cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.6418105
title: Dataset for "WUS256: An Adjoint Waveform Tomography Model of the Crust and Upper Mantle of the Western United States for Improved Waveform Simulations"

description: This dataset contains the WUS256 seismic model and auxiliary data used in the creation of the model (Rodgers et al., 2022). WUS256 is a three-dimensional model of the seismic properties of crust and upper mantle of the western United States. The WUS256 model is provided in NetCDF format (readable by for example, <em>xarray</em>, Hoyer & Hamman, 2017) and HDF5 format for viewing with <em>ParaView</em> (Ahrens et al., 2005) and interaction with <em>Salvus</em> (Afanasiev et al., 2019). Also included are the earthquake source parameters for the 72 inversion events and 18 validation events in ASCII text format. Lastly, we include a list of all waveforms used in the creation of WUS256. This is a simple ASCII file with the event name and receiver name (composed of the network_code and station_code). This effort was support by Lawrence Livermore National Laboratory’s Laboratory Directed Research and Development project 20-ERD-008. This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344. LLNL-MI-833624
DOI: 10.5281/zenodo.6418104
title: Dataset for "WUS256: An Adjoint Waveform Tomography Model of the Crust and Upper Mantle of the Western United States for Improved Waveform Simulations"

description: This dataset contains the WUS256 seismic model and auxiliary data used in the creation of the model (Rodgers et al., 2022). WUS256 is a three-dimensional model of the seismic properties of crust and upper mantle of the western United States. The WUS256 model is provided in NetCDF format (readable by for example, <em>xarray</em>, Hoyer & Hamman, 2017) and HDF5 format for viewing with <em>ParaView</em> (Ahrens et al., 2005) and interaction with <em>Salvus</em> (Afanasiev et al., 2019). Also included are the earthquake source parameters for the 72 inversion events and 18 validation events in ASCII text format. Lastly, we include a list of all waveforms used in the creation of WUS256. This is a simple ASCII file with the event name and receiver name (composed of the network_code and station_code). This effort was support by Lawrence Livermore National Laboratory’s Laboratory Directed Research and Development project 20-ERD-008. This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344. LLNL-MI-833624
DOI: 10.5063/f1445jxp
title: Reproductive consequences of shrub association, artificial herbivory, and supplemental pollination for Malacothrix glabrata in the Mojave Desert.

description: We tested the effects of shrub facilitation, two types of artificial herbivory (folivory and florivory), and supplemental pollination on floral production and seed set of Malacothrix glabrata in the Mojave Desert.
DOI: 10.5517/ccdc.csd.cc1mvjxx
title: CCDC 1515060: Experimental Crystal Structure Determination

description: Related Article: T. Hannah Clara, Johanan Christian Prasana, D. Reuben Jonathan, V. Vishwanathan|2022|J.Mol.Struct.|1261|132942|doi:10.1016/j.molstruc.2022.132942
DOI: 10.5517/ccdc.csd.cc27mkp4
title: CCDC 2074386: Experimental Crystal Structure Determination

description: Related Article: Pilar Narea, Benjamín Hernández, Jonathan Cisterna, Alejandro Cárdenas, Jaime Llanos, Pilar Amo-Ochoa, Félix Zamora, José Luis Priego, Miguel Cortijo, Gerzon E. Delgado, Iván Brito|2022|J.Solid State Chem.|310|123027|doi:10.1016/j.jssc.2022.123027
DOI: 10.5517/ccdc.csd.cc27mkq5
title: CCDC 2074387: Experimental Crystal Structure Determination

description: Related Article: Pilar Narea, Benjamín Hernández, Jonathan Cisterna, Alejandro Cárdenas, Jaime Llanos, Pilar Amo-Ochoa, Félix Zamora, José Luis Priego, Miguel Cortijo, Gerzon E. Delgado, Iván Brito|2022|J.Solid State Chem.|310|123027|doi:10.1016/j.jssc.2022.123027
DOI: 10.5517/ccdc.csd.cc27mkr6
title: CCDC 2074388: Experimental Crystal Structure Determination

description: Related Article: Pilar Narea, Benjamín Hernández, Jonathan Cisterna, Alejandro Cárdenas, Jaime Llanos, Pilar Amo-Ochoa, Félix Zamora, José Luis Priego, Miguel Cortijo, Gerzon E. Delgado, Iván Brito|2022|J.Solid State Chem.|310|123027|doi:10.1016/j.jssc.2022.123027
DOI: 10.5281/zenodo.6419097
title: OMEN data set: Tokheim pancancer data set with genome-wide interaction network

description: OMEN is a Network-based Driver Gene Identification method that exploits Mutual Exclusivity.<br> This repository stores the data used in a pancancer experiment showcasing this method. It consists of - [tokheim_pancancer_somatic_CADD.pl] A file containing CADD probabilities for gene-patient pairs (derived from the pancancer data set in Tokheim, Collin J., et al. "Evaluating the evaluation of cancer driver genes." <em>Proceedings of the National Academy of Sciences</em> 113.50 (2016): 14330-14335.) formatted to be used by OMEN.<br> - [tokheim_pancancer_somatic_coverage_ranks.pl] A file containing gene coverage data (derived from the CADD data) formatted to be used by OMEN.<br> - [network.pl] A file containing a genome-wide interaction network consisting of high quality metabolic interactions from Recon X and literature curated interactions from Intact. Recon X and Intact data was acquired from Pathway Commons version 8.<br> The resulting network covers 7901 samples, and contains 15.694 nodes and 178.051 edges.
DOI: 10.5281/zenodo.6419096
title: OMEN data set: Tokheim pancancer data set with genome-wide interaction network

description: OMEN is a Network-based Driver Gene Identification method that exploits Mutual Exclusivity.<br> This repository stores the data used in a pancancer experiment showcasing this method. It consists of - [tokheim_pancancer_somatic_CADD.pl] A file containing CADD probabilities for gene-patient pairs (derived from the pancancer data set in Tokheim, Collin J., et al. "Evaluating the evaluation of cancer driver genes." <em>Proceedings of the National Academy of Sciences</em> 113.50 (2016): 14330-14335.) formatted to be used by OMEN.<br> - [tokheim_pancancer_somatic_coverage_ranks.pl] A file containing gene coverage data (derived from the CADD data) formatted to be used by OMEN.<br> - [network.pl] A file containing a genome-wide interaction network consisting of high quality metabolic interactions from Recon X and literature curated interactions from Intact. Recon X and Intact data was acquired from Pathway Commons version 8.<br> The resulting network covers 7901 samples, and contains 15.694 nodes and 178.051 edges.
DOI: 10.3886/e114542v1-114380
title: Replication data for: Housing, Health, and Happiness

description: We investigate the impact of a large-scale Mexican program to replace dirt floors with cement floors on child health and adult happiness. We find that replacing dirt floors with cement significantly improves the health of young children measured by decreases in the incidence of parasitic infestations, diarrhea, and the prevalence of anemia, and an improvement in children's cognitive development. Additionally, we find significant improvements in adult welfare measured by increased satisfaction with their housing and quality of life, as well as by lower scores on depression and perceived stress scales. (JEL I12, I31, J13, O15)
DOI: 10.5066/p9j2mclj
title: Population genetic analysis of the snake-infecting fungus, Ophidiomyces ophidiicola, in the eastern United States

description: Snake fungal disease (SFD; ophidiomycosis), caused by the pathogen Ophidiomyces ophidiicola (Oo), has been documented in wild snakes in North America and Eurasia, and is a potentially emerging disease in the eastern USA. However, a lack of historical disease data has made it challenging to determine whether Oo is a recent arrival to the USA or whether SFD emergence is due to other factors. Here, we examined the genomes of 82 Oo strains to determine the pathogen's history in the eastern USA. This dataset contains metadata on the strains used in that study.
DOI: 10.5281/zenodo.6418651
title: Data from: Even low light pollution levels affect the spatial distribution and timing of activity of a "light tolerant" bat species

description: Abstract of the related publication : By disrupting nocturnal landscapes worldwide, light pollution caused by Artificial Light At Night (ALAN) is recognised as a major threat to biodiversity. As even low light intensities might affect some taxa, concerns are arising about biological responses to widespread low light levels. We used data from a French citizen science bat monitoring program (1,894 full-nights monitored on 1,055 sites) to explore the landscape-scale effects of light on an open-space-foraging bat species, the Serotine bat (<em>Eptesicus serotinus</em>). We assessed this species' abundance and timing of night-time activity (median time of activity) at foraging sites. ALAN, and to a lesser extent moonlight, reduced <em>E. serotinus</em> abundance. ALAN delayed activity, and this delay was amplified during overcast nights. On the contrary, where there was no ALAN, the higher the cloud cover, the earlier the activity occurred. Cloud cover likely darkened the night sky in rural locations, whereas it amplified skyglow in light-polluted places, increasing ALAN effects on bats. Interestingly, moonlight also delayed activity but this effect was weakened where there was ALAN. Our study shows that even fine variations of light levels could affect the spatiotemporal distribution of a common species usually considered to be “light tolerant”, with potential cascading effects on individual fitness and population dynamics. It stresses how urgent it is to preserve and restore dark areas to protect biodiversity from light pollution while working on light intensity and directivity where ALAN is needed.
DOI: 10.5281/zenodo.6418650
title: Data from: Even low light pollution levels affect the spatial distribution and timing of activity of a "light tolerant" bat species

description: Abstract of the related publication : By disrupting nocturnal landscapes worldwide, light pollution caused by Artificial Light At Night (ALAN) is recognised as a major threat to biodiversity. As even low light intensities might affect some taxa, concerns are arising about biological responses to widespread low light levels. We used data from a French citizen science bat monitoring program (1,894 full-nights monitored on 1,055 sites) to explore the landscape-scale effects of light on an open-space-foraging bat species, the Serotine bat (<em>Eptesicus serotinus</em>). We assessed this species' abundance and timing of night-time activity (median time of activity) at foraging sites. ALAN, and to a lesser extent moonlight, reduced <em>E. serotinus</em> abundance. ALAN delayed activity, and this delay was amplified during overcast nights. On the contrary, where there was no ALAN, the higher the cloud cover, the earlier the activity occurred. Cloud cover likely darkened the night sky in rural locations, whereas it amplified skyglow in light-polluted places, increasing ALAN effects on bats. Interestingly, moonlight also delayed activity but this effect was weakened where there was ALAN. Our study shows that even fine variations of light levels could affect the spatiotemporal distribution of a common species usually considered to be “light tolerant”, with potential cascading effects on individual fitness and population dynamics. It stresses how urgent it is to preserve and restore dark areas to protect biodiversity from light pollution while working on light intensity and directivity where ALAN is needed.
DOI: 10.6084/m9.figshare.19529479
title: Rat microbiome data

description: rat microbiome data source
DOI: 10.6084/m9.figshare.19529479.v1
title: Rat microbiome data

description: rat microbiome data source
DOI: 10.6084/m9.figshare.19529494
title: CRUD-Bolt Questionnaire Survey for MSc Computer Systems Thesis.csv

description: The data is as a result of a study done by the title An Enhanced Automatic Generation of CRUD Operations in React-JS. The tool coined CRUD-Bolt that would achieve automatic create, retrieve, update and delete operations in React-JS was shared amongst React-JS developers who tested it and filled a survey via Google Forms. This data is the result of those happenings.
DOI: 10.6084/m9.figshare.19529512
title: dataset06-04-22:48

description: This is a description
DOI: 10.6084/m9.figshare.19529512.v1
title: dataset06-04-22:48

description: This is a description
DOI: 10.6084/m9.figshare.19233780.v1
title: Sorting coefficient of loess sediments is a neglected proxy for wind intensity in eastern Central Asia

description: It contains five worksheet such as Raw grain size, Bulk grain size proxy, GSD of amphibole, GSD of epidote and Ratio between Amphibole and Epidote.
DOI: 10.6084/m9.figshare.19529524
title: dataset-06-04-22:43.pt

description: This is a description
DOI: 10.6084/m9.figshare.19529524.v1
title: dataset-06-04-22:43.pt

description: This is a description
DOI: 10.25606/surf.c6fdd0ce996b6879
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P000+38)

description: In this data release from the ongoing LOw-Frequency ARray (LOFAR) Two-metre Sky Survey (LoTSS) we present 120-168 MHz images covering 27% of the northern sky. Our coverage is split into two regions centred at approximately 12h45m +44◦30′ and 1h00m +28◦ 00′ and spanning 4178 and 1457 square degrees respectively. The images were derived from 3,451 hrs (7.6 PB) of LOFAR High Band Antenna data which were corrected for the direction-independent instrumental properties as well as direction-dependent ionospheric distortions during extensive, but fully automated, data processing. A catalogue of 4,396,228 radio sources is derived from our total intensity (Stokes I) maps, where the majority of these have never been detected at radio wavelengths before. At 6′′ resolution, our full bandwidth Stokes I continuum maps with a central frequency of 144 MHz have: a median rms sensitivity of 83 μ Jy/beam; a flux density scale accuracy of approximately 10%; an astrometric accuracy of 0.2′′; and we estimate the point-source completeness to be 90% at a peak brightness of 0.8 mJy/beam. By creating three 16 MHz bandwidth images across the band we are able to measure the in-band spectral index of many sources, albeit with an error on the derived spectral index of &gt; ±0.2 which is a consequence of our flux-density scale accuracy and small fractional bandwidth. Our circular polarisation (Stokes V) 20′′ resolution 120-168 MHz continuum images have a median rms sensitivity of 95 μ Jy/beam, and we estimate a Stokes I to Stokes V leakage of 0.056%. Our linear polarisation (Stokes Q and Stokes U) image cubes consist of 480 97.6 kHz wide planes and have a median rms sensitivity per plane of 10.8mJy/beam at 4′ and 2.2mJy/beam at 20′′; we estimate the Stokes I to Stokes Q/U leakage to be approximately 0.2%. Here we characterise and publicly release our Stokes I, Q, U and V images in addition to the calibrated uv-data to facilitate the thorough scientific exploitation of this unique dataset. This is field P000+38.
DOI: 10.6084/m9.figshare.19233780.v2
title: Variations of the intensity of the Siberian High during the Last Glacial revealed by the sorting coefficient of loess-paleosol deposits in Eastern Central Asia

description: It contains five worksheet such as Raw grain size, Bulk grain size proxy, GSD of amphibole, GSD of epidote and Ratio between Amphibole and Epidote.
DOI: 10.6084/m9.figshare.19529539
title: dataset-06-04-22:58

description: This is a description
DOI: 10.6084/m9.figshare.19529539.v1
title: dataset-06-04-22:58

description: This is a description
DOI: 10.6084/m9.figshare.19313822
title: Cognitive Reserve, Resting EEG and Cognition

description: Cognitive reserve (CR) is the ability to adapt cognitive function to resist the onslaught of brain-related injury or the normal aging process. The underlying brain mechanisms of CR through electroencephalogram (EEG) are scarcely reported; moreover, none of them consider dynamic proxy measures of CR. We explored the association of CR with cognition and resting-state EEG in older adults using three of the most representative dynamic proxy measures of CR: intellectual ability, leisure activities, and physical activities. Eighty-eight healthy older adults aged 60-77 (58 female) were selected from previous study data. A hierarchical cluster analysis considering scores on intellectual ability, leisure activities, and physical activities classified the participants into three groups of CR: Leisure-Active (n = 31), Active-Creative (n=27) and Passive-Receptive (n=30). Differences in cognitive performance and the absolute power (AP) on six resting-state EEG factors (beta, alpha1, alpha2, gamma, theta, and delta) were examined between the CR groups. Active-Creative and Leisure-Active groups reported a higher performance on processing speed compared to the Passive-Receptive group. The Active-Creative group reported a higher performance on phonological fluency than the other two groups and showed higher performance on motor programming than the Leisure-Active group. The Leisure-Active group displayed higher AP in alpha1 than the Passive-Receptive group and higher alpha2 than the Active-Creative group. The dynamic proxy variables of CR are differently associated with cognitive performance and resting-state EEG. Implementing leisure and physical activities may promote better cognitive performance through compensation or neural efficiency mechanisms.
DOI: 10.6084/m9.figshare.19529545
title: dataset-06-04-22:50

description: This is a description
DOI: 10.6084/m9.figshare.19529545.v1
title: dataset-06-04-22:50

description: This is a description
DOI: 10.6084/m9.figshare.19529548
title: dataset-06-04-22:57

description: This is a description
DOI: 10.6084/m9.figshare.19529548.v1
title: dataset-06-04-22:57

description: This is a description
DOI: 10.6084/m9.figshare.19529551
title: dataset-06-04-22:34

description: This is a description
DOI: 10.6084/m9.figshare.19529551.v1
title: dataset-06-04-22:34

description: This is a description
DOI: 10.6084/m9.figshare.19529560
title: model-06-04-22:41

description: This is a description
DOI: 10.6084/m9.figshare.19529560.v1
title: model-06-04-22:41

description: This is a description
DOI: 10.6084/m9.figshare.19529563
title: dataset-06-04-22:19

description: This is a description
DOI: 10.6084/m9.figshare.19529563.v1
title: dataset-06-04-22:19

description: This is a description
DOI: 10.6084/m9.figshare.19529566
title: model-06-04-22:32

description: This is a description
DOI: 10.6084/m9.figshare.19529566.v1
title: model-06-04-22:32

description: This is a description
DOI: 10.25919/jzj0-ha25
title: Parkes observations for project P1068 semester 2021APRS_35

description: In the fast-moving world of Fast Radio Bursts (FRBs), the critical question of what fraction of FRBs emit repeat bursts remains unanswered. Of order 20 repeating FRBs are now known, and their spectro-temporal properties hint at differences with apparently non-repeating bursts - the poor statistics preclude a definitive diagnosis. FRB 180301 is a promising source for further study for multiple reasons: it is an active repeater similar to the FRB 121102 and the most active FRB source visible to Parkes, and it shows diverse polarization properties across the repeat bursts. We have detected multiple repeat bursts from this source in our campaign last semester. The signal-to-noise ratio (S/N) of these detections are not sufficiently significant to measure their spectro-polarimetric properties. We request Parkes observations with the UWL receiver to continue the monitoring of this FRB source in order to characterize the broadband emission properties. Some of the key goals for these future observations are: to constrain the repetition rate, identify any variation of pulse characteristics over time, measure the polarimetric properties and provide insight into the emission mechanisms. The diverse polarization angle swings in the FAST detections and significant circular polarization in the original Parkes detection indicate the progenitor is embedded in an extreme magneto-ionic environment with complex field structure that has not been seen before. Understanding these diverse polarization properties from this source could be the key to distinguish repeater sources from the apparent non-repeaters ones.
DOI: 10.6084/m9.figshare.19529542
title: DATA 209.sav

description: Death attitudes and death anxiety
DOI: 10.6084/m9.figshare.19529542.v1
title: DATA 209.sav

description: Death attitudes and death anxiety
DOI: 10.5519/qd.1k8mbydx
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (5100619 records)
DOI: 10.25606/surf.f84b574bf377e107
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P173+35)

description: In this data release from the ongoing LOw-Frequency ARray (LOFAR) Two-metre Sky Survey (LoTSS) we present 120-168 MHz images covering 27% of the northern sky. Our coverage is split into two regions centred at approximately 12h45m +44◦30′ and 1h00m +28◦ 00′ and spanning 4178 and 1457 square degrees respectively. The images were derived from 3,451 hrs (7.6 PB) of LOFAR High Band Antenna data which were corrected for the direction-independent instrumental properties as well as direction-dependent ionospheric distortions during extensive, but fully automated, data processing. A catalogue of 4,396,228 radio sources is derived from our total intensity (Stokes I) maps, where the majority of these have never been detected at radio wavelengths before. At 6′′ resolution, our full bandwidth Stokes I continuum maps with a central frequency of 144 MHz have: a median rms sensitivity of 83 μ Jy/beam; a flux density scale accuracy of approximately 10%; an astrometric accuracy of 0.2′′; and we estimate the point-source completeness to be 90% at a peak brightness of 0.8 mJy/beam. By creating three 16 MHz bandwidth images across the band we are able to measure the in-band spectral index of many sources, albeit with an error on the derived spectral index of &gt; ±0.2 which is a consequence of our flux-density scale accuracy and small fractional bandwidth. Our circular polarisation (Stokes V) 20′′ resolution 120-168 MHz continuum images have a median rms sensitivity of 95 μ Jy/beam, and we estimate a Stokes I to Stokes V leakage of 0.056%. Our linear polarisation (Stokes Q and Stokes U) image cubes consist of 480 97.6 kHz wide planes and have a median rms sensitivity per plane of 10.8mJy/beam at 4′ and 2.2mJy/beam at 20′′; we estimate the Stokes I to Stokes Q/U leakage to be approximately 0.2%. Here we characterise and publicly release our Stokes I, Q, U and V images in addition to the calibrated uv-data to facilitate the thorough scientific exploitation of this unique dataset. This is field P173+35.