cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.25919/5cf2fa822ce4e
title: Parkes observations for project P1011 semester 2019APRS_08

description: Pulsars with features in their radio spectra, such as curvature or breaks seem to be special cases among the known pulsar population, with only about 20 per cent exhibiting them. Unfortunately, reliable flux density measurements besides at 1.4 GHz are often unavailable, so that their spectral morphologies and features cannot be determined accurately. We propose to utilize the unique capabilities of the newly commissioned UWL receiver at the Parkes telescope, its extremely wide instantaneous frequency coverage from about 700 to 4000 MHz together with its high sensitivity, to determine the spectra of 26 radio pulsars. These have previously been identified to exhibit spectral features or show hints thereof. The new Parkes data are crucial to determine their spectral morphologies in that frequency range, to characterize their spectral features and to resolve these within the recorded bandwidth. Our aim is to understand the physical origin of the features, namely, whether these are perhaps intrinsic to the pulsar emission in these sources, are caused by absorption processes inside the pulsar's magnetosphere, or along the line of sight.
DOI: 10.21227/aw71-6n07
title: Ultrasound/MRI Neck Muscle Image Semantic Segmentation Dataset

description: Segmentation of ultrasound (US) images of cervical muscles is required for visualisation, analysis of deep, muscle structure and function, and monitoring of patient specific treatment protocols.The lack of publicly available labelled data, benchmark methods and results, hinders development of this domain. Here, we contribute a labelled dataset of 1,100 US images of the human posterior cervical muscles during head motion, from 28 healthy adults(19 male, mean 31.4, s.d. 8.9), and a labelled static MRI/ultrasound dataset ofhuman posterior cervical muscles, from 25 healthy adults (age: 29.0 ± 6.6, male: 12).** NOTE: DATASET TEMPORARILY REMOVED UNTIL APPROVED BY PEER REVIEW - USE OF THIS DATASET PRIOR TO PEER REVIEW AND PUBLICATION IS NOT VALID, NOR APPROVED BY THE AUTHORS **
DOI: 10.7910/dvn/egmlqg/ypjtzk
title: TABLE4program.do

description: :unav
DOI: 10.6073/pasta/70af64bbe42413bbd6bf9efe4693fa78
title: Evaporation pan data from 1983 to March 2019 at Jornada Experimental Range Weather Station

description: Surface evaporation is measured weekly to twice weekly using an
  evaporation pan compatible with standard National Weather Service
  evaporation measurements. Measurements are made twice per week during
  hot periods because of high evaporation rate. The following data is
  collected: number of days between measurements, beginning and ending
  measurement period, current, minimum, and maximum water temperature;
  initial water level; final water level; rainfall since last
  evaporation measurement, and calculated evaporation (inches).
DOI: 10.7910/dvn/egmlqg/fwkrg5
title: GentzkowData.tab

description: :unav
DOI: 10.7910/dvn/egmlqg/hhif2o
title: TABLE2.smcl

description: :unav
DOI: 10.7910/dvn/egmlqg/jfrhjx
title: TABLE5.smcl

description: :unav
DOI: 10.7910/dvn/egmlqg/oo7ik6
title: TABLE2program.do

description: :unav
DOI: 10.7910/dvn/egmlqg/tmxmbw
title: TABLE3program.do

description: :unav
DOI: 10.7910/dvn/egmlqg/wrq0np
title: README.rtf

description: :unav
DOI: 10.7910/dvn/egmlqg/ympbei
title: TABLE5program.do

description: :unav
DOI: 10.7910/dvn/egmlqg/2zt67e
title: TABLE4.smcl

description: :unav
DOI: 10.7910/dvn/egmlqg/oxgvyy
title: TABLE1data.tab

description: :unav
DOI: 10.7910/dvn/egmlqg/uk1wmy
title: TABLE3.smcl

description: :unav
DOI: 10.5281/zenodo.3236595
title: Amateur Vocal Percussion Dataset

description: Dataset of vocal imitations of percussion sounds. It includes a total of 9895 utterances in 280 audio files recorded by 28 participants with little or no experience in beatboxing. Onsets and labels for kick drum, snare drum, closed hi-hat and opened hi-hat are annotated in separate .csv files.

All audio files were recorded with a MacBook Pro's built-in mic in an indoor environment and they are distributed into two modalities: personal imitations and fixed imitations. For each modality and participant, four files contain repetitions of utterances of the same class and one file corresponds to a rhythmic improvisation with these.
DOI: 10.25919/5cf30c6662366
title: Parkes observations for project P1011 semester 2019APRS_09

description: Pulsars with features in their radio spectra, such as curvature or breaks seem to be special cases among the known pulsar population, with only about 20 per cent exhibiting them. Unfortunately, reliable flux density measurements besides at 1.4 GHz are often unavailable, so that their spectral morphologies and features cannot be determined accurately. We propose to utilize the unique capabilities of the newly commissioned UWL receiver at the Parkes telescope, its extremely wide instantaneous frequency coverage from about 700 to 4000 MHz together with its high sensitivity, to determine the spectra of 26 radio pulsars. These have previously been identified to exhibit spectral features or show hints thereof. The new Parkes data are crucial to determine their spectral morphologies in that frequency range, to characterize their spectral features and to resolve these within the recorded bandwidth. Our aim is to understand the physical origin of the features, namely, whether these are perhaps intrinsic to the pulsar emission in these sources, are caused by absorption processes inside the pulsar's magnetosphere, or along the line of sight.
DOI: 10.25919/5cf30f306cfb1
title: Parkes observations for project PX501 semester 2019APRS_06

description: This proposal relates to time purchased by the Chinese Academy of Sciences for Parkes follow-up confirmation and timing of FAST discoveries.  As the observing time has been purchased this proposal (and the related PX500) does not require TAC grading.  The primary reason for submitting a proposal is to ensure an outreach statement and that the proposal is entered into OPAL for the data archive to access. The Chinese team have two time requests. The time scheduled for the first (PX500) will be allocated in blocks of 24 hours and the data will become available in the data archive with an 18 month embargo period.  The second type of time (relating to this proposal) will be scheduled in shorter blocks and the data archived with a 10 year embargo.
DOI: 10.5281/zenodo.3236923
title: Dataset of uGIM deployed in an office building

description: A dataset of sensor and energy data collected from uGIM system in an office building located in Portugal.

The dataset has a total of three days (24 hour records for each 10 seconds):

 - summer day

 - winter day

 - cloudy day
description: The present work has received funding from National Funds through FCT under the project UID/EEA/00760/2019 and SFRH/BD/109248/2015
DOI: 10.17632/bf76cyncdj.1
title: Data for: Developing a Holocene tephrostratigraphy for northern Japan using the sedimentary record from Lake Kushu, Rebun Island

description: Major element glass chemistry and glass standards for distal tephras identified in Lake Kushu and proximal deposits of Changbaishan volcano.
DOI: 10.17632/dcgyh5z772.1
title: Data for: A thermodynamic model for the solubility of N2, O2 and Ar in pure water and aqueous electrolyte solutions and its applications

description: The calculated solubilities of N2, O2, Ar and air in pure water and aqueous electrolyte solutions from our developed thermodynamic model are in the excel file, where experimental data of each corresponding system are also added for comparions.
DOI: 10.25919/5cf3c9095315f
title: Parkes observations for project P456 semester 2019APRS_34

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days over a wide bandwidth. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.6073/pasta/11f26c69eb5b133d9bfc6b623925d3da
title: Hubbard Brook Experimental Forest: Chemistry of Streamwater – Monthly Volume Weighted Concentrations, Watershed 8, 1995 - present

description: These data include volume-weighted, average, monthly concentrations of
  cations, anions, and pH measured in Watershed 8.

      
  HBWatER is a long-term record of stream and precipitation chemistry
  and volume. Currently this record is supported by NSF LTREB funding
  (for sample collection and processing), USDA Forest Service (USFS)
  funding (for maintenance of stream gauges, analytical chemistry and
  sample archiving), and LTER (for disposable supplies). The HBWatER
  supervisory team currently includes Emma Rosi (Cary Institute of
  Ecosystem Studies), Emily Bernhardt (Duke University), John Campbell
  (USFS), Charley Driscoll (Syracuse University.), Mark Green (Case
  Western Reserve University), Bill McDowell (University of NH ), and
  Lindsey Rustad (USFS).

      
  The long-term hydrologic record and calculation of fluxes are
  currently supervised by John Campbell (USFS). The collection and
  management of the long-term chemistry record is currently supervised
  by Emma Rosi (Cary Institute of Ecosystem Studies) and Emily Bernhardt
  (Duke University). At present field samples are collected by Tammy
  Wooster (Cary Institute of Ecosystem Studies), Chemical analyses are
  performed by Jeff Merriam (USFS). Data management and archiving is
  performed by Mary Martin (University of NH)

      
  HBWatER was initiated in 1963 by G.E. Likens, F. H. Bormann, R.
  Pierce, and N. Johnson. The record has been funded over its lifetime
  by the Mary Flagler Cary Charitable Trust, The Andrew W. Mellon
  Foundation, HBR LTER grants (#8702331, #9211768, #9810221, #0423259,
  #1114804, #1637685) and NSF LTREB (# 1256696). A full list of
  contributors to the HBWatER over its lifetime is provided at:
  Bernhardt E., G. Likens, E. Rosi. 2019. Continuous
  precipitation and stream chemistry data, Hubbard Brook Ecosystem
  Study, 1963 – present.. Environmental Data Initiative.
  https://doi.org/10.6073/pasta/4022d829f3a1fa4057b63b5db8b1a172.

      
  These data were gathered as part of the Hubbard Brook Ecosystem Study
  (HBES). The HBES is a collaborative effort at the Hubbard Brook
  Experimental Forest, which is operated and maintained by the USDA
  Forest Service, Northern Research Station.
DOI: 10.17632/psm4d995yx.1
title: Data for: COSMOS Trader – Chaotic Neuro-oscillatory Multiagent Financial Prediction and Trading System

description: Dataset#2 consists of the time series data for 129 worldwide financial products (Table 4), which include: - 9 major cryptocurrencies - 84 major forex - 19 major commodities - 17 worldwide financial indices The raw data contains the daily time series of the daily OPEN, HIGH, LOW, CLOSE and VOLUME. These raw time series data are provided by AvaTrade.com – one of the world major cryptocurrency trading platforms and Forex.com – one of the world major Forex MT4 trading platforms. To facilitate chaotic neural network training and system testing, we have generated time series data of 15 major financial technical indicators for these 129 financial products. Fellow researchers can base on these financial time series to test for the chaotic neural networks for time series financial prediction under different categories and products.
DOI: 10.25919/5cf320308d4eb
title: Parkes observations for project P456 semester 2019APRS_31

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days over a wide bandwidth. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.6073/pasta/dffd665c34907717722ff009d968a23a
title: Hubbard Brook Experimental Forest: Chemistry of Streamwater – Monthly Volume Weighted Concentrations, Watershed 9, 1995 - present

description: These data include volume-weighted, average, monthly concentrations of
  cations, anions, and pH measured in Watershed 9.

      
  HBWatER is a long-term record of stream and precipitation chemistry
  and volume. Currently this record is supported by NSF LTREB funding
  (for sample collection and processing), USDA Forest Service (USFS)
  funding (for maintenance of stream gauges, analytical chemistry and
  sample archiving), and LTER (for disposable supplies). The HBWatER
  supervisory team currently includes Emma Rosi (Cary Institute of
  Ecosystem Studies), Emily Bernhardt (Duke University), John Campbell
  (USFS), Charley Driscoll (Syracuse University.), Mark Green (Case
  Western Reserve University), Bill McDowell (University of NH ), and
  Lindsey Rustad (USFS).

      
  The long-term hydrologic record and calculation of fluxes are
  currently supervised by John Campbell (USFS). The collection and
  management of the long-term chemistry record is currently supervised
  by Emma Rosi (Cary Institute of Ecosystem Studies) and Emily Bernhardt
  (Duke University). At present field samples are collected by Tammy
  Wooster (Cary Institute of Ecosystem Studies), Chemical analyses are
  performed by Jeff Merriam (USFS). Data management and archiving is
  performed by Mary Martin (University of NH)

      
  HBWatER was initiated in 1963 by G.E. Likens, F. H. Bormann, R.
  Pierce, and N. Johnson. The record has been funded over its lifetime
  by the Mary Flagler Cary Charitable Trust, The Andrew W. Mellon
  Foundation, HBR LTER grants (#8702331, #9211768, #9810221, #0423259,
  #1114804, #1637685) and NSF LTREB (# 1256696). A full list of
  contributors to the HBWatER over its lifetime is provided at:
  Bernhardt E., G. Likens, E. Rosi. 2019. Continuous
  precipitation and stream chemistry data, Hubbard Brook Ecosystem
  Study, 1963 – present.. Environmental Data Initiative.
  https://doi.org/10.6073/pasta/4022d829f3a1fa4057b63b5db8b1a172.

      
  These data were gathered as part of the Hubbard Brook Ecosystem Study
  (HBES). The HBES is a collaborative effort at the Hubbard Brook
  Experimental Forest, which is operated and maintained by the USDA
  Forest Service, Northern Research Station.
DOI: 10.25919/5cf325e15fb88
title: Parkes observations for project P456 semester 2019APRS_32

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days over a wide bandwidth. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.5281/zenodo.3236929
title: BIDS Data for "A Whole-Brain Map and Assay Parameter Analysis of Mouse VTA Dopaminergic Activation"

description: Base data package for the “"A Whole-Brain Map and Assay Parameter Analysis of Mouse VTA Dopaminergic Activation” article, formatted corresponding to the Brain Imaging Data Structure.
DOI: 10.5281/zenodo.3236930
title: BIDS Data for "A Whole-Brain Map and Assay Parameter Analysis of Mouse VTA Dopaminergic Act ivation"

description: Base data package for the “Multivariate Guide to Magnetic Resonance Imaging and Optogenetic Control of the Mouse VTA” article, formatted corresponding to the Brain Imaging Data Structure.
DOI: 10.25919/5cf328111a9c5
title: Parkes observations for project P971 semester 2019APRS_08

description: We propose timing observations of the relativistic pulsar - white-dwarf binary PSR J1141-6545. This unique system offers access to a wide range of physics, from relativistic phenomena through pulsar emission cone studies, to the structure and distribution of interstellar plasma along our line-of-sight. The recently installed Parkes Ultra Wide Band Low Frequency (UWL) receiver has opened up the possibility of performing first-ever studies of its orbital dynamics at high temporal resolution and study of the effects of the intra-binary medium on the dispersion and polarisation of the pulse profile. Our analysis of data obtained to date suggests that the pulsar would precess away from our line-of-sight in the next 3-5 years. Hence, regular observations are crucial to maximizing its science outcome
DOI: 10.25919/5cf3d571945c4
title: Parkes observations for project P456 semester 2019APRS_35

description: The Parkes Pulsar Timing Array (PPTA) project has three primary goals: (a) detection of gravitational waves from astronomical sources, (b) establishment of a pulsar timescale, and (c) improvement of our understanding of Solar-system dynamics. The PPTA is the oldest of three international pulsar timing groups. We have the smallest telescope and the smallest group, but the best measurements and the best results. Our bound on the strength of the incoherent gravitational wave background is the only bound which significantly constrains theoretical models. We have maintained our leading position because: we have the southern sky; we have a small but well-focussed group; we have the best-calibrated receivers; and we have been able to observe with an almost regular cadence of 15 to 20 days over a wide bandwidth. With this proposal we aim to maintain our pre-eminent position in the field.

Unlike most observing proposals, this is a continuing proposal for which the observations will continue to improve bounds on ultra-low-frequency gravitational waves until they are finally detected. Continued Parkes observations will remain valuable at least until the first stage of the SKA is able to improve on our sensitivity and observing cadence. Even after the gravitational wave background is detected we will want to continue observations in support of the nascent field of gravitational wave astronomy!
DOI: 10.17632/m86b4kvwmh.1
title: Data for: Corruption in Space: A closer look at the world's subnations

description: Dataset and do-file to replicate manuscript.
DOI: 10.7910/dvn/o5ks5o/glchmi
title: MainDataset.tab

description: :unav
DOI: 10.17632/dx7fwfj28g.1
title: Data for: LONG-TERM DIVERSIFICATION PATHS AND ENERGY TRANSITIONS IN EUROPE

description: The data set provides the raw data we used in our research: energy use by primary energy source in United Kingdom, Italy, Netherlands, Portugal, Spain, Sweden, Germany and France, from 1800 to 2009, expressed in petajoules (the data do not cover the first decades of the period for some countries); the calculation process, based on the Herfindahl-Hirschman concentration index; and the outputs we obtained: the Energy Mix Concentration Index in the mentioned countries for the period covered. Our starting point are the historical databases developed by a number of energy researchers, that is, United Kingdom (Fouquet, 2014), Italy (Malanima, 2006), Netherlands (Gales et al., 2007), Portugal (Henriques, 2011), Spain (Rubio, 2005), Sweden (Kander, 2002) and Germany and France (Kander et al., 2014, where all the data, but the United Kingdom’s, have been collected - an alternative set of data is included for England and Wales by Warde (2007)-). The basic data set on energy consumption is available at http://www.fas.harvard.edu/~histecon/energyhistory/energydata.html
DOI: 10.5519/qd.498ry15d
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (7466 records)
DOI: 10.5519/qd.s8rgn800
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (7 records)