cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25606/surf.578c6039-c81e728d
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-002)

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 002 of the 1024³ resolution collection.
DOI: 10.5519/qd.zo3oobql
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (26 records)
DOI: 10.17171/1-6-724-1
title: 3d model of steelyard 1356

description: Ancient Steelyards
DOI: 10.17171/1-6-725-1
title: PDF of 3d model of steelyard 1356 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-727-1
title: 3d model of steelyard 1357

description: Ancient Steelyards
DOI: 10.17171/1-6-728-1
title: PDF of 3d model of steelyard 1357 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-730-1
title: 3d model of steelyard 1358

description: Ancient Steelyards
DOI: 10.17171/1-6-731-1
title: PDF of 3d model of steelyard 1358 including basic dimensions

description: Ancient Steelyards
DOI: 10.25606/surf.578c6039-e4da3b7f
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-005)

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 005 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-eccbc87e
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-003)

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 003 of the 1024³ resolution collection.
DOI: 10.17171/1-6-733-1
title: 3d model of steelyard 1359

description: Ancient Steelyards
DOI: 10.17171/1-6-734-1
title: PDF of 3d model of steelyard 1359 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-736-1
title: 3d model of steelyard 1360

description: Ancient Steelyards
DOI: 10.17171/1-6-737-1
title: PDF of 3d model of steelyard 1360 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-739-1
title: 3d model of steelyard 1361

description: Ancient Steelyards
DOI: 10.17171/1-6-740-1
title: PDF of 3d model of steelyard 1361 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-742-1
title: 3d model of steelyard 1362

description: Ancient Steelyards
DOI: 10.17171/1-6-743-1
title: PDF of 3d model of steelyard 1362 including basic dimensions

description: Ancient Steelyards
DOI: 10.25606/surf.578c6039-8f14e45f
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-007)

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 007 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-c9f0f895
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-008)

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 008 of the 1024³ resolution collection.
DOI: 10.17171/1-6-951-1
title: 3d model of steelyard 1381

description: Ancient Steelyards
DOI: 10.17171/1-6-952-1
title: PDF of 3d model of steelyard 1381 including basic dimensions

description: Ancient Steelyards
DOI: 10.25606/surf.578c6039-3295c76a
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-066)

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 066 of the 1024³ resolution collection.
DOI: 10.5281/zenodo.3520641
title: Dataset: Risk Transfer Model for Flood Risk Evolution in a Multi-reservoir System

description: The files in this record contain data for real-time optimal flood control decision making and risk propagation under multiple uncertainties considered for publication in Water Resources Research. The files consist of: Data: Figure 11; Figure 12; Figure S1; Figure S4 Relative prediction error Reservoir information Streamflow Model code: Calculation of entropy Forecasting error simulation model LHS Analytic code of transfer model
DOI: 10.5281/zenodo.3520642
title: Dataset: Risk Transfer Model for Flood Risk Evolution in a Multi-reservoir System

description: The files in this record contain data for real-time optimal flood control decision making and risk propagation under multiple uncertainties considered for publication in Water Resources Research. The files consist of: Data: Figure 11; Figure 12; Figure S1; Figure S4 Relative prediction error Reservoir information Streamflow Model code: Calculation of entropy Forecasting error simulation model LHS Analytic code of transfer model
DOI: 10.5519/qd.qthp88hd
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (182 records)
DOI: 10.15468/mgpwv6
title: Charmon ramagei sp. nov., a new Charmontinae (Hymenoptera: Braconidae) from Reunion, with a synopsis of world species

description: This dataset contains the digitized treatments in Plazi based on the original journal article Rousse, Pascal (2013): Charmon ramagei sp. nov., a new Charmontinae (Hymenoptera: Braconidae) from Reunion, with a synopsis of world species. Zootaxa 3626 (4): 583-588, DOI: http://dx.doi.org/10.11646/zootaxa.3626.4.12
DOI: 10.17171/1-6-748-1
title: 3d model of steelyard 1395

description: Ancient Steelyards
DOI: 10.17171/1-6-749-1
title: PDF of 3d model of steelyard 1395 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-752-1
title: 3d model of steelyard 1397

description: Ancient Steelyards
DOI: 10.17171/1-6-753-1
title: PDF of 3d model of steelyard 1397 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-754-1
title: 3d model of steelyard 1407

description: Ancient Steelyards
DOI: 10.17171/1-6-755-1
title: PDF of 3d model of steelyard 1407 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-954-1
title: 3d model of steelyard 1392

description: Ancient Steelyards
DOI: 10.17171/1-6-955-1
title: PDF of 3d model of steelyard 1392 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-756-1
title: 3d model of steelyard 1410

description: Ancient Steelyards
DOI: 10.17171/1-6-757-1
title: PDF of 3d model of steelyard 1410 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-758-1
title: 3d model of steelyard 1411

description: Ancient Steelyards
DOI: 10.17171/1-6-759-1
title: PDF of 3d model of steelyard 1411 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-760-1
title: 3d model of steelyard 1412

description: Ancient Steelyards
DOI: 10.17171/1-6-761-1
title: PDF of 3d model of steelyard 1412 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-762-1
title: 3d model of steelyard 1413

description: Ancient Steelyards
DOI: 10.17171/1-6-763-1
title: PDF of 3d model of steelyard 1413 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-764-1
title: 3d model of steelyard 1414

description: Ancient Steelyards
DOI: 10.17171/1-6-765-1
title: PDF of 3d model of steelyard 1414 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-766-1
title: 3d model of steelyard 1415

description: Ancient Steelyards
DOI: 10.17171/1-6-767-1
title: PDF of 3d model of steelyard 1415 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-768-1
title: 3d model of steelyard 1416

description: Ancient Steelyards
DOI: 10.17171/1-6-769-1
title: PDF of 3d model of steelyard 1416 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-770-1
title: 3d model of steelyard 1418

description: Ancient Steelyards
DOI: 10.17171/1-6-771-1
title: PDF of 3d model of steelyard 1418 including basic dimensions

description: Ancient Steelyards
DOI: 10.25606/surf.578c6039-34ed066d
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: 10.25606/surf.578c6039-8c19f571
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-172)

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 172 of the 2048³ resolution collection.
DOI: 10.17171/1-6-772-1
title: 3d model of steelyard 1420

description: Ancient Steelyards
DOI: 10.17171/1-6-773-1
title: PDF of 3d model of steelyard 1420 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-774-1
title: 3d model of steelyard 1423

description: Ancient Steelyards
DOI: 10.17171/1-6-775-1
title: PDF of 3d model of steelyard 1423 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-777-1
title: 3d model of steelyard 1428

description: Ancient Steelyards
DOI: 10.17171/1-6-778-1
title: PDF of 3d model of steelyard 1428 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-779-1
title: 3d model of steelyard 1429

description: Ancient Steelyards
DOI: 10.17171/1-6-780-1
title: PDF of 3d model of steelyard 1429 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-781-1
title: PDF of 3d model of steelyard 1430 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-782-1
title: PDF of 3d model of steelyard 1431 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-783-1
title: 3d model of steelyard 1432

description: Ancient Steelyards
DOI: 10.17171/1-6-784-1
title: PDF of 3d model of steelyard 1432 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-785-1
title: 3d model of steelyard 1434

description: Ancient Steelyards
DOI: 10.17171/1-6-786-1
title: PDF of 3d model of steelyard 1434 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-787-1
title: PDF of 3d model of steelyard 1441 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-956-1
title: 3d model of steelyard 1437

description: Ancient Steelyards
DOI: 10.17171/1-6-957-1
title: PDF of 3d model of steelyard 1437 including basic dimensions

description: Ancient Steelyards
DOI: 10.7910/dvn/dymeqr/dvicnw
title: Shotgun mass spectrometry for brain specific autoantibodies.tab

description: :unav
DOI: 10.7910/dvn/dymeqr/jxp79p
title: Patient descriptives.txt

description: :unav
DOI: 10.17171/1-6-788-1
title: 3d model of steelyard 1443

description: Ancient Steelyards
DOI: 10.17171/1-6-789-1
title: PDF of 3d model of steelyard 1443 including basic dimensions

description: Ancient Steelyards
DOI: 10.15468/bjqvfm
title: A new species of Galendromimus (Acari: Phytoseiidae) from Brazil

description: This dataset contains the digitized treatments in Plazi based on the original journal article Zacarias, M. S., De Moraes, G. J., McMurtry, J. A. (2002): A new species of Galendromimus (Acari: Phytoseiidae) from Brazil. Zootaxa 102: 1-6, DOI: 10.5072/zenodo.155636
DOI: 10.17171/1-6-790-1
title: 3d model of steelyard 1444

description: Ancient Steelyards
DOI: 10.17171/1-6-791-1
title: PDF of 3d model of steelyard 1444 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-793-1
title: 3d model of steelyard 1450

description: Ancient Steelyards
DOI: 10.17171/1-6-794-1
title: PDF of 3d model of steelyard 1450 including basic dimensions

description: Ancient Steelyards
DOI: 10.5281/zenodo.3520696
title: Common biochemical and topological properties of metabolic genes recurrently dysregulated in tumors

description: Although tumors exhibit numerous metabolic alterations, it’s unclear if common objectives and constraints underlie diverse metabolic changes. Here we interpret cancer gene expression, copy number variation, and survival data using a computational model, MetOncoFit. MetOncoFit evaluates142 metabolic features that can impact tumor fitness, including enzyme catalytic activity, pathway association, network topological attributes, and reaction flux. Meta-analysis of tumor databases using MetOncoFit revealed that metabolic enzymes with high catalytic activity were frequently up-regulated in many tumors and associated with poor survival. MetOncoFit also identified metabolites that were hot-spots of dysregulation. MetOncoFit illuminates how enzyme activity and metabolic network architecture influences tumorigenesis.
DOI: 10.17171/1-6-795-1
title: 3d model of steelyard 1451

description: Ancient Steelyards
DOI: 10.17171/1-6-796-1
title: PDF of 3d model of steelyard 1451 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-797-1
title: 3d model of steelyard 1452

description: Ancient Steelyards
DOI: 10.17171/1-6-798-1
title: PDF of 3d model of steelyard 1452 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-799-1
title: 3d model of steelyard 1453

description: Ancient Steelyards
DOI: 10.17171/1-6-800-1
title: PDF of 3d model of steelyard 1453 including basic dimensions

description: Ancient Steelyards
DOI: 10.5281/zenodo.3520695
title: Common biochemical and topological properties of metabolic genes recurrently dysregulated in tumors

description: Although tumors exhibit numerous metabolic alterations, it’s unclear if common objectives and constraints underlie diverse metabolic changes. Here we interpret cancer gene expression, copy number variation, and survival data using a computational model, MetOncoFit. MetOncoFit evaluates142 metabolic features that can impact tumor fitness, including enzyme catalytic activity, pathway association, network topological attributes, and reaction flux. Meta-analysis of tumor databases using MetOncoFit revealed that metabolic enzymes with high catalytic activity were frequently up-regulated in many tumors and associated with poor survival. MetOncoFit also identified metabolites that were hot-spots of dysregulation. MetOncoFit illuminates how enzyme activity and metabolic network architecture influences tumorigenesis.
DOI: 10.17171/1-6-801-1
title: 3d model of steelyard 1454

description: Ancient Steelyards
DOI: 10.17171/1-6-802-1
title: PDF of 3d model of steelyard 1454 including basic dimensions

description: Ancient Steelyards
DOI: 10.17171/1-6-804-1
title: 3d model of steelyard 1467

description: Ancient Steelyards
DOI: 10.17171/1-6-805-1
title: PDF of 3d model of steelyard 1467 including basic dimensions

description: Ancient Steelyards