cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25606/surf.578c6039-8526b53e
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-093)

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 093 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-b7725292
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-096)

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 096 of the 1024³ resolution collection.
DOI: 10.25606/surf.578c6039-f373b9a5
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (1024-092)

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 092 of the 1024³ resolution collection.
DOI: 10.5281/zenodo.2648178
title: FT9 Blockley 4-key tenoroon: measurements, photos

description: Dataset of FT9 Blockley 4-key tenoroon containing detailed external and internal measurements, photos. Some incomplete measurement details will be collected at a later date.
DOI: 10.17632/yy2kvb9k4y.1
title: Data for: Genetic diversity of chemokine XCL1 and its receptor XCR1 in murine rodents
DOI: 10.5281/zenodo.2648177
title: FT9 Blockley 4-key tenoroon: measurements, photos

description: Dataset of FT9 Blockley 4-key tenoroon containing detailed external and internal measurements, photos. Some incomplete measurement details will be collected at a later date.
DOI: 10.5281/zenodo.2652907
title: FT31 Tauber (1) 6-key tenoroon: basic data

description: Dataset of FT31 Tauber (1) 6-key tenoroon containing basic data.  Measurement data will be collected at a later date.
DOI: 10.5519/qd.xbm5fti0
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (32 records)
DOI: 10.15139/s3/6cjviq
title: Replication Data for: Preserving racial hierarchy amidst changing racial demographics: How neighborhood racial preferences are changing while maintaining segregation.

description: Replication/Extension assignment for POLI 784 for Leah Campbell - Preserving Racial Hierarchy Amidst Changing Racial Demographics. Package includes data file, R script, replication/extension write-up, codebook on the data set, and a PDF of the original paper.
DOI: 10.7910/dvn/h4dv8n
title: Yoga Burn

description: Yoga Burn is a instructional yoga program that teaches you the specific yoga poses that increases your body’s metabolism to burn fat, and, at the same time, tone your whole body. The follow along yoga videos in the program can be streamed online via its private member page or be downloaded into your computer or smartphone. The program is split into 3 phases: Foundational Flow, Transitional Flow, and Mastery Flow. In each phase, there are 4 videos: instruction video, and 3 workout videos. And with the latest update (2017), you can now download the program’s instructional videos to your phone and follow along with it at the comfort of your home or anywhere you like.Specifically designed for women, this program is a concise and informative collation of the all relevant information to help you achieve the best you can from your workout regime. Created by Zoe Bray-Cotton, a certified yoga instructor and personal trainer, this program can help women from any walk of life to completely change their bodies. Focusing primarily on helping people to get the most out of yoga, Zoe’s dynamic sequencing strategy is what sets her Yoga Burn apart from other programs on the market. Yoga Burn is accessed entirely online and comprises a 12 week follow-along video series. Access the sequential videos via smartphone, tablet or PC and implement the valuable information anywhere with connectivity. Comprised of 3 unique phases, each phase lasts around 4 weeks and breaks yoga down into manageable chunks.
DOI: 10.5519/qd.oe5dfble
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (115 records)
DOI: 10.7910/dvn/gmbpsq
title: Unlock Your Hip Flexors

description: Unlock Your Hip Flexors program contains a 63-page manual guide and 2 videos – a coaching video and a follow-along video, which shows you on how to do the exercises as taught in the manual. The goal of the program is teaching readers on how to loosen and strengthen their hip flexors. Clients who purchased the program are also entitled to 2 free bonuses: Unlock Your Tight Hamstrings program (manual and video guides) and The 7-Day Anti-Inflammatory Diet.It’s rare that a program of this calibre is created by two respected professionals, which is what makes us sure that the Unlock Your Hip Flexors program is the top of its game in the market. Co-authored by Rick Kaselj and Mike Westerdal, the program allows you to benefit from the combined expertise of two of the leading professionals in the exercise, weight training and core strength industry.
DOI: 10.17632/yr5sdcfg27.1
title: Data for: One size does not fit all: quantile regression estimates of cross-country risk of poverty and social exclusion. An application to European data

description: Stata data set
DOI: 10.5281/zenodo.2653236
title: Exploring Internal Quality Metric Fluctuations in Revision Histories – An Empirical Study

description: Datasets and analysis script for the article "Exploring Internal Quality Metric Fluctuations in Revision Histories – An Empirical Study" submitted to ESEM'19 under double-blind review and provided as-is.
DOI: 10.17632/yr5sdcfg27.2
title: Data for: One size does not fit all: quantile regression estimates of cross-country risk of poverty and social exclusion. An application to European data

description: Stata data set
DOI: 10.5281/zenodo.2652934
title: mapbiomas_lu_historical_data

description: Brazilian land use data from 1985 to 2017 derived from Project MapBiomas - Collection 3.1 to be used as historical data in MAgPIE-Brazil.
DOI: 10.5281/zenodo.2652935
title: mapbiomas_lu_historical_data

description: Land use data from 1985 to 2017 for Brazil is aggregated from Project MapBiomas - Collection 3.1 of Brazilian Land Cover & Use Map Series, accessed on 27/04/2019 through the link: http://mapbiomas.org/pages/estatisticas".

File mapbiomas_other_no_croppast.mz aggregates data from MapBiomas as follows:<br>
Resources|Land Cover|Forest|+|Managed Forest = Forest Plantation<br>
Resources|Land Cover|+|Forest = Forest<br>
Resources|Land Cover|+|Urban Area = Urban Infrastructure<br>
Resources|Land Cover|+|Cropland = Agriculture<br>
Resources|Land Cover|+|Pastures and Rangelands = Pasture<br>
Resources|Land Cover|+|Other Land = Non-Forest Natural Formation + Non-Vegeted Area except Urban Infrastructure + Water Bodies + Non Observed

<br>
File mapbiomas_other_plus_croppast.mz aggregates data from MapBiomas as follows:<br>
Resources|Land Cover|Forest|+|Managed Forest = Forest Plantation<br>
Resources|Land Cover|+|Forest = Forest<br>
Resources|Land Cover|+|Urban Area = Urban Infrastructure<br>
Resources|Land Cover|+|Cropland = Agriculture<br>
Resources|Land Cover|+|Pastures and Rangelands = Pasture<br>
Resources|Land Cover|+|Other Land = Non-Forest Natural Formation + Non-Vegeted Area except Urban Infrastructure + Water Bodies + Non Observed + Mosaic of Agriculture and Pasture
DOI: 10.5281/zenodo.2653235
title: Exploring Internal Quality Metric Fluctuations in Revision Histories – An Empirical Study

description: Datasets and analysis script for the article "Exploring Internal Quality Metric Fluctuations in Revision Histories – An Empirical Study" submitted to ESEM'19 under double-blind review and provided as-is.
DOI: 10.17632/8gwn2ghk44.1
title: Data for: Review of Methods to Assess Sustainability of Industrial Water Use

description: This file contains the raw data from the EPPI reviewer software concerning methodologies employed to evaluate the sustainability of water use in industry.
DOI: 10.3886/e104860v3
title: Foreign Policy Assertiveness of Six Major Nations

description: These variables are indicators of the foreign policy assertiveness of six major nations: Great Britain, France, Germany, Japan, Russia, and the United States. Assertiveness is defined as the magnitude and intensity of actions by a nation to influence the foreign environment. The following indicators are considered to reflect a nation's changing assertiveness: the number of active duty naval personnel, the number of military personnel in foreign areas, the number of military attaches stationed abroad, and the number of diplomatic, consular, and other civilian government officials posted abroad. Percentage changes in those indicators are considered to reflect the relative foreign policy assertiveness of the six nations. The variables span the period from 1815 to 2005, but the coverage varies with each country. Primary sources are used to the extent possible and are cited in each file.<br><br><br><br><br><br><br><br><br><br><br><br><br><br><br><br><br><br>
DOI: 10.17632/mgm7fdrwkn.1
title: Data for: Disentangling the connections: a network analysis of approaches on urban green infrastructures
DOI: 10.25845/5cc64f29b35a1
title: Reef Plan Monitoring Of Inshore Coral Reef Communities, Great Barrier Reef (RRMMP)
DOI: 10.7910/dvn/p9kgwd
title: Le Miracle De La Grossesse, Avis 2019 - Fiable ou arnaque ?

description: Si vous êtes à la recherche d’une revue honnête et détaillée sur“ Le Miracle De La Grossesse ” de Lisa Olson, alors je vous assure que vous êtes au bon endroit. Ici, vous allez trouver la revue la plus fiable et la plus authentique de ce produit. Cette étude est basée sur des expériences réelles, alors vous serez complètement satisfait par les informations que vous trouverez ici. Si vous avez une question sur le sujet de lagrossesse, lisez cet article jusqu’à la fin et il y a de fortes chances que vous allez y trouver la réponse. Chaque femme souhaite vivre ce magnifique sentiment de la maternité dans un moment donné de sa vie. Ce sentiment complète votre féminité alors que votre enfant complète votre existence et votre individualité. Mais malheureusement, en présence de quelques sérieux problèmes comme l’infertilité, la femme devient incapable de tomber enceinte. Elle peut dans ce cas se retrouver dans des situations embarrassantes on optant pour des médicaments forts, des chirurgies, et d’autres méthodes de traitement qui ne sont pas efficaces. Pouvez-vous imaginer que vous n’allez jamais entendre votre enfant vous appeler « maman » ! C’est effrayant non? Ne vous inquiétez pas ! Comme son nom l’indique, le programme“ Le Miracle De La Grossesse ”a réussi à surprendre le monde entier avec son efficacité. Dans cet article nous allons vous parler de ce programme d’une manière détaillée.
DOI: 10.14457/nida.the.1995.1
title: Determinants and consequences of legal marriage dissolution among Thai women
DOI: 10.14457/nida.the.1995.2
title: Determinants and consequences of early marriage among adolescent women in the rural northeast of Thailand
DOI: 10.14457/nida.the.1995.3
title: Levels trends determinants and demographic consequences of contraceptive sterilization in Thailand
DOI: 10.14457/nida.the.2006.257
title: Segment reporting in practice and quality of segment information of listed companies in Thailand
DOI: 10.14457/nida.the.2010.40
title: A critical discourse analysis of Thainess in children's literature : a case study of TK Park books for children in the three southernmost provinces of Thailand
DOI: 10.17632/67sjx5y6xc.1
title: Data for: Preparation 2-(anthracen-9-yl)-1,3-dithiolane as a novel dual-channel AIE-active fluorescent probe for mercury (II) ion with excellent performance

description: A novel fluorescent probe molecule, 2-(anthracen-9-yl)-1,3-dithiolane (AADT), is designed and synthesized for Hg2+ detection successfully, based on a good aggregation induced emission (AIE) fluorescent mechanism and a specific reaction type. DMF-H2O mixed solvent (Fw 80% V/V) is suitable to disperse AADT for forming 1×10-5 mol·L-1 solution with an AIE-active fluorescence probe system. With the increase of trace Hg (II), the AADT probe shows dual-channel, (turn-off at 429 nm, and turn–on at 511nm) fluorescence probe character. (R2&gt;0.994), which does not interfere each other. The probe demonstrates excellent selectivity, anti-inference properties, and several metal ions and acid ions hardly affect its performance. The LOD of the AADT probe is lower than 2.34×10-8 mol·L-1.
DOI: 10.17632/p8hzhj45ph.1
title: Data for: Building sectoral job search indices for the United States

description: This file contains US sectoral job search indices.
DOI: 10.14457/nida.res.1989.1
title: Industrial demand for energy in Thailand
DOI: 10.14457/nida.res.1990.1
title: Business memos, letters and telex
DOI: 10.14457/nida.res.2013.8
title: The role of the oil fund in Thailand: past, present, and future
DOI: 10.14457/nida.the.1987.1
title: Consequences of population changes on compulsory education in Thailand : 1986-1996
DOI: 10.14457/nida.the.1988.1
title: Identification of target population needing health services : basic minimum needs approach
DOI: 10.14457/nida.the.1990.3
title: Education management for the generation of self-employment of graduated
DOI: 10.14457/nida.the.1995.4
title: The role of the family in supporting the elderly : a comparative study between urban and rural areas
DOI: 10.17632/vb8w48w9zm.1
title: Data for: Evolution of the Singhbhum Craton and supracrustal provinces from age, isotopic and chemical constraints

description: Supplementary Material to Olierook et al., Earth-Science Reviews 2019
DOI: 10.25919/5cc4e490bf191
title: Parkes observations for project P958 semester 2019APRS_10

description: Fast radio bursts (FRBs) continue to raise more questions than they answer. Until a few months ago, only one burst – the only one known to repeat -  had been localized to a bright radio nebula (either a young supernova remnant or pulsar wind nebulae) in a distant dwarf galaxy.   
Over the last year searches with the Australian Square Kilometre Array Pathfinder (ASKAP) have detected 28 bursts, two of which have been localised to host galaxies at redshifts &gt; 0.3. These bursts and their hosts are very unlike the repeater, suggesting there may be a dichotomy in the population.  Over the next six months we expect to detect another 12 FRBs, which will also have sub-arcsecond localisations.   Here we propose to search this population for repeats.  Our comprehensive sample and a dense monitoring campaign of well localised bursts, at a fluence limit more than 60 times lower than that of their detections, will either confirm the presence of additional repeating FRBs or the uniqueness of FRB 121102 amongst the population.
DOI: 10.5281/zenodo.2652930
title: Recla 8-state founder allele dosages

description: 8-state founder allele dosages for the Recla data. Created by R/qtl2 (https://kbroman.org/qtl2/).
DOI: 10.5281/zenodo.2652931
title: Recla 8-state founder allele dosages

description: 8-state founder allele dosages for the Recla data. Created by R/qtl2 (https://kbroman.org/qtl2/).
DOI: 10.14457/nida.res.1990.2
title: Impacts of uncertainty of input supply on production of manufacture : a case study of natural gas curtailments
DOI: 10.5281/zenodo.2653099
title: Data for "Measurement of the atom-surface van der Waals interaction by transmission spectroscopy in a wedged nano-cell"

description: The data presented in publication "Measurement of the atom-surface van der Waals interaction by transmission spectroscopy in a wedged nano-cell" . Published version: https://doi.org/10.1103/PhysRevA.100.022503 The data are in HDF5 format, with associated metadata. To see examples of how to use the data, and the theoretical model for analysis, see https://github.com/thermal-vapours/TAS-Transmission-Atom-Surface
DOI: 10.5281/zenodo.2653100
title: Data for "Measurement of the atom-surface van der Waals interaction by transmission spectroscopy in a wedged nano-cell"

description: The data presented in publication "Measurement of the atom-surface van der Waals interaction by transmission spectroscopy in a wedged nano-cell" . Published version: https://doi.org/10.1103/PhysRevA.100.022503 The data are in HDF5 format, with associated metadata. To see examples of how to use the data, and the theoretical model for analysis, see https://github.com/thermal-vapours/TAS-Transmission-Atom-Surface
DOI: 10.14272/nvqfhmagcydrgo-byyhnaklsa-n/13cnmr
title: 13C NMR (, InChI=1S/C26H18N2O4/c29-25(30)19-10-6-17(7-11-19)21-14-15-23(18-8-12-20(13-9-18)26(31)32)24(16-21)28-27-22-4-2-1-3-5-22/h1-16H,(H,29,30)(H,31,32)/b28-27+)

description: dataset for 13C NMR
      
      13C NMR (100 MHz, DMSO-d6, ppm) δ = 167.2 (1C, CO2H), 167.0 (1C, CO2H), 152.2 (1C, Cq), 149.3 (1C, Cq), 143.0 (1C, Cq), 142.0 (1C, Cq), 139.7 (1C, Cq), 139.1 (1C, Cq), 131.7 (1C, CH), 131.7 (1C, CH), 130.8 (2C, CH), 130.2 (1C, Cq), 130.1 (2C, CH), 129.8 (1C, Cq), 129.7 (1C, CH), 129.5 (2C, CH), 128.8 (2C, CH), 127.0 (2C, CH), 122.9 (2C, CH), 114.0 (1C, CH).This spectrum shows additional signals corresponding to the cis isomer, due to isomerization under the conditions of the measurement: 167.0 (1C, CO2H), 166.9 (1C, CO2H), 153.1 (1C, Cq), 152.0 (1C, Cq), 142.5 (1C, Cq), 141.4 (1C, Cq), 138.9 (1C, Cq), 131.5 (1C, Cq), 131.0 (1C, CH), 129.9 (2C, CH), 129.4 (2C, CH), 129.0 (2C, CH), 127.8 (1C, CH), 127.1 (1C, CH), 126.7 (2C, CH), 126.2 (2C, CH), 119.5 (2C, CH), 117.6 (1C, CH).
DOI: 10.14272/nvqfhmagcydrgo-byyhnaklsa-n/1hnmr
title: 1H NMR (, InChI=1S/C26H18N2O4/c29-25(30)19-10-6-17(7-11-19)21-14-15-23(18-8-12-20(13-9-18)26(31)32)24(16-21)28-27-22-4-2-1-3-5-22/h1-16H,(H,29,30)(H,31,32)/b28-27+)

description: dataset for 1H NMR
      
      1H NMR (500 MHz, DMSO-d6, ppm) δ = 13.04 (bs, 2H, CO2H), 8.09–8.02 (m, 6H, CH), 7.93–7.92 (m, 2H, CH), 7.83–7.78 (m, 3H, CH), 7.66–7.64 (m, 2H, CH), 7.59–7.57 (m, 3H, CH). This spectrum shows additional signals corresponding to the cis isomer, due to isomerization under the conditions of the measurement.
DOI: 10.14272/nvqfhmagcydrgo-byyhnaklsa-n/ea
title: EA (, InChI=1S/C26H18N2O4/c29-25(30)19-10-6-17(7-11-19)21-14-15-23(18-8-12-20(13-9-18)26(31)32)24(16-21)28-27-22-4-2-1-3-5-22/h1-16H,(H,29,30)(H,31,32)/b28-27+)

description: dataset for EA
      
      EA (C26H18N2O4): Calcd C 73.92; H 4.30; N 6.63. Found C 74.35; H 4.49; N 6.52.
DOI: 10.14272/nvqfhmagcydrgo-byyhnaklsa-n/ir
title: IR (, InChI=1S/C26H18N2O4/c29-25(30)19-10-6-17(7-11-19)21-14-15-23(18-8-12-20(13-9-18)26(31)32)24(16-21)28-27-22-4-2-1-3-5-22/h1-16H,(H,29,30)(H,31,32)/b28-27+)

description: dataset for IR
      
      IR (ATR, ṽ) = 2920, 2874, 1683, 1606, 1422, 1317, 1289, 1179, 1128, 1019 cm–1.
DOI: 10.14272/nvqfhmagcydrgo-byyhnaklsa-n/mass
title: Mass (, InChI=1S/C26H18N2O4/c29-25(30)19-10-6-17(7-11-19)21-14-15-23(18-8-12-20(13-9-18)26(31)32)24(16-21)28-27-22-4-2-1-3-5-22/h1-16H,(H,29,30)(H,31,32)/b28-27+)

description: dataset for Mass
      
      EI (m/z, 70 eV, 220 °C): 284 [M–C6H4CO2H–OH]+.
DOI: 10.14272/nvqfhmagcydrgo-byyhnaklsa-n/others
title: Others (, InChI=1S/C26H18N2O4/c29-25(30)19-10-6-17(7-11-19)21-14-15-23(18-8-12-20(13-9-18)26(31)32)24(16-21)28-27-22-4-2-1-3-5-22/h1-16H,(H,29,30)(H,31,32)/b28-27+)

description: dataset for Others
      
      UV-VIS (CH2Cl2), λmax = 291 nm.
DOI: 10.5519/qd.d7iwfhi6
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1 records)
DOI: 10.5281/zenodo.2652948
title: Data Intervals To Study Statistics of Whistler Waves in the Solar Wind

description: This dataset contains a list of intervals that were used to study the statistics of whistler waves in the solar wind. It is created in companion to a manuscript submitted to ApJ.
DOI: 10.5281/zenodo.2652949
title: Data Intervals To Study Statistics of Whistler Waves in the Solar Wind

description: This dataset contains a list of intervals that were used to study the statistics of whistler waves in the solar wind. It is created in companion to a manuscript submitted to ApJ.