cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.14457/msu.res.2019.24
title: Phytochemical Screening, Antioxidant, and alpha-Glucosidase Inhibitory Activities of Different Solvent Extracts from Leersia hexandra and Elephantopus scaber

description: The aim of this research was to determine on phytochemical screening, antioxidant and alpha glucosidase inhibitory activities of Leersia hexandra and Elephantopus scaber by using different solvent extractions. Both plants (1:1
description: w:w) of recipe were extracted using by different solvents including aqueous (ALE) and 80% ethanol (ELE). Phytochemical screening was determined on total phenolic (TPC) and flavonoid (TFC) contents in plants. The antioxidant activities were determined by, 2,2-diphenyl-1- picrylhydrazy (DPPH) radical scavenging and 2,2-azinobis(3-ethylbenzothiazoline-6-sulphonate) (ABTS+ ) assay. The -glucosidase inhibitory assay was evaluated on glucose transferase mechanism. This experimental study found that the recipe showed high among of total phenolic and flavonoid contents especially ELE (40.024?0.952 mgGE/gExt and 0.072?0.001 mgQE/gExt,). The ELE (IC50 = 0.082?0.0025 mg/mL) was significantly exerted on free radical scavenging activity higher than ALE (IC50 = 0.122?0.0033 mg/mL). ABTS+ radical scavenging activity, the ELE (IC50 = 0.0048?0.00018 mg/mL) was significantly stronger than Trolox (IC50 = 0.0086?0.00063 mg/mL), known as standard substances. ?-glucosidase inhibitory activity, ALE (IC50 = 0.022?0.001 mg/mL) and ELE (IC50 = 0.098?0.002 mg/mL) were significantly more effect in inhibited ?-glucosidase enzyme than acarbose (IC50 =1.054?0.113 mg/mL), known anti-diabetic drug. The recipe has been having the phenolic and flavonoid contents which chemical substances were known as anti-oxidation and anti-diabetic property, Pharmaceutical activities were showed on antioxidant and ?-glucosidase inhibitory activities. Further, also chemical compositions, major active compound(s) and in vivo were clarified in next study.
DOI: 10.14457/msu.res.2019.25
title: Plant Diversity in Burapha University, Sa Kaeo Campus

description: Plant diversity in Burapha University, Sa Kaeo campus was investigated from June 2016June 2019. Field expedition and specimen collection was done and deposited at the herbarium of the Faculty of Agricultural Technology. 400 plant species from 271 genera 98 families were identified. Three species were pteridophytes, one species was gymnosperm, and 396 species were angiosperms. Flowering plants were categorized as Magnoliids 7 species in 7 genera 3 families, Monocots 106 species in 58 genera 22 families and Eudicots 283 species in 201 genera 69 families. Fabaceae has the greatest number of species among those flowering plant families.
DOI: 10.14457/msu.res.2019.26
title: Parasitic Infection in Common Lowland Frog (Hoplobatrachus rugulosus Wiegmann) and Disease Treatment

description: Parasitic infection in common lowland frog (Hoplobatrachus rugulosus Wiegmann) in Maha Sarakham and Roi-et Provinces was studied. The samples of the present study were collected from 3 stages of frog (Tadpole, young and adult frog), totally 833 frogs. The results revealed that all stages were affected by parasites throughout the year, in which 91.72% evidently. Both ectoparasite and endoparasite were found to affect the frogs at 9.89 and 90.11%, respectively. The 2 genera of ectoparasite, belonging to ciliate protozoa including Epistylis and Acineta, while endoparasite especially intestinal parasite found 2 genera of ciliate protozoa including Opalina and Balantidium and 4 genera of parasitic rotifer including Monostyla, Lecane, Philodina and Bracheonus. The finding shows that Opalina and Balantidium were the highest prevalence and abundance in each stage. Sodium chloride, potassium permanganate and formalin were used as chemicals to treat ectoparasite and applied to control the parasites in tadpole and young frog. The results showed that 0.5-1% of sodium chloride could reduce number of parasites, showing 3-4% of tadpole and young frog died within 1 hour. Potassium permanganate and formalin could be effective to control the parasite at 10 ppm and 50-60 ppm, while the concentration at 30-40 ppm showed high survival rate after treament. For endoparasite treatment, 3 internal anti-parasite drugs including Albendazole, Metronidazole and Piperazine were used to treat Opalina sp. and Balantidium in tadpole and young frog via oral administration. This study found that Metronidazole showed high effectiveness to treat the parasites whereas another drugs were not effective to treat parasite.
DOI: 10.5066/p91fl2gy
title: Suspended sediment, total nitrogen, and total phosphorus loads for Iroquois River near Foresman, Indiana, April 2015 to July 2018

description: This data release contains the calibration data set and R code used to create regression models for estimating daily loads of suspended sediment, total nitrogen, and total phosphorus at the Iroquois River near Foresman, Indiana streamgage (05524500). The USGS R software package, rloadest, was used to develop the regression models and estimate loads. The models were developed using discrete water-quality data and concurrent daily streamflow data measured/determined at the streamgage for the period April 2015 through July 2018. Also included in this data release is the input data set of daily streamflow data and the daily load output data sets that were produced by the regression models. Summary information for the model development for each constituent are included in this data release.
DOI: 10.5281/zenodo.2554877
title: Uganda Malaise trapping 2014–2015 Rhyssinae taxonomy data

description: This dataset contains the data and scripts of our paper on the taxonomy of African Rhyssinae. We collected rhyssines by Malaise trapping and hand-netting in tropical forest in Kibale National Park 2014–2015. The dataset contains data on the 456 rhyssines we caught and 13 other African specimens we examined, a table of diagnostic characters, and scripts for generating an identification key and automating the writing of species descriptions. It also contains images used to take measurements of the rhyssines. <br> The specimen data (<em>1 Specimen data</em>) and table of diagnostic characters (<em>Uganda Rhyssinae diagnosis characters.csv</em>) will usually be of the greatest interest.
description: Funded by the Finnish Cultural Foundation, Oskar Öflunds Stiftelse, the Helsinki Entomology Society and Waldemar von Frenckells Stiftelse
DOI: 10.5281/zenodo.2554876
title: Uganda Malaise trapping 2014–2015 Rhyssinae taxonomy data

description: This dataset contains the data and scripts of our paper on the taxonomy of African Rhyssinae. We collected rhyssines by Malaise trapping and hand-netting in tropical forest in Kibale National Park 2014–2015. The dataset contains data on the 456 rhyssines we caught and 13 other African specimens we examined, a table of diagnostic characters, and scripts for generating an identification key and automating the writing of species descriptions. It also contains images used to take measurements of the rhyssines. <br> The specimen data (<em>1 Specimen data</em>) and table of diagnostic characters (<em>Uganda Rhyssinae diagnosis characters.csv</em>) will usually be of the greatest interest.
description: Funded by the Finnish Cultural Foundation, Oskar Öflunds Stiftelse, the Helsinki Entomology Society and Waldemar von Frenckells Stiftelse
DOI: 10.21227/zd98-mt55
title: Real-world DNS dataset (2016)

description: · We captured ten days real-world DNS traffic from campus network comprising of 4000 hosts in peak load hours.
DOI: 10.25606/surf.578c6039-a7c441b5
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-069)

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 069 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-1faf0b2b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-150)

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 150 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-26b3abae
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-502)

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 502 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-53f8fb14
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-458)

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 458 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-87e13341
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-631)

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 631 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-3e848e8e
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-668)

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 668 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-b90ae391
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-602)

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 602 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-e541c81c
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-071)

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 071 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-6bf42138
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-681)

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 681 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-3665a76e
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-680)

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 680 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-682d8eaf
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-625)

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 625 of the 2048³ resolution collection.