cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.34725/dvn/fnvtbd/cyclag
title: 1.SENTINEL LANDSCAPE HH v1 1 (TRADUIT) +comment questionnaire.doc
DOI: 10.34725/dvn/fnvtbd/cyxuoa
title: 4.HH_CAFHUT_Ver.tab

description: SPSS data file for the cleaned and verified household data
DOI: 10.34725/dvn/fnvtbd/d5brdf
title: Household_Instrument_CAFHUT.xls

description: ODK form for data collection using tablets.
DOI: 10.34725/dvn/fnvtbd/g6kqg9
title: 0.Disclaimer.pdf
DOI: 10.34725/dvn/fnvtbd/luxil1
title: 1.SENTINEL LANDSCAPE HH v1 1 (TRADUIT) +comment questionnaire.doc

description: Questionnaire used
DOI: 10.34725/dvn/fnvtbd/p5arrk
title: 3.HH_EtiolomoMintom_Raw.tab

description: Raw household data colleted in Etiolomo and Mintom sites in the CAFHUT SL.
DOI: 10.34725/dvn/fnvtbd/pqm0fg
title: 4.HH_CAFHUT_Ver-2.tab

description: SPSS data file for the cleaned and verified household data
DOI: 10.34725/dvn/fnvtbd/ww1qvr
title: 3.HH_CAFHUT_Raw.csv

description: CSV data file for the raw household data collected in the CAFHUT SL.
DOI: 10.34725/dvn/fnvtbd/gtopau
title: 4.HH_CAFHUT_Ver.tab

description: Cleaned and verified household data from CAFHUT SL
DOI: 10.34725/dvn/fnvtbd/hsoncf
title: Generic Codebook.csv

description: Description of variables for the household data collected.
DOI: 10.34725/dvn/fnvtbd/yajtea
title: 0.Disclaimer.pdf
DOI: 10.34725/dvn/fnvtbd/ylsbhq
title: 4.HH_CAFHUT_Ver.tab

description: SPSS data file for the cleaned and verified household data
DOI: 10.25606/surf.578c6039-28af7762
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-488)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 488 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3445281
title: European Union Summary Reports on surveillance for the presence of TSE: historical reported cases

description: The tables contain all historical cases reported until 2016 for classical and atypical BSE, classical and atypical scrapie in sheep and goats. A new version has been added with numbered order of uploaded files.
description: xls; EU; biocontam@efsa.europa.eu
DOI: 10.18430/m36et8
title: X-ray diffraction data for the crystal structure of AlbA in complex with albicidin (6ET8)
DOI: 10.18430/m36g70
title: X-ray diffraction data for the structure of murine Prpf39 (6G70)
DOI: 10.25606/surf.578c6039-ce5cf5c9
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-601)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 601 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-95fb2d08
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-532)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 532 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-52da34ab
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-696)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 696 of the 2048³ resolution collection.
DOI: 10.15468/atl470
title: Checklist of fungi of the Onega Pomorie National Park

description: The fungi occurring in the park’s area have been studied by a team of the park’s research officers in cooperation with the scientists of Lomonosov Moscow State University’s Biological Faculty, and Russian Academy of Sciences’ Botanical Institute (Saint-Petersburg).
DOI: 10.25606/surf.578c6039-1f9a332a
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-598)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 598 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3444498
title: Demonstration case study reports

description: As part of the PLAID project an in-depth assessments of the processes involved in achieving efficient and effective on-farm demonstration activities was investigated. 24 year-long studies of demonstration events and activities were selected and followed 2 case studies in each partner country were selected, which followed demonstration from initial commissioning through to impact assessment. The specific objectives were Improved understanding of the key elements that contribute to successful and effective demonstration activities on commercial farms, looking specifically at: commissioning and financing, topic selection, accessibility, mediation techniques, and embeddedness. Gender will be specifically addressed. Improved understanding of the effectiveness of demonstration activities in terms of learning by participants (at the individual level and the network level: what is learned, by whom, how and why?) and the subsequent impact (i.e. actual implementation of what farmers have learned on their own farm, new network development, innovation inception). Assess the role of demonstration within the wider AKIS systems and what the impact of demonstration is on learning and technology adoption Develop insights into critical success factors, best (and poor) practices, and indicators for effective and successful demonstration activities.
DOI: 10.5281/zenodo.3444499
title: Demonstration case study reports

description: As part of the PLAID project an in-depth assessments of the processes involved in achieving efficient and effective on-farm demonstration activities was investigated. 24 year-long studies of demonstration events and activities were selected and followed 2 case studies in each partner country were selected, which followed demonstration from initial commissioning through to impact assessment. The specific objectives were Improved understanding of the key elements that contribute to successful and effective demonstration activities on commercial farms, looking specifically at: commissioning and financing, topic selection, accessibility, mediation techniques, and embeddedness. Gender will be specifically addressed. Improved understanding of the effectiveness of demonstration activities in terms of learning by participants (at the individual level and the network level: what is learned, by whom, how and why?) and the subsequent impact (i.e. actual implementation of what farmers have learned on their own farm, new network development, innovation inception). Assess the role of demonstration within the wider AKIS systems and what the impact of demonstration is on learning and technology adoption Develop insights into critical success factors, best (and poor) practices, and indicators for effective and successful demonstration activities.
DOI: 10.25606/surf.578c6039-c1d2fe46
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-145)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 145 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-ef0100ec
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-600)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 600 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3445395
title: Database for comparison between Hybrid Capture and PCR techniques for HPV-HR detection

description: This database displays the results from the HPV-HR detection with the gold standard technique Hybrid Capture 2 (HC2) and different PCR-based techniques. These results are compared in order to determine the degree of agreement between theses techniques.
DOI: 10.24378/exe.1883
title: On the optimal position of an emitter in a wavelength-scale parabolic reflector (dataset)

description: We investigate the optimum emitter position within reflecting parabolic antennas whose size is comparable to the emission wavelength. Using finite-element modelling we calculate the dependence of the amount of power directed into a 20° half-angle cone on the emitter’s position and compare with results obtained using geometrical optics. The spatially varying density of states within the wavelength-scale reflector is mapped and its impact discussed. In addition, it is demonstrated that changing the characteristic size of the reflector within the range from 0.5 to 1.5 times the emission wavelength has a strong bearing on the optimum emitter position, a position that does not in general coincide with the parabola’s focus. We calculate that the optimal antenna size and emitter position allow for the maximum directed power to exceed that obtained in the geometrical optics regime.
description: The dataset is divided into folders referring to each applicable figure in the corresponding publication. Within each of these folders (or subfolders within) is a .txt file beginning 'Descrip' which explains the contents of the files and how they were used to generate the figures seen in the publication. Where practical there is both the 'raw' data straight from COMSOL multiphysics simulations and the processed version which can be directly used to generate the figures in the paper.
description: The article associated with this dataset is available on open access in ORE at http://hdl.handle.net/10871/39155, with the title 'Optimal position of an emitter in a wavelength-scale parabolic reflector'
DOI: 10.25606/surf.578c6039-f0111585
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-468)

description: We present the results of the "Cosmogrid" cosmological N-body simulation suites based on the concordance LCDM model. The Cosmogrid simulation was performed in a 30 Mpc box with 2048³ particles. The mass of each particle is 1.28x10^5 Msun, which is sufficient to resolve ultra-faint dwarfs. We found that the halo mass function shows good agreement with the Sheth & Tormen fitting function down to ~10^7 Msun. We have analyzed the spherically averaged density profiles of the three most massive halos which are of galaxy group size and contain at least 170 million particles. The slopes of these density profiles become shallower than -1 at the inner most radius. We also find a clear correlation of halo concentration with mass. The mass dependence of the concentration parameter cannot be expressed by a single power law, however a simple model based on the Press-Schechter theory proposed by Navarro et al. gives reasonable agreement with this dependence. The spin parameter does not show a correlation with the halo mass. The probability distribution functions for both concentration and spin are well fitted by the log-normal distribution for halos with the masses larger than ~10^8 Msun. The subhalo abundance depends on the halo mass. Galaxy-sized halos have 50% more subhalos than ~10^11 Msun halos have. This is snapshot 468 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3444088
title: Data for manuscript Marmet, Studer, Lemoine, Grazioli, Bertholet & Gmel (2019). Reconsidering the associations between self-reported alcohol use disorder and mental health problems in the light of co-occurring addictions in young Swiss men. Plos One. DOI: 10.1371/journal.pone.0222806.

description: Dataset for the manuscript Marmet, Studer, Lemoine, Grazioli, Bertholet & Gmel (2019). Reconsidering the associations between self-reported alcohol use disorder and mental health problems in the light of co-occurring addictions in young Swiss men. Plos One. DOI: 10.1371/journal.pone.0222806. The dataset contains all data needed to reproduce the results in the above cited manuscript. Variable description and labels can be found in the codebook. For further information on the instruments used please refer to the manuscript. The data was collected between April 2016 and March 2018 in Switzerland by the C-SURF study (www.c-surf.ch). Participants were on average 25 years old when they answered the questionnaires. The final sample size used in the manuscript is 5516. Please note that the dataset contains 25 datasets created with multiple imputation, therefore there are no missing values in the dataset. The research protocol for this study was approved by the Human Research Ethics Committee of the Canton Vaud (Protocol No. 15/07). Data collection was funded by the Swiss National Science Foundation (FN 33CSC0-122679, FN 33CS30_139467, FN 33CS30_148493)
DOI: 10.5281/zenodo.3444089
title: Data for manuscript Marmet, Studer, Lemoine, Grazioli, Bertholet & Gmel (2019). Reconsidering the associations between self-reported alcohol use disorder and mental health problems in the light of co-occurring addictions in young Swiss men. Plos One. DOI: 10.1371/journal.pone.0222806.

description: Dataset for the manuscript Marmet, Studer, Lemoine, Grazioli, Bertholet & Gmel (2019). Reconsidering the associations between self-reported alcohol use disorder and mental health problems in the light of co-occurring addictions in young Swiss men. Plos One. DOI: 10.1371/journal.pone.0222806. The dataset contains all data needed to reproduce the results in the above cited manuscript. Variable description and labels can be found in the codebook. For further information on the instruments used please refer to the manuscript. The data was collected between April 2016 and March 2018 in Switzerland by the C-SURF study (www.c-surf.ch). Participants were on average 25 years old when they answered the questionnaires. The final sample size used in the manuscript is 5516. Please note that the dataset contains 25 datasets created with multiple imputation, therefore there are no missing values in the dataset. The research protocol for this study was approved by the Human Research Ethics Committee of the Canton Vaud (Protocol No. 15/07). Data collection was funded by the Swiss National Science Foundation (FN 33CSC0-122679, FN 33CS30_139467, FN 33CS30_148493)
DOI: 10.5281/zenodo.3445360
title: Dynamics of Phase Separation from Holography

description: We use holography to develop a physical picture of the real-time evolution of the spinodal instability of a four-dimensional, strongly-coupled gauge theory with a first-order thermal phase transition. The implemented planar symmetry on the gravity side reduces the dynamics to $1+1$ dimensions in the gauge theory. In this dataset, we publish the boundary data of several simulations each in its respective archive. The simulations are all for the same theory as the first evolution of the inhomogeneous triple peak solution published in <strong>arXiv:1703.02948</strong>. They differ in their initial state (initial<strong><em> </em></strong>homogeneous energy density or initial excitation) and longitudinal extent, but are all on a circle in that longitudinal direction due to the periodic boundary condition. Most evolution finish in the preferred universal final state with a single phase separated domain. Their detailed physical analysis can be found in the upcoming paper<strong> arXiv:1905.12544</strong>. 000_Readme.txt provides a quick explanation on the content of each archive. We also provide an optional Mathematica script to plot properties of the stress tensor.
DOI: 10.5281/zenodo.3416448
title: Grey-white matter contrast surface files in ABIDE 1&2 datasets

description: Computed with FreeSurfer. https://surfer.nmr.mgh.harvard.edu/ ABIDE dataset: http://fcon_1000.projects.nitrc.org/indi/abide/ Used in: Fouquet, M., Traut, N., Beggiato, A., Delorme, R., Bourgeron, T., & Toro, R. (2019). Increased contrast of the grey-white matter boundary in the motor, visual and auditory areas in Autism Spectrum Disorders. <em>BioRxiv</em>, 750117. https://doi.org/10.1101/750117 https://github.com/neuroanatomy/GWPC