cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25606/surf.578c6039-92d39715
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-155)

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 155 of the 2048³ resolution collection.
DOI: 10.7910/dvn/wan2gi/8ucq7d
title: part 1_educ_health(20190928).do

description: do command
DOI: 10.7910/dvn/wan2gi/cpmbo0
title: part 1 20190928.smcl

description: :unav
DOI: 10.7910/dvn/wan2gi/vsiidl
title: Part2 Results(20181220).smcl

description: :unav
DOI: 10.7910/dvn/wan2gi/07czgu
title: StudyList(20190928).xls

description: :unav
DOI: 10.7910/dvn/wan2gi/m1n12p
title: Part2 _educ_health(20190928).do

description: :unav
DOI: 10.7910/dvn/wan2gi/dnvtqy
title: part 2 20190928.smcl

description: :unav
DOI: 10.14457/cu.the.2006.1711
title: Adsorption of polycyclic aromatic hydrocarbons from synthetic wastewater by organoclays

description: The effect of the amount of organic cation on the characteristics and PAHs sorption of organoclays were investigated. Dodecylpyridinium chloride (DPC), naphthalene, and phenanthrene were selected to represent organic cation and PAHs, respectively. Eight organoclays were synthesized by exchanging the inorganic cations on the clay surfaces with DPC at loading level of 0.25-2.00 times the cation exchanged capacity (CEC). Organoclays were characterized by Accelerated surface area and porosimetry system, X-ray diffraction (XRD), and Fourier transform infrared spectroscopy (FTIR). The adsorption of DPC noto clay and the sorption of PAHs from aqueous solution by organoclays were studied by batch experiment. The results showed that DPC could be adsorbed ontto clay in excess of the CEC of clay, The characteristics (e. g., the BET surface area, the interlayer spacing, and structural features) of organoclays and sorption capacities of PAHs noto organoclays depended on the amount of DPC applied. The sorption isotherms of PAHs onto organoclays were linear, indicated that partition was the main mechanism of PAHs sorption by organoclyas. The sorption capacities of PAHs increased with the amount of DPC increased from 0.25 to 1.25 times the CEC. When the amount of DPC increased from 1.25 to 2.00 times the CEC, the sorption capacities were not different. The distribution coefficient (K ) of naphthalene ranged from 0.151 to 1.675 L/g and phenanthrene from 0.426 to 36.184 L/g.
DOI: 10.21227/zbp2-zq39
title: MultiModal dataset from Instragram

description: We collect almost 248,166 public microblogsaccording to selected 97 hashtags of "Top 100" on Instagram.The final collection contains 56861 microblogswhich include both text and image, called MultiModaldata from Instagram (MM-INS). We filter duplicate hashtagsin one sample and drop out those microblogs withouttexts.
DOI: 10.5281/zenodo.3457236
title: British English Cued Speech--interspeech 2019

description: The first British English Cued Speech (CS) dataset is recorded for this work in Cued Speech UK association without using any artificial mark, and it is also the first one especially for the continuous recognition in British English CS. A professional CS interpreter (with no hearing impairment) is asked to simultaneously utter and encode a set of 97 British English sentences (e.g., I feel it is a time to move to a new chapter in my career). 97 sentences are chosen from the uploaded text file. There are totally 907 monophthongs and 138 diphthongs in the dataset. Color video images of the interpreter’s upper body are recorded at 25 fps, with a spatial resolution of 720x1280. If you use this dataset, please cite the following: <pre>@inproceedings{Liu2019, author={Li Liu and Jianze Li and Gang Feng and Xiao-Ping Zhang}, title={{Automatic Detection of the Temporal Segmentation of Hand Movements in British English Cued Speech}}, year=2019, booktitle={Proc. Interspeech 2019}, pages={2285--2289}, doi={10.21437/Interspeech.2019-2353}, url={http://dx.doi.org/10.21437/Interspeech.2019-2353} }</pre>
description: The authors would like to thank the professional CS teacher Cate Calder from Cued Speech UK association for her time spent on the British English CS dataset recording.
description: {"references": ["interspeech 2019"]}
DOI: 10.5281/zenodo.3457237
title: British English Cued Speech--interspeech 2019

description: The first British English CS dataset is recorded for this work in Cued Speech UK association without using any artificial mark, and it is also the first one especially for the continuous recognition in British English CS. A professional CS interpreter (with no hearing impairment) is asked to simultaneously utter and encode a set of 97 British English sentences (e.g., I feel it is a time to move to a new chapter in my career). There are totally 907 monophthongs and 138 diphthongs in the dataset. Color video images of the interpreter’s upper body are recorded at 25 fps, with a spatial resolution of 720x1280. If you use this dataset, please cite the following: <pre>@inproceedings{Liu2019, author={Li Liu and Jianze Li and Gang Feng and Xiao-Ping Zhang}, title={{Automatic Detection of the Temporal Segmentation of Hand Movements in British English Cued Speech}}, year=2019, booktitle={Proc. Interspeech 2019}, pages={2285--2289}, doi={10.21437/Interspeech.2019-2353}, url={http://dx.doi.org/10.21437/Interspeech.2019-2353} }</pre>
description: {"references": ["interspeech 2019"]}
DOI: 10.5281/zenodo.3464319
title: Muti-type Aircraft of Remote Sensing Images: MTARSI

description: MTARSI has a total of 9'385 remote sensing images acquired from Google Earth satellite imagery and manually expanded, including 20~different types of aircraft covering 36~airports.<br> The new data set is made up of the following 20 aircraft types: B-1, B-2, B-29, B-52, Boeing, C-130, C-135, C-17, C-5, E-3, F-16, F-22, KC-10, C-21, U-2, A-10, A-26, P-63, T-6, T-43.<br> All the sample images are carefully labeled by seven specialists in the field of remote sensing images interpretation. <br> Each image contains one and only one complete aircraft.
DOI: 10.14457/cu.the.2006.1712
title: Copolymerization of ethylene/1-octene with boron-modified MCM-41-supported zirconocene catalyst

description: In this research, effect of boron modification on the catalytic activity of the ethylene/1-octene copolymerization with rac-ethylenebis (indeny) zirconium dichloride [rac-Et(Ind) )[subscript 2]ZrCl[subscript 2]] catalyst system using MCM-41 with different pore sizes as support was studied. The properties of polymer produced were also investigated. The MCM-41 having small pore system with boron (B) modification gave higher activity than that of the MCM-41 having large pore at the same condition. This was attributed to the dispersion and interaction between [Al][subscript dMMAO] and supports as proven by EDX and TGA techniques. It was found that small pore system exhibited higher amounts of [Al][subscript dMMAO] than the large pore system. The highest activity was observed from MCM-41 with 1% wt of B modification. The molecular weight of polymer obtained from this supported system was higher than for the copolymer normally produced from the corresponding homogeneous system. For the small pore system, the inhibition of chain transfer reaction during polymerization apparently occurred upon the B modification indicating higher MW of polymer. On the contrary for the large pore system, it exhibited lower MW of polymer with B modification. For both the MCM-41 small pore and large pore (especially at low content of B) system, it was also suggested that B modification rendered more uniform catalytic sites leading to narrow MWD of polymer observed. There was no significant change in the polymer molecular structure by means of [superscript 13]C NMR. It can be also stated that the addition of B into MCM-41 support affected the insertion of 1-octene, T[subscript m] and crystallinity of polymer produced.
DOI: 10.25606/surf.578c6039-1babab00
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-152)

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 152 of the 2048³ resolution collection.
DOI: 10.21227/jz0h-0q26
title: Agent3 Data

description: A synthetic dataset supporting a submission.
DOI: 10.21227/khyr-k082
title: Agent3 Data

description: A synthetic dataset supporting a submission.
DOI: 10.14457/cu.the.2006.1713
title: Cosmetic actives from rice husk

description: In this work, rice husks from five strains of rice cultivar Chai-nat 1 (CN), Look Daeng Pattani (LD), Leb Nok Pattani (LN), Go Ko 1 (GK) and Jasmine (JM), were extracted and screened for biological activities including anti-tyrosinase, antioxidant and UV screening activity. The dichlormethane and ethylacetate crude extracts of CN possess potent radical scavenging effect, moderate inhibition effect toward tyrosinase, and some UV (290-400 nm) absorption property. The active compounds in CN crude extract were isolated by chromatographic techniques and identified as dipentyl phthalate (0.16% w/w yield) and 4-hydroxy-3-methoxycinnamaldehyde (0.22% w/w yield) by [superscript1]H and [superscript13]C NMR, IR and mass spectroscopy. Dipentyl phthalate showed inhibitory effect toward typrosinase while 4-hydroxy-3-methoxycinnamaldehyde exhibited strong antioxidant activity and UV screening activity. Anti-tyrosinase activity of dipentyl phthalate at concentration of 750 mug/ml was equivalent to that of reference kojic acid at concentration of 30 mug/ml. A 4-hydroxy-3methoxycinnamaldehyde possessed similar 2,2-diphenyl-l-picrylhydrazyl (DPPH) radical scavenging activity to that of the reference butylated hydroxytoluene (BHT). The IC[subscript50] values were 69.49 and 42.3 ug/ml for 4-hydroxy-3methoxycinnamaldehyde and BHT respectively. In addition, 4-hydroxy-3-methoxycinnamaldehyde possessed UVA absorption property with 339 nm and the molar absorptivity of 32,000 cm[superscript-1]M[superscript-1]. Furthermore, alkene and anthracene were also found in CN extract.
DOI: 10.17632/s9smyhnpvz.1
title: Data for: External photon radiation treatment for prostate cancer: uncomplicated and cancer-free control probability assessment of 36 plans

description: Tables list neutron and photon dose to peripheral organs in a prostate cancer treatment as well as second primary cancer risk (per 100 patients for age at exposure of 60 y) at each organ for all studied plans. The code is a matlab routine to compute photon peripheral doses.
DOI: 10.25606/surf.578c6039-92f1a52b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-559)

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 559 of the 2048³ resolution collection.
DOI: 10.5281/zenodo.3464212
title: British English Cued Speech--interspeech 2019

description: The first British English Cued Speech (CS) dataset is recorded for this work in Cued Speech UK association without using any artificial mark, and it is also the first one especially for the continuous recognition in British English CS. A professional CS interpreter (with no hearing impairment) is asked to simultaneously utter and encode a set of 97 British English sentences (e.g., I feel it is a time to move to a new chapter in my career). 97 sentences are chosen from the uploaded text file. There are totally 907 monophthongs and 138 diphthongs in the dataset. Color video images of the interpreter’s upper body are recorded at 25 fps, with a spatial resolution of 720x1280. If you use this dataset, please cite the following: <pre>@inproceedings{Liu2019, author={Li Liu and Jianze Li and Gang Feng and Xiao-Ping Zhang}, title={{Automatic Detection of the Temporal Segmentation of Hand Movements in British English Cued Speech}}, year=2019, booktitle={Proc. Interspeech 2019}, pages={2285--2289}, doi={10.21437/Interspeech.2019-2353}, url={http://dx.doi.org/10.21437/Interspeech.2019-2353} }</pre>
description: The authors would like to thank the professional CS teacher Cate Calder from Cued Speech UK association for her time spent on the British English CS dataset recording.
description: {"references": ["interspeech 2019"]}
DOI: 10.25606/surf.578c6039-2c58b578
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-560)

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 560 of the 2048³ resolution collection.
DOI: 10.14457/cu.the.2006.1714
title: Design and control of a reactive distillation column for the production of butyl acetate from dilute acetic acid

description: Recovery of the dilute acetic acid becomes important issues due to economic and environmental awareness. The present research is focused on the application of a reactive distillation as a potential alternative method for dilute acetic acid recovery. The synthesis of butyl acetate, from esterification of dilute acetic acid with butanol in the reactive distillation is investigated with HYSYS commercial software. The model prediction by the HYSYS simulator is validated with experimental results reported in literature and a good agreement is observed. The effect of dilute acetic acid concentration on reactive distillation performances in terms of butyl acetate production is first studied. The influences of key operating variables on the performance of the reactive distillation are also evaluated in order to design the reactive distillation. Finally, the closed-loop control of a reactive distillation column is explored. Two alternative control structures are evaluated using 80 wt% acetic acid concentration for the production of butyl acetate. Disturbances in fresh feed flow rate and compositions are made to examine the rangeability of the control structures.
DOI: 10.5519/qd.2quyddqj
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (432705 records)
DOI: 10.5519/qd.on9qxyj1
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1755 records)
DOI: 10.5519/qd.qwbd20sr
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (986 records)
DOI: 10.5519/qd.rd5wadp8
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (946 records)
DOI: 10.5519/qd.znrj0ytc
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1223 records)
DOI: 10.5519/qd.amr6bxi1
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (36 records)
DOI: 10.5519/qd.kedojvmu
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (69 records)
DOI: 10.14457/cu.the.2006.1715
title: Defect structure controlling on TIO₂ nanocrystal and its applications

description: The objectives of this work are the study for understanding surface defect (Ti³+) TiO₂ nanocrystal in anatase phase in the points of controlling, probing, and investigating its effect on the thermal stability, photoactivity, metal-support strong interaction, and the forming of metal-support compound. In this work, the surface defect (Ti³+) has been successfully controlled on TiO₂ nanocrystal at the same time with the preparation of anatase via sol-gel technique. This new method consumes less step and energy than the common technique. For the application of TiO₂ having different amount of surface defect on the photocatalysis, it was found that the increase in number of surface defect can enhance the photoactivity of TiO₂ nanocrystal because it can inhibit the recombination process between photo-electron and hole generated after UV irradiation. For another application of TiO₂ nanocrystal as a support of cobalt, it can be concluded that the increase in number of surface defect (Ti³+) can enhance the cobalt dispersion on TiO₂ support and also inhibit the formation of Co-SCF after standard reduction which led to increase in activity of cobalt for CO-hydrogenation. In this work, moreover, the effect of surface defect on the thermal stability was also investigated via the Piyasan's equation showing that the increase in number of surface defect have no effect on the rate of crystal growth and the surface defect can be created as mush as required. In the last part, the probing surface defect by using metal carbonyls in the atom level was also studied. It can monitor the behavior of surface defect and make a deeply understanding over it.
DOI: 10.25606/surf.578c6039-fdbc4747
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-141)

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 141 of the 2048³ resolution collection.