cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25606/surf.578c6039-c8e388bb
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-611)

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 611 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-e685020e
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-607)

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 607 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-fde91617
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-604)

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 604 of the 2048³ resolution collection.
DOI: 10.25835/0007088
title: Condensates of SO(5)_N anyons

description: Plots, data and Mathematica notebooks for the paper\r\n\r\nDaniel Borcherding and Holger Frahm: "Condensates of interacting non-Abelian $SO(5)_{N_f}$ anyons", JHEP __1910__ (2019) 054, arXiv:1906.09929\r\n\r\nand the doctoral thesis\r\n\r\nDaniel Borcherding: "Non-Abelian quasi-particles in electronic systems". Gottfried Wilhelm Leibniz Universit\xe4t Hannover, Diss.
DOI: 10.5281/zenodo.3245361
title: X-ray diffraction images of Anti-CD20 crystals

description: Original X-ray diffraction images from Pilatus detector taken at Diamond Light Source Synchrotron (I04 beamline).

Images can be read by AXDV (or similar) software.

These datasets were used for diffraction and crystallographic analyses reported in Yang et al., Crystals 2019, 9, 230.
DOI: 10.5281/zenodo.3245362
title: X-ray diffraction images of Anti-CD20 crystals

description: Original X-ray diffraction images from Pilatus detector taken at Diamond Light Source Synchrotron (I04 beamline).

Images can be read by AXDV (or similar) software.

These datasets were used for diffraction and crystallographic analyses reported in Yang et al., Crystals 2019, 9, 230.
DOI: 10.6073/pasta/adbd8a51eeb4b76bdbbf40a5db30d210
title: Rainfall Stable Isotopes collected at Florida International University-MMC (FCE LTER), Miami Florida, from October 2007 to Present

description: A precipitation collector was placed on top of the roof of the HLS-1 buidling at the main campus of FIU. The collector only. opens when the sensor is activated by water and closes when it is not raining to prevent evaportation. Water samples were collected and analyzed for stable isotopes of hydrogen and oxygen.
DOI: 10.5281/zenodo.3255138
title: Systematic mapping data for translation-enabling technologies for sign languages

description: These data correspond to the papers selected for a systematic mapping of that translation-enabling technologies for sign languages.
DOI: 10.5281/zenodo.3255139
title: Systematic mapping data for translation-enabling technologies for sign languages

description: These data correspond to the papers selected for a systematic mapping of that translation-enabling technologies for sign languages.
DOI: 10.17632/rdv35w5xcz.1
title: Data for: ‘You are where you shop’: Examining stereotypes about town center shoppers

description: Data set for the article entitled: ‘You are where you shop’: Examining stereotypes about town center shoppers. Please contact burak.tunca@fek.lu.se or burtunca@gmail.com for more information.
DOI: 10.5281/zenodo.3256193
title: Localized admittance and correlation

description: Localized admittance and correlation data from Broquet & Wieczorek (2019)
DOI: 10.5281/zenodo.3256194
title: Localized admittance and correlation

description: Localized admittance and correlation data from Broquet & Wieczorek (2019)
DOI: 10.17632/mk5xz9jy5d.1
title: Data for: Fault Detection of Sludge Bulking Using a Self-Organizing Type-2 Fuzzy-Neural-Network
DOI: 10.17632/cxbtk83r43.1
title: Data for: Broad spectrum antiviral remdesivir inhibits human endemic and zoonotic deltacoronaviruses with a highly divergent RNA dependent RNA polymerase
DOI: 10.5281/zenodo.3256095
title: Statistics on Smoking, England, 2017

description: This statistical report presents a range of information on smoking which is drawn together from a variety of sources. The report aims to present a broad picture of health issues relating to smoking in England and covers topics such as smoking prevalence, habits, behaviours and attitudes among adults and school children, smoking-related ill health and mortality and smoking-related costs.

This report combines data from different sources presenting it in a user-friendly format. It contains data and information previously published by the Health and Social Care Information Centre (HSCIC), Department of Health, the Office for National Statistics and Her Majesty’s Revenue and Customs. The report also includes new analyses carried out by the Health and Social Care Information Centre.
DOI: 10.5281/zenodo.3256096
title: Statistics on Smoking, England, 2017

description: This statistical report presents a range of information on smoking which is drawn together from a variety of sources. The report aims to present a broad picture of health issues relating to smoking in England and covers topics such as smoking prevalence, habits, behaviours and attitudes among adults and school children, smoking-related ill health and mortality and smoking-related costs.

This report combines data from different sources presenting it in a user-friendly format. It contains data and information previously published by the Health and Social Care Information Centre (HSCIC), Department of Health, the Office for National Statistics and Her Majesty’s Revenue and Customs. The report also includes new analyses carried out by the Health and Social Care Information Centre.
DOI: 10.5255/ukda-sn-853729
title: Party survey and follow up survey 2017-2019
DOI: 10.5281/zenodo.3253760
title: Comparison of three types of laser optical disdrometers under natural rainfall conditions

description: This dataset contains the raw files of one rain gauge and four disdrometers used for a comparative study of rainfall characteristics measured by optical laser-based disdrometers.

Please see data description file for further information.
DOI: 10.5281/zenodo.3253761
title: Comparison of three types of laser optical disdrometers under natural rainfall conditions

description: This dataset contains the raw files of one rain gauge and four disdrometers used for a comparative study of rainfall characteristics measured by optical laser-based disdrometers.

Please see data description file for further information.
DOI: 10.5519/qd.m36cl2nt
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (13 records)
DOI: 10.25606/surf.578c6039-e595596f
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-059)

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 059 of the 2048³ resolution collection.
DOI: 10.5063/f1ng4nz3
title: Oostvaardersplassen carrion experiment

description: We collected insects and plants at five carrion sites (1 month old red deer Cervus elaphus carcasses) and at paired control sites in spring (May) and summer (late August) 2013 to test whether carrion has lasting trophic effects on taxa other than carrion associated species.In spring we collected arthropods using 3 pitfall traps at each carrion and control site, and in summer we took 3 destructive suction samples at each site.The following groups were identified to species level: Spiders (Araneae) and harvestmen (Opiliones), woodlice (Isopoda), millipedes and centipedes (Myriapoda), earwigs (Dermaptera), beetles (Coleoptera),true bugs (Heteroptera), plant and leafhoppers (Hemiptera: Auchenorrhyncha). The following groups were counted: fly larvae, ants (not analyses in the original paper), larvae of fruit flies and Microlepidoptera living in the flower heads of Carduus crispus (also not analyses in the original paper).In late summer we also collected plant material at the sites of the suction sampling to measure plant biomass and C:N ratios of the plant tissue.During the summer sampling, 2 of the original carrion sites could not be found back and were substituted with 2 carcasses that looked approximately of the same age (died at the end of the previous winter).
DOI: 10.5519/qd.cipxnyhh
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (8 records)
DOI: 10.5281/zenodo.3256099
title: Data and results for Cochrane systematic review and network meta-analysis on hepatorenal syndrome

description: This contains the data and the raw results for the Cochrane systematic review and network meta-analysis on hepatorenal syndrome (https://doi.org/10.1002/14651858.CD013103). Please unzip the file and read the instructions before using the data.
DOI: 10.5281/zenodo.3256100
title: Data and results for Cochrane systematic review and network meta-analysis on hepatorenal syndrome

description: This contains the data and the raw results for the Cochrane systematic review and network meta-analysis on hepatorenal syndrome (https://doi.org/10.1002/14651858.CD013103). Please unzip the file and read the instructions before using the data.
DOI: 10.5519/qd.cvdyqj7d
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (53 records)
DOI: 10.25606/surf.578c6039-525b6c2e
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-052)

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 052 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-8ff3e26d
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-090)

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 090 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-0076f3ee
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-082)

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 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-796f08f9
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-089)

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 089 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-8b12e928
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-088)

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 088 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-a87f84f1
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-055)

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 055 of the 2048³ resolution collection.