions and prior to a significant pressure increase in the downstream reservoir. The analytical model considers gas compressibility and slippage effects. In order to validate the proposed method, measurements were performed on a core sample of the Cretaceous Eagle Ford shale, Texas, USA, under different pore and confining pressures. Helium was used as the test fluid to minimize effects from adsorption. Permeability coefficients obtained from this new approach agree well with those from the classical pulse decay evaluation while the duration of tests was reduced from hours to minutes. The present model is a good supplement for the pulse decay method and suitable for measurements of ultra-low-permeability rocks.
DOI: 10.5285/a2fb07be9622439fa191f0e596f5e4f9
title: HadUK-Grid Gridded Climate Observations on a 60km grid over the UK, v1.0.0.0 (1862-2017)

description: HadUK-Grid is a collection of gridded climate variables derived from the network of UK land surface observations. The data have been interpolated from meteorological station data onto a uniform grid to provide complete and consistent coverage across the UK. The data set at 60 km resolution is derived from the associated 1km x 1km resolution to allow for comparison to data from UKCP18 climate projections. The dataset spans the period from 1862 to 2017, but the start time is dependent on climate variable and temporal resolution. The grids are produced for daily, monthly, seasonal and annual timescales, as well as long term averages for a set of climatological reference periods. Variables include air temperature (maximum, minimum and mean), precipitation, sunshine, mean sea level pressure, wind speed, relative humidity, vapour pressure, days of snow lying, and days of ground frost. This data set supersedes the UKCP09 gridded observations. Subsequent versions may be released in due course and will follow the version numbering as outlined by Hollis et al. (2018, see linked documentation). The primary purpose of these data are to facilitate monitoring of UK climate and research into climate change, impacts and adaptation. The datasets have been created by the Met Office with financial support from the Department for Business, Energy and Industrial Strategy (BEIS) and Department for Environment, Food and Rural Affairs (DEFRA) in order to support the Public Weather Service Customer Group (PWSCG), the Hadley Centre Climate Programme, and the UK Climate Projections (UKCP18) project. The data recovery activity to supplement 19th and early 20th Century data availability has also been funded by the Natural Environment Research Council (NERC grant ref: NE/L01016X/1) project "Analysis of historic drought and water scarcity in the UK". The dataset is provided under Open Government Licence.
DOI: 10.5286/isis.e.rb1920013
title: The role of defects in the pressure-induced octahedral tilting in Prussian blue analogues

description: We propose a high-pressure study of two Prussian blue analogues, Mn[Co(CN)6]0.67 and MnPt(CN)6. Our high-pressure XRD study shows a phase transition from cubic to rhombohedral symmetry driven by octahedral tilting---like the octahedral rotations in perovskites. However, we could not reliably compare the magnitude of the tilting, as it is manifested in the positions of the cyanide linkers, which cannot be accurately determined from XRD in the presence of heavy metals. Understanding the factors that influence the amplitude of the tilting distortion is important, as tilting impacts the magnetic pathways and the electrochemical performance. In addition, exploring tilting in Prussian blue analogues is of interest from a fundamental viewpoint, to compare to the wealth of literature on oxide perovskites. This will be the first neutron study on pressure-induced rotations in these systems.
DOI: 10.5286/isis.e.rb1920013-1
title: The role of defects in the pressure-induced octahedral tilting in Prussian blue analogues

description: We propose a high-pressure study of two Prussian blue analogues, Mn[Co(CN)6]0.67 and MnPt(CN)6. Our high-pressure XRD study shows a phase transition from cubic to rhombohedral symmetry driven by octahedral tilting---like the octahedral rotations in perovskites. However, we could not reliably compare the magnitude of the tilting, as it is manifested in the positions of the cyanide linkers, which cannot be accurately determined from XRD in the presence of heavy metals. Understanding the factors that influence the amplitude of the tilting distortion is important, as tilting impacts the magnetic pathways and the electrochemical performance. In addition, exploring tilting in Prussian blue analogues is of interest from a fundamental viewpoint, to compare to the wealth of literature on oxide perovskites. This will be the first neutron study on pressure-induced rotations in these systems.
DOI: 10.5286/isis.e.rb1920023
title: Rod reversed micelles with mixtures of optimized surfactants and hydrotropes

description: Contrast variation SANS will be used to study structures of reversed micelles in cyclohexane, and in particular to reveal effects of hydrotrope addition for promotion and growth of cylindrical micellar aggregates. This equilibrium study represents the first stage of a broader project, which will involve future high pressure/temperature and shear SANS experiments, aimed at understanding the recently discovered role of reversed micelles in lubricants. This is the first stage in a new 3.5-year PhD program to develop optimized lubricant fluids, and Georgina Moody is a 1st year PhD student, fully funded by Infineum.
DOI: 10.5286/isis.e.rb1920023-1
title: Rod reversed micelles with mixtures of optimized surfactants and hydrotropes

description: Contrast variation SANS will be used to study structures of reversed micelles in cyclohexane, and in particular to reveal effects of hydrotrope addition for promotion and growth of cylindrical micellar aggregates. This equilibrium study represents the first stage of a broader project, which will involve future high pressure/temperature and shear SANS experiments, aimed at understanding the recently discovered role of reversed micelles in lubricants. This is the first stage in a new 3.5-year PhD program to develop optimized lubricant fluids, and Georgina Moody is a 1st year PhD student, fully funded by Infineum.