cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.2652034
title: Pileup Jet Dataset for PUMML

description: Dataset of events used in the PUMML paper. One file contains datasets with 2k events per pileup vertex number (mu) for mu=0-180 and the other contains 50k events for different signal processes (specified by the mass of a scalar particle decaying to quarks) all with mu=140. A notebook demonstrating how to use the files can be found at https://github.com/pkomiske/PUMML/blob/master/PUMML%20Events.ipynb.
description: {"references": ["P. T. Komiske, E. M. Metodiev, B. Nachman, M. D. Schwartz, Pileup Mitigation with Machine Learning, JHEP 1712 (2017) 051, arXiv:1707.08600."]}
DOI: 10.5519/qd.pyfq0oe9
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1024 records)
DOI: 10.5519/qd.g60cbpm2
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (13033 records)
DOI: 10.5519/qd.ozimldyi
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (730 records)
DOI: 10.25919/5cc405c3df7fe
title: Parkes observations for project P958 semester 2019APRS_09

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: 10.5517/ccdc.csd.cc20klt0
title: CCDC 1863962: Experimental Crystal Structure Determination

description: Related Article: Sahar Usefi, Kamran Akhbari, Jonathan White|2019|J.Solid State Chem.|276|61|doi:10.1016/j.jssc.2019.04.016
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc20twf5
title: CCDC 1871917: Experimental Crystal Structure Determination

description: Related Article: Tuanli Yao, Xiujuan Liang, Zhen Guo, Dong Yang|2019|Tetrahedron|75|3088|doi:10.1016/j.tet.2019.04.036
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21fxhx
title: CCDC 1890209: Experimental Crystal Structure Determination

description: Related Article: Pavel S. Kulyabin, Ivan A. Portnyagin, Alexey N. Tsarev, Andrey F. Asachenko, Georgy P. Goryunov, Vyatcheslav V. Izmer, Dmitry V. Uborsky, Alexander Z. Voskoboynikov, Noureddine Ajellal, Tiina Vanne, Riitta Varzeshkhah, Luigi Resconi, Pascal Castro|2019|J.Organomet.Chem.|892|41|doi:10.1016/j.jorganchem.2019.04.027
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc21fxkz
title: CCDC 1890211: Experimental Crystal Structure Determination

description: Related Article: Pavel S. Kulyabin, Ivan A. Portnyagin, Alexey N. Tsarev, Andrey F. Asachenko, Georgy P. Goryunov, Vyatcheslav V. Izmer, Dmitry V. Uborsky, Alexander Z. Voskoboynikov, Noureddine Ajellal, Tiina Vanne, Riitta Varzeshkhah, Luigi Resconi, Pascal Castro|2019|J.Organomet.Chem.|892|41|doi:10.1016/j.jorganchem.2019.04.027
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5517/ccdc.csd.cc2225fs
title: CCDC 1908714: Experimental Crystal Structure Determination

description: Related Article: Qing-Qing Huang, Yang-Jie Lin, Rui Zheng, Wei-Hua Deng, Chiranjeevulu Kashi, P. Naresh Kumar, Guan-E Wang, Gang Xu|2019|Inorg.Chem.Commun.|105|119|doi:10.1016/j.inoche.2019.04.037
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.5281/zenodo.2652854
title: Apprenticeship in Early Modern Venice - Supporting data and code

description: A dataset of contracts of apprenticeship from early modern Venice, along with R code to analyse them. These were used for a chapter on Apprenticeship in Early Modern Venice for the CUP. This work is part of the Garzoni project: https://garzoni.hypotheses.org.
DOI: 10.5281/zenodo.2652855
title: Apprenticeship in Early Modern Venice - Supporting data and code

description: A dataset of contracts of apprenticeship from early modern Venice, along with R code to analyse them. These were used for a chapter on Apprenticeship in Early Modern Venice for the CUP. This work is part of the Garzoni project: https://garzoni.hypotheses.org.
DOI: 10.17632/bf5svxhzb5.1
title: Data for: Water-soluble rare earth elements in atmospheric deposition at Shihua Cave, Beijing, North China
DOI: 10.17632/2w38zxxkh6.1
title: Data for: Numerical Simulations of Guided self-propelled jumping of droplets on a Wettability Gradient Surface

description: This is a simulation example，the openfoam version used in this paper is 2.4.
DOI: 10.17632/xhxhb556wn.1
title: Data for: Numerical Simulations of Guided self-propelled jumping of droplets on a Wettability Gradient Surface
DOI: 10.17632/vrk2tpbtt3.1
title: Data for: Growth mechanism of Sb2Se3 thin films for photovoltaic application by vapor transport deposition

description: Data contain scanning electron microscopy and X-ray diffraction results of all thin films tested in this study.
DOI: 10.25919/5cc52053ce174
title: Parkes observations for project P958 semester 2019APRS_11

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: 10.17632/2w38zxxkh6.2
title: Data for: Numerical Simulations of Guided self-propelled jumping of droplets on a Wettability Gradient Surface

description: This is a simulation example，the openfoam version used in this paper is 2.4.
DOI: 10.17632/2jyrhy5f9x.1
title: Data for: The Investigation of Visual Scan Patterns on Different Designs of Crew Alerting System in the Flight Deck
DOI: 10.17632/p3pgccc3hn.1
title: Data for: The Investigation of Visual Scan Patterns on Different Designs of Crew Alerting System in the Flight Deck
DOI: 10.17632/y88tf3fybf.1
title: Data for: Modeling of a charged dielectric interface: Comparison of continuum and discrete lattice representations of surface charges

description: 1. Numerical calculations on the ratio of electrostatic force between discrete and continuum representations of surface charges. 2. Raw data and Gnuplot scripts
DOI: 10.17632/6zt5c9gzw6.1
title: Data for: Multi-gene global phylogeography of the Gypsy Moth, reveals misaligned subspecies concepts and a cryptic lineage

description: Various datasets used in this study are uploaded here.
DOI: 10.17632/2shpbgndb5.1
title: Data for: Surveying the future of science, technology and business – a 35 year perspective

description: Science, Nature and Harvard Business Review readers report their expectations for advances in science, technology, and business over a 35-year time horizon.
DOI: 10.17632/vtmd7smjz7.1
title: Data for: Effects of Photoperiod and Light Spectrum on Growth Performance, Digestive Enzymes, Hepatic Biochemistry and Peripheral Hormones in Spotted Sea Bass (Lateolabrax maculatus)
DOI: 10.5281/zenodo.2653215
title: S37 | LITMINEDNEURO | Neurotoxicants from literature mining PubMed

description: This is the collection associated with list S37 LITMINEDNEURO on the NORMAN Suspect List Exchange.

https://www.norman-network.com/?q=suspect-list-exchange

S37

LITMINEDNEURO

<strong>Neurotoxicants from literature mining PubMed</strong>

LITMINEDNEURO CSV, XLSX (25/01/2019)<br>
CompTox LITMINEDNEURO List

LITMINEDNEURO InChIKeys (25/01/2019)

A list of chemicals associated with neurotoxicity compiled through systematic literature mining of PubMed using MeSH terms, compiled by Nancy Baker, Antony Williams (US EPA) and Emma Schymanski (LCSB), details in Schymanski et al (submitted) and on CompTox list.
DOI: 10.17632/2shpbgndb5.2
title: Data for: Surveying the future of science, technology and business – a 35 year perspective

description: Science, Nature and Harvard Business Review readers report their expectations for advances in science, technology, and business over a 35-year time horizon.
DOI: 10.25919/5cc6175f5dba9
title: Parkes observations for project P991 semester 2019APRS_01

description: Finding radio pulsars orbiting near Sgr A* is a major goal of pulsar surveys with existing telescopes and future telescopes such as the Square Kilometer Array (SKA). The discovery of such pulsars will allow us to measure relativistic effects through timing of pulsars in tight orbits around Sgr A*, to characterise the distribution of dark matter near Sgr A*, to study the stellar population in the GC region and to probe the scattering region around Sgr A*. Although several surveys of the GC region have done, the Ultra-Wideband Low (UWL) receiver provides us a much wider frequency coverage with great sensitivity and therefore it is an excellent chance to revisit the GC region. At around 4GHz, a survey with UWL will achieve a sensitivity significantly higher than previous Parkes and Green Bank surveys, especially for pulsars with short spin periods and high dispersion measures.
DOI: 10.25919/5cc61c92d341c
title: Parkes observations for project P885 semester 2019APRS_01

description: We propose to observe the magnetars 1E 1547.0-5408 and PSR J1622-4950
approximately weekly, to track their rotation, flux density, and
polarisation, as we have been doing through this project. As of
this week (8 Dec 2018), XTE J1810-197 is again a radio magnetar,
after 10 years dormant! (We have been observing it sporadically
during its low state waiting for such an event.) Its likely chaotic
rotation will be better tracked in detail elsewhere, but weekly
observations with the UWL receiver will provide unique measurements
of its radio spectrum and broad-band behaviour. Our observations
provide an important window into remarkably dynamic magnetar
magnetospheres, and characterise the conditions under which radio
emission takes place therein, placing constraints on the emission
mechanisms, which in at least some significant respects differ from
those of ordinary pulsars.
DOI: 10.26300/jwv9-ew20
title: Data from "Encoding Information in Synthetic Metabolomes"
DOI: 10.5517/ccdc.csd.cc2268rb
title: CCDC 1912661: Experimental Crystal Structure Determination

description: Related Article: Brian W. Skelton, Murray V. Baker, Rosenani A. Haque|2019|CSD Communication|||
description: An entry from the Cambridge Structural Database, the world’s repository for small molecule crystal structures. The entry contains experimental data from a crystal diffraction study. The deposited dataset for this entry is freely available from the CCDC and typically includes 3D coordinates, cell parameters, space group, experimental conditions and quality measures.
DOI: 10.25606/surf.578c6039-1d4fd770
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-644)

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 644 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-49ae3b15
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-645)

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 645 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-bcdd5958
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-647)

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 647 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-c9ded29b
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-646)

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 646 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-1c99da62
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-098)

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 098 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-25cfab2c
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-094)

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 094 of the 2048³ resolution collection.
DOI: 10.25606/surf.578c6039-41aecf4d
title: The Cosmogrid Simulation: Statistical Properties of Small Dark Matter Halos (2048-076)

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 076 of the 2048³ resolution collection.