cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.14457/msu.res.2019.10
title: Variation of Inulin Content inBanana Peels at Different Maturity Stages

description: Banana is an inexpensive source of vitamin and dietary fiber. The objective of the present study was to determine inulin content of Kluai Nam Thai (Musa acuminata) peel at different maturity stages. The experiment was conducted at the experimental farm of the Faculty of Agricultural Technology, Burapha University, Sakaeo Campus, Sakaeo, Thailand. Banana peels at four maturity stages (light three-quarters, light full three-quarters, full three-quarters and full) were used and arranged in a completely randomized design with three replications. Data were recorded for number of fruits/finger, peel fresh weight/finger, peel dry weight/finger, total fruit (pulp and peel) fresh weight, peel fresh weight/fruit, percentage of peel fresh weight/fruit, total fruit dry weight, peel dry weight/fruit, percentage of peel dry weight/fruit and inulin content. Maturity stages were significantly different (P &lt; 0.05) for totalfruit fresh and dry weight, percentage of peel fresh and dry weight/fruit and inulin content. Banana peel harvested at light three-quartersstage had the highest inulin content of 0.57% dry weight, whereas banana peel at light full three-quarters stage, full three-quartersstage and full stage had inulin content of 0.39, 0.35 and 0.32% dry weight, respectively. Banana peels at light three-quarters had the highest of percentage of peel fresh and dry weight/fruit of 51.4 and 45.3%, respectively. The results indicated that banana peel at light three-quarters stage had a significant amount of inulin (0.57% dry weight) for use as an alternative source of a raw material for functional food producers and animal feed.
DOI: 10.14457/msu.res.2019.17
title: Screening and Identification of Bacteria that Produce Chitinase Enzymes from Soil in Na Si Nuan Forest, Maha Sarakham, Thailand

description: This research aimed to screen the bacteria that produce chitinase enzymes from soil in Na Si Nuan forest located at Kantarawichai District, Maha Sarakham Province, Thailand. The conservation project in response to Plant Genetic Conservation Project under the Royal initiative of Her Royal Highness Princess Maha Chakri Sirindhorn has occupied the community forest of 19.2 ha in this study. Isolation of bacteria was performed from soil on chitin agar. Our results were found two isolates of chitinase-positive bacterial strains. The isolate of 3.2 CT1 was showed the highest of halo: colony ratios with 4.5. The morphology isolate of 3.2 CT1 is gram negative, and rod shaped. The optimum temperature for chitinase activity was 40 ?C with enzyme activity of 0.40 ? 0.01 U/mL and given a specific enzyme activity of 0.49 ? 0.01 U/mg. protein. The optimum pH was 6.0 with activity of 0.70 ? 0.01 U /mL. This chitinase may be used for agricultural purposes, such as plant pathogen inhibition and as insecticide for insect pest control.
DOI: 10.14457/msu.res.2019.8
title: Effect of Acid-Alkaline Pretreatment on Reducing Sugar Yield and Lignocellulosic Compositions of Rice (Oryza sativa L.) Residues

description: Rice residues (RRs) are classified as an agricultural waste, which refer to rice bran, rice husk and rice straw. In the present study, the chemical compositions of each RRs were analyzed. The determination of lignocellulosic compositions of rice bran was revealed and represented as an outstanding biomass that consisted of high cellulose and low hemicellulose and lignin. While the compositions of rice husk and rice straw was obviously contrasted from rice bran. Furthermore, the acid-alkaline pretreatment of RRs under autoclaving at 121 ?C for 90 min was investigated for determination of the reducing sugar yield and lignocellulosic compositions change. The study consists of four pretreatment conditions for disruption of RRs structure with different solutions, including the condition (1): 1%(v/v) H2SO4, (2): 1%(w/v) NaOH, (3): 1%(w/v) NaOH following by 1%(v/v) H2SO4, and (4): distilled water (control). The result showed that the acid pretreatment with 1%(v/v) H2SO4 solution (condition 1) was the best condition that provided the highest reducing sugar yield from all RRs kinds. The dilute acid and alkaline pretreatment of RRs under 121 ?C for 90 min illustrated a clearly variation of its lignocellulosic compositions. The acid pretreated rice bran showed that cellulose reduction which correlated with concentration of reducing sugar yield released in the same experiment condition
DOI: 10.14457/msu.res.2019.9
title: Mixture of Parawood Sawdust and Dried Napier Grass as a Substrate on Lentinus squarrusulus Mont. Cultivatio

description: Lentinus squarrosulus Mont. , or Hed Khon Khao, is a commercial mushroom in Thailand. Parawood sawdust is a main substrate for bag mushroom cultivation but it is quite expensive. Napier grass is a fast growing grass which can be used as an alternative source for mushroom cultivation. This study aims to investigate the effect of parawood sawdust and Napier grass mixture on mycelial growth and fruiting body production of L. squarrosulus. Parawood sawdust and Napier grass mixtures in the ratio of 100:0(T1), 90:10(T2), 80:20(T3), 70:30(T4) and 50:50(T5) were used as a main substrate in bag cultivation. C/N ratio, substrate pH, mycelial growth, fruiting body and biological efficiency (BE) were determined. The results showed that all substrates had pH value and C/N ratio in the range of 6.23-6.80 and 107.56- 160.57, respectively. Mycelial running on T1 to T4 substrates was faster than T5 substrate. T2 substrate gave higher fresh fruiting body weight (59.42?16.14 g/bag) than T1 (54.53 ? 10.67 g/bag), T3 (27.17 ? 11.98 g/bag), T4 (22.33 ? 13.70 g/bag) and T5 (4.14 ? 4.05 g/bag), respectively. In addition, there was no significant difference between BE of T1 (12.36?2.42%) and T2 (13.47?3.66%). These results suggested that 10% dried Napier grass mixture (T2) could be used to culture L. squarrosulus the same as parawood sawdust (T1) whereas higher amount of dried Napier grass resulted in significant decreasing in mushroom production. In conclusion, dried Napier grass can be used to mix with parawood sawdust for L. squarrosulus cultivation leading to the decrease of parawood sawdust usage
DOI: 10.25606/surf.578c6039-77c9749b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-456)

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 456 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-e8015f2a
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-628)

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 628 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-f2277844
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-528)

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 528 of the 2048³ resolution collection.
DOI: 10.26050/wdcc/topoi-cs_cosmo-clm
title: TOPOI-CS_COSMO-CLM

description: Project: TOPOI-CLIMATE-SIMULATION - It is well known that climate conditions affect human living conditions. Prominent examples are water availability or heat spells like in the European summer in 2003. The project addressed the question how climate may have changed in the past 6000 years and thus affected living conditions. As an example, in the last millennia, changes in orbital parameters such as the shape of the elliptical path of the earth around the sun were a source of climate change. However, due to the sparseness of regional reconstructions of climatic variables such as temperature and precipitation, climate models are a useful tool for analyzing possible changes. In the project, state-of-the-art climate models were employed to simulate climate for the period from 6000 years ago until the present. Orbital parameters, greenhouse gases and solar activity are viewed as external forces. Simulations were carried out with low-resolution coupled ocean-atmosphere general circulation models and high-resolution atmosphere models. The research data of the last 6000 years were produced using global and regional climate simulations. Climate models of the present and future climate are applied as background for the simulations. The global climate was simulated in a high spatial resolution by using the so-called time slice approach for chosen periods in the past 6000 years. The subsequent refinement with the regional model allows a gain of information in Europe. Further Information: https://www.topoi.org/ Summary: High-resolution simulations of the palaeoclimate are carried out throughout Europe. A set of climate simulations will be performed, based on the so-called time slicing technique. The simulations are performed with the state-of-the-art regional climate model COSMO-CLM (cosmo_4.8_clm19) at a horizontal resolution of 0.44° longitude and 40 vertical levels. The COSMO-CLM is a non-hydrostatic RCM with rotated geographical coordinates and a terrain following height coordinate (Rockel et al., 2008), developed by the German Weather Service (DWD) of the COSMO model (Doms and Schättler, 2003). The ECHAM5 output is used as a boundary data set for the dynamic downscaling approach. Detailed information on the model set-up can be found in Russo and Cubasch (2016). Russo, E. and Cubasch, U.: Mid-to-late Holocene temperature evolution and atmospheric dynamics over Europe in regional model simulations, Clim. Past, 12, 1645-1662, https://doi.org/10.5194/cp-12-1645-2016, 2016.
DOI: 10.7910/dvn/mv25mz/77sckm
title: f_variety_mechanisms.do

description: :unav
DOI: 10.7910/dvn/mv25mz/cp38au
title: read_in_TUS.do

description: :unav
DOI: 10.7910/dvn/mv25mz/gnspp9
title: Round61.tar

description: :unav
DOI: 10.7910/dvn/mv25mz/j26of4
title: nic04_98.tab

description: :unav
DOI: 10.7910/dvn/mv25mz/stsjb7
title: Round55.tar

description: :unav
DOI: 10.7910/dvn/mv25mz/vm4oru
title: f_variety_districts.do

description: :unav
DOI: 10.7910/dvn/mv25mz/xk2653
title: Round43.tar

description: :unav
DOI: 10.7910/dvn/mv25mz/zqrs5a
title: README.pdf

description: READ ME
DOI: 10.21227/0hnv-5h95
title: Forecasting Box-Office Revenue with Random Forest Algorithm – Evidence from Taiwanese Film Market

description: Data are used for the paper titled "Box-Office Forecasting Using the Random Forest Algorithm: Evidence from the Taiwanese Film Market"
DOI: 10.21227/cc49-8k21
title: Forecasting Box-Office Revenue with Random Forest Algorithm – Evidence from Taiwanese Film Market

description: Data are used for the paper titled "Box-Office Forecasting Using the Random Forest Algorithm: Evidence from the Taiwanese Film Market"
DOI: 10.7910/dvn/mv25mz/alrkmo
title: Round66.tar

description: :unav
DOI: 10.7910/dvn/mv25mz/nanslf
title: common_consumption_NSS.do

description: :unav
DOI: 10.7910/dvn/mv25mz/odqhgm
title: f_boostrap_se.do

description: :unav
DOI: 10.7910/dvn/mv25mz/oiuotk
title: f_elasticity_final.do

description: :unav
DOI: 10.7910/dvn/mv25mz/tz00v7
title: nic70_87_2digit.tab

description: :unav
DOI: 10.7910/dvn/mv25mz/uq1bmm
title: nss61_nm61.tab

description: :unav
DOI: 10.7910/dvn/mv25mz/z5a5vw
title: district_conversion.tab

description: :unav
DOI: 10.5281/zenodo.3469654
title: Observed and predicted variables of in vitro methanogenesis

description: This data sets shows the dynamics of <em>in vitro </em>methanogenesis by three gut archaea: <em>Methanobrevibacter smithii</em>, <em>Methanobrevibacter ruminantium</em> and <em>Methanobacterium formicium</em>. Experimental data are compared against variables predicted by a kinetic model.
DOI: 10.5281/zenodo.3469655
title: Observed and predicted variables of in vitro methanogenesis

description: This data sets shows the dynamics of <em>in vitro </em>methanogenesis by three gut archaea: <em>Methanobrevibacter smithii</em>, <em>Methanobrevibacter ruminantium</em> and <em>Methanobacterium formicium</em>. Experimental data are compared against variables predicted by a kinetic model.
DOI: 10.7910/dvn/mv25mz/1nkdsk
title: districts.tar

description: :unav
DOI: 10.7910/dvn/mv25mz/3lq0wi
title: nss43_nm61.tab

description: :unav
DOI: 10.7910/dvn/mv25mz/7xvfp0
title: Round38.tar

description: :unav
DOI: 10.7910/dvn/mv25mz/czhbab
title: f_stylizedfacts.do

description: :unav
DOI: 10.7910/dvn/mv25mz/lo7r0o
title: Other.tar

description: :unav
DOI: 10.7910/dvn/mv25mz/mevzzq
title: nss66_nm61.tab

description: :unav
DOI: 10.7910/dvn/mv25mz/uxmnlr
title: nss55_nm61.tab

description: :unav
DOI: 10.7910/dvn/mv25mz/wcpwcr
title: nic87_87_2digit.tab

description: :unav
DOI: 10.7910/dvn/mv25mz/hbee6x
title: TUS.tar

description: :unav
DOI: 10.7910/dvn/mv25mz/hzxmxm
title: nic98_87.tab

description: :unav
DOI: 10.7910/dvn/mv25mz/mo9fkj
title: read_in_NSS_sch1.do

description: :unav
DOI: 10.7910/dvn/mv25mz/nfzecc
title: common_hh_NSS_sch10.do

description: :unav
DOI: 10.7910/dvn/mv25mz/nowpag
title: common_hh_NSS_sch1.do

description: :unav
DOI: 10.7910/dvn/mv25mz/tegbto
title: f_parameters.do

description: :unav
DOI: 10.7910/dvn/mv25mz/xixbhy
title: prices_indexes_final.do

description: :unav
DOI: 10.7910/dvn/mv25mz/z7l5iw
title: nco_cross.tab

description: :unav
DOI: 10.7910/dvn/mv25mz/zamq2w
title: f_ceswelfare_overtime.do

description: :unav
DOI: 10.7910/dvn/mv25mz/zzwj1e
title: f_other.do

description: :unav
DOI: 10.15468/udr5tt
title: Two Hexapleomera species from Japan, with a new species description and discussion of phylogenetic relationships within Hexapleomera (Crustacea: Tanaidacea)

description: This dataset contains the digitized treatments in Plazi based on the original journal article Tanabe, Yuki, Kakui, Keiichi (2019): Two Hexapleomera species from Japan, with a new species description and discussion of phylogenetic relationships within Hexapleomera (Crustacea: Tanaidacea). Zootaxa 4648 (2): 318-336, DOI: https://doi.org/10.11646/zootaxa.4648.2.7
DOI: 10.25606/surf.578c6039-b9adad3e
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-695)

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 695 of the 2048³ resolution collection.
DOI: 10.7910/dvn/mv25mz/nfrake
title: f_ceswelfare_ru.do

description: :unav
DOI: 10.25606/surf.578c6039-a13df244
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-500)

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 500 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-ba73ccef
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-481)

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 481 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-e160b466
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-207)

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 207 of the 2048³ resolution collection.