cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.6227390
title: Full Datasets for the "Molecular Mimicry Map of SARS-CoV-2" Web Application

description: A Full Dataset for the "Molecular Mimicry Map of SARS-CoV-2" Web Application This TAR archive file contains the minimally filtered list of potentially cross-reactive epitopes of SARS-CoV-2 and human proteins predicted by the CRESSP analysis pipeline (https://pypi.org/project/cressp/). Our web application, "Molecular Mimicry Map of SARS-CoV-2" (https://ahs2202.github.io/3M/), only visualizes the high-scoring potential cross-reactive epitope pairs (40,000 epitope pairs maximum). However, for the researchers who want to access the complete list of potentially cross-reactive epitope pairs for further analysis, these full datasets can be used.
description: For the descriptions of the columns of this dataset, please refer to the documentation of our web application (https://ahs2202.github.io/3M/documentation/)
DOI: 10.5281/zenodo.6227389
title: Full Datasets for the "Molecular Mimicry Map of SARS-CoV-2" Web Application

description: A Full Dataset for the "Molecular Mimicry Map of SARS-CoV-2" Web Application This TAR archive file contains the minimally filtered list of potentially cross-reactive epitopes of SARS-CoV-2 and human proteins predicted by the CRESSP analysis pipeline (https://pypi.org/project/cressp/). Our web application, "Molecular Mimicry Map of SARS-CoV-2" (https://ahs2202.github.io/3M/), only visualizes the high-scoring potential cross-reactive epitope pairs (40,000 epitope pairs maximum). However, for the researchers who want to access the complete list of potentially cross-reactive epitope pairs for further analysis, these full datasets can be used.
description: For the descriptions of the columns of this dataset, please refer to the documentation of our web application (https://ahs2202.github.io/3M/documentation/)
DOI: 10.5281/zenodo.6413272
title: DataSet Inmobiliario

description: Datos obtenidos mediante un proceso de Web Scraping a la pagina web https://www.inmovision.com.ec/
DOI: 10.5281/zenodo.6413271
title: DataSet Inmobiliario

description: Datos obtenidos mediante un proceso de Web Scraping a la pagina web https://www.inmovision.com.ec/
DOI: 10.5281/zenodo.6409813
title: GSM896803.bam

description: GSM896803.bam
DOI: 10.5281/zenodo.6409812
title: GSM896803.bam

description: GSM896803.bam
DOI: 10.5281/zenodo.6409374
title: Erythroxylum coriaceum decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6409373
title: Erythroxylum coriaceum decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6408522
title: Leptodoras oyakawai decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6408483
title: Geranospiza caerulescens decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6408521
title: Leptodoras oyakawai decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6408482
title: Geranospiza caerulescens decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6408400
title: Elanoides forficatus decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6408399
title: Elanoides forficatus decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6408364
title: Rostrhamus sociabilis decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6408363
title: Rostrhamus sociabilis decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6408348
title: Polyboroides typus decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6408347
title: Polyboroides typus decontaminated FSCR

description: .
DOI: 10.5281/zenodo.6406278
title: Molecular Genetic Analysis of SARS-CoV-2 Lineages in Armenia - additional data

description: Sequencing of SARS-CoV-2 provides essential information on viral evolution, transmission, and epidemiology. In this study, we performed whole-genome sequencing of SARS-CoV-2 using nanopore and Illumina short-read sequencing to describe the circulation of the virus lineage in Armenia. This dataset contains Nextstrain configuration files, the auspice JSON file, BEAST output logs, and trees files, and resulting log and tree files as well as R scripts and data files used in phylogenetic and functional analyses.
DOI: 10.5281/zenodo.6406277
title: Molecular Genetic Analysis of SARS-CoV-2 Lineages in Armenia - additional data

description: Sequencing of SARS-CoV-2 provides essential information on viral evolution, transmission, and epidemiology. In this study, we performed whole-genome sequencing of SARS-CoV-2 using nanopore and Illumina short-read sequencing to describe the circulation of the virus lineage in Armenia. This dataset contains Nextstrain configuration files, the auspice JSON file, BEAST output logs, and trees files, and resulting log and tree files as well as R scripts and data files used in phylogenetic and functional analyses.
DOI: 10.6084/m9.figshare.19527712
title: Factors Affecting Decision-making in Gaelic Football: A Focus Group Approach

description: Using a focus group approach, this study identified four factors that affect the decision-making processes of expert Gaelic Football players. Three factors were information sources used to make the decisions: <i>pre-match context, current match context and visual information</i>. The decision-making process itself was moderated by the final theme, <i>individual differences</i>.
DOI: 10.6084/m9.figshare.19527712.v1
title: Factors Affecting Decision-making in Gaelic Football: A Focus Group Approach

description: Using a focus group approach, this study identified four factors that affect the decision-making processes of expert Gaelic Football players. Three factors were information sources used to make the decisions: <i>pre-match context, current match context and visual information</i>. The decision-making process itself was moderated by the final theme, <i>individual differences</i>.
DOI: 10.34740/kaggle/dsv/3418018
title: Russian Invasion of Ukraine
DOI: 10.6073/pasta/bfdaf2eb56c99e6369b4a58467ed3ed3
title: CAP LTER weather stations at Papago Park and Lost Dutchman State Park in the greater Phoenix metropolitan area, ongoing since 2010

description: The CAP LTER maintains two micrometeorological stations (10-m height) in the greater Phoenix metropolitan area, including at Lost Dutchman State Park and near the Desert Botanical Garden at Papago Park. The local terrain at both sites is flat or gently sloping Sonoran desert, and the vegetation canopy consists of patchy coverage of desert shrubs and trees. The dominant vegetation species include bursage (*Ambrosia deltoidea*) and creosote bush (*Larrea tridentata*), while minor species include palo verde (*Parkinsonia microphylla*) and saguaro cactus (*Carnegiea gigantea*). Wind speed and direction, incoming solar radiation, air temperature, relative humidity, and precipitation have been monitored nearly continuously since the fall of 2010. Each variable is measured every 5 seconds and the average (or total for precipitation and total solar radiation) saved to a data logger every 10 minutes.
DOI: 10.25606/surf.e6ce5ae52bd1dcf2
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P334+23)

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 P334+23.
DOI: 10.5281/zenodo.6418643
title: Verkehrsperspektiven 2050: VISUM-Versionen (Strassenverkehr), DWV, Szenario BASIS 2030/2040/2050

description: Transport model versions in the transport planning software VISUM containing road transport volumes on networks of the average workday traffic (monday-friday, so called DWV, Scenario BASIS).
DOI: 10.5281/zenodo.6419024
title: Understanding the Influence of Receptive Field and Network Complexity in Neural-Network-Guided TEM Image Analysis

description: TEM images of Au nanoparticles of various sizes on ultra-thin carbon substrates and their corresponding labels for semantic segmentation. The images have a dataset label of "images" and the labels have a dataset label of "labels".
DOI: 10.5281/zenodo.6419023
title: Understanding the Influence of Receptive Field and Network Complexity in Neural-Network-Guided TEM Image Analysis

description: TEM images of Au nanoparticles of various sizes on ultra-thin carbon substrates and their corresponding labels for semantic segmentation. The images have a dataset label of "images" and the labels have a dataset label of "labels".
DOI: 10.5281/zenodo.6419675
title: Modelled data - Energy Transition in Bolivia

description: Model structure, input data and output files from MoManI
DOI: 10.5281/zenodo.6419674
title: Modelled data - Energy Transition in Bolivia

description: Model structure, input data and output files from MoManI
DOI: 10.6084/m9.figshare.3761562.v2180
title: Online Labour Index: Measuring the Online Gig Economy for Policy and Research

description: Data repository for the data underlying the Online Labour Index. See http://ilabour.oii.ox.ac.uk online-labour-index/ for details.
DOI: 10.25606/surf.42ec7216bcc568d2
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P116+34)

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 P116+34.
DOI: 10.25606/surf.d93c933f728241a7
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P13Hetdex12)

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 P13Hetdex12.
DOI: 10.25606/surf.9acd87c6ebec4b7f
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P154+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 P154+35.
DOI: 10.25606/surf.671f263a1965bb9f
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P169+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 P169+35.
DOI: 10.25606/surf.54e26c11dfb80e63
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P188+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 P188+35.
DOI: 10.25606/surf.faeab288db18e404
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P241+65)

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 P241+65.