cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.2992179
title: Russian social contact data relative to reactive school closure policies

description: The dataset consists of individual contact diaries collected in Tomsk, Russia, in 2016. The dataset contains contact information for both for regular school/work days and for days when classes/schools are closed as a consequence of a reactive school closure strategy.<br> <br> This record consists of the dataset associated with M. Litvinova, Q.-H. Liu, E. S. Kulikov, M. Ajelli, Reactive school closure weakens the network of social interactions and reduces the spread of influenza. PNAS, 116(27):13174-13181, 2019.
DOI: 10.7910/dvn/iwmh4t/iqthxi
title: lobby_outcomes_v3_all.tab

description: :unav
DOI: 10.7910/dvn/iwmh4t/k3n9ni
title: lobby_outcomes_v3_hilo.tab

description: :unav
DOI: 10.7910/dvn/iwmh4t/km0wly
title: Categorical_EPU_Data.tab

description: :unav
DOI: 10.7910/dvn/iwmh4t/oc1avm
title: lobby_outcomes_v3_50.tab

description: :unav
DOI: 10.7910/dvn/iwmh4t/qqwx2c
title: matched_HouseCandidates_Vote_LobbyistIDs_v5.tab

description: :unav
DOI: 10.7910/dvn/iwmh4t/su9y1m
title: rev_door_dstats.tab

description: :unav
DOI: 10.7910/dvn/iwmh4t/u6hfqg
title: analyze_officeholder_lobbying.do

description: :unav
DOI: 10.7910/dvn/iwmh4t/zvj5im
title: lobbyist_final_all_covs.tab

description: :unav
DOI: 10.25919/5cf2c34592b36
title: Parkes observations for project P456 semester 2019APRS_27

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.3236856
title: Dataset for strain-localisation in  helium implanted tungsten: CPFE, Laue diffraction, AFM

description: The folder includes dataset for helium-implanted tungsten and pure tungsten. The data includes measurement of the following for both materials  as observed experimentally, and predicted using crystal-plasticity simulations:

1. Surface morphology of nano-indents,

2. Lattice-distortions around and under nano-indents

3. Computed geometrically necessary dislocations field around and under nano-indents in both materials

4. Load-displacement curves

Guidelines for using dataset:

1. Extracting the folder will generate five individual folders

2. In the AFM plots folder, use the matlab code and dataset in the the folder to generate the surface morphology of nano-indents.

3. In the "CPFE implanted sample data" folder --&gt; use "CPFE implanted matlab code" --&gt; load "variables2" --&gt; run the code (raw data is also provided in the folder)

4. In the "CPFE unimplanted sample data" folder --&gt; use "CPFE unimp matlab code" --&gt; load "variables3" --&gt; run the code (raw data is also provided in the folder)

5. In the "Laue unimplanted data" folder --&gt; use matlab code with relevant raw data provided in folder

6. In the "Laue implanted data" folder --&gt; use matlab code with relevant raw data provided in folder

7. Excel sheet provides nano-indentation and CPFE predictions of load-displacement curves

8. The folder "HR-EBSD code and data" includes related raw data and codes.
DOI: 10.5281/zenodo.3236857
title: Dataset for helium implanted tungsten: CPFE, Laue diffraction, AFM

description: The folder includes dataset for helium-implanted tungsten and pure tungsten. The data includes measurement of the following for both materials  as observed experimentally, and predicted using crystal-plasticity simulations:

1. Surface morphology of nano-indents,

2. Lattice-distortions around and under nano-indents

3. Computed geometrically necessary dislocations field around and under nano-indents in both materials

4. Load-displacement curves

Guidelines for using dataset:

1. Extracting the folder will generate five individual folders

2. In the AFM plots folder, use the matlab code and dataset in the the folder to generate the surface morphology of nano-indents.

3. In the "CPFE implanted sample data" folder --&gt; use "CPFE implanted matlab code" --&gt; load "variables2" --&gt; run the code (raw data is also provided in the folder)

4. In the "CPFE unimplanted sample data" folder --&gt; use "CPFE unimp matlab code" --&gt; load "variables3" --&gt; run the code (raw data is also provided in the folder)

5. In the "Laue unimplanted data" folder --&gt; use matlab code with relevant raw data provided in folder

6. In the "Laue implanted data" folder --&gt; use matlab code with relevant raw data provided in folder

7. Excel sheet provides nano-indentation and CPFE predictions of load-displacement curves
DOI: 10.21227/3axa-an23
title: Antenna simulation and measurement_01

description: These files contain all the simulated and measured dataset for the paper entitled "Design and measurement of a high gain V-fed dipole antenna," which was submitted to IEEE Antennas and Wireless Propagation Letters in 2019.All the simulation data were obtained using FEKO, and those were imported and visualized using MATLAB.The scattering parameters of the antenna were measured using Keysight E8362B vector network analyzer, while the gain patterns were measured in the anechoic chamber.
DOI: 10.21227/77ex-wf32
title: Antenna simulation and measurement_01

description: These filesare the dataset of the antenna simulation and measurement.All the simulation data were obtained using FEKO, and those were imported and visualized using MATLAB.The scattering parameters of the antenna were measured using Keysight E8362B vector network analyzer, while the gain patterns were measured in the anechoic chamber.
DOI: 10.5281/zenodo.3234218
title: Laser Disdrometer Particle Size and Velocities Distributions Raw data (2014-2017) for Melbourne, Australia

description: This dataset includes raw data obtained from Laser Disdrometers installed in the proximity of Melbourne, Australia. It includes data from 2 Thies LPM and 2 OTT Parsivel. The description of this dataset as well as a first step in the processing are described in Guyot et al. (under review) at Hydrology and Earth Sciences Systems (publisher EGU) under an open-source Discussion format.
DOI: 10.5281/zenodo.3234217
title: Laser Disdrometer Particle Size and Velocities Distributions Raw data (2014-2017) for Melbourne, Australia

description: This dataset includes raw data obtained from Laser Disdrometers installed in the proximity of Melbourne, Australia. It includes data from 2 Thies LPM and 2 OTT Parsivel. The description of this dataset as well as a first step in the processing are described in Guyot et al. (under review) at Hydrology and Earth Sciences Systems (publisher EGU) under an open-source Discussion format.
DOI: 10.5281/zenodo.3237001
title: Data for "Temporal and Spatial Characteristics of Preliminary Breakdown Pulses in Intracloud Lightning Flashes"

description: In the manuscript entitled "Temporal and Spatial Characteristics of Preliminary Breakdown Pulses in Intracloud Lightning Flashes", the corresponding data is provided in the following attachment. These files can be opened by Matlab 2016 (or later).
DOI: 10.5281/zenodo.3237002
title: Data for "Temporal and Spatial Characteristics of Preliminary Breakdown Pulses in Intracloud Lightning Flashes"

description: In the manuscript entitled "Temporal and Spatial Characteristics of Preliminary Breakdown Pulses in Intracloud Lightning Flashes", the corresponding data is provided in the following attachment. These files can be opened by Matlab 2016 (or later).
DOI: 10.25919/5cf39df54138f
title: Parkes observations for project P985 semester 2019APRS_05

description: We propose to use the ultra-wide-bandwidth, low frequency receiver installed at the Parkes telescope in order to quantify the broad-band intermittency time scale, polarization, quasi-periodicities, and mode changing of a newly discovered pulsar, PSR J1926-0653. The pulsar is unique in its emission properties. It has multiple pulse components, that change with time (both mode- changing and sub-pulse drifting phenomena are evident). The pulsar exhibits nulls in which a few individual pulses seem to be missing. It also exhibits longer-scale (hour-scale) intermittency behaviour in which the emission switches off for long periods of time. The pulse flux densities often, but not always, seem to exhibit quasi-periodic variations. Clearly this pulsar may hold the key to many different emission phenomena and we request time on Parkes, FAST and ATCA to parameterise the pulsar and its emission properties in detail.
DOI: 10.25919/5cf39eaf8baf9
title: Parkes observations for project P1011 semester 2019APRS_10

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: 10.5281/zenodo.3237266
title: UK Biobank GWAS of WHRadjBMI in combined, women only, and men only

description: GWAS of WHRadjBMI in UK Biobank. GWAS was performed in BOLT-LMM and full details can be found here: https://www.ncbi.nlm.nih.gov/pubmed/30239722 (the paper is open access). Columns: SNP, SNP identifier CHR, chromosome BP, position (hg19) GENPOS, genetic position ALLELE1, tested allele ALLELE0, other allele A1FREQ, frequency of the tested allele INFO, imputation quality (info score) CHISQ_LINREG, chi-square from linear regression P_LINREG, p-value from linear regression BETA, beta (effect) from the linear mixed model SE, standard error from the linear mixed model CHISQ_BOLT_LMM_INF, chi-square from linear mixed model P_BOLT_LMM_INF, p-value from the linear mixed model
DOI: 10.5281/zenodo.3237267
title: UK Biobank GWAS of WHRadjBMI in combined, women only, and men only

description: GWAS of WHRadjBMI in UK Biobank. GWAS was performed in BOLT-LMM and full details can be found here: https://www.ncbi.nlm.nih.gov/pubmed/30239722 (the paper is open access). Columns: SNP, SNP identifier CHR, chromosome BP, position (hg19) GENPOS, genetic position ALLELE1, tested allele ALLELE0, other allele A1FREQ, frequency of the tested allele INFO, imputation quality (info score) CHISQ_LINREG, chi-square from linear regression P_LINREG, p-value from linear regression BETA, beta (effect) from the linear mixed model SE, standard error from the linear mixed model CHISQ_BOLT_LMM_INF, chi-square from linear mixed model P_BOLT_LMM_INF, p-value from the linear mixed model
DOI: 10.5281/zenodo.3237281
title: Chemical Profiles of Shexiang Tongxin Dropping Pill Based on HPLC Fingerprints Combined with HPLC-Q-TOF-MSMS Method

description: supporting information
DOI: 10.5281/zenodo.3237282
title: Chemical Profiles of Shexiang Tongxin Dropping Pill Based on HPLC Fingerprints Combined with HPLC-Q-TOF-MSMS Method

description: supporting information
DOI: 10.5281/zenodo.3237210
title: 2014 US National Emissions Inventory data

description: This is the emissions dataset used in the following publication:

Inequity in consumption of goods and services adds to racial–ethnic disparities in air pollution exposure. Christopher W. Tessum, Joshua S. Apte, Andrew L. Goodkind, Nicholas Z.Muller, Kimberley A. Mullins, David A. Paolella, Stephen Polasky, Nathaniel P. Springer, Sumil K. Thakrar, Julian D. Marshall, Jason D. Hill. <em>Proceedings of the National Academy of Sciences.</em> 2019, 116 (13) 6001-6006; DOI:10.1073/pnas.1818859116

All data is originally from the U.S. Environmental Protection Agency and is subject to any licenses or restrictions applicable to the original data. The dataset is reproduced here for archival purposes.
DOI: 10.5281/zenodo.3237211
title: 2014 US National Emissions Inventory data

description: This is the emissions dataset used in the following publication:

Inequity in consumption of goods and services adds to racial–ethnic disparities in air pollution exposure. Christopher W. Tessum, Joshua S. Apte, Andrew L. Goodkind, Nicholas Z.Muller, Kimberley A. Mullins, David A. Paolella, Stephen Polasky, Nathaniel P. Springer, Sumil K. Thakrar, Julian D. Marshall, Jason D. Hill. <em>Proceedings of the National Academy of Sciences.</em> 2019, 116 (13) 6001-6006; DOI:10.1073/pnas.1818859116

All data is originally from the U.S. Environmental Protection Agency and is subject to any licenses or restrictions applicable to the original data. The dataset is reproduced here for archival purposes.
DOI: 10.21227/cjw6-rm59
title: Saudi Dialect Twitter Corpus (SDTwittC)

description: SDTwittC consists of 200 authors evenly balanced by gender (100 for each). We identified the gender of the tweeters via their names and profile pictures. As potential copy-and-paste texts, both tweets and retweets are discarded in the first place. Only replies are compiled. The number of replies for each author varies from hundreds to thousands. Male authors produced 233926 replies whereas 219740 replies are generated by the female group
DOI: 10.21227/ekmr-e053
title: Saudi Dialect Twitter Corpus (SDTwittC)

description: SDTwittC consists of 200 authors evenly balanced by gender (100 for each). We identified the gender of the tweeters via their names and profile pictures. As potential copy-and-paste texts, both tweets and retweets are discarded in the first place. Only replies are compiled. The number of replies for each author varies from hundreds to thousands. Male authors produced 233926 replies whereas 219740 replies are generated by the female group
DOI: 10.5281/zenodo.2653962
title: Early-Universe Simulations of the Cosmological Axion: Supplementary Data

description: Public release of the axion field state obtained through simulations of the post-inflationary QCD axion as performed in "Early-Universe Simulations of the Cosmological Axion," from arXiv:1906.00967v1[astro-ph.CO].

This dataset should enable researchers to construct density fields for gravitational simulations for axion structure formation. Alternatively, it provides initial conditions for the further evolution of a realistic axion field configuration to arbitrary late times under classical field dynamics. For detailed instructions regarding the data formatting, units, and density field construction, see README.pdf.
DOI: 10.5281/zenodo.2653964
title: Early-Universe Simulations of the Cosmological Axion: Supplementary Data

description: Public release of the axion field state obtained through simulations of the post-inflationary QCD axion as performed in "Early-Universe Simulations of the Cosmological Axion," from arXiv:1906.00967v1[astro-ph.CO].

This dataset should enable researchers to construct density fields for gravitational simulations for axion structure formation. Alternatively, it provides initial conditions for the further evolution of a realistic axion field configuration to arbitrary late times under classical field dynamics. For detailed instructions regarding the data formatting, units, and density field construction, see README.pdf.
DOI: 10.25919/5cf3a837bd151
title: Parkes observations for project P1011 semester 2019APRS_11

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: 10.7910/dvn/tsbhic/bfetcz
title: ReplicationDataset.tab

description: :unav
DOI: 10.7910/dvn/tsbhic/e7vzfe
title: Replication do-file.do

description: :unav
DOI: 10.7910/dvn/tsbhic/wywxra
title: SpendingData_countryyear.tab

description: :unav
DOI: 10.7910/dvn/tsbhic/0mmyq6
title: Contracts_2000-2003.tab

description: :unav
DOI: 10.7910/dvn/tsbhic/2n3lnp
title: Contracts_2004-2007.tab

description: :unav
DOI: 10.7910/dvn/tsbhic/61tp6q
title: ReadMe.txt

description: :unav
DOI: 10.7910/dvn/tsbhic/cem5yx
title: Contracts_2008-2011.tab

description: :unav
DOI: 10.7910/dvn/tsbhic/cetjmi
title: Contracts_2012-2015.tab

description: :unav
DOI: 10.7910/dvn/tsbhic/en8twj
title: BlankenshipJoyce_ProcurementSpending_Codebook.pdf

description: :unav
DOI: 10.7910/dvn/tsbhic/kaksn6
title: Africa location coding.do

description: :unav
DOI: 10.7910/dvn/tsbhic/y2t4f1
title: Contracts_Africa.tab

description: :unav
DOI: 10.5281/zenodo.3237016
title: Biocrusts on dryland road slopes

description: Biocrust abundance on dryland road slopes and associated environmental variables
DOI: 10.5281/zenodo.3237017
title: Biocrusts on dryland road slopes

description: Biocrust abundance on dryland road slopes and associated environmental variables
DOI: 10.25919/5cf3b5614307a
title: Parkes observations for project P456 semester 2019APRS_33

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: 10.15468/hqzdc1
title: Lestes secula, a new species of damselfly (Odonata: Zygoptera: Lestidae) from Panama

description: This dataset contains the digitized treatments in Plazi based on the original journal article May, M. L. (1993): Lestes secula, a new species of damselfly (Odonata: Zygoptera: Lestidae) from Panama. J. New York Entomol. Soc. 101: 410-416, DOI: 10.5281/zenodo.3237470
DOI: 10.18716/nmrshiftdb2/30001353
title: NMR data for borane
DOI: 10.5281/zenodo.3234779
title: The Aerial Elephant Dataset

description: Aerial surveying is a key tool for effective wildlife management. However, the high costs associated with large scale surveys means that this tool is often underutilized. We believe that computer vision can be used to dramatically decrease the costs associated with surveying, while at the same time improving the consistency of results. We present the Aerial Elephant Dataset, a challenging dataset to enable research on game detection under real-world conditions. The dataset consists of 2 074 images containing a total of 15 581 African bush elephants in their natural habitats, imaged with a consistent methodology over a range of background types, resolutions and times-of-day.
DOI: 10.5281/zenodo.3234780
title: The Aerial Elephant Dataset

description: Aerial surveying is a key tool for effective wildlife management. However, the high costs associated with large scale surveys means that this tool is often underutilized. We believe that computer vision can be used to dramatically decrease the costs associated with surveying, while at the same time improving the consistency of results. We present the Aerial Elephant Dataset, a challenging dataset to enable research on game detection under real-world conditions. The dataset consists of 2 074 images containing a total of 15 581 African bush elephants in their natural habitats, imaged with a consistent methodology over a range of background types, resolutions and times-of-day.
DOI: 10.5519/qd.v74mi5j8
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1304 records)
DOI: 10.7910/dvn/dkesrc/5mjmk1
title: uspto.citation.1926-1975.tab

description: :unav
DOI: 10.7910/dvn/dkesrc/63jizs
title: uspto.ocr.1926-1975.z04

description: :unav
DOI: 10.7910/dvn/dkesrc/8hg0dq
title: uspto.ocr.1926-1975.z01

description: :unav
DOI: 10.7910/dvn/dkesrc/95l6wp
title: uspto.govt.reliance.category.tab

description: :unav
DOI: 10.7910/dvn/dkesrc/dp2ejd
title: uspto.govt.reliance.statistics.tsv

description: :unav
DOI: 10.7910/dvn/dkesrc/sfqijh
title: uspto.govt.reliance.metadata.tsv

description: :unav
DOI: 10.7910/dvn/dkesrc/st0e2p
title: uspto.ocr.1926-1975.z03

description: :unav
DOI: 10.7910/dvn/dkesrc/vaqvjg
title: command

description: This SQL script generates "	uspto.govt.reliance.statistics.tsv" from 	"uspto.govt.reliance.metadata.tsv"
DOI: 10.7910/dvn/dkesrc/yg0o7i
title: uspto.ocr.1926-1975.zip

description: OCRed raw texts from the USPTO Image Files in PDF.  Due to the DVN single file size limit, we had to split the zip into six chunks.  Please put uspto.ocr.1926-1975.zip as well as uspto.ocr.1926-1975.z0[1-5] under the same folder, so the unzipper can extract all raw texts without running into an error.