cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25606/surf.636f736d6f67-99
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-002)

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 2048³ resolution collection.
DOI: 10.25606/surf.636f736d6f67-642
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-767)

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 767 of the 2048³ resolution collection.
DOI: 10.25606/surf.636f736d6f67-673
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-026)

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 026 of the 512³ resolution collection.
DOI: 10.5066/f7rr1wf0
title: Geochemical data supporting analysis of geochemical conditions and nitrogen transport in nearshore groundwater and the subterranean estuary at a Cape Cod embayment, East Falmouth, Massachusetts

description: This data release provides analytical and other data in support of an analysis of nitrogen transport and transformation in groundwater and in a subterranean estuary in the Eel River and onshore locations on the Seacoast Shores peninsula, Falmouth, Massachusetts. The analysis is described in U.S. Geological Survey Scientific Investigations Report 2018-5095 by Colman and others (2018). This data release is structured as a set of comma-separated values (CSV) files, each of which contains data columns for laboratory (if applicable), USGS Site Name, date sampled, time sampled, and columns of specific analytical and(or) other data. The .csv data files have the same number of rows and each row in each .csv file corresponds to the same sample. Blank cells in a .csv file indicate that the sample was not analyzed for that constituent. The data release also provides a Data Dictionary (Data_Dictionary.csv) that provides the following information for each constituent (analyte): laboratory or data source, data type, description of units, method, minimum reporting limit, limit of quantitation if appropriate, method reference citations, minimum, maximum, median, and average values for each analyte. The data release also contains a file called Abbreviations in Data_Dictionary.pdf that contains all of the abbreviations in the Data Dictionary and in the well characteristics file in the companion report, Colman and others (2018).
DOI: 10.5281/zenodo.1319539
title: ROS-Specific Huntingtin Interactions: Reproducible high and medium confidence huntingtin interacting proteins

description: Mass spec identification of DNA damage-specific huntingtin protein-protein interactions.
description: This work is funded by the HDSA Berman/Topper HD Career Development Fellowship.
DOI: 10.5281/zenodo.1319540
title: ROS-Specific Huntingtin Interactions: Reproducible high and medium confidence huntingtin interacting proteins

description: Mass spec identification of DNA damage-specific huntingtin protein-protein interactions.
description: This work is funded by the HDSA Berman/Topper HD Career Development Fellowship.
DOI: 10.7910/dvn/wgwmav/3uhtlp
title: Paglayan Dataset.tab

description: Original longitudinal dataset on student-teacher ratios, teacher salaries, per-pupil spending, and collective bargaining rights for teachers across U.S. states
DOI: 10.7910/dvn/wgwmav/6wp7lo
title: UScoord.tab

description: Geographic coordinates for Figure 1
DOI: 10.7910/dvn/wgwmav/cd2e6b
title: AJPS Replication Code.do

description: Replication code for all Tables and Figures in the main text and Online Appendix
DOI: 10.7910/dvn/wgwmav/el7mfv
title: Data Appendix.pdf

description: Data Appendix
DOI: 10.7910/dvn/wgwmav/ggnd0s
title: Codebook.pdf

description: Codebook
DOI: 10.7910/dvn/wgwmav/gmhxox
title: CBA_Coverage.tab

description: Teachers covered by collective bargaining agreements (from Saltzman)
DOI: 10.7910/dvn/wgwmav/lzecpr
title: Paglayan Dataset-1.tab

description: Original longitudinal dataset on student-teacher ratios, teacher salaries, per-pupil spending, and collective bargaining rights for teachers across U.S. states
DOI: 10.7910/dvn/wgwmav/v64del
title: CBA_Coverage-1.tab

description: Teachers covered by collective bargaining agreements (from Saltzman)
DOI: 10.7910/dvn/wgwmav/x2kcrx
title: Readme.txt

description: List of files and short description of their content
DOI: 10.7910/dvn/ywzbuj/icy3t0
title: China_DemilitarizationAgreement.tab

description: :unav
DOI: 10.7910/dvn/ywzbuj/ntp7et
title: Russia_Sanctions.tab

description: :unav
DOI: 10.7910/dvn/ywzbuj/rk8wdr
title: mattesweeksAJPS.tab

description: :unav
DOI: 10.7910/dvn/ywzbuj/vleyhr
title: mattesweeksAJPS.do

description: :unav
DOI: 10.7910/dvn/ywzbuj/x5thww
title: Russia_TroopWithdrawal.do

description: :unav
DOI: 10.5063/f1ms3qzb
title: Alaska Local and Regional Information (ALARI) data on Alaska's workforce: characteristics, tax revenue, and industries

description: These three datasets are a consolidated version of the many found on http://live.laborstats.alaska.gov/alari/. Data were initially collected by the Alaska Department of Labor and Workforce Development, Research and Analysis Section and stored on the Alaska Local and Regional Information (ALARI) site. In this archived version, a web scrape was performed from the ALARI site with the help of R's 'rvest' package. The .html code on the ALARI site was inspected and certain codes were targeted to generate correct web URLs for each location's data on worker characteristics, tax revenue, and industries. The data were then copied from the contents of these URLs and stored into three separate datasets; one each for worker characteristics, tax revenue, and industries. The purpose of this project is to compile all separate records for each unique documented location within Alaska into one dataset. Three records for Alaskan locations were of interest: tax revenue, industry information, and worker characteristics. In all, the three datasets are intended for inference into the nature of the Alaskan labor force from 2001 to 2016.
DOI: 10.7910/dvn/ywzbuj/5ww2tn
title: Russia_TroopWithdrawal.tab

description: :unav
DOI: 10.7910/dvn/ywzbuj/dsxqqn
title: Russia_Sanctions.do

description: :unav
DOI: 10.7910/dvn/ywzbuj/f4hpug
title: China_DemilitarizationAgreement.do

description: :unav
DOI: 10.7910/dvn/ywzbuj/kit6nk
title: readme.txt

description: :unav
DOI: 10.7910/dvn/ywzbuj/qixd19
title: MattesWeeks_Codebook.pdf

description: :unav
DOI: 10.15468/vzsq52
title: Mozambique Endemic and Near-Endemic Red Listed Plant Species

description: In February 2018 the Southern African Plant Specialist Group (SASPG) under the IUCN Species Survival Commission (SSC) met in Maputo to assess conservation status of about 100 plant species. The group focused on the endemic and near-endemic plants of Mozambique. The SAPSG brings together institutions including the two National herbaria in Mozambique (LMA and LMU), the South African National Biodiversity Institute (SANBI), the Royal Botanic Gardens, Kew (K) as well as independent specialists. The assessments are now being independently reviewed and thereafter they will be published on the IUCN web page. These assessments will inform conservation planning, development planning as well as to inform consultants conducting environmental impact assessments.
DOI: 10.25606/surf.636f736d6f67-696
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-049)

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 049 of the 512³ resolution collection.
DOI: 10.25606/surf.636f736d6f67-641
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-766)

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 766 of the 2048³ resolution collection.
DOI: 10.25606/surf.636f736d6f67-648
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-001)

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 001 of the 512³ resolution collection.
DOI: 10.25606/surf.636f736d6f67-695
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (512-048)

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 048 of the 512³ resolution collection.
DOI: 10.15129/7bf114fc-a3ce-4036-ae84-54b6c0ae7131
title: Data for: Binary Sintering of Polymeric Powder

description: Results of numerical simulations and hot stage microscopy of binary sintering of polymeric powder grains
DOI: 10.15468/2gbkf0
title: Checklist derived from occurrence data published on animalia on GBIF site

description: Occurrence data were collected throughout Benin and published on GBIF site. The datasets were then downloaded and the checklist extracted. It therefore cover the whole list of species published up to date on GBIF site
DOI: 10.5066/f7416wbq
title: Host Feeding Ecology and Trophic Position Significantly influence Isotopic discrimination between a Generalist Ectoparasite and its hosts: Implications for parasite host trophic studies

description: Despite being one of the most prevalent forms of consumerism in ecological communities, parasitism has largely been excluded from food-web models. Stable isotope analysis of consumers and their diets has been widely used in the study of food-webs for decades. However, the amount of information regarding parasite stable isotope ecology is limited, restricting the ability of ecologists to use stable isotope analysis to study parasites in food-webs. This study took advantage of distinct differences in the feeding ecology and trophic position of different species of fish known to host the same common micropredatory gnathiid isopod, to study the effects of host stable isotope ecology on that of the associated micropredator. Blood engorged juvenile gnathiids were in most cases indistinguishable from their hosts' blood, but significant isotope discrimination was observed for adults. Adult males were generally lower in delta-13C and delta-15N than host blood whereas host specific isotopic discrimination for females varied among the different host species. Model predictions indicated that there is a significant effect of host blood isotope ratios on the rate of stable carbon and nitrogen isotopic discrimination between gnathiids' host blood. As such, general differences in the feeding ecology and trophic positions of the different host species were reflected in their associated gnathiids, indicating that stable isotope analysis of wild caught gnathiids can provide significant details concerning previous hosts. The results present herein have significant implications for how stable isotopes may be used as a tool to study the trophic dynamics and feeding ecology of gnathiids.
DOI: 10.5066/p9srshv2
title: Molecular and morphological data on two species complexes in the freshwater mussel genus Cyclonaias

description: We examined species boundaries within an imperiled group of freshwater mussels in the genus Cyclonaias (Bivalvia: Unionidae) using morphometrics, molecular phylogenetics, and multispecies coalescent models to help guide pending conservation assessments and legislative decisions. Congruence across all lines of evidence indicated that current taxonomy overestimates diversity in the C. pustulosa species complex, while underestimating diversity in the C. petrina species complex. Here we provide all molecular, morphological, and collection information collected and analyzed in our investigation.
DOI: 10.5281/zenodo.1320312
title: EU Pesticide monitoring data 2016

description: The file presents the results of the 2016 EU pesticide monitoring activities of EU Member States, Iceland and Norway.
description: EU; en; xls; pesticides.mrl@efsa.europa.eu
DOI: 10.7910/dvn/0tjnt4
title: Morphological Characterization of Adansonia digitata fruits, 2016

description: This dataset was moved to: https://doi.org/10.34725/DVN/0TJNT4Adansonia digitata fruit characterization
DOI: 10.7910/dvn/0tjnt4/gcpala
title: Adansonia_digitata.jpg

description: :unav
DOI: 10.7910/dvn/0tjnt4/l6qhoy
title: Adansonia_digitata Fruit_characterization_dataverse_Genesys.xlsx

description: :unav
DOI: 10.7910/dvn/twqvda/jnv0iq
title: Sclerocarya birrea_evaluation.xls

description: :unav
DOI: 10.7910/dvn/xjjbb2
title: Morphological Characterization of Adansonia digitata Seed, 2016

description: This dataset was moved to: https://doi.org/10.34725/DVN/XJJBB2Adansonia digitata seed characterization
DOI: 10.7910/dvn/xjjbb2/p2fsst
title: Adansonia_digitata.jpg

description: Fruits, seeds and seedlings
DOI: 10.7910/dvn/xjjbb2/zr2ocw
title: ICRAF_Genebank_Adansonia_seed_characterisation_dataverse_genesys.xlsx

description: :unav
DOI: 10.5066/p9stbz0t
title: USGS Menlo Park Vertebrate Cenozoic Paleontology Collection

description: Data is primarily type fossils from the USGS Menlo Park vertebrate Cenozioc Paleontology Collection created and maintained by U.S. Geological Survey (USGS). Data was collected by paleontologist Charles A. Repenning during his forty years of service within the USGS Paleontology And Stratigraphy Branch. His catalog was converted into digital form, Excel and Filemaker Pro database. The Catalog is 516 fossil localities. His supplementary data has been added whenever possible - sources field map locality points, E&R files with enhanced faunal lists, as well as formal publications. For the complete traditional dataset, please contact Kevin Mckinney (kcmckinney@usgs.gov) and/or Kathy Hollis (HollisK@si.edu)
DOI: 10.5063/f1g44nh8
title: State of Alaska's Salmon and People Regional Boundaries

description: This dataset depicts the boundaries of the State of Alaska's Salmon and People (SASAP) regions. The SASAP region boundaries were updated in 2017 to better reflect HUC 8 watershed boundaries and to repair gaps, overlaps, and other topological errors.
DOI: 10.5066/p9dwv93u
title: Novel protocol for moose DNA extraction from Tempus blood tube supernatant following RNA extraction

description: Data were collected to validate the use of supernatant from the isolation of RNA from Tempus blood RNA tubes to obtain genomic DNA in the associated blood sample from moose. Data represent the metrics measured to validate the novel technique for isolating DNA from the supernatant of an RNA isolation protocol using blood collected into Tempus blood RNA tubes.