cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.7910/dvn/pjomf1/ocnib9
title: 1930_45.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/wfnxda
title: 1925_14.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/wja372
title: 1920_Book30_188.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/xu7lz7
title: 1930_46.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/adbrjb
title: 1930_141.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/ajz7zz
title: 1920_Book30_220.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/bmhktd
title: 1920-02-11 New Bungalows Being Built Here (MES).jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/dfzmyk
title: 1920-10-1 A Place to Live p2 (MES).jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/euh37f
title: 1930_54.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/f1g65k
title: 1920_Book30_183.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/gwkywc
title: sfr_all.tab

description: :unav
DOI: 10.7910/dvn/pjomf1/u1thqa
title: 1925_116.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/xy68ve
title: 1930_95.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/5xzxzg
title: 1930_104.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/6nwaci
title: 1930_49.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/dskcaf
title: 1930_105.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/kl1g3l
title: 1925_18.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/l1mpht
title: 1925_25.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/qm79fi
title: 1920-09-08 Tax Figures Indicate Merced Co Growth B p1 (MES) .jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/qqnte2
title: 1920_Book30_152-1.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/sbvmcu
title: 1923-11-16 Mercy Hospital Opened with Reception p6 (MES).jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/wc7rmn
title: 1920_Book30_134-1.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/0pllsr
title: assessment_data.tab

description: :unav
DOI: 10.7910/dvn/pjomf1/4pnslc
title: 1925_55.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/6g8rqy
title: 1923-12-12 Buy Now Where Building Restrictions Protect You, in the John Muir Tract p8 (MES).jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/dege3j
title: 1930_18.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/kgjoxd
title: 1930_14.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/lod8cn
title: 1922-02-04 Bids Now In On School House p4 (MES).jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/nzvz3e
title: 1925_101.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/qey0b1
title: 1920_Book30_46-1.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/tksvoz
title: 1923-03-08 Twenty-Six New Homes Going Up p6 (MES).jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/z8cx0x
title: 1925_80.jpg

description: :unav
DOI: 10.7910/dvn/pjomf1/na8fcz
title: 1920_Book30_158-1.jpg

description: :unav
DOI: 10.5281/zenodo.3407801
title: Natural history specimens collected and/or identified and deposited.

description: Natural history specimen data collected and/or identified by Rainer, Heimo, https://orcid.org/0000-0002-5963-349X. Claims were made on Bloodhound, https://bloodhound-tracker.net using specimen data from the Global Biodiversity Information Facility, https://gbif.org.
DOI: 10.25919/5d7ed23c09baa
title: Model scenarios for sustainable expansion of irrigated agriculture and horticulture in Northern Adelaide Corridor

description: Long-term modelling scenarios under historical (1970-2017) and future climate (2018-2050) using UNSATCHEM module in HYDRUS-1D to assess the longevity of irrigation, using a range of available water resources, in four main soil groups. File extensions: .in = input file, .out = output file, .dat and .h1d are system files that can't be opened.
DOI: 10.5281/zenodo.3409456
title: DWD European Weather 2

description: opendata.dwd.de - OpenData by Deutscher Wetter Dienst Conditions: https://www.dwd.de/EN/service/copyright/copyright_node.html dates and times are UTC.
DOI: 10.5281/zenodo.3408817
title: Data and R-code on a cross-sectional study of factors associated with lameness in dairy cows housed in freestall and compost-bedded pack dairy farms in southern Brazil

description: The data correspond to a cross-sectional study designed to investigate factors associated with lameness in dairy cows on intensive farms in southern Brazil.<br> Farms: 38 freestall and 12 compost-bedded pack visited once in 2016. All lactating cows (n = 13,716) were examined and body condition score (BCS) and gait score were assessed. Additionally, some variables were collected through inspection of facilities and using data from an interview with farmers on routine herd management practices.<br> Additional information is provided in the published paper ("Factors associated with lameness prevalence in lactating cows housed in freestall and compost-bedded pack dairy farms in southern Brazil" https://doi.org/10.1016/j.prevetmed.2019.104773)
DOI: 10.5281/zenodo.3408818
title: Data and R-code on a cross-sectional study of factors associated with lameness in dairy cows housed in freestall and compost-bedded pack dairy farms in southern Brazil

description: The data correspond to a cross-sectional study designed to investigate factors associated with lameness in dairy cows on intensive farms in southern Brazil.<br> Farms: 38 freestall and 12 compost-bedded pack visited once in 2016. All lactating cows (n = 13,716) were examined and body condition score (BCS) and gait score were assessed. Additionally, some variables were collected through inspection of facilities and using data from an interview with farmers on routine herd management practices.<br> Additional information is provided in the published paper ("Factors associated with lameness prevalence in lactating cows housed in freestall and compost-bedded pack dairy farms in southern Brazil" https://doi.org/10.1016/j.prevetmed.2019.104773)
DOI: 10.25345/c5707b
title: MassIVE MSV000084325 - GNPS-carnitine treatment, acute stage Chagas disease, liver and oesophagus, positive mode
title: Male C3H/HeJ mice were infected with 50,000 luciferase-expressing strain CL Brener trypanosoma cruzi parasites. Beginning 7 days post-infection, mice were treated with carnitine in drinking water (100 mg/kg/day dosing equivalent), benznidazole (100 mg/kg/day by intraperitoneal injection), or left untreated (vehicle group). One additional control group was uninfected. Mice were euthanized and liver and oesophagus collected at day 17 post-infection. Tissue was extracted with 50% methanol followed by 3:1 dichloromethane:methanol, and analyzed by C8 chromatography, with detection by MS in positive mode.
DOI: 10.18112/openneuro.ds002179.v1.0.0
title: 7 Tesla MRI of the ex vivo human brain at 100 micron resolution
DOI: 10.25345/c5395f
title: MassIVE MSV000084326 - GNPS-carnitine treatment, acute stage Chagas disease, liver and oesophagus, negative mode
title: Male C3H/HeJ mice were infected with 50,000 luciferase-expressing strain CL Brener trypanosoma cruzi parasites. Beginning 7 days post-infection, mice were treated with carnitine in drinking water (100 mg/kg/day dosing equivalent), benznidazole (100 mg/kg/day by intraperitoneal injection), or left untreated (vehicle group). One additional control group was uninfected. Mice were euthanized and liver and oesophagus collected at day 17 post-infection. Tissue was extracted with 50% methanol followed by 3:1 dichloromethane:methanol, and analyzed by C8 chromatography, with detection by MS in negative mode.
DOI: 10.25606/surf.578c6039-4408939d
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-437)

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 437 of the 2048³ resolution collection.
DOI: 10.7910/dvn/a2hfof/eimi6x
title: Wheat_test2.csv

description: Data for Spatial variability in regional scale drought index insurance viability across Australia’s wheat growing regions
DOI: 10.7910/dvn/vhcaau/35rwdr
title: coffee_quality_dataframe.tab

description: Robusta coffee bean quality data
DOI: 10.5281/zenodo.3408464
title: DWD European Weather 2

description: opendata.dwd.de - OpenData by Deutscher Wetter Dienst Conditions: https://www.dwd.de/EN/service/copyright/copyright_node.html dates and times are UTC.
DOI: 10.5281/zenodo.3408690
title: Experimental dataset

description: Data set of Geophysical Research Letter paper "The entrainment rate of non Boussinesq hazardous geophysical gas-particle flows: an experimental model Ewith application to pyroclastic density currents "
DOI: 10.5281/zenodo.3408691
title: Experimental dataset

description: Data set of Geophysical Research Letter paper "The entrainment rate of non Boussinesq hazardous geophysical gas-particle flows: an experimental model Ewith application to pyroclastic density currents "
DOI: 10.25919/5d7ee3d833001
title: Parkes observations for project P958 semester 2019APRS_85

description: Fast radio bursts (FRBs) continue to raise more questions than they answer. Until a few months ago, 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 year searches with the Australian Square Kilometre Array Pathfinder (ASKAP) have detected 28 bursts, two of which have been localised to host galaxies at redshifts &gt; 0.3. These bursts and their hosts are very unlike the repeater, suggesting there may be a dichotomy in the population. Over the next six months we expect to detect another 12 FRBs, which will also have sub-arcsecond localisations. Here we propose to search this population for repeats. 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, will either confirm the presence of additional repeating FRBs or the uniqueness of FRB 121102 amongst the population.
DOI: 10.34725/dvn/wdvcu5
title: Simple Crop Corg Model

description: The model was set up to generate “soil carbon transition curves” that are consistent with simple assumptions about soil carbon dynamics during fallow and cropping stages. The model provides estimates of yield, organic matter dynamics, yield per unit labor and net GHG emissions per unit yield.
DOI: 10.34725/dvn/wdvcu5/b70kzc
title: 0.Disclaimer.pdf
DOI: 10.34725/dvn/wdvcu5/tqu05z
title: Simple Crop Corg Model.xls
DOI: 10.5281/zenodo.3408462
title: A semi-implicit relaxed Douglas-Rachford algorithm (sDR) for Ptychography

description: Alternating projection based methods, such as ePIE and rPIE, have been used widely in ptychography. However, they only work well if there are adequate measurements (diffraction patterns); in the case of sparse data (i.e. fewer measurements) alternating projection underperforms and might not even converge. In this paper, we propose semi-implicit relaxed Douglas-Rachford (sDR), an accelerated iterative method, to solve the classical ptychography problem. Using both simulated and experimental data, we show that sDR improves the convergence speed and the reconstruction quality relative to extended ptychographic iterative engine (ePIE) and regularized ptychographic iterative engine (rPIE). Furthermore, in certain cases when sparsity is high, sDR converges while ePIE and rPIE fail or encounter slow convergence. To facilitate others to use the algorithm, we post the Matlab source code of sDR on a public website (www.physics.ucla.edu/research/imaging/sDR) and data con zenodo. We anticipate that this algorithm can be generally applied to the ptychographic reconstruction of a wide range of samples in the physical and biological sciences.
DOI: 10.5281/zenodo.3408463
title: A semi-implicit relaxed Douglas-Rachford algorithm (sDR) for Ptychography

description: Alternating projection based methods, such as ePIE and rPIE, have been used widely in ptychography. However, they only work well if there are adequate measurements (diffraction patterns); in the case of sparse data (i.e. fewer measurements) alternating projection underperforms and might not even converge. In this paper, we propose semi-implicit relaxed Douglas-Rachford (sDR), an accelerated iterative method, to solve the classical ptychography problem. Using both simulated and experimental data, we show that sDR improves the convergence speed and the reconstruction quality relative to extended ptychographic iterative engine (ePIE) and regularized ptychographic iterative engine (rPIE). Furthermore, in certain cases when sparsity is high, sDR converges while ePIE and rPIE fail or encounter slow convergence. To facilitate others to use the algorithm, we post the Matlab source code of sDR on a public website (www.physics.ucla.edu/research/imaging/sDR) and data con zenodo. We anticipate that this algorithm can be generally applied to the ptychographic reconstruction of a wide range of samples in the physical and biological sciences.
DOI: 10.5281/zenodo.3408604
title: Offensive Content: A Tale of Two Classes

description: This dataset contains 6000 rows evenly distributed between hate speech, trolling and normal. Data source primary from Twitter, Reddit and Wikipedia Talk pages. No metadata about posts is included. Posts have been anonymized to protect user privacy.
DOI: 10.5281/zenodo.3408605
title: Offensive Content: A Tale of Two Classes

description: This dataset contains 6000 rows evenly distributed between hate speech, trolling and normal. Data source primary from Twitter, Reddit and Wikipedia Talk pages. No metadata about posts is included. Posts have been anonymized to protect user privacy.
DOI: 10.7910/dvn/jgvf9a/mgzgm1
title: fb_200M_uint32.xz

description: :unav
DOI: 10.7910/dvn/jgvf9a/y54si9
title: fb_200M_uint64.xz

description: :unav
DOI: 10.18170/dvn/82lohs
title: dynamic rupture on branched fault

description: Numerical simulation data of dynamic ruptures on branched fault
DOI: 10.21251/9418b7a2-fa37-4a16-b241-ddd4b09e7b57
title: test dataset for doi creation
DOI: 10.21251/cbb9f1e0-df68-47d8-8833-ce3884cb6b50
title: test dataset 2
DOI: 10.25606/surf.578c6039-5a9ac010
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-745)

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 745 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-e2901170
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-669)

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 669 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3234804
title: Monitoring of the UHPFRC strengthened Chillon viaduct under environmental and operational variability

description: Datasets corresponding to 3 months of data of the monitoring of Chillon viaduct. Each file contains: the vibration data from 11 acelerometers, in vertical direction the sampling ratio Temperature Humidity The accelerometer positions are illustarted in the pdf "accelerometres Position.pdf". When employing this dataset, please cite:"Martín-Sanz, Henar, Konstantinos Tatsis, Vasilis K. Dertimanis, Luis David Avendaño-Valencia, Eugen Brühwiler, and Eleni Chatzi. "Monitoring of the UHPFRC strengthened Chillon viaduct under environmental and operational variability." <em>Structure and Infrastructure Engineering</em> (2019): 1-31."
description: When employing this dataset, please cite:"Martín-Sanz, Henar, Konstantinos Tatsis, Vasilis K. Dertimanis, Luis David Avendaño-Valencia, Eugen Brühwiler, and Eleni Chatzi. "Monitoring of the UHPFRC strengthened Chillon viaduct under environmental and operational variability." Structure and Infrastructure Engineering (2019): 1-31."
DOI: 10.5281/zenodo.3234805
title: Monitoring of the UHPFRC strengthened Chillon viaduct under environmental and operational variability

description: Datasets corresponding to 3 months of data of the monitoring of Chillon viaduct. Each file contains: the vibration data from 11 acelerometers, in vertical direction the sampling ratio Temperature Humidity The accelerometer positions are illustarted in the pdf "accelerometres Position.pdf". When employing this dataset, please cite:"Martín-Sanz, Henar, Konstantinos Tatsis, Vasilis K. Dertimanis, Luis David Avendaño-Valencia, Eugen Brühwiler, and Eleni Chatzi. "Monitoring of the UHPFRC strengthened Chillon viaduct under environmental and operational variability." <em>Structure and Infrastructure Engineering</em> (2019): 1-31."
description: When employing this dataset, please cite:"Martín-Sanz, Henar, Konstantinos Tatsis, Vasilis K. Dertimanis, Luis David Avendaño-Valencia, Eugen Brühwiler, and Eleni Chatzi. "Monitoring of the UHPFRC strengthened Chillon viaduct under environmental and operational variability." Structure and Infrastructure Engineering (2019): 1-31."
DOI: 10.21227/v6ff-cz03
title: Clustering by the way of atomic fission

description: Cluster analysis which focuses on the grouping and categorization of similar elements is widely used in various fields of research. Inspired by the phenomenon of atomic fission, a novel density-based clustering algorithm is proposed in this paper, called fission clustering (FC). It focuses on mining the dense families of a dataset and utilizes the information of the distance matrix to fissure clustering dataset into subsets. When we face the dataset which has a few points surround the dense families of clusters, K-nearest neighbors local density indicator is applied to distinguish and remove the points of sparse areas so as to obtain a dense subset that is constituted by the dense families of clusters. A number of frequently-used datasets were used to test the performance of this clustering approach, and to compare the results with those of algorithms. The proposed algorithm is found to outperform other algorithms in speed and accuracy.
DOI: 10.25606/surf.578c6039-01add094
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-616)

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 616 of the 2048³ resolution collection.