cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25606/surf.578c6039-b9991e5b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-087)

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 087 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-dac8f1ee
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-060)

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 060 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-2b009c5b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-054)

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 054 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-617e0bcd
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-056)

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 056 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-7244477c
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-061)

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 061 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-dcd63252
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-072)

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 072 of the 2048³ resolution collection.
DOI: 10.5255/ukda-sn-853774
title: Do students behave like real taxpayers? Experimental evidence on taxpayer compliance from the lab and from the field 2013-2018
DOI: 10.5281/zenodo.3256233
title: Data for Energy Landscapes for Digital Alchemy

description: Data relating to the paper 'Energy Landscapes for Digital Alchemy'. See the README for details.
DOI: 10.5281/zenodo.3256234
title: Data for Energy Landscapes for Digital Alchemy

description: Data relating to the paper 'Energy Landscapes for Digital Alchemy'. See the README for details.
DOI: 10.5255/ukda-sn-853775
title: The role of negative emotions on error and non-compliance 2013-2018
DOI: 10.18430/m3.irrmc.4978
title: X-ray diffraction data for the HDAC6-x2 project
DOI: 10.5281/zenodo.3256400
title: Test de DOI événementiel pour Espace temps

description: Production Formation aux métadonnées culturelles

Variante Atelier de préparation

Artiste principal Jean-Robert Bisaillon

Artiste principal ISNI http://isni.org/isni/0000000466242395

Discipline Conférence

Genre

Artiste secondaire

Artiste secondaire ISNI

Promoteur

Date 2019-06-25

Event Name (EN) Brainstorm your data

Nom de l'événement (FR) Tempête de données

Type d'événement Conférence

Type d'événement détaillé

URL de l'événement

URL de l'événement Facebook

DoorTime 14:30:00

BeginTime 15:00:00

AnnounceDateTime 11:00:00

PointOfSale ID

Description billetterie Gratuit

Description billetterie (alternative)

OnsaleDate

Nom du lieu Temps libre

UN-LOCODE du lieu CA MTR

Adresse rue 5605 Avenue de Gaspé #106

Adresse ville Montréal

Adresse code postal H2T 2A4

Media Context (EN)

Accroche médiatique (FR)

Image (.jpg)

Lead Performer Bio (EN)

Bio de l'artiste principal (FR)

Autre URL (1) http://tempslibre.coop/
DOI: 10.5281/zenodo.3256401
title: Test de DOI événementiel pour Espace temps

description: Production Formation aux métadonnées culturelles

Variante Atelier de préparation

Artiste principal Jean-Robert Bisaillon

Artiste principal ISNI http://isni.org/isni/0000000466242395

Discipline Conférence

Genre

Artiste secondaire

Artiste secondaire ISNI

Promoteur

Date 2019-06-25

Event Name (EN) Brainstorm your data

Nom de l'événement (FR) Tempête de données

Type d'événement Conférence

Type d'événement détaillé

URL de l'événement

URL de l'événement Facebook

DoorTime 14:30:00

BeginTime 15:00:00

AnnounceDateTime 11:00:00

PointOfSale ID

Description billetterie Gratuit

Description billetterie (alternative)

OnsaleDate

Nom du lieu Temps libre

UN-LOCODE du lieu CA MTR

Adresse rue 5605 Avenue de Gaspé #106

Adresse ville Montréal

Adresse code postal H2T 2A4

Media Context (EN)

Accroche médiatique (FR)

Image (.jpg)

Lead Performer Bio (EN)

Bio de l'artiste principal (FR)

Autre URL (1) http://tempslibre.coop/
DOI: 10.5061/dryad.gq60sj7/1
title: Dryad Item 10.5061/DRYAD.GQ60SJ7/1

description: (:tba)
DOI: 10.5519/qd.xmu7qdyi
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (15 records)
DOI: 10.5281/zenodo.3256110
title: Project STORM: monitoring the masonry of Hall I, at the Baths of Diocletian, with Fiber Bragg Grating (FBG) sensors. RAW Dataset 2017 - 2019

description: This dataset for monitoring the masonry of Hall I at the Baths of Diocletian (Rome) was created by the University of Tuscia.<br> The measurements are carried out with a Fiber Bragg Grating (FBG) sensors, have been investigated: Strain of lesions (sensors S0, S2 and S3); Temperature of masonry (sensors S1, and S8); Humidity of masonry (sensors S4, S5, S6 and S7). The data produced by the sensors were automatically saved them every 30 seconds. The dataset is composed of the data raw obtained from October 2017 to May 2019 and separated by month in 14 sheets. In total more than 4 million values were registered, used to understand the slow hazard phenomena present on the monitored masonry. STORM (Safeguarding Cultural Heritage through Technical and Organisational Resources Management) is a HORIZON 2020 funded European Union Cultural Heritage project that aims at the protection of Cultural Heritage through a combination of technical and organizational resources (http://www.storm-project.eu).
DOI: 10.5281/zenodo.3256111
title: Project STORM: monitoring the masonry of Hall I, at the Baths of Diocletian, with Fiber Bragg Grating (FBG) sensors. RAW Dataset 2017 - 2019

description: This dataset for monitoring the masonry of Hall I at the Baths of Diocletian (Rome) was created by the University of Tuscia.<br> The measurements are carried out with a Fiber Bragg Grating (FBG) sensors, have been investigated: Strain of lesions (sensors S0, S2 and S3); Temperature of masonry (sensors S1, and S8); Humidity of masonry (sensors S4, S5, S6 and S7). The data produced by the sensors were automatically saved them every 30 seconds. The dataset is composed of the data raw obtained from October 2017 to May 2019 and separated by month in 14 sheets. In total more than 4 million values were registered, used to understand the slow hazard phenomena present on the monitored masonry. STORM (Safeguarding Cultural Heritage through Technical and Organisational Resources Management) is a HORIZON 2020 funded European Union Cultural Heritage project that aims at the protection of Cultural Heritage through a combination of technical and organizational resources (http://www.storm-project.eu).
DOI: 10.14459/2019mp1487154
title: Oktoberfest Food Dataset
DOI: 10.14459/2018mp1506524
title: Phenomenology of bubble-collapse-driven penetration of biomaterial-surrogate liquid-liquid interfaces
DOI: 10.5519/qd.xc0d0uec
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (859 records)
DOI: 10.5519/qd.2m3ptyh0
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (377 records)
DOI: 10.17632/8rfzwb72nk.1
title: Data for: A Novel Energy Pile: The Thermo-Syphon Helical Pile
DOI: 10.17632/wk3z3gzrzy.3
title: Data for: Performance Analysis of a Hybrid Ground Source Heat Pump System Integrated with Liquid Dry Cooler

description: The uploaded file is a zipped file containing major raw data collected as a result of running simulation models.
DOI: 10.18169/papdeott007953
title: Verfahren zum Betrieb eines Lüftungsgerätes
DOI: 10.17632/mw925jcwy2.1
title: Data for: Response Surface Based Experimental Analysis and Thermal Resistance Model of a Thermoelectric Power Generation System
DOI: 10.18430/m3.irrmc.4977
title: X-ray diffraction data for the HDAC6-x3 project
DOI: 10.5281/zenodo.3256071
title: SpikeInterface Tutorial Dataset - Spike Sorting Workshop - Edinburgh 2019

description: Synthetic extracellular recording generated by MEArec (https://github.com/alejoe91/MEArec) for the SpikeIntrafece tutorial in Edunburgh, 25 June 2019.

Clone this repo (https://github.com/SpikeInterface/spiketutorials/) and follow the notebook in the <em>Spike_Sorting_Workshop_2019 </em>folder.

Enjoy!
DOI: 10.17632/gjfxzhmphx.1
title: Data for: Performance analysis and design optimization of heat pipe sink with a variable height fin array under natural convection

description: NSGA2 multi-objective genetic optimization
DOI: 10.5281/zenodo.3254448
title: Carbon-latitude analysis of the ocean carbon cycle computed from NEMO-Medusa

description: NetCDF files containing carbon-latitude stream functions computed from the coupled physical-biogeochemical model NEMO-Medusa. The stream functions have been computed for the last years of a historical run and the first years of the RCP 8.5 scenario run (2000-2009). The dataset includes a climatology of the most important tracers, the computed meridional carbon transports in the ocean, and volume distribution in the carbon-latitude space.
DOI: 10.5281/zenodo.3254449
title: Carbon-latitude analysis of the ocean carbon cycle computed from NEMO-Medusa

description: NetCDF files containing carbon-latitude stream functions computed from the coupled physical-biogeochemical model NEMO-Medusa. The stream functions have been computed for the last years of a historical run and the first years of the RCP 8.5 scenario run (2000-2009). The dataset includes a climatology of the most important tracers, the computed meridional carbon transports in the ocean, and volume distribution in the carbon-latitude space.
DOI: 10.5281/zenodo.3256113
title: A New Approach for Computing the Asymptotes of a Parametric Curve

description: [This repository contains the source data and the implementation for the manuscript "<strong>A New Approach for Computing the Asymptotes of a Parametric Curve</strong>" published in the Journal of Computational and Applied Mathematics; see Section 4.3] The file "implementation-zenodo-BlascoPerez-v3.mws" contains the last version of the implementation of the algorithm presented in the paper "<strong>A New Approach for Computing the Asymptotes of a Parametric Curve</strong>". Furthermore, the implementations of the algorithms presented in [Asymptotes of Space Curves. Journal of Computational and Applied Mathematics. Volume 278, pp. 231-247. DOI: 10.1016/j.cam.2014.10.013. (2015)] and [Asymptotes and Perfect Curves. Computer Aided Geometric Design. Volume 31, Issue 2, pp. 81-96. (2014)], can be found in this file.
description: The final version is the file "implementation-zenodo-BlascoPerez-v3.mws". Please, use download this file.
DOI: 10.5281/zenodo.3256114
title: Recent Advances in the Computation of Asymptotes for Parametric Curves

description: [This repository contains the source data and the implementation for the manuscript "<strong>Recent Advances in the Computation of Asymptotes for Parametric Curves</strong>" submitted to Journal of Computational and Applied Mathematics; see Section 4.3]
DOI: 10.5281/zenodo.3256132
title: Data and results for Cochrane systematic review and network meta-analysis on treatment of spontaneous bacterial peritonitis

description: This contains the data and the raw results for the Cochrane systematic review and network meta-analysis on the treatment of spontaneous bacterial peritonitis (https://doi.org/10.1002/14651858.CD013120). Please unzip the file and read the instructions before using the data.
DOI: 10.5281/zenodo.3256133
title: Data and results for Cochrane systematic review and network meta-analysis on treatment of spontaneous bacterial peritonitis

description: This contains the data and the raw results for the Cochrane systematic review and network meta-analysis on the treatment of spontaneous bacterial peritonitis (https://doi.org/10.1002/14651858.CD013120). Please unzip the file and read the instructions before using the data.
DOI: 10.18430/m3.irrmc.4793
title: X-ray diffraction data for the HDAC6-x519 project
DOI: 10.18430/m3.irrmc.4794
title: X-ray diffraction data for the HDAC6-x518 project
DOI: 10.18430/m3.irrmc.4803
title: X-ray diffraction data for the HDAC6-x517 project
DOI: 10.18430/m3.irrmc.4804
title: X-ray diffraction data for the HDAC6-x516 project
DOI: 10.18430/m3.irrmc.4805
title: X-ray diffraction data for the HDAC6-x515 project
DOI: 10.7910/dvn/voqchq/cyzign
title: countypres_2000-2016.tab

description: :unav
DOI: 10.18430/m3.irrmc.4732
title: X-ray diffraction data for the HDAC6-x52 project
DOI: 10.18430/m3.irrmc.4888
title: X-ray diffraction data for the HDAC6-x522 project
DOI: 10.18430/m3.irrmc.4889
title: X-ray diffraction data for the HDAC6-x523 project
DOI: 10.18430/m3.irrmc.4891
title: X-ray diffraction data for the HDAC6-x521 project
DOI: 10.18430/m3.irrmc.4894
title: X-ray diffraction data for the HDAC6-x524 project
DOI: 10.18430/m3.irrmc.4895
title: X-ray diffraction data for the HDAC6-x525 project
DOI: 10.18430/m3.irrmc.5302
title: X-ray diffraction data for the HDAC6-x520 project
DOI: 10.18430/m3.irrmc.4731
title: X-ray diffraction data for the HDAC6-x53 project
DOI: 10.18430/m3.irrmc.4892
title: X-ray diffraction data for the HDAC6-x526 project
DOI: 10.18430/m3.irrmc.4893
title: X-ray diffraction data for the HDAC6-x527 project
DOI: 10.18430/m3.irrmc.4898
title: X-ray diffraction data for the HDAC6-x528 project
DOI: 10.18430/m3.irrmc.4899
title: X-ray diffraction data for the HDAC6-x529 project
DOI: 10.18430/m3.irrmc.4592
title: X-ray diffraction data for the HDAC6-x536 project
DOI: 10.18430/m3.irrmc.5176
title: X-ray diffraction data for the HDAC6-x531 project
DOI: 10.18430/m3.irrmc.5177
title: X-ray diffraction data for the HDAC6-x530 project
DOI: 10.18430/m3.irrmc.5178
title: X-ray diffraction data for the HDAC6-x533 project
DOI: 10.18430/m3.irrmc.5179
title: X-ray diffraction data for the HDAC6-x532 project
DOI: 10.18430/m3.irrmc.5180
title: X-ray diffraction data for the HDAC6-x535 project
DOI: 10.18430/m3.irrmc.5181
title: X-ray diffraction data for the HDAC6-x534 project
DOI: 10.18430/m3.irrmc.4591
title: X-ray diffraction data for the HDAC6-x537 project
DOI: 10.18430/m3.irrmc.4637
title: X-ray diffraction data for the HDAC6-x540 project
DOI: 10.18430/m3.irrmc.5033
title: X-ray diffraction data for the HDAC6-x54 project
DOI: 10.18430/m3.irrmc.5184
title: X-ray diffraction data for the HDAC6-x539 project
DOI: 10.18430/m3.irrmc.5185
title: X-ray diffraction data for the HDAC6-x538 project
DOI: 10.5281/zenodo.3256486
title: The Hidden Midden – Geoarchaeological investigation of sedimentation processes, waste disposal practices and resource management at the La Tène settlement of Basel-Gasfabrik (Switzerland) - Dataset

description: Data set to the paper " The Hidden Midden – Geoarchaeological investigation of sedimentation processes, waste disposal practices and resource management at the La Tène settlement of Basel-Gasfabrik (Switzerland)" (Geoarchaeology; An International Journal). Supplementary Information 1: Profile photos, polished sections and thin sections scans Supplementary Information 2: Data set of the micromorpological analysis. Most of the data are given in a semiquantitative way: absent [0%] – single [&lt;2%] – few [2–10%] – frequent [10–25%] – numerous [25–50%] – dominant [&gt;50%]
DOI: 10.5281/zenodo.3256487
title: The Hidden Midden – Geoarchaeological investigation of sedimentation processes, waste disposal practices and resource management at the La Tène settlement of Basel-Gasfabrik (Switzerland) - Dataset

description: Data set to the paper " The Hidden Midden – Geoarchaeological investigation of sedimentation processes, waste disposal practices and resource management at the La Tène settlement of Basel-Gasfabrik (Switzerland)" (Geoarchaeology; An International Journal).

Supplementary Information 1: Profile photos, polished sections and thin sections scans

Supplementary Information 2: Data set of the micromorpological analysis. Most of the data are given in a semiquantitative way: absent [0%] – single [&lt;2%] – few [2–10%] – frequent [10–25%] – numerous [25–50%] – dominant [&gt;50%]
DOI: 10.18430/m3.irrmc.4638
title: X-ray diffraction data for the HDAC6-x541 project
DOI: 10.18430/m3.irrmc.4641
title: X-ray diffraction data for the HDAC6-x544 project
DOI: 10.18430/m3.irrmc.4642
title: X-ray diffraction data for the HDAC6-x545 project
DOI: 10.18430/m3.irrmc.5123
title: X-ray diffraction data for the HDAC6-x542 project
DOI: 10.18430/m3.irrmc.5131
title: X-ray diffraction data for the HDAC6-x543 project
DOI: 10.18430/m3.irrmc.5172
title: X-ray diffraction data for the HDAC6-x546 project