cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25606/surf.578c6039-0be4acef
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-195)

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 195 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-32ff715b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-752)

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 752 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-4410d552
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-684)

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 684 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-85bbe597
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-538)

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 538 of the 2048³ resolution collection.
DOI: 10.25919/5d7efc6adae9a
title: Parkes observations for project P885 semester 2019APRS_13

description: We propose to observe the magnetars 1E 1547.0-5408 and PSR J1622-4950 approximately weekly, to track their rotation, flux density, and polarisation, as we have been doing through this project. As of this week (8 Dec 2018), XTE J1810-197 is again a radio magnetar, after 10 years dormant! (We have been observing it sporadically during its low state waiting for such an event.) Its likely chaotic rotation will be better tracked in detail elsewhere, but weekly observations with the UWL receiver will provide unique measurements of its radio spectrum and broad-band behaviour. Our observations provide an important window into remarkably dynamic magnetar magnetospheres, and characterise the conditions under which radio emission takes place therein, placing constraints on the emission mechanisms, which in at least some significant respects differ from those of ordinary pulsars.
DOI: 10.25606/surf.578c6039-59a9e27e
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-535)

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 535 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-8464742d
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-590)

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 590 of the 2048³ resolution collection.
DOI: 10.5519/qd.2xw0khf4
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (0 records)
DOI: 10.25606/surf.578c6039-f6b17200
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-618)

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 618 of the 2048³ resolution collection.
DOI: 10.21227/4w0x-ww05
title: Data for arc light and temperature reconstruction

description: 'Onion-Kasuga' algorithm was proposed to simplify the energy distribution reconstruction process. The research work discussed and supplied an effective method for energy/temperature distribution welding arc discharge analysis. That is also believed to be important for relevant field because the arc is usually used as the heat or force source. It is crucial to understand and control the arc behavior.
DOI: 10.21227/5mfa-3k68
title: Data for arc light and temperature reconstruction

description: 'Onion-Kasuga' algorithm was proposed to simplify the energy distribution reconstruction process. The research work discussed and supplied an effective method for energy/temperature distribution welding arc discharge analysis. That is also believed to be important for relevant field because the arc is usually used as the heat or force source. It is crucial to understand and control the arc behavior.
DOI: 10.21227/t9mt-et97
title: 300-Dimensional Word Embeddings for Nepali Language

description: This pre-trained Word2Vec model has 300-dimensional vectors for more than 0.5 million Nepali words and phrases. A separate Nepali language text corpus was created using the news contents freely available in the public domain. The text corpus contained more than 100 million running words.Word2Vec model details: Embeddings Dimension: 300, Architecture: Continuous - BOW, Training algorithm: Negative sampling = 15, Context (window) size: 10, Token minimum count: 2, Encoded in UTF-8.
DOI: 10.25919/5d7f3c5ac3e84
title: Parkes observations for project P958 semester 2019APRS_86

description: Fast radio bursts (FRBs) continue to raise more questions than they answer. Until a few months ago, only one burst – the only one known to repeat - had been localized to a bright radio nebula (either a young supernova remnant or pulsar wind nebulae) in a distant dwarf galaxy. Over the last year searches with the Australian Square Kilometre Array Pathfinder (ASKAP) have detected 28 bursts, two of which have been localised to host galaxies at redshifts &gt; 0.3. These bursts and their hosts are very unlike the repeater, suggesting there may be a dichotomy in the population. Over the next six months we expect to detect another 12 FRBs, which will also have sub-arcsecond localisations. Here we propose to search this population for repeats. Our comprehensive sample and a dense monitoring campaign of well localised bursts, at a fluence limit more than 60 times lower than that of their detections, will either confirm the presence of additional repeating FRBs or the uniqueness of FRB 121102 amongst the population.
DOI: 10.7910/dvn/jn4eyu/qtv4gw
title: MeTooMA.tab

description: :unav
DOI: 10.5519/qd.hc3yjead
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1 records)
DOI: 10.5281/zenodo.3414419
title: GNNWR Code and Simulated Data

description: GNNWR Code and Simulated Data
DOI: 10.5281/zenodo.3414515
title: Picture assessments

description: This is a full overview of picture assessments.
DOI: 10.5281/zenodo.3414516
title: Picture assessments

description: This is a full overview of picture assessments.
DOI: 10.17632/fm7v4dzpfs.1
title: Data for: Data-driven hybrid multiple attribute decision-making model for green supplier evaluation and performance improvement
DOI: 10.5281/zenodo.3412757
title: Analysis of opposing histone modifications H3K4me3 and H3K27me3 reveals candidate diagnostic biomarkers for triple negative breast cancer and gene set prediction combinations

description: Supplementary data of manuscript <strong>'Analysis of opposing histone modifications H3K4me3 and H3K27me3 reveals candidate diagnostic biomarkers for triple negative breast cancer and gene set prediction combinations </strong><strong>Analysis of opposing histone modifications H3K4me3 and H3K27me3 reveals candidate diagnostic biomarkers for triple negative breast cancer and gene set prediction combinations'</strong>
DOI: 10.5281/zenodo.3412758
title: Analysis of opposing histone modifications H3K4me3 and H3K27me3 reveals candidate diagnostic biomarkers for triple negative breast cancer and gene set prediction combinations

description: Supplementary data of manuscript <strong>'Analysis of opposing histone modifications H3K4me3 and H3K27me3 reveals candidate diagnostic biomarkers for triple negative breast cancer and gene set prediction combinations </strong><strong>Analysis of opposing histone modifications H3K4me3 and H3K27me3 reveals candidate diagnostic biomarkers for triple negative breast cancer and gene set prediction combinations'</strong>
DOI: 10.15468/xbrdpp
title: A taxonomic review of the Xanthonia species occurring in Texas (Coleoptera: Chrysomelidae, Eumolpinae)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Riley, Edward G., Weisman, Donald M., Quinn, Michael A. (2019): A taxonomic review of the Xanthonia species occurring in Texas (Coleoptera: Chrysomelidae, Eumolpinae). Zootaxa 4668 (1): 1-29, DOI: https://doi.org/10.11646/zootaxa.4668.1.1
DOI: 10.5258/soton/d0759
title: Dataset: Fibre-optic based particle sensing via deep learning

description: Dataset to support the publication: Grant-Jacob, James et al."Fibre-optic based particle sensing via deep learning". Journal of Physics: Photonics. 2019.
DOI: 10.5258/soton/d1070
title: Monitoring data from Mill Hill pile stabilised railway embankment

description: Dataset supports: Smethurst, J., Bicocchi, N., Powrie, W., & O'Brien, A. S. (2019). Behaviour of discrete piles used to stabilise a tree-covered railway embankment. Géotechnique, [18-P-150R1].A data set from the monitoring of a pile-stabilised railway embankment at Mill Hill, between November 2004 and July 2010. The data set contains measured pile strains, bending moments and displacements, slope (soil) displacements, pore water pressures, soil water content, and the results of some analysis (such as fitted curves).Data can be requested via http://library.soton.ac.uk/datarequest
DOI: 10.5258/soton/d1029
title: O-band bismuth-doped fiber amplifier and its temperature dependent performance

description: This dataset supports the publication: Yu Wang, Naresh K Thipparapu, Siyi Wang, Pranabesh Barua, Andrey A Umnikov, David J Richardson, Jayanta Sahu. (2019) O-band bismuth-doped fiber amplifier and its temperature dependent performance, 6th Workshop on Specialty Optical Fiber and Their Applications (WSOF 2019)
DOI: 10.5281/zenodo.3415146
title: Supporting transcriptomic data and code for: "Rapid and dose-dependent Natural Killer (NK) cell modulation and cytokine correlations after human rVSV-ZEBOV Ebolavirus vaccination"

description: The counts_NK.csv file contains gene expression data (counts) for genes in the Ion Ampliseq human Gene expression kit panel. Data were obtained from whole blood RNA. Subjects were vaccinated with a high dose of the rVSV-ZEBOV vaccine against Ebola virus disease in the Geneva clinical trial. The Descriptive_Table_NK_2.csv contains descriptive data of the subjects for differential expression analysis. The NK_analysis_code.R file contains the code used for analysis.
DOI: 10.5281/zenodo.3415147
title: Supporting transcriptomic data and code for: "Rapid and dose-dependent Natural Killer (NK) cell modulation and cytokine correlations after human rVSV-ZEBOV Ebolavirus vaccination"

description: The counts_NK.csv file contains gene expression data (counts) for genes in the Ion Ampliseq human Gene expression kit panel. Data were obtained from whole blood RNA. Subjects were vaccinated with a high dose of the rVSV-ZEBOV vaccine against Ebola virus disease in the Geneva clinical trial. The Descriptive_Table_NK_2.csv contains descriptive data of the subjects for differential expression analysis. The NK_analysis_code.R file contains the code used for analysis.
DOI: 10.5519/qd.ab4p8rej
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (113 records)
DOI: 10.21421/d2/to4jwo
title: Fine mapping for shoot fly resistance and stay-green QTL's in Sorghum

description: This study was conducted to dissect the genetic basis of stay-green Quantitative Trait Loci (QTL) and shoot fly resistance morphological QTLs on sorghum chromosome SBI-10 long arm (L) using high-density single nucleotide polymorphism (SNP) genetic markers. A fine-mapping population of 1,894 F2 individuals was developed from a cross involving introgression lines- RSG04008-6 (stay-green, but shoot fly susceptible) × J2614-11 (moderately senescent, but shoot fly resistant). Based on genotyping and phenotyping data 182 selective recombinants were subjected to Genotyping by Sequencing (GBS). SNPs were derived from the sequencing data by aligning the reads to the Sorghum bicolor reference genome v1.4 and v3.1 which identified 32,836 and 29,507 SNPs respectively, from the aligned reads using the TASSEL GBS pipeline. SNPs with 0.05 minimum minor allele frequency (MAF) were retained. Finally, 1515(v1.4) and 1184(v3.1) SNPs were found within the target region on SBI-10L (chromosome 10; 45Mb-60Mb). Experimental location on Google Map
DOI: 10.5258/soton/d0880
title: Temperature-dependent gain and noise figure characteristics in O-band bismuth-doped fibre amplifier

description: This dataset supports the publication: Wang, Yu et al (2019). Temperature dependent gain and noise figure characteristics of O-band bismuth-doped fibre amplifier. ECOC 2019.
DOI: 10.7910/dvn/ezdwzh/1mj4ae
title: CJPS_Schimpf_Replication_MasterFile.R

description: :unav
DOI: 10.7910/dvn/ezdwzh/3qippe
title: CJPS_Schimpf_Replication_Analyses_20190107.R

description: :unav
DOI: 10.7910/dvn/ezdwzh/dyn1ii
title: READ ME.txt

description: :unav
DOI: 10.7910/dvn/ezdwzh/slfwpx
title: .Rhistory

description: :unav
DOI: 10.7910/dvn/ezdwzh/snhpv5
title: CJPS_Schimpf_Replication_DataPrep2_20190107.R

description: :unav
DOI: 10.7910/dvn/ezdwzh/vya7ij
title: CJPS_Schimpf_Replication_DataPrep1_20190107.R

description: :unav
DOI: 10.7910/dvn/ezdwzh/ximowy
title: dfCan2015.RData

description: :unav
DOI: 10.5284/1056618
title: Photographs from the archive of the IUO Italian Archaeological Mission to Upper Egypt (1977-1986)

description: null
DOI: 10.5258/soton/d1077
title: Dataset supporting the article entitled "Collaborative Adaptation for Energy-Efficient Heterogeneous Mobile SoCs"

description: This dataset supports the article entitled "Collaborative Adaptation for Energy-Efficient Heterogeneous Mobile SoCs" accepted for publication in IEEE Transactions on Computers, August 2019.
DOI: 10.17171/2-7-31-1
title: Fit grid lines on wall
title: Olstzyn Castle

description: Copernicus' Heliograph
DOI: 10.17632/mccvkb3m59.3
title: Quantitative mapping of the East Australian Current encroachment

description: This dataset includes a compelete statistics of the EAC mapping validation, data of sensitivity experiments, and the quantitative results of EAC encroachment (area and distance) during July 2015 to September 2017.
DOI: 10.15468/kmwh6u
title: A Revision of the Holarctic Genus Rocetelion Matile (Diptera: Keroplatidae)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Fitzgerald, Scott J. (2019): A Revision of the Holarctic Genus Rocetelion Matile (Diptera: Keroplatidae). Zootaxa 4648 (3): 568-580, DOI: https://doi.org/10.11646/zootaxa.4648.3.10
DOI: 10.15468/s07h57
title: A new stygobiotic Xiphocaridinella (Crustacea: Decapoda: Atyidae) from the Motena Cave, Samegrelo-Zemo Svaneti region of Georgia, Caucasus

description: This dataset contains the digitized treatments in Plazi based on the original journal article Marin, Ivan (2019): A new stygobiotic Xiphocaridinella (Crustacea: Decapoda: Atyidae) from the Motena Cave, Samegrelo-Zemo Svaneti region of Georgia, Caucasus. Zootaxa 4648 (3): 592-600, DOI: https://doi.org/10.11646/zootaxa.4648.3.12