cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.3465825
title: emmetaobrien/mm_neo_atlas: Transcriptomic Atlas of Mouse Neocortical Layers

description: In the mammalian cortex, neurons and glia form a patterned structure across six layers whose complex cytoarchitectonic arrangement is likely to contribute to cognition. This dataset contains transcriptomes from layers 1-6b of different areas (primary and secondary) of the adult (postnatal day 56) mouse somatosensory cortex. A total of 5,835 protein-coding genes and 66 noncoding RNA loci are differentially expressed ("patterned") across the layers. Layers 2-6b are each associated with specific functional and disease annotations that provide insights into their biological roles. This dataset extends currently available resources by providing quantitative expression levels, by being genome-wide, by including novel loci, and by identifying candidate alternatively spliced transcripts that are differentially expressed across layers. "A transcriptomic atlas of mouse neocortical layers", TG Belgard et al. Neuron, 25:605-616 (2011). http://wwwfgu.anat.ox.ac.uk/~grantb/mouse_layers/
DOI: 10.7910/dvn/pmwyi5/hp1xe6
title: PresCab_BASIC_Chile_18.xlsx

description: :unav
DOI: 10.7910/dvn/qpc6iv/suu7dk
title: PresCab_BASIC_Colombia_18.r

description: :unav
DOI: 10.7910/dvn/qpc6iv/yr6pkz
title: PresCab_BASIC_Colombia_18.xlsx

description: :unav
DOI: 10.7910/dvn/wzzqje/f0wtp6
title: PresCab_BASIC_Ecuador_18.r

description: :unav
DOI: 10.7910/dvn/wzzqje/mjemlt
title: PresCab_BASIC_Ecuador_18.xlsx

description: :unav
DOI: 10.5255/ukda-sn-853948
title: Digital hoarding survey 2017
DOI: 10.7910/dvn/d0rx90/fhjh81
title: PresCab_BASIC_Uruguay_18.r

description: :unav
DOI: 10.7910/dvn/d0rx90/tbrbrn
title: PresCab_BASIC_Uruguay_18.xlsx

description: :unav
DOI: 10.7910/dvn/gerijb/m4vcwx
title: PresCab_BASIC_Peru_18.xlsx

description: :unav
DOI: 10.7910/dvn/gerijb/slwbj6
title: PresCab_BASIC_Peru_18.r

description: :unav
DOI: 10.7910/dvn/3s2wvb/s0bcnx
title: PresCab_BASIC_Argentina_18.r

description: :unav
DOI: 10.7910/dvn/3s2wvb/tk6eaz
title: PresCab_BASIC_Argentina_18.xlsx

description: :unav
DOI: 10.7910/dvn/ad1lt2/1s9vdr
title: PresCab_BASIC_USA_18.r

description: :unav
DOI: 10.7910/dvn/ad1lt2/a0qjfp
title: PresCab_BASIC_USA_18.xlsx

description: :unav
DOI: 10.5281/zenodo.3465498
title: Affine Policies for Flexibility Provision by Natural Gas Networks to Power Systems

description: Online appendix for the paper - "Affine Policies for Flexibility Provision by Natural Gas Networks to Power Systems", containing the power generators, gas producers and demand data as well as physical characteristics of the electrical transmission lines and gas pipelines. The empirically estimated forecast error covariance matrix used in the model is provided as well. The power systems and natural gas systems data is adapted from: C. Ordoudis, P. Pinson and J. M. González, "An integrated market for electricity and natural gas systems with stochastic power producers", European Journal of Operational Research, vol. 272, no. 2, pp. 642-654, 2019.
DOI: 10.5281/zenodo.3465499
title: Data-Driven Affine Policies for Flexibility Provision by Natural Gas Networks to Power Systems

description: Online appendix for the paper - "Data-Driven Affine Policies for Flexibility Provision by Natural Gas Networks to Power Systems", containing the power generators, gas producers and demand data as well as physical characteristics of the electrical transmission lines and gas pipelines. The empirically estimated forecast error covariance matrix used in the model is provided as well. The power systems and natural gas systems data is adapted from: C. Ordoudis, P. Pinson and J. M. González, "An integrated market for electricity and natural gas systems with stochastic power producers", European Journal of Operational Research, vol. 272, no. 2, pp. 642-654, 2019.
DOI: 10.5281/zenodo.3465552
title: Unison Source Separation Dataset

description: The unison source separation data set consist of several single, isolated instruments notes all of the same fundamental frequency (C4). For more information our accompanying website
DOI: 10.5519/qd.aoid9dmj
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (41 records)
DOI: 10.5281/zenodo.3465842
title: emmetaobrien/celltypes: Allen Brain Atlas Cell Types

description: This brain cell database contains a survey of biological features derived from single cell data, from both human and mouse. It is part of a multi-year project to create a census of cells in the mammalian brain. The database contains electrophysiological, morphological, and transcriptomic data measured from individual cells, as well as models simulating cell activity. Thus far, data generation has focused on select areas of cerebral cortex, and thalamic neurons. https://celltypes.brain-map.org/
DOI: 10.5066/p9fm835b
title: Microplastics in the water column and sediment in Milwaukee-Area streams, the Milwaukee Harbor, and Lake Michigan, 2016

description: This dataset describes the quantity, morphology, and polymer identity of microplastics in the water column and surficial sediments of Milwaukee-Area streams, the Milwaukee Harbor, and Lake Michigan (Wisconsin). Water samples were collected at 10 locations, 2-4 times each, from May to September, 2016. At the 4 shallowest locations, water was collected only at the water surface. At the remaining 6 locations, water was collected at the water surface and at 1-4 depths below the surface. Sediment samples were collected once, in June 2016, at a subset of 9 locations. Sampling and analysis methods are described in the Processing Steps section of the metadata. These data are interpreted in a journal article (TBD).
DOI: 10.17632/mcfzsf47zf.1
title: Data for: Establishment and validation of a prediction model for vaginal delivery after cesarean and its pregnancy outcomes —— based on a prospective study

description: data
DOI: 10.17632/2j6bhypszt.1
title: Swiming Pool Fixed Data for: A geometry conforming isogeometric method for the self-adjoint angular flux (SAAF) form of the neutron transport equation with a discrete ordinate (SN) angular discretisation

description: Solutions for the IAEA swimming pool fixed source problem, solved using ICARUS
DOI: 10.17632/dzrwgg6h8x.1
title: Swimming Pool Fission Data for: A geometry conforming isogeometric method for the self-adjoint angular flux (SAAF) form of the neutron transport equation with a discrete ordinate (SN) angular discretisation

description: Solution Keff data for the IAEA swimming pool fission problem solved by ICARUS
DOI: 10.17632/j8yy9dttgv.1
title: MMS Data for: A geometry conforming isogeometric method for the self-adjoint angular flux (SAAF) form of the neutron transport equation with a discrete ordinate (SN) angular discretisation

description: Log error in MMS solution for the MMS test case specified in the paper from the title. Solved using ICARUS.
DOI: 10.17632/j224bw7grv.1
title: Bare Fuel Pin Data for: A geometry conforming isogeometric method for the self-adjoint angular flux (SAAF) form of the neutron transport equation with a discrete ordinate (SN) angular discretisation

description: Data for the bare fuel pin problem, solved by ICARUS.
DOI: 10.17632/rjff4g9z8m.1
title: C5G7 Data for: A geometry conforming isogeometric method for the self-adjoint angular flux (SAAF) form of the neutron transport equation with a discrete ordinate (SN) angular discretisation

description: Data from the C5G7 benchmark problem run using ICARUS
DOI: 10.5519/qd.8wy3slbj
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1 records)
DOI: 10.5281/zenodo.3966704
title: Vasp calculation and local structures of NdFeB substituted structures

description: This dataset summary Density Functional Theory calculations using VASP[1] with Nd-Fe-B substituted structures. The source calculated VASP results are found in [2]. In addition, the dataset includes local structures extracted from the Nd-Fe-B substituted structures and Nd-Fe-B structures collected from OQMD that used to create tSNE maps of local structures.<br> <br> [1] VASP: Vienna Ab initio Simulation Package: https://www.vasp.at/ [2] VASP calculation of Nd-Fe-B at NOMAD repository: https://dx.doi.org/10.17172/NOMAD/2020.07.30-1 [3] OQMD: Open Quantum Materials Database: http://www.oqmd.org/
DOI: 10.5519/qd.h0qyxh77
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (5 records)
DOI: 10.25606/surf.578c6039-4628ef55
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-188)

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 188 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-a60d9b00
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-764)

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 764 of the 2048³ resolution collection.
DOI: 10.5525/gla.researchdata.892
title: The rapid electrochemical activation of MoTe2 for the hydrogen evolution reaction

description: The data set includes raw experimental files of electrochemical data, XRD and Raman spectroscopy as well as optimised coordinates for structures from computational studies. A comprehensive description is provided within description file.
DOI: 10.5066/p9t6p5sm
title: 2015 Georgia water-use information by county and water-use trends by water-planning region

description: Water-withdrawal, water-use, and water-return information have been collected and compiled for each county in Georgia every 5 years since 1980 using data obtained from various Federal, State, private agencies, and on-line sources. For 2015, water use, water withdrawal, and water returns were estimated for each county in Georgia. Off-stream water use in 2015 is estimated for the categories of domestic use, commercial use, industrial use processing, mining use, irrigation use (subdivided into crop and golf course irrigation), livestock, aquaculture, and thermoelectric power cooling. Water-use trends from 1985-2015 have also been compiled for each water-planning region in Georgia.
DOI: 10.25606/surf.578c6039-011c79a0
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-065)

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 065 of the 2048³ resolution collection.
DOI: 10.25573/data.9920336
title: Supporting data for 'Assessing the accuracy of paleodischarge estimates for rivers on Mars'

description: Supporting information for 'Assessing the accuracy of paleodischarge estimates for rivers on Mars', by A.M. Morgan and R.A. Craddock (2019) in Geophysical Research Letters
DOI: 10.7910/dvn/2kv3eg/8u3rfp
title: distances_JS.tgzab

description: :unav
DOI: 10.7910/dvn/2kv3eg/kns5ip
title: distances_JS.tgzaa

description: :unav
DOI: 10.7910/dvn/2kv3eg/ofdae4
title: distances_energy.tgzaa

description: :unav
DOI: 10.7910/dvn/2kv3eg/hngud5
title: distances_KL.tgzac

description: :unav
DOI: 10.7910/dvn/2kv3eg/g8alki
title: distances_KL.tgzab

description: :unav
DOI: 10.7910/dvn/2kv3eg/nhmb34
title: distances_energy.tgzac

description: :unav
DOI: 10.7910/dvn/2kv3eg/rpwm3d
title: distances_energy.tgzab

description: :unav
DOI: 10.7910/dvn/2kv3eg/eczgx4
title: distances_KL.tgzaa

description: :unav
DOI: 10.25606/surf.578c6039-42c1f9af
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-184)

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 184 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-13e58e8f
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-540)

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 540 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-d8dd27e7
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-474)

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 474 of the 2048³ resolution collection.
DOI: 10.25387/g3.9808379
title: Supplemental Material for Palu et al., 2019

description: Source code for GSEA analysis run in "Natural genetic variation screen in Drosophila identifies Wnt signaling, mitochondrial metabolism, and redox homeostasis genes as modifiers of apoptosis." Included is the code itself as well as instructions for that code (README)
DOI: 10.25387/g3.9808379.v1
title: Supplemental Material for Chow et al., 2019

description: Source code for GSEA analysis run in "Natural genetic variation screen in Drosophila identifies Wnt signaling, mitochondrial metabolism, and redox homeostasis genes as modifiers of apoptosis." Included is the code itself as well as instructions for that code (README)
DOI: 10.5281/zenodo.3465889
title: Underlying data of the project "Are CONSORT checklists submitted by authors adequately reflecting what information is actually reported in published papers?"

description: <em><strong>Supplementary file 3.xlsx</strong></em> contains the evaluations for the 12 papers included in the study.
DOI: 10.5281/zenodo.3465890
title: Underlying data of the project "Are CONSORT checklists submitted by authors adequately reflecting what information is actually reported in published papers?"

description: <em><strong>Supplementary file 3.xlsx</strong></em> contains the evaluations for the 12 papers included in the study.
DOI: 10.7910/dvn/pjs21l/fwvfbq
title: SM_Extraction results_commented.json

description: RambleON cleaned output.
DOI: 10.7910/dvn/pjs21l/yg43ph
title: SM_Processed_results.tsv

description: Positions, cities, population: full merged data.
DOI: 10.7910/dvn/pjs21l/yhhxsl
title: README.txt

description: Description of the two datasets.
DOI: 10.25606/surf.578c6039-9a5135d3
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-670)

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 670 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3465904
title: Data for "How to use scale invariant properties of imperviousness in urban areas to handle missing data ?"

description: The data set corresponds the data presented in the data paper : “How to use scale invariant properties of imperviousness in urban areas to handle missing data ?“ which has been submitted to Water Resources Research ” (https://agupubs.onlinelibrary.wiley.com/journal/19447973). It corresponds to : - the rainfall data collected on 2019-06-02 with 5 min and 30 s time steps by a disdrometer installed on the roof of Ecole des Ponts ParisTech building. - land use distribution for the Jouy-en-Josas catchment (1 = forest, 2= road, 3=Grass, 4=building, 5=Gully, 6=missing data), with pixel size of 10 m and 2 m. More details can be found in the file and in the paper.