cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.2653095
title: Quantitative modeling method for geolocating pollen samples

description: Pollen producing plants are present on every continent and the taxa of these plans can be distinguished based on the pollen grains. As a pollen assemblage can only come from a vegetation that produces the pollen types in that assemblage, pollen can give an indication of vegetation composition. Knowing the assemblage that produced a specific sample can be used to determine the origins of pollen on objects of interest such as footwear, drugs and poached goods. Most studies that used forensic palynology for geolocation were qualitative analyses of regions with low biodiversity. None are studies on a continental scale that involve the tropics. There is a need for objective qualitative forensic methods, which are expected to be effective and efficient with both high and low biodiversity regions.

In this study a qualitative modeling method was developed using pollen samples from 705 neotropical sites and tested on pollen samples from 55 European sites. These samples came from pollen traps, soil samples, mud water interfaces of lakes and rivers, and moss samples.  Ensemble species distribution models based on presence data were run for all genera present in these samples. The predicted range of all genera present in each individual sample were combined to produce a predicted range of origin of the site. A rate of 89.9% of all Neotropical sites was correctly predicted. The highest accuracy was achieved with samples from pollen traps, which were correct in 96.2% of cases. The results of European and Neotropical sites of the same sample origin were comparable. The results indicate that qualitative analysis can be accurate and efficient in the tropics at a continental scale.

This file contains all used data and R scripts. With the contents the results can be recreated. Instructions on use are enclosed
DOI: 10.5281/zenodo.2653096
title: Quantitative modeling method for geolocating pollen samples

description: Pollen producing plants are present on every continent and the taxa of these plans can be distinguished based on the pollen grains. As a pollen assemblage can only come from a vegetation that produces the pollen types in that assemblage, pollen can give an indication of vegetation composition. Knowing the assemblage that produced a specific sample can be used to determine the origins of pollen on objects of interest such as footwear, drugs and poached goods. Most studies that used forensic palynology for geolocation were qualitative analyses of regions with low biodiversity. None are studies on a continental scale that involve the tropics. There is a need for objective qualitative forensic methods, which are expected to be effective and efficient with both high and low biodiversity regions.

In this study a qualitative modeling method was developed using pollen samples from 705 neotropical sites and tested on pollen samples from 55 European sites. These samples came from pollen traps, soil samples, mud water interfaces of lakes and rivers, and moss samples.  Ensemble species distribution models based on presence data were run for all genera present in these samples. The predicted range of all genera present in each individual sample were combined to produce a predicted range of origin of the site. A rate of 89.9% of all Neotropical sites was correctly predicted. The highest accuracy was achieved with samples from pollen traps, which were correct in 96.2% of cases. The results of European and Neotropical sites of the same sample origin were comparable. The results indicate that qualitative analysis can be accurate and efficient in the tropics at a continental scale.

This file contains all used data and R scripts. With the contents the results can be recreated. Instructions on use are enclosed
DOI: 10.5281/zenodo.2653248
title: All observational data for the study "Mixing, stratification and plankton under lake-ice: implications for summertime oxygen levels in the hypolimnion of a large lake"

description: All field measurements of temperature, oxygen, conductivity, and velocity used in this study
DOI: 10.5286/isis.e.rb1890263
title: Lattice and magnetic dynamics in thermoeelctric AgCrSE2
DOI: 10.17632/3rvcwn4f7y.1
title: Data for: Re-examining the time-varying nature and determinants of exchange rate pass-through into import prices

description: This study collected 1975Q1-2016Q1 quarterly data from 16 OECD countries, including Australia, Austria, Canada, Denmark, Finland, Germany, Italy, Japan, the Netherlands, New Zealand, Norway, Spain, Sweden, Switzerland, the UK, and the US. All data were derived from IMF-IFS and the OECD Statistical Compendium. For details, please refer to the Manustript.
DOI: 10.21227/prvh-es90
title: Audio Steganalysis Dataset

description: This is a dataset for audio steganalysis.
DOI: 10.3886/e109524v1
title: The impact of adapting the jurisprudence of the objectives of Sharia Controls (Contemporary financial transactions as a model)

description: The adaptation of the jurisprudence is a practical
method of jurisprudence to judge the hew cases and matters. It can only be
achieved after verifying the availability of its basic elements, including the
objectives of Shari'a to deal with the new issues and developments in
contemporary financial transactions. Therefore, this study aims to reveal the
importance of the practice of adapting the jurisprudence to meet the challenges
of the age and to show their role in practical cases.
DOI: 10.5281/zenodo.2653247
title: All observational data for the study "Mixing, stratification and plankton under lake-ice: implications for summertime oxygen levels in the hypolimnion of a large lake"

description: All field measurements of temperature, oxygen, conductivity, and velocity used in this study
DOI: 10.5517/ccdc.csd.cc2267k3
title: CCDC 1912624: Experimental Crystal Structure Determination

description: Related Article: Brian W. Skelton, Murray V. Baker, Rosenani A. Haque|2019|CSD Communication|||
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5281/zenodo.2653257
title: sEMG data

description: Data set used by the "Exploration of feature extraction methods and dimension for sEMG signal classification"
DOI: 10.5281/zenodo.2653258
title: sEMG data

description: Data set used by the "Exploration of feature extraction methods and dimension for sEMG signal classification"
DOI: 10.5281/zenodo.2653478
title: Transkripte von drei TV-Debatten mit Schweizer PolitikerInnen vor eidgenössischen Abstimmungen. Transcripts of three TV debates with Swiss politicians before popular votes.

description: Der Datensatz enthält Transkripte (doc, htm, PDF) von drei 'Arena'-Abstimmungssendungen mit Schweizer PolitikerInnen vor eidgenössischen Abstimmungen. Die TV-Sendungen wurden nach GAT 2 transkribiert / The dataset contains transcripts (doc, htm, PDF) of three 'Arena' TV-debates with Swiss politicians before popular votes. The debates were transcribed according to GAT 2.
DOI: 10.5281/zenodo.2653479
title: Transkripte von drei TV-Debatten mit Schweizer PolitikerInnen vor eidgenössischen Abstimmungen. Transcripts of three TV debates with Swiss politicians before popular votes.

description: Der Datensatz enthält Transkripte (doc, htm, PDF) von drei 'Arena'-Abstimmungssendungen mit Schweizer PolitikerInnen vor eidgenössischen Abstimmungen. Die TV-Sendungen wurden nach GAT 2 transkribiert / The dataset contains transcripts (doc, htm, PDF) of three 'Arena' TV-debates with Swiss politicians before popular votes. The debates were transcribed according to GAT 2.
DOI: 10.14455/nrct.img.2019.360
title: กรณีศึกษาออกแบบผลิตภัณฑ์จากเศษไม้เหลือใช้ในอุตสาหกรรมแปรรูปไม้ เพื่อส่งเสริมงานตกแต่งทางสถาปัตยกรรม
DOI: 10.14455/nrct.img.2019.365
title: เครื่องปลูกข้าวแบบหย่อนต้นกล้า
DOI: 10.25606/surf.578c6039-499dfaf9
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-013)

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 013 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-4b9df86a
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-017)

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 017 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-4cbc0da4
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-084)

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 084 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-508b7a04
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-083)

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 083 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-a1413d21
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-086)

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 086 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-a88d6dba
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-087)

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 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-a9d39ae0
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-085)

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 085 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-eded17f5
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-016)

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 016 of the 2048³ resolution collection.
DOI: 10.14455/nrct.fas.2019.11
title: การบริหารจัดการน้ำโป่งแดง โครงการชลประทานแม่ฮ่องสอน
DOI: 10.14455/nrct.fas.2019.12
title: บริหารจัดการน้ำอย่างไร ให้มีน้ำใช้อย่างยั่งยืน
DOI: 10.14455/nrct.fas.2019.14
title: การบริหารจัดการน้ำและการพัฒนาระบบชลประทาน
DOI: 10.14455/nrct.fas.2019.15
title: การบริหารจัดการน้ำเพื่อสร้างความมั่นคงด้านการผลิต ทั้งภาคการเกษตร/อุตสาหกรรม
DOI: 10.14455/nrct.fas.2019.16
title: โครงการพัฒนาแหล่งน้ำขนาดใหญ่ตามแผนยุทธศาสตร์การริหารจัดการน้ำของประเทศ (พ.ศ. 2558-2569)
DOI: 10.14455/nrct.img.2019.366
title: เครื่องลำเลียงทะลายปาล์มน้ำมันชนิดผ่อนแรง
DOI: 10.14455/nrct.img.2019.367
title: โมเดลโครงสร้างความสัมพันธ์เชิงสาเหตุและประสิทธิผลของรูปแบบการปรับเปลี่ยนพฤติกรรมการดื่มเครื่องดื่มแอลกอฮอล์ของนักศึกษาปริญญาตรี
DOI: 10.25606/surf.578c6039-3d3163c4
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-015)

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 015 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-73558e74
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-082)

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 082 of the 1024³ resolution collection.