cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.3886/e181742
title: OTOPIST

description: <b>Question</b>: Is there any difference in the incidence of prosthesis loop dislocation from the incus between manual crimping Teflon and Titanium stapes prostheses over time? <b>Findings</b>: In this retrospective survival analysis on 855 patients, we observed 23/755 cases (2.9%) of dislocation in the Teflon group and 0/97 In the Titanium group but this difference was not statistically significant. <b>Meaning</b>: Titanium stapes prostheses seem more stable than Teflon prostheses over time. Further prospective studies are encouraged to confirm these findings.
DOI: 10.3886/e181742v1
title: OTOPIST

description: <b>Question</b>: Is there any difference in the incidence of prosthesis loop dislocation from the incus between manual crimping Teflon and Titanium stapes prostheses over time? <b>Findings</b>: In this retrospective survival analysis on 855 patients, we observed 23/755 cases (2.9%) of dislocation in the Teflon group and 0/97 In the Titanium group but this difference was not statistically significant. <b>Meaning</b>: Titanium stapes prostheses seem more stable than Teflon prostheses over time. Further prospective studies are encouraged to confirm these findings.
DOI: 10.3886/e181742v2
title: OTOPIST

description: <b>Question</b>: Is there any difference in the incidence of prosthesis loop dislocation from the incus between manual crimping Teflon and Titanium stapes prostheses over time? <b>Findings</b>: In this retrospective survival analysis on 855 patients, we observed 23/755 cases (2.9%) of dislocation in the Teflon group and 0/97 In the Titanium group but this difference was not statistically significant. <b>Meaning</b>: Titanium stapes prostheses seem more stable than Teflon prostheses over time. Further prospective studies are encouraged to confirm these findings.
DOI: 10.6084/m9.figshare.17087319
title: Persistent sexual dysfunction after SSRI withdrawal: a scoping review and presentation of 86 cases from the Netherlands

description: Sexual dysfunction is highly prevalent worldwide. A specific form is persistent sexual dysfunction after SSRI withdrawal. We conducted a systematic literature review in order to characterize factors related to post SSRI sexual dysfunction (PSSD) and analyzed spontaneous reports of persistent sexual dysfunction reported to the Netherlands Pharmacovigilance Center Lareb. A systematic literature review was conducted following the PRISMA-ScR guidelines. In addition, reports of PSSD submitted to the Netherlands Pharmacovigilance Center Lareb between 1992 and 2021 were analyzed. A total of 237 articles were retrieved through the search and 33 articles were selected for inclusion in this review, in accordance with the inclusion criteria. Information regarding the characteristics of the condition, its clinical management, patient characteristics, and impact of PSSD is presented. A total of 86 reports of persistent sexual dysfunction were analyzed. The longest case being a patient with PSSD for 23 years. The main symptoms were: loss or decreased libido (n = 53), erectile dysfunction (n = 23) and anorgasmia (n = 5). PSSD impact includes sexual, psychological, and social consequences. Little is known about the mechanisms underlying PSSD and no effective treatment exists. It is necessary to increase recognition of PSSD among prescribers and improve its management at the clinical level.
DOI: 10.6084/m9.figshare.17087319.v1
title: Persistent sexual dysfunction after SSRI withdrawal: a scoping review and presentation of 86 cases from the Netherlands

description: Sexual dysfunction is highly prevalent worldwide. A specific form is persistent sexual dysfunction after SSRI withdrawal. We conducted a systematic literature review in order to characterize factors related to post SSRI sexual dysfunction (PSSD) and analyzed spontaneous reports of persistent sexual dysfunction reported to the Netherlands Pharmacovigilance Center Lareb. A systematic literature review was conducted following the PRISMA-ScR guidelines. In addition, reports of PSSD submitted to the Netherlands Pharmacovigilance Center Lareb between 1992 and 2021 were analyzed. A total of 237 articles were retrieved through the search and 33 articles were selected for inclusion in this review, in accordance with the inclusion criteria. Information regarding the characteristics of the condition, its clinical management, patient characteristics, and impact of PSSD is presented. A total of 86 reports of persistent sexual dysfunction were analyzed. The longest case being a patient with PSSD for 23 years. The main symptoms were: loss or decreased libido (n = 53), erectile dysfunction (n = 23) and anorgasmia (n = 5). PSSD impact includes sexual, psychological, and social consequences. Little is known about the mechanisms underlying PSSD and no effective treatment exists. It is necessary to increase recognition of PSSD among prescribers and improve its management at the clinical level.
DOI: 10.6084/m9.figshare.22109018
title: Feeding data

description: Data of pollen feeding bumblebees.
DOI: 10.6084/m9.figshare.22109018.v2
title: Feeding data

description: Data of pollen feeding bumblebees.
DOI: 10.34740/kaggle/dsv/5008161
title: Health Workforce Shortage Areas
DOI: 10.6084/m9.figshare.22109018.v1
title: Feeding data

description: Data of pollen feeding bumblebees.
DOI: 10.34740/kaggle/dsv/5008171
title: AutoXGB
DOI: 10.5281/zenodo.7011026
title: Stereoretentive Post-Translational Protein Editing

description: This dataset contains raw LCMSMS files used to confirm chemical post-translational modifications described in the article.
DOI: 10.5281/zenodo.7011025
title: Stereoretentive Post-Translational Protein Editing

description: This dataset contains raw LCMSMS files used to confirm chemical post-translational modifications described in the article.
DOI: 10.4119/unibi/2968974
title: Data publication for: Stigmatization in the Context of the COVID-19 Pandemic: A Survey Experiment Using Attribution Theory and the Familiarity Hypothesis

description: Background: The COVID-19 pandemic has created a global health crisis, leading to stigmatization and discriminatory behaviors against people who have contracted or are suspected of having contracted the virus. Yet the causes of stigmatization in the context of COVID-19 remain only partially understood. Using attribution theory, we examine to what extent attributes of a fictitious person affect the formation of stigmatizing attitudes towards this person, and whether suspected COVID-19 infection (vs. flu) intensifies such attitudes. We also use the familiarity hypothesis to explore whether familiarity with COVID-19 reduces stigma and whether it moderates the effect of a COVID-19 infection on stigmatization. Methods: We conducted a multifactorial vignette survey experiment (2x2x2x2x2x2x2x2-design, i.e., number of vignettes = 256) in Germany (Number of respondents = 4,059) in which we experimentally varied signals and signaling events (i.e., information that may trigger stigma) concerning a fictitious person in the context of COVID-19. We assessed respondents’ cognitive (e.g., blameworthiness) and affective (e.g., anger) responses as well as their discriminatory inclinations (e.g., avoidance) towards the character. Furthermore, we measured different indicators of respondents’ familiarity with COVID-19. Results: Results revealed higher levels of stigma towards people who were diagnosed with COVID-19 versus a regular flu. In addition, stigma was higher towards those who were considered responsible for their infection due to irresponsible behavior. Knowing someone who died from a COVID infection increased stigma. While higher self-reported knowledge about COVID-19 was associated with more stigma, higher factual knowledge was associated with less. Conclusion: Attribution theory and to a lesser extent the familiarity hypothesis can help better understand stigma in the context of COVID-19. This study provides insights about who is at risk of stigmatization and stigmatizing others in this context. It thereby allows identifying the groups that require more support in accessing healthcare services and suggests that basic, factually oriented public health interventions would be promising for reducing stigma.
DOI: 10.34740/kaggle/dsv/5008217
title: Survey on Employment Trends
DOI: 10.5519/qd.flldcrz0
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (1001 records)
DOI: 10.5519/qd.ussp9w3n
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (4 records)
DOI: 10.5519/qd.yoe08sfk
title: Query on the Natural History Museum Data Portal (data.nhm.ac.uk) (44 records)
DOI: 10.34740/kaggle/dsv/5008263
title: Elon Musk Tweets
DOI: 10.5281/zenodo.7505674
title: RT Dataset -- Updated radiative transfer model for Titan in the near-infrared wavelength range: Validation against Huygens atmospheric and surface measurements and application to the Cassini/VIMS observations of the Dragonfly landing area

description: This dataset contains all Radiative Transfer (RT) results made for the paper. The data are stored in 5 zipped-folders names with the Cassini/VIMS cube flyby and id, or explicitly for Huygens/ULIS calibrated observations: TB_C1481624349_1 T40_C1578266417_1 T38_C1575509158_1 T40_C1578263500_1 T40_C1578263152_1 ULIS_observations The TB_C1481624349_1 folder contains the Cassini/VIMS cube over HLS, the HLS end-member (End_member.txt), the surface albedo retrieved by Karkoschka et al. (2016) corrected for the photometry (HLS_Karkoschka_2016_spectrum.txt), and the inverted surface albedo (Surface_albedo.txt). In these folders, each VIMS pixel is stored in a .txt file with the following pattern: &lt;CUBE_ID&gt;_&lt;PIXEL_SAMPLE&gt;_&lt;PIXEL_LINE&gt; .txt It starts with a header describing the observation: CUBE_ID: the VIMS cube id (`C1234567890_1` format) SAMPLE: the pixel sample number. LINE: the pixel line number. LONG: the pixel longitude (in degree). LAT: the pixel latitude (in degree). INC: the surface incident angle (in degree). EMI: the surface emergent angle (in degree). PHASE: the surface phase angle (in degree). For the Selk crater cubes (T40_C1578266417_1, T38_C1575509158_1, T40_C1578263500_1, T40_C1578263152_1), the header also contains the spatial sampling and the radiative transfer model outputs: Spatial sampling (km/pix). Fh: the haze scaling factor. Fm: the mist scaling factor. 1-sigma (Fh): the 1-sigma uncertainty on Fh. 1-sigma (Fm): the 1-sigma uncertainty on Fm. Reduced chi2: the reduced chi2. Then contains the observed spectra: Column 1: the VIMS channel central wavelength (in micrometers). Column 2: the VIMS pixel I/F. Column 3: the VIMS pixel I/F 1-sigma uncertainty. For the Selk crater cubes (T40_C1578266417_1, T38_C1575509158_1, T40_C1578263500_1, T40_C1578263152_1), 3 columns are added for: Column 4: the surface albedo. Column 5: the upper 1-sigma uncertainty on the surface albedo. Column 6 : the lower 1-sigma uncertainty on the surface albedo. The ULIS folder contains the Huygens/ULIS calibrated observations (in I/F) and the simulations with 1-sigma uncertainties as a function of the altitude (in km): Column 1: the VIMS channel central wavelength (in micrometers), stopped at the end of the Huygens/ULIS wavelength range. Column 2: the ULIS I/F. Column 3 : the simulated I/F. Column 4: the lower 1-sigma uncertainty on the simulation. Column 5 : the upper 1-sigma uncertainty on the simulation.
DOI: 10.5281/zenodo.7505675
title: RT Dataset -- Updated radiative transfer model for Titan in the near-infrared wavelength range: Validation against Huygens atmospheric and surface measurements and application to the Cassini/VIMS observations of the Dragonfly landing area

description: This dataset contains all Radiative Transfer (RT) results made for the paper. The data are stored in 4 zipped-folders names with the VIMS cube flyby and id: TB_C1481624349_1 T40_C1578266417_1 T38_C1575509158_1 T40_C1578263500_1 T40_C1578263152_1 The HLS folder contains the VIMS cubes, the HLS end-member (End_member.txt), and the corresponding surface albedo (Surface_albedo.txt). In these folders, each VIMS pixel is stored in a .txt file with the following pattern: &lt;CUBE_ID&gt;_&lt;PIXEL_SAMPLE&gt;_&lt;PIXEL_LINE&gt; .txt It starts with a header describing the observation: CUBE_ID: the VIMS cube id (`C1234567890_1` format) SAMPLE: the pixel sample number. LINE: the pixel line number. LONG: the pixel longitude (in degree). LAT: the pixel latitude (in degree). INC: the surface incident angle (in degree). EMI: the surface emergent angle (in degree). PHASE: the surface phase angle (in degree). For the Selk crater cubes (T40_C1578266417_1, T38_C1575509158_1, T40_C1578263500_1, T40_C1578263152_1), the header also contains the spatial sampling and the radiative transfer model outputs: Spatial sampling (km/pix). Fh: the haze scaling factor. Fm: the mist scaling factor. 1-sigma (Fh): the 1-sigma uncertainty on Fh. 1-sigma (Fm): the 1-sigma uncertainty on Fm. Reduced chi2: the reduced chi2. Then contains the observed spectra: Column 1: the VIMS channel central wavelength (in micrometers). Column 2: the VIMS pixel I/F. Column 3: the VIMS pixel I/F 1-sigma uncertainty. For the Selk crater cubes (T40_C1578266417_1, T38_C1575509158_1, T40_C1578263500_1, T40_C1578263152_1), 3 columns are added for: Column 4: the surface albedo. Column 5: the upper 1-sigma uncertainty on the surface albedo. Column 6 : the lower 1-sigma uncertainty on the surface albedo.
DOI: 10.5281/zenodo.7630258
title: RT Dataset -- Updated radiative transfer model for Titan in the near-infrared wavelength range: Validation against Huygens atmospheric and surface measurements and application to the Cassini/VIMS observations of the Dragonfly landing area

description: This dataset contains all Radiative Transfer (RT) results made for the paper. The data are stored in 5 zipped-folders names with the Cassini/VIMS cube flyby and id, or explicitly for Huygens/ULIS calibrated observations: TB_C1481624349_1 T40_C1578266417_1 T38_C1575509158_1 T40_C1578263500_1 T40_C1578263152_1 ULIS_observations The HLS folder contains the Cassini/VIMS cubes, the HLS end-member (End_member.txt), and the corresponding surface albedo (Surface_albedo.txt). In these folders, each VIMS pixel is stored in a .txt file with the following pattern: &lt;CUBE_ID&gt;_&lt;PIXEL_SAMPLE&gt;_&lt;PIXEL_LINE&gt; .txt It starts with a header describing the observation: CUBE_ID: the VIMS cube id (`C1234567890_1` format) SAMPLE: the pixel sample number. LINE: the pixel line number. LONG: the pixel longitude (in degree). LAT: the pixel latitude (in degree). INC: the surface incident angle (in degree). EMI: the surface emergent angle (in degree). PHASE: the surface phase angle (in degree). For the Selk crater cubes (T40_C1578266417_1, T38_C1575509158_1, T40_C1578263500_1, T40_C1578263152_1), the header also contains the spatial sampling and the radiative transfer model outputs: Spatial sampling (km/pix). Fh: the haze scaling factor. Fm: the mist scaling factor. 1-sigma (Fh): the 1-sigma uncertainty on Fh. 1-sigma (Fm): the 1-sigma uncertainty on Fm. Reduced chi2: the reduced chi2. Then contains the observed spectra: Column 1: the VIMS channel central wavelength (in micrometers). Column 2: the VIMS pixel I/F. Column 3: the VIMS pixel I/F 1-sigma uncertainty. For the Selk crater cubes (T40_C1578266417_1, T38_C1575509158_1, T40_C1578263500_1, T40_C1578263152_1), 3 columns are added for: Column 4: the surface albedo. Column 5: the upper 1-sigma uncertainty on the surface albedo. Column 6 : the lower 1-sigma uncertainty on the surface albedo. The ULIS folder contains the Huygens/ULIS calibrated observations (in I/F) and the simulations with 1-sigma uncertainties as a function of the altitude (in km): Column 1: the VIMS channel central wavelength (in micrometers), stopped at the end of the Huygens/ULIS wavelength range. Column 2: the ULIS I/F. Column 3 : the simulated I/F. Column 4: the lower 1-sigma uncertainty on the simulation. Column 5 : the upper 1-sigma uncertainty on the simulation.
DOI: 10.5281/zenodo.7645466
title: RT Dataset -- Updated radiative transfer model for Titan in the near-infrared wavelength range: Validation against Huygens atmospheric and surface measurements and application to the Cassini/VIMS observations of the Dragonfly landing area

description: This dataset contains all Radiative Transfer (RT) results made for the paper. The data are stored in 5 zipped-folders names with the Cassini/VIMS cube flyby and id, or explicitly for Huygens/ULIS calibrated observations: TB_C1481624349_1 T40_C1578266417_1 T38_C1575509158_1 T40_C1578263500_1 T40_C1578263152_1 ULIS_observations The TB_C1481624349_1 folder contains the Cassini/VIMS cube over HLS, the HLS end-member (End_member.txt), the surface albedo retrieved by Karkoschka et al. (2016) corrected for the photometry (HLS_Karkoschka_2016_spectrum.txt), and the inverted surface albedo (Surface_albedo.txt). In these folders, each VIMS pixel is stored in a .txt file with the following pattern: &lt;CUBE_ID&gt;_&lt;PIXEL_SAMPLE&gt;_&lt;PIXEL_LINE&gt; .txt It starts with a header describing the observation: CUBE_ID: the VIMS cube id (`C1234567890_1` format) SAMPLE: the pixel sample number. LINE: the pixel line number. LONG: the pixel longitude (in degree). LAT: the pixel latitude (in degree). INC: the surface incident angle (in degree). EMI: the surface emergent angle (in degree). PHASE: the surface phase angle (in degree). For the Selk crater cubes (T40_C1578266417_1, T38_C1575509158_1, T40_C1578263500_1, T40_C1578263152_1), the header also contains the spatial sampling and the radiative transfer model outputs: Spatial sampling (km/pix). Fh: the haze scaling factor. Fm: the mist scaling factor. 1-sigma (Fh): the 1-sigma uncertainty on Fh. 1-sigma (Fm): the 1-sigma uncertainty on Fm. Reduced chi2: the reduced chi2. Then contains the observed spectra: Column 1: the VIMS channel central wavelength (in micrometers). Column 2: the VIMS pixel I/F. Column 3: the VIMS pixel I/F 1-sigma uncertainty. For the Selk crater cubes (T40_C1578266417_1, T38_C1575509158_1, T40_C1578263500_1, T40_C1578263152_1), 3 columns are added for: Column 4: the surface albedo. Column 5: the upper 1-sigma uncertainty on the surface albedo. Column 6 : the lower 1-sigma uncertainty on the surface albedo. The ULIS folder contains the Huygens/ULIS calibrated observations (in I/F) and the simulations with 1-sigma uncertainties as a function of the altitude (in km): Column 1: the VIMS channel central wavelength (in micrometers), stopped at the end of the Huygens/ULIS wavelength range. Column 2: the ULIS I/F. Column 3 : the simulated I/F. Column 4: the lower 1-sigma uncertainty on the simulation. Column 5 : the upper 1-sigma uncertainty on the simulation.
DOI: 10.5281/zenodo.7619946
title: Datasets and R script to replicate the theoretical modeling from the article entitled Multiple hosts, multiple impacts: the role of vertebrate host diversity in shaping mosquito life history and pathogen transmission

description: Datasets and R script to replicate the theoretical modeling from the article entitled "<strong> </strong>Multiple hosts, multiple impacts: the role of vertebrate host diversity in shaping mosquito life history and pathogen transmission" by Vantaux A., Moiroux N., Dabire K. R., Cohuet A., Lefevre T. 2023
DOI: 10.5281/zenodo.7619947
title: Datasets and R script to replicate the theoretical modeling from the article entitled Multiple hosts, multiple impacts: the role of vertebrate host diversity in shaping mosquito life history and pathogen transmission

description: Datasets and R script to replicate the theoretical modeling from the article entitled "<strong> </strong>Multiple hosts, multiple impacts: the role of vertebrate host diversity in shaping mosquito life history and pathogen transmission" by Vantaux A., Moiroux N., Dabire K. R., Cohuet A., Lefevre T. 2023
DOI: 10.5281/zenodo.7645483
title: Datasets and R script to replicate the theoretical modeling from the article entitled Multiple hosts, multiple impacts: the role of vertebrate host diversity in shaping mosquito life history and pathogen transmission

description: Datasets and R script to replicate the theoretical modeling from the article entitled "<strong> </strong>Multiple hosts, multiple impacts: the role of vertebrate host diversity in shaping mosquito life history and pathogen transmission" by Vantaux A., Moiroux N., Dabire K. R., Cohuet A., Lefevre T. 2023
DOI: 10.6084/m9.figshare.22091294
title: sdm tests raw-data

description: test raw data
DOI: 10.6084/m9.figshare.22091294.v1
title: sdm tests raw-data

description: test raw data
DOI: 10.5281/zenodo.7645485
title: Single-molecule datasets for Slitflow tutorials

description: Datasets used in tutorials on Slitflow, a Python framework for single-molecule dynamics and localization analysis. For more information see https://slitflow.readthedocs.io
DOI: 10.5281/zenodo.7645484
title: Single-molecule datasets for Slitflow tutorials

description: Datasets used in tutorials on Slitflow, a Python framework for single-molecule dynamics and localization analysis. For more information see https://slitflow.readthedocs.io
DOI: 10.5281/zenodo.7561154
title: Survey I4.0 in the Marche Region

description: This dataset contains the answers to a survey to a sample of 7 innovative firms of the Marche Region regarding their use of Industry 4.0 technologies, including blockchain, the collaborations that they have with regional, national, and European actors, and which measures they believe are useful for the diffusion of Industry 4.0 technologies in firms of the Marche Region.
DOI: 10.5281/zenodo.7561153
title: Survey I4.0 in the Marche Region

description: This dataset contains the answers to a survey to a sample of 7 innovative firms of the Marche Region regarding their use of Industry 4.0 technologies, including blockchain, the collaborations that they have with regional, national, and European actors, and which measures they believe are useful for the diffusion of Industry 4.0 technologies in firms of the Marche Region.
DOI: 10.5285/409dc3f0-f371-4322-bdc3-39cd439c28c9
title: X-discontinuity observations beneath the African continent

description: X-discontinuity observations recorded from receiver function stacks of passive-source seismic data. Receiver functions are recorded between January 1990 and October 2021 at numerous seismometers on the African continent (see Pugh et al., 2023 for details). Receiver functions are downloaded, processed using SMURFPy (Cottaar et al., 2020). They are subsequently stacked in the depth and time-slowness domains in 1 degree radius overlapping bins and interpreted for the presence of the X-discontinuity. The dataset comprises 597 stacks, their location, the depth of the X-discontinuity, a classification of the stack and the amplitudes of the X-discontinuity. See Pugh et al., 2023 for further details on the method, the code used to download, process and stack receiver functions can be found at: https://doi.org/10.5281/zenodo.4337258
Pugh et al., 2023 - Multigenetic Origin of the X-discontinuity Below Continents: Insights from African Receiver Functions.
DOI: 10.6084/m9.figshare.21673097
title: bioinformatic analyses

description: Mice NAFLD and rhythms disturbance models to analyze the relationships of the key circadian clock genes and NAFLD.
DOI: 10.6084/m9.figshare.21673097.v1
title: bioinformatic analyses

description: Mice NAFLD and rhythms disturbance models to analyze the relationships of the key circadian clock genes and NAFLD.