cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.7910/dvn/scfl3l/lb7ppo
title: prq_fig4_5.tab

description: :unav
DOI: 10.7910/dvn/scfl3l/s9lpfg
title: prq_fig4_5.R

description: :unav
DOI: 10.7910/dvn/scfl3l/cjrwvl
title: prq_fig2_3.r

description: :unav
DOI: 10.7910/dvn/scfl3l/kwhghk
title: prq_fig1.tab

description: :unav
DOI: 10.25606/surf.578c6039-3e540164
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-151)

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 151 of the 2048³ resolution collection.
DOI: 10.7910/dvn/gxmoxs/be2tg2
title: TABLE1.do

description: :unav
DOI: 10.7910/dvn/gxmoxs/hdc0s2
title: TABLE3.do

description: :unav
DOI: 10.7910/dvn/gxmoxs/nhasov
title: TABLE2.do

description: :unav
DOI: 10.7910/dvn/gxmoxs/nibcrv
title: README.txt

description: :unav
DOI: 10.7910/dvn/gxmoxs/w0ybhp
title: TABLE1.tab

description: :unav
DOI: 10.7910/dvn/gxmoxs/yprrkf
title: TABLE2.tab

description: :unav
DOI: 10.7910/dvn/hvpvxh/uewjxz
title: Lucid pre-registration.pdf

description: :unav
DOI: 10.25606/surf.578c6039-b4106b40
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-555)

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 555 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3466110
title: Benchmarking algorithms for gene regulatory network inference from single-cell transcriptomic data

description: This repository contains input files from the synthetic, curated, and processed experimental single-cell gene expression datasets used in BEELINE.
DOI: 10.25606/surf.578c6039-5d77a092
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-562)

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 562 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-9f1ea183
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-064)

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 064 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-0c595caa
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-736)

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 736 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3465969
title: "Laser wakefield accelerator driven by the super-Gaussian laser beam in the focus" - Input files for the PIC simulations in the EPOCH Code

description: These are particle-in-cell simulation set-ups for the EPOCH code. The simulations show the super-Gaussian beam diffraction in free space and in plasma (LWFA acceleration). Coresponding publication is currently reviewed.
DOI: 10.5281/zenodo.3465970
title: "Laser wakefield accelerator driven by the super-Gaussian laser beam in the focus" - Input files for the PIC simulations in the EPOCH Code

description: These are particle-in-cell simulation set-ups for the EPOCH code. The simulations show the super-Gaussian beam diffraction in free space and in plasma (LWFA acceleration). Coresponding publication is currently reviewed.
DOI: 10.15468/cndfec
title: Description of a new species of the genus Bagauda (Heteroptera: Reduviidae: Emesinae) from Maharashtra State, India

description: This dataset contains the digitized treatments in Plazi based on the original journal article Ghate, Hemant V., Boyane, Swapnil S., Joshi, Nikhil U. (2019): Description of a new species of the genus Bagauda (Heteroptera: Reduviidae: Emesinae) from Maharashtra State, India. Zootaxa 4652 (3): 591-600, DOI: https://doi.org/10.11646/zootaxa.4652.3.14
DOI: 10.25606/surf.578c6039-b846240b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-205)

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 205 of the 2048³ resolution collection.
DOI: 10.15468/8ektwt
title: Taxonomic revision of the aequata - group of the subgenus Eucera s. str. (Hymenoptera, Apidae, Eucerini)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Dorchin, Achik (2019): Taxonomic revision of the aequata - group of the subgenus Eucera s. str. (Hymenoptera, Apidae, Eucerini). Zootaxa 4652 (3): 457-472, DOI: https://doi.org/10.11646/zootaxa.4652.3.3
DOI: 10.15468/yv26hm
title: Tropical sand-bubblers heading north? First discovery of Scopimera curtelsona Shen, 1936 (Crustacea: Decapoda: Dotillidae) populations in Hong Kong: possible range expansion from Hainan, China

description: This dataset contains the digitized treatments in Plazi based on the original journal article Hui, T. Y., Wong, Kingsley J. H. (2019): Tropical sand-bubblers heading north? First discovery of Scopimera curtelsona Shen, 1936 (Crustacea: Decapoda: Dotillidae) populations in Hong Kong: possible range expansion from Hainan, China. Zootaxa 4652 (3): 520-532, DOI: https://doi.org/10.11646/zootaxa.4652.3.8
DOI: 10.25606/surf.578c6039-cf99c3ad
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-501)

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 501 of the 2048³ resolution collection.
DOI: 10.25919/5d9277328afc2
title: Gravity fracturing simulation results

description: Simulation results for gravity hydraulic fracturing. The data is in an Excel spreadsheet with figures embedded.
DOI: 10.21227/03q7-2n91
title: Ruling Power Tautology: Error in Big Bang Theory

description: -If Ruling Power were able and willing to create Sun/Mars, he would do so. If Ruling Power were unable to create Sun/Mars, he would be incapable; if he were unwilling to create Sun/Mars, he would be malevolent. Ruling Power creates Sun/Mars. If Ruling Power exists, he is neither incapable nor malevolent. Therefore, Ruling Power exists. The World of PC can’t be created itself just from one factor light. I (programmer) die & consequently light (big bang) become useless.
DOI: 10.25606/surf.578c6039-1847614e
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-603)

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 603 of the 2048³ resolution collection.
DOI: 10.6073/pasta/ef23f8617d3db6c1ca3a3cdd4cc40853
title: Cone production of upper slope conifers in the Cascade Range of Oregon and Washington, 1959 to present

description: Seed supply is a key feature of tree population dynamics, and seed production may be indicative of environmental and biological drivers. This study examines cone production in upper-slope, true fir-hemlock forests of the Pacific Northwest, starting in 1959 to the present. Annual surveys of cone counts of Abies spp. (A. amabilis, A. concolor, A. grandis, A. lasiocarpa, A. magnifica, A. procera), Pinus spp. (P. engelmannii, P. lamberti, P. monticola), and Tsuga spp. (T mertsiana) have been conducted at sixty-one plots in 37 locations in nine national forests in Washington and Oregon (originally 10 national forests, but Mt. Baker and Snoqualimie were combined). At each site, a visual count is made of cone production in each of a number (20-30) trees in a stand of one tree species. At some plots, additional trees were added in the 1980s. Primary data include numbers of counts per tree per year, periodic measurements of tree diameter, and the names of the sites. These data illustrate the periodicity of cone production cycles, as well as longer trends associated with climate change and variability in the region.
DOI: 10.6073/pasta/2143c0c75491d2923e3302032ddca1f8
title: Cone production of upper slope conifers in the Cascade Range of Oregon and Washington, 1959 to present

description: Seed supply is a key feature of tree population dynamics, and seed production may be indicative of environmental and biological drivers. This study examines cone production in upper-slope, true fir-hemlock forests of the Pacific Northwest, starting in 1959 to the present. Annual surveys of cone counts of Abies spp. (A. amabilis, A. concolor, A. grandis, A. lasiocarpa, A. magnifica, A. procera), Pinus spp. (P. engelmannii, P. lamberti, P. monticola), and Tsuga spp. (T mertsiana) have been conducted at sixty-one plots in 37 locations in nine national forests in Washington and Oregon (originally 10 national forests, but Mt. Baker and Snoqualimie were combined). At each site, a visual count is made of cone production in each of a number (20-30) trees in a stand of one tree species. At some plots, additional trees were added in the 1980s. Primary data include numbers of counts per tree per year, periodic measurements of tree diameter, and the names of the sites. These data illustrate the periodicity of cone production cycles, as well as longer trends associated with climate change and variability in the region.
DOI: 10.1285/i24995835v2019n10p1
title: Frontespizio e pagine iniziali
DOI: 10.25606/surf.578c6039-cdc82bd1
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-453)

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 453 of the 2048³ resolution collection.
DOI: 10.1285/i24995835v2019n10p4
title: Indice
DOI: 10.1285/i24995835v2019n10p5
title: Editoriale
DOI: 10.15468/pqggbj
title: A new species of Crocidosema Zeller (Lepidoptera, Tortricidae) from the Andes of northern Chile

description: This dataset contains the digitized treatments in Plazi based on the original journal article Vargas, Hector A. (2019): A new species of Crocidosema Zeller (Lepidoptera, Tortricidae) from the Andes of northern Chile. Nota Lepidopterologica 42 (2): 129-136, DOI: http://dx.doi.org/10.3897/nl.42.38341, URL: http://dx.doi.org/10.3897/nl.42.38341
DOI: 10.15468/shn2lp
title: Phylogenetic differentiation and taxonomic consequences in the Saurodactylus brosseti species complex (Squamata: Sphaerodactylidae), with description of four new species

description: This dataset contains the digitized treatments in Plazi based on the original journal article Javanmardi, Soheila, Vogler, Sven, Joger, Ulrich (2019): Phylogenetic differentiation and taxonomic consequences in the Saurodactylus brosseti species complex (Squamata: Sphaerodactylidae), with description of four new species. Zootaxa 4674 (4): 401-425, DOI: http://doi.org/10.5281/zenodo.3465002
DOI: 10.25606/surf.578c6039-34db6d7c
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-478)

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 478 of the 2048³ resolution collection.
DOI: 10.1285/i24995835v2019n10p8
title: Sezione Didattica