cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.17632/gkzhmg4yng.1
title: Data for: A new compensation method for insulated core transformer power supply and its optimization using genetic algorithm

description: The file“M0_test” is the single-turn winding mutual inductance data. It was measured experimentally. The file“fullloadfeedback.slx” is a circuit simulation model of the ICT power supply. It was created in Matlab / simulink. The file“GA_opt_turn_cap.m” is the program code of the genetic algorithm optimization process. It is the m file format of matlab. It calls “M0_test” and “fullloadfeedback.slx” when it executes.
DOI: 10.5519/qd.v4zft3p0
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (332 records)
DOI: 10.7910/dvn/rrimzy/gjl0xt
title: Third and Fourth Wave Elections.tab

description: :unav
DOI: 10.7910/dvn/rrimzy/tksulm
title: Codebook - Do Elections Create or Further Path Dependencies.pdf

description: :unav
DOI: 10.7910/dvn/rrimzy/ujjsq9
title: Codebook - Do Elections Create or Further Path Dependencies.pdf

description: :unav
DOI: 10.17632/gpphys79dh.1
title: Data for: Precipitation variations recorded in tree rings from the upper Salween and Brahmaputra River valleys, China

description: Here we reconstruct precipitation variations from prior September to current June (r2 = 43%, 1600-2016 CE) in the upper Salween River valley and from prior July to current April (r2 = 44%, 1650-2016 CE) in the upper Brahmaputra River valley based on tree ring width records collected from the Salween and Brahmaputra River basins.
DOI: 10.14469/hpc/6898
title: Figure 2 (Wright BMC Biology 2020)

description: excel file (combined data for Figure 2)
DOI: 10.25345/c5jb2p
title: MassIVE MSV000085864 - GNPS - Bacterial extracts from Spur Estremadura
title: Crude extracts produced by marine bacteria recovered from Spur Stremadura, Portugal.
DOI: 10.14469/hpc/6899
title: Figure 3 (Wright BMC Biology 2020)

description: All primary data files for Figure 3 in Wright et al. BMC Biology 2020
DOI: 10.14469/hpc/6901
title: Figure 5 (Wright BMC Biology 2020)

description: All primary data files for Figure 5 in Wright et al. BMC Biology 2020.
DOI: 10.14469/hpc/6902
title: Figure 6 (Wright BMC Biology 2020)

description: Primary data for Figure 7 in Wright et al. BMC Biology 2020.
DOI: 10.14469/hpc/6900
title: Figure 4 (Wright BMC Biology 2020)

description: All primary data accompanying Figure 4 in Wright et al BMC Biology 2020.
DOI: 10.14469/hpc/6903
title: Figure 7 (Wright BMC Biology 2020)

description: Primary data for Figure 7 in Wright et al. BMC Biology 2020.
DOI: 10.15784/601260
title: Measurements of 14CH4 and 14CO in ice from Taylor Glacier: Last Deglaciation

description: This data set contains measurements of 14CH4 and 14CO in ice cores from Taylor Glacier, Antarctica. This includes measurements in ice from the last deglaciation (18 - 8 kyr), for the purposes of paleoatmospheric 14CH4 reconstruction.
DOI: 10.5281/zenodo.3692742
title: Protecting against Website Fingerprinting with Multihoming – dataset

description: This folder contains the dataset gathered for the paper Protecting against Website Fingerprinting with Multihoming, published at PoPETS 2020. It consists in real Tor traces gathered with different single path and multipath algorithms. The files consist in timestamp and direction (incoming or outgoing) of the Tor cells. More details about the architecture can be found in the paper. More details about this dataset can be found in Section 7 of our paper.
description: https://github.com/sebhenri/HyWF
DOI: 10.5281/zenodo.3692743
title: Protecting against Website Fingerprinting with Multihoming – dataset

description: This folder contains the dataset gathered for the paper Protecting against Website Fingerprinting with Multihoming, published at PoPETS 2020. It consists in real Tor traces gathered with different single path and multipath algorithms. The files consist in timestamp and direction (incoming or outgoing) of the Tor cells. More details about the architecture can be found in the paper. More details about this dataset can be found in Section 7 of our paper.
description: https://github.com/sebhenri/HyWF
DOI: 10.6084/m9.figshare.11918190.v2
title: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment r1i1p1f1

description: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment (one of future scenarios) r1i1p1f1. The grid, named gx1v6, is the displaced pole (the North Pole displaced to the Greenland) grid with 1.1 degree in longitude and 0.27-0.54 degree in latitude.
DOI: 10.5519/qd.7ykfqjrk
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1 records)
DOI: 10.25919/5e5b35c55a268
title: Parkes observations for project P1027 semester 2019OCTS_08

description: We propose to carry out Parkes follow-up observations of the new millisecond pulsar, J1431-6328, discovered by the Australian SKA Pathfinder (ASKAP) and Parkes Ultra-Wideband Low (UWL) receiver. The discovery demonstrated the power of identifying pulsar candidates in radio continuum images and then following up with high time resolution observations. The discovery itself is also interesting. PSR J1431-6328 has a spin period of 2.77 ms, and is likely to be in a binary system. Follow-up observations will enable us to measure the binary parameters, which will guide future multi-wavelength observations and might shed new lights on the binary evolution. The short spin period, relatively large flux density and sky location of PSR J1431-6328 also make it a promising candidate for pulsar timing arrays. The proposed observations will allow us to obtain a timing solution of this new pulsar, and are therefore essential for future timing observations.
DOI: 10.6084/m9.figshare.11918190.v3
title: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment r1i1p1f1

description: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment (one of future scenarios) r1i1p1f1. The grid, named gx1v6, is the displaced pole (the North Pole displaced to the Greenland) grid with 1.1 degree in longitude and 0.27-0.54 degree in latitude.
DOI: 10.25919/5e5b4323cd4f7
title: Parkes observations for project P595 semester 2019OCTS_08

description: We propose to continue the PULSE@Parkes project in which high school students from Australia and around the World use the Parkes radio telescope in a remote observing model to observe and analyse pulsar data. The data from some PULSE@Parkes observations are used to support the FERMI Gamma ray mission, other observations supplement the P456 Pulsar Timing Array project and the remainder were chosen in order to make a detailed analysis of pulsar timing irregularities and intermittency.
DOI: 10.3886/e111201v2
title: Values and Beliefs, Welfare Evaluations, and Attitudes Towards a Universal Basic Income in Europe

description: This study investigates the determinants of public support for a universal basic income (UBI), using the European Social Survey Round 8 (2016), which is a cross-national survey that asked respondents for the first time whether or not they support a UBI scheme. Among the determinants, this article focuses on the three sets of factors: basic human values (universalism, benevolence, power, and achievement), beliefs about economic differences (economic individualism and economic fairness), and evaluations of current social benefits and services. The findings show that young, leftist, and economically vulnerable people who are unemployed or low-income earners are more supportive of UBI, as expected. Regarding the predictors of the values and beliefs, those who are in favor of enhancing equality in a broad sense are more likely to support UBI; those who support economic individualism and worry about a lack of work ethic and economic burden imposed by welfare policies are less likely to support UBI, as hypothesized. However, the results are unexpected that those who are more inclined to self-enhancement values (power and achievement) and targeted welfare policies are more supportive of UBI, which reveals that UBI is not just an egalitarian policy. <br>
DOI: 10.6084/m9.figshare.11918190.v4
title: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment r1i1p1f1

description: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment (one of future scenarios) r1i1p1f1. The grid, named gx1v6, is the displaced pole (the North Pole displaced to the Greenland) grid with 1.1 degree in longitude and 0.27-0.54 degree in latitude.
DOI: 10.5517/ccdc.csd.cc252kvp
title: CCDC 1998472: Experimental Crystal Structure Determination

description: Related Article: Lorel M. Scriven, Katharina Kaiser, Fabian Schulz, Alistair J. Sterling, Steffen L. Woltering, Przemyslaw Gawel, Kirsten E. Christensen, Harry L. Anderson, Leo Gross|2020|J.Am.Chem.Soc.|142|12921|doi:10.1021/jacs.0c05033
DOI: 10.5517/ccdc.csd.cc2534zf
title: CCDC 1999034: Experimental Crystal Structure Determination

description: Related Article: Giorgio Olivo, Giorgio Capocasa, Barbara Ticconi, Osvaldo Lanzalunga, Stefano Di Stefano, Miquel Costas|2020|Angew.Chem.,Int.Ed.|59|12703|doi:10.1002/anie.202003078
DOI: 10.5517/ccdc.csd.cc25350h
title: CCDC 1999035: Experimental Crystal Structure Determination

description: Related Article: Giorgio Olivo, Giorgio Capocasa, Barbara Ticconi, Osvaldo Lanzalunga, Stefano Di Stefano, Miquel Costas|2020|Angew.Chem.,Int.Ed.|59|12703|doi:10.1002/anie.202003078
DOI: 10.5281/zenodo.3692811
title: MoMA Collection - Automatic Monthly Update

description: Temporary Description
DOI: 10.5281/zenodo.3692810
title: MoMA Collection - Automatic Monthly Update

description: Temporary Description
DOI: 10.5519/qd.2plodvwg
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1607 records)
DOI: 10.25919/5e5b6ce0ca9d5
title: Parkes observations for project P1034 semester 2019OCTS_09

description: We recently discovered two millisecond pulsars (MSPs) in the globular cluster, Omega Centauri, the first pulsar discovery in this globular cluster. The discovery of these MSPs will enable us to study the stellar population and dynamics in the core of Omega Centauri, and to probe the ionised interstellar medium in Omega Centauri. These two MSPs are potentially in extreme eclipsing systems, and are useful for us to understand the formation of such systems. More importantly, our discoveries, for the first time, allow us to carry out a deep, coherently de-dispersed, high time resolution survey of pulsars in Omega Centauri, which might lead to exciting discoveries. We propose to carry out follow-up timing observations of the new discoveries, and a new coherently de-dispersed, high time resolution survey of Omega Centauri.
DOI: 10.25345/c55t23
title: MassIVE MSV000085041 - Candidate stress biomarkers for queen failure diagnostics
title: Spermathecal fluid proteins were cleaned up via acetone precipitation overnight at 20 C. The precipitated protein was pelleted and washed twice with 500 ul of 80% acetone, then the pellet was allowed to air dry (ca. 5 min) prior to solubilization in 50 ul of digestion buffer (6 M urea, 2 M thiourea). Approximately 25 ug of protein were reduced (0.5 ug dithiothreitol, 20 min), alkylated (2.5 ug iodoacetamide, 30 min, dark), and digested (0.5 ug Lys-C for 3 h, then 0.5 ug trypsin overnight). Digested peptides were acidified with one volume of 1% trifluoroacetic acid and desalted with high-capacity STAGE tips. Eluted samples were dried (SpeedVac, Eppendorf, 45 min) and resuspended in Buffer A (0.1% formic acid). Peptide concentrations were determined using a NanoDrop (Thermo, 280 nm) and sample orders were randomized for liquid chromatography-tandem mass spectrometry (LC-MS/MS) analysis. Peptides (0.5 ug for each sample) were injected on an EASY-nLC 1000 liquid chromatography system (Thermo) coupled to an Impact II Q-TOF mass spectrometer (Bruker). The LC system included a fused-silica (5 um Aqua C18 particles (Phenomenex)) fritted 2 cm trap column connected to a 50 cm analytical column packed with ReproSil C18 (3 um C18 particles (Dr. Maisch)). The separation gradient ran from 5% to 35% Buffer B (80% acetonitrile, 0.1% formic acid) over 120 min, followed by a 15 min wash at 95% Buffer B (flow rate: 250 uL/min). The instrument parameters were: scan from 150 to 2200 m/z, 100 us transient time, 10 us prepulse storage, 7 eV collision energy, 1500 Vpp Collision RF, a +2 default charge state, 18 Hz spectral acquisition rate, 3.0 s cycle time, and the intensity threshold was 250 counts. Mass spectrometry data were searched using MaxQuant (v1.6.1.0) using default parameters, except match between runs was enabled. Peptide spectral matches, peptide identifications and protein identifications were controlled at 1% false discovery rates (FDRs). Data were analyzed in Perseus (v1.6.1.1). Proteins differentially expressed between heat-shocked and non-heat-shocked samples, as well as among tissues (semen, virgin spermathecae, and mated spermathecae), were identified using t-tests and significant results were corrected to either 5% (heat-shock and cold-shock) or 10% FDR (pesticide stress) (Banjamini-Hochberg method).
DOI: 10.6084/m9.figshare.11918190.v5
title: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment r1i1p1f1

description: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment (one of future scenarios) r1i1p1f1. The grid, named gx1v6, is the displaced pole (the North Pole displaced to the Greenland) grid with 1.1 degree in longitude and 0.27-0.54 degree in latitude.
DOI: 10.25919/5e5b76c125f19
title: Parkes observations for project P958 semester 2019OCTS_61

description: Fast radio bursts (FRBs) continue to raise more questions than they answer. Until last year, only one burst – the only one known to repeat - had been localized to a bright radio nebula (either a young supernova remnant or pulsar wind nebulae) in a distant dwarf galaxy. Over the last two year searches with the Australian Square Kilometre Array Pathfinder (ASKAP) have detected 31 bursts, five of which have been localised to host galaxies at redshifts ranging from 0.1 to 0.5. These bursts and their hosts are very unlike the repeater, suggesting there may be a dichotomy in the population. However one of the arcminute-localised ASKAP FRBs has recently been found to repeat. Here we propose to search and study repetitions in this FRB population. Our comprehensive sample and a dense monitoring campaign of well localised bursts, at a fluence limit more than 60 times lower than that of their detections to characterise the fraction of bursts that repeat. For bursts that repeat the unique wide bandwidth observations will be used to test leading models of burst emission.
DOI: 10.3886/e112669v1-22703
title: Replication data for: The Effect of Education on Adult Mortality and Health: Evidence from Britain

description: There is a strong, positive, and well-documented correlation between education and health outcomes. In this paper, we attempt to understand to what extent this relationship is causal. Our approach exploits two changes to British compulsory schooling laws that generated sharp across-cohort differences in educational attainment. Using regression discontinuity methods, we find the reforms did not affect health although the reforms impacted educational attainment and wages. Our results suggest caution as to the likely health returns to educational interventions focused on increasing educational attainment among those at risk of dropping out of high school, a target of recent health policy efforts.
DOI: 10.25606/surf.578c6039-7c42c21c
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-210)

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 210 of the 2048³ resolution collection.
DOI: 10.21227/ew8w-ze25
title: QUEKO-Benchmark

description: Quantum Mapping Example with Known Optimal Depth
DOI: 10.21227/zbnb-hc98
title: QUEKO-Benchmark

description: Quantum Mapping Example with Known Optimal Depth
DOI: 10.6084/m9.figshare.11918190.v6
title: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment r1i1p1f1

description: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment (one of future scenarios) r1i1p1f1. The grid, named gx1v6, is the displaced pole (the North Pole displaced to the Greenland) grid with 1.1 degree in longitude and 0.27-0.54 degree in latitude.
DOI: 10.6084/m9.figshare.11918190.v7
title: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment r1i1p1f1

description: Simulated spectrum peak wave period (3-hourly, 2015.01-2100.12) from FIO-ESM v2.0 ssp585 experiment (one of future scenarios) r1i1p1f1. The grid, named gx1v6, is the displaced pole (the North Pole displaced to the Greenland) grid with 1.1 degree in longitude and 0.27-0.54 degree in latitude.
DOI: 10.5281/zenodo.3692891
title: doppant/etika-profesi: Data Penelitian

description: Berisi file-file(data) yang digunakan sebagai sumber membuat paper
DOI: 10.5281/zenodo.3692892
title: doppant/etika-profesi: Data Penelitian

description: Berisi file-file(data) yang digunakan sebagai sumber membuat paper
DOI: 10.21227/2b2c-mf88
title: Development of Industrial IoT System for Anomaly Detection in Smart Factory

description: Development of Industrial IoT System for Anomaly Detection in Smart Factory
DOI: 10.21227/vhec-0q55
title: Development of Industrial IoT System for Anomaly Detection in Smart Factory

description: Development of Industrial IoT System for Anomaly Detection in Smart Factory
DOI: 10.5281/zenodo.3692923
title: Supplementary code and visualisations for "Seizure pathways change on circadian and slower timescales in individual patients with focal epilepsy"

description: MATLAB code and workspaces for reproducing the main results and figures of the paper "Seizure pathways change on circadian and slower timescales in individual patients with focal epilepsy." Additional supplementary visualisations for all patients are also provided as PDFs. The paper preprint is available on bioRxiv: https://www.biorxiv.org/content/10.1101/661371v2
DOI: 10.6073/pasta/246d4eaf296697e4a8a99b98e703bb8d
title: Jornada Basin LTER Cross-scale Interactions Study (CSIS) Block 10 meteorological station: 1-hour summary data: 2017 - ongoing

description: This data package contains hourly air temperature, relative humidity, wind speed, wind direction, and precipitation summary data from Jornada Basin LTER Cross Scale Interactions Study (CSIS) Block-10 met station. Air temperature, relative humidity, wind speed, wind direction, and precipitation are measured and calculated at an automated meteorological station connected to a 900 MHz spread spectrum wireless network. Wind speed is measured at 37cm, 75 cm, 150 cm, and 300 cm, wind direction at approximately 3m, and air temperature and relative humidity at approximate 2.5m. Measurements are aggregated at intervals of 5, 30, 60 minutes and daily, with precipitation additionally provided with 1 second aggregation during precipitation events. Precipitation is not measured at Block 1 and Block 12 because of proximity to Block 2 and Block 13, respectively . This is an ONGOING dataset.
DOI: 10.6073/pasta/452840c3a652f167a2701b7e34ebd35f
title: Jornada Basin LTER Cross-scale Interactions Study (CSIS) Block 1 meteorological station: Daily average soil volumetric water content data: 2013 - ongoing

description: Daily Average of 30-minute Soil Volumetric Water Content data at 10 cm at CSIS Block-1. Collection of soil water content data at Jornada LTER Cross-scale Interactions Study (CSIS) blocks, New Mexico, supports the environmental monitoring objectives of the Jornada LTER monitoring program that look at plant-soil water dynamics. Soil volumetric water content is measured every 30 minutes at 10 cm depth at 3 locations at each of the 4 plots per block and averaged for the daily value. The locations in each plot are under bare soil, under perennial grass, and under shrub. Volumetric water content, bulk electrical conductivity, soil temperature, and bulk dielectric permittivity are recorded at an automated meteorological station installed at Jornada LTER CSIS Block-1 site. This is an ONGOING dataset.
DOI: 10.6073/pasta/3b4487d5ab0e5a19dafc7dc6b891a276
title: Jornada Basin LTER Cross-scale Interactions Study (CSIS) Block 10 meteorological station: 30-minute soil volumetric water content data: 2013 - ongoing

description: 30-minute Soil Moisture data at 10 cm at CSIS Block-10. Collection of soil volumetric water content data at Jornada LTER Cross-scale Interactions Study (CSIS) blocks, New Mexico, supports the environmental monitoring objectives of the Jornada LTER monitoring program that look at plant-soil water dynamics. Soil volumetric water content is measured at 10 cm depth at 3 locations at each of the 4 plots per block. The locations in each plot are under bare soil, under perennial grass, and under shrub. Volumetric water content, bulk electrical conductivity, soil temperature, and bulk dielectric permittivity are recorded every 30 minutes at an automated meteorological station installed at Jornada LTER CSIS Block-10 site. This is an ONGOING dataset.
DOI: 10.6073/pasta/ff3cd357f5c44b9c4166a85c3e2b20cf
title: Jornada Basin LTER Cross-scale Interactions Study (CSIS) Block 1 meteorological station: Daily summary data: 2013 - ongoing

description: This data package contains hourly air temperature, relative humidity, wind speed, wind direction, and precipitation summary data from Jornada Basin LTER Cross Scale Interactions Study (CSIS) Block-1 met station. Air temperature, relative humidity, wind speed and wind direction are measured and calculated at an automated meteorological station connected to a 900 MHz spread spectrum wireless network. Wind speed is measured at 37cm, 75 cm, 150 cm, and 300 cm, wind direction at approximately 3m, and air temperature and relative humidity at approximate 2.5m. Measurements are aggregated at intervals of 5, 30, 60 minutes and daily, with precipitation additionally provided with 1 second aggregation during precipitation events. The met station variables measured include air temperature, precipitation, relative humidity, wind direction, wind speed. Precipitation is not measured at Block 1 and Block 12 because of proximity to Block 2 and Block 13, respectively . This is an ONGOING dataset.