cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5517/ccdc.csd.cc290yjt
title: CCDC 2116076: Experimental Crystal Structure Determination

description: Related Article: He-Qun Cai, Guang Zeng, Zi-Xin You, Chen Wang, Li-Xian Sun, Feng-Ying Bai, Yong-Heng Xing|2022|Dalton Trans.|51|5457|doi:10.1039/D2DT00067A
DOI: 10.5517/ccdc.csd.cc2914gz
title: CCDC 2116260: Experimental Crystal Structure Determination

description: Related Article: He-Qun Cai, Guang Zeng, Zi-Xin You, Chen Wang, Li-Xian Sun, Feng-Ying Bai, Yong-Heng Xing|2022|Dalton Trans.|51|5457|doi:10.1039/D2DT00067A
DOI: 10.5517/ccdc.csd.cc29zmdb
title: CCDC 2144592: Experimental Crystal Structure Determination

description: Related Article: I.G. Grosu, F. Martin, A. Turza, M. Miclaus, I. Kacso, G. Borodi|2022|Acta Crystallogr.,Sect.C:Cryst.Struct.Chem.|78|240|doi:10.1107/S2053229622002984
DOI: 10.5517/ccdc.csd.cc29zmfc
title: CCDC 2144593: Experimental Crystal Structure Determination

description: Related Article: I.G. Grosu, F. Martin, A. Turza, M. Miclaus, I. Kacso, G. Borodi|2022|Acta Crystallogr.,Sect.C:Cryst.Struct.Chem.|78|240|doi:10.1107/S2053229622002984
DOI: 10.5517/ccdc.csd.cc29zmgd
title: CCDC 2144594: Experimental Crystal Structure Determination

description: Related Article: I.G. Grosu, F. Martin, A. Turza, M. Miclaus, I. Kacso, G. Borodi|2022|Acta Crystallogr.,Sect.C:Cryst.Struct.Chem.|78|240|doi:10.1107/S2053229622002984
DOI: 10.5517/ccdc.csd.cc29zmhf
title: CCDC 2144595: Experimental Crystal Structure Determination

description: Related Article: I.G. Grosu, F. Martin, A. Turza, M. Miclaus, I. Kacso, G. Borodi|2022|Acta Crystallogr.,Sect.C:Cryst.Struct.Chem.|78|240|doi:10.1107/S2053229622002984
DOI: 10.5517/ccdc.csd.cc29zmjg
title: CCDC 2144596: Experimental Crystal Structure Determination

description: Related Article: I.G. Grosu, F. Martin, A. Turza, M. Miclaus, I. Kacso, G. Borodi|2022|Acta Crystallogr.,Sect.C:Cryst.Struct.Chem.|78|240|doi:10.1107/S2053229622002984
DOI: 10.5517/ccdc.csd.cc29zmkh
title: CCDC 2144597: Experimental Crystal Structure Determination

description: Related Article: I.G. Grosu, F. Martin, A. Turza, M. Miclaus, I. Kacso, G. Borodi|2022|Acta Crystallogr.,Sect.C:Cryst.Struct.Chem.|78|240|doi:10.1107/S2053229622002984
DOI: 10.5517/ccdc.csd.cc29zmlj
title: CCDC 2144598: Experimental Crystal Structure Determination

description: Related Article: I.G. Grosu, F. Martin, A. Turza, M. Miclaus, I. Kacso, G. Borodi|2022|Acta Crystallogr.,Sect.C:Cryst.Struct.Chem.|78|240|doi:10.1107/S2053229622002984
DOI: 10.5281/zenodo.5822484
title: DNA sequence and taxonomic gap analyses to quantify the coverage of aquatic cyanobacteria and eukaryotic microalgae in reference databases: Results of a survey in the Alpine region

description: This dataset has been prepared as part of the Interreg Alpine Space project Eco-AlpsWater (ASP569) - <em>Innovative Ecological Assessment and Water Management Strategy for the Protection of Ecosystem Services in Alpine Lakes and Rivers</em>, https://www.alpine-space.eu/projects/eco-alpswater/en/home Individual archives include 16S rRNA (cyanobacteria) and 18S rRNA (microalgae) FASTA sequences and associated blastn results obtained from the high throughput sequencing of plankton and biofilm bulk/eDNA samples collected in 2019 in 37 lakes and 22 rivers across the Alpine region. These are supporting files for the paper by Salmaso et al., 2022. DNA sequence and taxonomic gap analyses to quantify the coverage of aquatic cyanobacteria and eukaryotic microalgae in reference databases: Results of a survey in the Alpine region. Science of the Total Environment, in press.
description: This dataset has been prepared with the support and co-financing of the European Regional Development Fund through the Interreg Alpine Space program, project Eco-AlpsWater (EAW), grant number ASP569 (www.alpine-space.org/projects/eco-alpswater/en/home) and national programs (15% of project co-funding for EC countries); in Switzerland, the project EAW received support and funds from the Federal Office for Spatial Development (ARE), within the Swiss Confederation's New Regional Policy (NRP).
DOI: 10.5281/zenodo.5822483
title: DNA sequence and taxonomic gap analyses to quantify the coverage of aquatic cyanobacteria and eukaryotic microalgae in reference databases: Results of a survey in the Alpine region

description: This dataset has been prepared as part of the Interreg Alpine Space project Eco-AlpsWater (ASP569) - <em>Innovative Ecological Assessment and Water Management Strategy for the Protection of Ecosystem Services in Alpine Lakes and Rivers</em>, https://www.alpine-space.eu/projects/eco-alpswater/en/home Individual archives include 16S rRNA (cyanobacteria) and 18S rRNA (microalgae) FASTA sequences and associated blastn results obtained from the high throughput sequencing of plankton and biofilm bulk/eDNA samples collected in 2019 in 37 lakes and 22 rivers across the Alpine region. These are supporting files for the paper by Salmaso et al., 2022. DNA sequence and taxonomic gap analyses to quantify the coverage of aquatic cyanobacteria and eukaryotic microalgae in reference databases: Results of a survey in the Alpine region. Science of the Total Environment, in press.
description: This dataset has been prepared with the support and co-financing of the European Regional Development Fund through the Interreg Alpine Space program, project Eco-AlpsWater (EAW), grant number ASP569 (www.alpine-space.org/projects/eco-alpswater/en/home) and national programs (15% of project co-funding for EC countries); in Switzerland, the project EAW received support and funds from the Federal Office for Spatial Development (ARE), within the Swiss Confederation's New Regional Policy (NRP).
DOI: 10.15161/oar.it/75466
title: CovidStat project data

description: This record contains the daily updated data of the CovidStat project. CovidStat is a project carried out by the CovidStat Working Group at INFN, whose creation was promoted within the Italian National Institute of Nuclear Physics with the aim of making a statistical analysis of the data provided daily by the Civil Protection on the spread of the pandemic in Italy. CovidStat data can interactively be browsed at https://covid19.infn.it.
description: The software to process this Root TTree is in the related identifier. Be sure to use the right corresponding version, based on the data in which Root TTree was generated..
DOI: 10.5281/zenodo.6433541
title: Animals Characteristics of the Fuengirola bioparc in Spain

description: In the dataset you will find information about the animals found in the Fuengirola Bioparc. In this dataset we will find the family, species, order, habitat, classification, area, diet, gestation and degree of threat of each animal.
DOI: 10.5281/zenodo.6433540
title: Animals Characteristics of the Fuengirola bioparc in Spain

description: In the dataset you will find information about the animals found in the Fuengirola Bioparc. In this dataset we will find the family, species, order, habitat, classification, area, diet, gestation and degree of threat of each animal.
DOI: 10.23728/b2share.0b02d78b523544a3a76c621da6c723d2
title: Dataset about consumption of single-use plastics.

description: Spreadsheet containing participant answers. Approved by the Committee of Research Ethics of Asturias Principality (Spain) with the reference CEImPA:2021.116.
DOI: 10.25606/surf.db360b7d575f09e5
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P149+32)

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 P149+32.
DOI: 10.5281/zenodo.6433623
title: El tiempo en España durante la próxima semana

description: Este dataset es fruto de un proyecto que es parte de una Práctica de la asignatura Tipología y ciclo de vida de los datos, que pertenece al Máster Universitario de Ciencia de Datos de la Universitat Oberta de Catalunya. En esta práctica se pide elaborar un caso práctico orientado a aprender a identificar los datos relevantes para un proyecto analítico y usar herramientas de extracción de datos.
DOI: 10.5281/zenodo.6433622
title: El tiempo en España durante la próxima semana

description: Este dataset es fruto de un proyecto que es parte de una Práctica de la asignatura Tipología y ciclo de vida de los datos, que pertenece al Máster Universitario de Ciencia de Datos de la Universitat Oberta de Catalunya. En esta práctica se pide elaborar un caso práctico orientado a aprender a identificar los datos relevantes para un proyecto analítico y usar herramientas de extracción de datos.
DOI: 10.5281/zenodo.6433609
title: Third Way: A Puzzle that Dual-Route Model of Lexical Access Cannot Solve

description: The dataset needed to replicate the study findings.
DOI: 10.5281/zenodo.6433608
title: Third Way: A Puzzle that Dual-Route Model of Lexical Access Cannot Solve

description: The dataset needed to replicate the study findings.
DOI: 10.25606/surf.9788d66f2392ff39
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P191+62)

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 P191+62.
DOI: 10.6084/m9.figshare.19561609
title: Raw data of survivor bias in ozone-volatile organic compounds system.xlsx

description: Raw data of survivor bias in ozone-volatile organic compounds system.
DOI: 10.6084/m9.figshare.19123637
title: Sexual Violence and the Object of Attribution of Responsibility in Georgian Students

description: Transcripts of interviews, Quantitative results data (the percentages relating to the participants assessments of each case), Copy of the interview guide.
DOI: 10.6084/m9.figshare.19123637.v9
title: Sexual Violence and the Object of Attribution of Responsibility in Georgian Students

description: Transcripts of interviews, Quantitative results data (the percentages relating to the participants assessments of each case), Copy of the interview guide.
DOI: 10.6084/m9.figshare.19262366
title: 2022 electron-only reconnection

description: In the data files, 'ax', 'ay', 'az' mean vector potential A_x, A_y, A_z; 'bx', 'by', 'bz' mean magnetic field B_x, B_y, B_z; 'ex', 'ey', 'ez' mean electric field E_x, E_y, E_z; 'jx', 'jy', 'jz' mean current density j_x, j_y, j_z; 'uix', 'uiy', 'uiz' mean ion flow velocity V_ix, V_iy, V_iz; 'uex', 'uey', 'uez' mean electron flow velocity V_ex, V_ey, V_ez; 'dde' means electron density; 'ddi' means ion density; 'pixx', 'piyy', 'pizz' mean ion pressure tensor components P_ixx, P_iyy, P_izz; 'pexx', 'peyy', 'pezz' mean electron pressure tensor components P_exx, P_eyy, P_ezz; the numbers in the file names divided by 4000 are the corresponding time in units of Omega_i^-1. The data format is 2048*1024f15.7. <br> “time_histories.dat” contains the time histories of the maximum electron and ion outflows in the L direction V_eL and V_iL at N = 0 and the maximum energy conversion j*E' and ion temperature T_i at L = L_R, where L_R is where B_N at N = 0 minimizes before reconnection and reverses after reconnection. The data format is 5f15.7 in each line.
DOI: 10.6084/m9.figshare.19262366.v2
title: 2022 electron-only reconnection

description: In the data files, 'ax', 'ay', 'az' mean vector potential A_x, A_y, A_z; 'bx', 'by', 'bz' mean magnetic field B_x, B_y, B_z; 'ex', 'ey', 'ez' mean electric field E_x, E_y, E_z; 'jx', 'jy', 'jz' mean current density j_x, j_y, j_z; 'uix', 'uiy', 'uiz' mean ion flow velocity V_ix, V_iy, V_iz; 'uex', 'uey', 'uez' mean electron flow velocity V_ex, V_ey, V_ez; 'dde' means electron density; 'ddi' means ion density; 'pixx', 'piyy', 'pizz' mean ion pressure tensor components P_ixx, P_iyy, P_izz; 'pexx', 'peyy', 'pezz' mean electron pressure tensor components P_exx, P_eyy, P_ezz; the numbers in the file names divided by 4000 are the corresponding time in units of Omega_i^-1. The data format is 2048*1024f15.7. <br> “time_histories.dat” contains the time histories of the maximum electron and ion outflows in the L direction V_eL and V_iL at N = 0 and the maximum energy conversion j*E' and ion temperature T_i at L = L_R, where L_R is where B_N at N = 0 minimizes before reconnection and reverses after reconnection. The data format is 5f15.7 in each line.
DOI: 10.6084/m9.figshare.19262366.v1
title: 2022 electron-only reconnection

description: In the data files, 'ax', 'ay', 'az' mean vector potential A_x, A_y, A_z; 'bx', 'by', 'bz' mean magnetic field B_x, B_y, B_z; 'ex', 'ey', 'ez' mean electric field E_x, E_y, E_z; 'jx', 'jy', 'jz' mean current density j_x, j_y, j_z; 'uix', 'uiy', 'uiz' mean ion flow velocity V_ix, V_iy, V_iz; 'uex', 'uey', 'uez' mean electron flow velocity V_ex, V_ey, V_ez; 'dde' means electron density; 'ddi' means ion density; 'pixx', 'piyy', 'pizz' mean ion pressure tensor components P_ixx, P_iyy, P_izz; 'pexx', 'peyy', 'pezz' mean electron pressure tensor components P_exx, P_eyy, P_ezz; the numbers in the file names divided by 4000 are the corresponding time in units of Omega_i^-1. The data format is 2048*1024f15.7.
DOI: 10.25606/surf.60083e00f1f0a22f
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P011+41)

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 P011+41.
DOI: 10.6084/m9.figshare.14371652.v1
title: JNU-IFM

description: The JNU-IFM dataset for segmenting symphysis pubis-fetal head
DOI: 10.25606/surf.4f4106c22a188d95
title: The LOFAR Two-metre Sky Survey (LoTSS) V. Second data release (P336+28)

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 P336+28.
DOI: 10.15151/esrf-es-698651895
title: The Israeli BAG

description: The BAG is quite large with 24 principal investigators covering almost all groups in Israel. The scientific topics are diverse and so different that depicting them in a short Abstract is extremely difficult. In this context BAG members are studying the parameters that govern protein assemblage, structural impacts of signaling processes in different cascades. There are several projects that are directed towards molecular recognition with implementation towards drug design. In addition, we still have the ribosome project and the design of unique antibiotics with specific functional interactions from the mycinamycins family and their resistance related mechanism compared with other macrolides and the photosystem and how it converts light into energy. Since Covid-19 is still a relevant topic as are other viral infections BAG members are and have been involved in the understanding of the infection process and the means to hinder it.
DOI: 10.25919/ckf0-w763
title: Parkes observations for project P1131 semester 2021OCTS_12

description: Fast Radio Bursts (FRBs) are extragalactic radio transients with the duration time in the range of several microseconds to tens of milliseconds. The origin of them is still unclear. Ultraluminous X-ray Sources (ULXs) are objects that mostly discovered in external galaxies which host black holes or neutron stars, with isotropic luminosities exceeding the usual Eddington value for stellar-mass black holes. The host galaxies of ULXs, and their spatial offsets within their hosts, show broad similarities to those of FRB. Periodicity of days to years of some repeated FRBs could be attributed to the companion effect of ULXs. Moreover, pulsing ULXs (PULXs) which hots neutron stars may be the manifestation of accreting magnetars. Therefore, we propose targeted FRB searches of known PULXs, which have not yet been carried out by other telescopes according to published literature to date. Our observations will play an important role in investigating the FRB progenitors. If FRBs were detected in our selected ULXs, then puzzle of FRBs' origin would be directly resolved. If no FRB is detected, we can still constrain some ULX-related models statistically, e.g. the upper limit of the burst rate, the period of duty cycle, etc. Our observations can also be used to hunt for radio pulsars in PULXs.
DOI: 10.6084/m9.figshare.19565242
title: Himawari-8

description: The netcdf files contain Himawari-8 observations for cloud top temperatures, types etc.
DOI: 10.6084/m9.figshare.19565242.v1
title: Himawari-8

description: The netcdf files contain Himawari-8 observations for cloud top temperatures, types etc.
DOI: 10.5519/qd.9gb6txjy
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (5101468 records)
DOI: 10.34740/kaggle/dsv/3437203
title: YouTube Trending Video Dataset (updated daily)
DOI: 10.34740/kaggle/dsv/3437242
title: 2021 World Population (updated daily)
DOI: 10.6084/m9.figshare.19565719
title: accuracy assessment

description: 1-S and 2-S case