cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.15468/dl.jw7ntu
title: Occurrence Download

description: A dataset containing 474299 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Geometry POLYGON((-88.071 41.05,-86.236 41.05,-86.236 42.176,-88.071 42.176,-88.071 41.05))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "TaxonKey is one of (Lepidoptera, Hymenoptera, Diptera, Coleoptera)"
 ]
}

 The dataset includes 474299 records from 110 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0069360-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.5281/zenodo.18056368
title: Dataset for "Predictability and interrelations of spectral indicators for PV performance in multiple latitudes and climates". Solar Energy, 259, 174–187. https://doi.org/10.1016/j.solener.2023.04.067

description: This dataset comprises spectral global irradiance on the plane of array (tilted) data (Excel files) measured in Madrid and Jaén using EKO MS-700 spectroradiometers during 2015–2016 and 2016–2017, respectively, together with a README file explaining how to interpret the Excel files. An additional Excel file providing the spectral response of the PV materials analysed in the paper is also included.

These data support part of the experimental analysis presented in the following paper:

Sevillano-Bendezú, M. A., Khenkin, M., Nofuentes, G., de la Casa, J., Ulbrich, C., & Töfflinger, J. A. (2023). Predictability and interrelations of spectral indicators for PV performance in multiple latitudes and climates. Solar Energy, 259, 174–187. https://doi.org/10.1016/j.solener.2023.04.067
DOI: 10.5281/zenodo.18056369
title: Dataset for "Predictability and interrelations of spectral indicators for PV performance in multiple latitudes and climates". Solar Energy, 259, 174–187. https://doi.org/10.1016/j.solener.2023.04.067

description: This dataset comprises spectral global irradiance on the plane of array (tilted) data (Excel files) measured in Madrid and Jaén using EKO MS-700 spectroradiometers during 2015–2016 and 2016–2017, respectively, together with a README file explaining how to interpret the Excel files. An additional Excel file providing the spectral response of the PV materials analysed in the paper is also included.

These data support part of the experimental analysis presented in the following paper:

Sevillano-Bendezú, M. A., Khenkin, M., Nofuentes, G., de la Casa, J., Ulbrich, C., & Töfflinger, J. A. (2023). Predictability and interrelations of spectral indicators for PV performance in multiple latitudes and climates. Solar Energy, 259, 174–187. https://doi.org/10.1016/j.solener.2023.04.067
DOI: 10.5281/zenodo.17613648
title: African American Burial Grounds in the Louisiana River Parishes

description: This dataset documents African American burial grounds in the Louisiana River Parishes. The sites were recorded from 2023-2024 using drone lidar, neural rendering, and ambisonics. This project was funded by the National Park Service, the Architecture Research Centers Consortium, and Louisiana State University. The project leads were Brendan Harmon, Nicholas Serrano, and Annicia Streete. Read about the project in our paper: Endangered African American Burial Grounds of the Lower Mississippi: Acts of Reparation and Preservation. This dataset is released under the Creative Commons Zero public domain dedication. This dataset is divided into the following parts: lidar (28 GB), scans (15 GB), and soundscapes (41 GB). See the collection online at xyz.cct.lsu.edu.
DOI: 10.15468/dl.rvh9vj
title: Occurrence Download

description: A dataset containing 214 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Geometry POLYGON((13.19649 41.22494,13.72972 41.23206,13.72423 41.51365,13.1887 41.50646,13.19649 41.22494))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "OccurrenceStatus is Present",
 "TaxonKey is Corvus cornix",
 "Year 1990-2025"
 ]
}

 The dataset includes 214 records from 3 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0069363-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.48577/jpl.hootst
title: Weak, extended water vapor emission in the Horsehead nebula

description: We have analyzed archival Herschel observations of water vapor emission toward the Horsehead photon dominated region (PDR), along with supporting ground-based and airborne observations of CO isotopologues and fine structure lines of ionized and atomic carbon to determine the distribution and abundance of water vapor in this low-UV illumination PDR. Water emission in the Horsehead nebula is very weak and, surprisingly, extends outward beyond other PDR tracers such as CO isotopologues or [C i] 609 µm, and as far out as [C ii] 158 µm. We model the observations using a newly developed a PDR wrapper that takes into account the geometry of this region. PDR modeling provides strong constraints on the thermal pressure, but not on the UV illumination. Maximum model line intensities agree to within 40% with the observations. Spatial profiles are also well reproduced, except for CO isotopologues, where the increase on the illuminated side of the PDR is steeper than observed. Water vapor abundance in the model reaches 3.6 ×10−7 at AV∼3 mag. However, the ground state o-H2O 557 GHz line is systematically overestimated by the models. This line has a very high optical depth and the emergent line intensity is sensitive to radiative transfer effects such as line scattering by low-density halos and the assumed microturbulent line width. A more accurate model of the water surface chemistry is required.
DOI: 10.5281/zenodo.17482129
title: Data and code for "Agroforestry Optimisation for Climate Policy: Mapping Silvopastoral Carbon Sequestration Trade-Offs in the Mediterranean"

description: This repository contains the R scripts that execute the full workflow for modeling the potential distribution of silvopastoral systems in the Mediterranean and quantifying their associated carbon sequestration potential. The maps are stored in the `maps/` directory, while R scripts used to generate and analyse them are located in the `scripts/` directory.
DOI: 10.5281/zenodo.17482130
title: Data and code for "Agroforestry Optimisation for Climate Policy: Mapping Silvopastoral Carbon Sequestration Trade-Offs in the Mediterranean"

description: This repository contains the R scripts that execute the full workflow for modeling the potential distribution of silvopastoral systems in the Mediterranean and quantifying their associated carbon sequestration potential. The maps are stored in the `maps/` directory, while R scripts used to generate and analyse them are located in the `scripts/` directory.
DOI: 10.5281/zenodo.18098564
title: Deroubaix et al. (in preparation for Nature NPJ ) – gas–aerosol statistical relationships in EMeRGe

description: In headers
DOI: 10.5281/zenodo.18098563
title: Deroubaix et al. (in preparation for Nature NPJ ) – gas–aerosol statistical relationships in EMeRGe

description: In headers
DOI: 10.13140/rg.2.2.11177.45929
title: Formaldehyde Volume-Gas Concentration Calibration Calculator
DOI: 10.48577/jpl.zqpz5g
title: Multi-StarWavefront Control: Science Case and Technological Prospects with High-Contrast Imaging of Exoplanets in Multi-Star Systems for Roman and HWO

description: Binary and other multi-star systems pose an additional challenge for starlight suppression systems due to the combined stellar components’ diffraction and aberration leakage into the region of interest. As a result, many multi-star systems are considered unsuitable for direct imaging by the Habitable worlds Observatory (HWO). Multi-Star Wavefront Control (MSWC) is a method that uses the deformable mirror (DM) on a coronagraph instrument to directly image planets and disks in multi-star systems such as Alpha Centauri. MSWC can thus enable missions such as the Roman Space Telescope and HWO to handle binary targets. Imaging planets around multi-star systems enables exciting science, in part because about half of Sun-like stars have stellar companions, and in part because multi-star systems differ from single stars in terms of planet formation, dynamics, and demographics. MSWC is a “contributed mode” on the Roman Space Telescope Coronagraph Instrument, and is compatible with HWO. We review the prospects and science case for exoplanets around binaries using Roman and HWO coronagraphs, and the results of the technology development for MSWC obtained on the Occulting mask coronagraph (OMC) in JPL’s High Contrast Imaging Testbed (HCIT) representative of the Roman coronagraph instrument. These experiments used a binary star source representative of the Alpha Centauri stars and demonstrated 2.1e-8 contrast for planets around the A component and 1.8e-7 for planets around the B in Band-3d. These contrast levels are consistent with potential detection in reflected light of the planet candidate identified with NEAR and JWST. Further contrast improvements are expected in planned future tests, including those with configurations relevant for HWO that will require deeper contrast levels.
DOI: 10.5281/zenodo.18098482
title: Bubble dissolution kinetics in porous media-Simulation and Experimental Data

description: Raw data for all plots in the paper "Bubble dissolution kinetics in porous media" submitted to Physical Review Fluids.
DOI: 10.5281/zenodo.18098481
title: Bubble dissolution kinetics in porous media-Simulation and Experimental Data

description: Raw data for all plots in the paper "Bubble dissolution kinetics in porous media" submitted to Physical Review Fluids.
DOI: 10.15468/dl.xxjcc7
title: Occurrence Download

description: A dataset containing 282 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Geometry POLYGON((-70.81996 -33.431,-70.7668 -33.42977,-70.76762 -33.35399,-70.8216 -33.35412,-70.81996 -33.431))",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "OccurrenceStatus is Present",
 "TaxonKey is Plantae"
 ]
}

 The dataset includes 282 records from 7 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0069365-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.6084/m9.figshare.28700648
title: Chromosome-Level Haplotype Resolved Genome Assembly of the Linguliform Brachiopod <i>Discradisca antillarum</i> (d'Orbigny, 1845)

description: Supplementary data including the proteomes used for annotations, Hi-C .agp, .hic and assembly files. <br><br>From the manuscript titled:<br><br>Chromosome-Level Haplotype Resolved Genome Assembly of the Linguliform Brachiopod <i>Discradisca antillarum</i> (d'Orbigny, 1845)<br><br>
DOI: 10.6084/m9.figshare.28700648.v2
title: Chromosome-Level Haplotype Resolved Genome Assembly of the Linguliform Brachiopod <i>Discradisca antillarum</i> (d'Orbigny, 1845)

description: Supplementary data including the proteomes used for annotations, Hi-C .agp, .hic and assembly files. <br><br>From the manuscript titled:<br><br>Chromosome-Level Haplotype Resolved Genome Assembly of the Linguliform Brachiopod <i>Discradisca antillarum</i> (d'Orbigny, 1845)<br><br>
DOI: 10.6084/m9.figshare.28700648.v1
title: Chromosome-Level Haplotype Resolved Genome Assembly of the Linguliform Brachiopod <i>Discradisca antillarum</i> (d'Orbigny, 1845)

description: Supplementary data including the proteomes used for annotations, Hi-C .agp, .hic and assembly files. <br><br>From the manuscript titled:<br><br>Chromosome-Level Haplotype Resolved Genome Assembly of the Linguliform Brachiopod <i>Discradisca antillarum</i> (d'Orbigny, 1845)<br><br>
DOI: 10.6084/m9.figshare.30972058
title: Related data for CF4 global model

description: Related data and code for low-pressure radio frequency CF4 capacitively coupled plasma
DOI: 10.6084/m9.figshare.30972058.v1
title: Related data for CF4 global model

description: Related data and code for low-pressure radio frequency CF4 capacitively coupled plasma
DOI: 10.6084/m9.figshare.30972058.v2
title: Related data for CF4 global model

description: Related data and code for low-pressure radio frequency CF4 capacitively coupled plasma
DOI: 10.48577/jpl.az1cim
title: First abundance estimate for the East Greenland polar bear subpopulation

description: Evaluating the demographic status of large mammals in dynamic habitats is challenging. The East Greenland (EG) polar bear subpopulation ranges over approximately 1.5 million km2 of sea ice and 18 degrees of latitude along a mostly uninhabited coastline, making it the most expansive of the world’s 20 polar bear subpopulations. We report on a distance-sampling aerial survey that provided the first estimate of abundance for EG polar bears. We used a density surface model (DSM) that corrected for incomplete detection on the transect line using mark-recapture methods, accounted for overall detectability via distance-sampling methods, and modeled bear density as a function of environmental covariates with a Generalized Additive Model. Our study design was informed by Indigenous Knowledge surveys and three decades of polar bear movement data obtained from satellite telemetry. During March–May 2023, we flew 106.5 hours on-effort over 26 survey days and sighted 84 groups of bears (108 individuals). Mean observed litter size was 1.6 (95% CI = 1.2–2.0) for cubs-of-the-year and 1.6 (95% CI = 1.3–1.8) for yearlings. Polar bear density was higher closer to land and along the continental shelf break offshore, where bathymetry deepens from 300 to 1,000 m. Polar bear density was approximately five times lower within 50 km of subsistence hunting communities (0.06 per 100 km2) compared to the rest to the study area (0.31 bears per 100 km2). The best estimate of abundance for the EG subpopulation, adjusted for animals located outside the sampling area, was 2,275 bears (CV = 0.27, 95% CI = 1,360–3,807). This estimate can be used to identify a sustainable level of subsistence harvest, manage human-bear conflicts, and monitor the effects of climate warming on EG polar bears. Our methods also provide a template for designing and conducting aerial surveys for wildlife populations inhabiting vast and remote regions.
DOI: 10.5281/zenodo.18098616
title: Airfoil Stall Divergence-Free Dataset (Re1000 & Re5000)

description: Preprocessed divergence-free trajectory data for Airfoil Stall at Re1000 and Re5000.
DOI: 10.34740/kaggle/dsv/14346374
title: Peer-to-Peer Boliviano (BOB) Exchange Data
DOI: 10.48577/jpl.4w8bod
title: Discovery of a rich population of compact hub-filament systems in a single star-forming complex

description: We report the discovery of 45 compact hub-filament systems (HFSs; median size ∼2.4 pc) in infrareddark clouds (IRDCs) in the W33 complex, located at the junction of the Scutum and Norma spiral arms. These HFSs are identified using Spitzer 8 and 24 μm, and unWISE 12 μm images, which reveal intertwined substructures in absorption toward IRDCs. In each IRDC, HFSs are mainly located at the intersections of substructures, associated with groups of protostars and lacking radio continuum emission. Minimum Spanning Tree (MST) analysis shows that protostars are closely associated with the HFSs, with protostellar core separations of ≤ 0.7 pc, indicating strong clustering within fragmented structures. The HFSs form two main groupings spanning 10–15 pc, with member separations of 1–3.3 pc. Around 65% are tightly clustered (&lt; 2 pc), exhibiting rich small-scale structures and emphasizing the uniqueness of the complex. MST analysis of ALMAGAL 1.38 mm continuum cores—predominantly low-mass and embedded in ten HFSs containing more than five cores each—reveals a median core separation of ∼0.03 pc. The protostellar spacing (∼0.7 pc) significantly exceeds the thermal Jeans length (∼0.08 pc for temperature ∼18 K and density ∼105 cm−3), whereas the core spacing is smaller than the Jeans length, suggesting that thermal fragmentation may influence core formation but alone cannot explain the larger-scale protostellar distribution. All these findings together support a picture in which fragments of clouds/filaments form clumps hosting compact HFSs that facilitate efficient and clustered star formation, often yielding massive stars.
DOI: 10.5281/zenodo.18097706
title: Datasets for Stefano Riva's PhD Thesis

description: Datasets needed to replicate the results from Stefano Riva's PhD Thesis: Advanced Data Driven Techniques for State Estimation in Nuclear Reactors.

Supervisor: Prof. Antonio CammiCo-Supervisors: Dr. Carolina Introini, Prof. J. Nathan KutzDifferent cases are included:



Molten Salt Fast Reactor: EVOL geometry

Flow over cylinder with dolfinx

Flow over cylinder from CFD Bench

MultiPhysics model of TWIGL reactor
DOI: 10.5281/zenodo.18097707
title: Datasets for Stefano Riva's PhD Thesis

description: Datasets needed to replicate the results from Stefano Riva's PhD Thesis: Advanced Data Driven Techniques for State Estimation in Nuclear Reactors.

Supervisor: Prof. Antonio CammiCo-Supervisors: Dr. Carolina Introini, Prof. J. Nathan KutzDifferent cases are included:



Molten Salt Fast Reactor: EVOL geometry

Flow over cylinder with dolfinx

Flow over cylinder from CFD Bench

MultiPhysics model of TWIGL reactor
DOI: 10.26030/a9qb-d730
title: Skeletal muscle-specific inducible AMPKα1/α2 knockout mice develop muscle weakness, glycogen depletion, and fibrosis that persists during disuse atrophy.

description: The 5' adenosine monophosphate-activated protein kinase (AMPK) is an important skeletal muscle regulator implicated as a possible therapeutic target to ameliorate the local undesired deconditioning of disuse atrophy. However, the muscle-specific role of AMPK in regulating muscle function, fibrosis, and transcriptional reprogramming during physical disuse is unknown. The purpose of this study was to determine how the absence of both catalytic subunits of AMPK in skeletal muscle influences muscle force production, collagen deposition, and the transcriptional landscape. We generated skeletal muscle-specific tamoxifen-inducible AMPKα1/α2 knockout mice that underwent 14 days of hindlimb unloading (HU) or remained ambulatory for 14 days (AMB). We found that AMPKα-/- during ambulatory conditions altered body weight and myofiber size, decreased muscle function, depleted glycogen stores and TBC1 domain family member 1 (TBC1D1) phosphorylation, increased collagen deposition, and altered transcriptional pathways. Primarily, pathways related to cellular senescence and mitochondrial biogenesis and function were influenced by the absence of AMPKα. The effects of AMPKα-/- persisted, but were not worsened, following hindlimb unloading. Together, we report that AMPKα is necessary to maintain skeletal muscle quality.
DOI: 10.5281/zenodo.18098524
title: Analysis Scripts and Datasets for a Longitudinal Study on Yoga Nidra

description: This repository contains the research data and analysis pipeline for a longitudinal study evaluating the impact of Yoga Nidra on psychological well-being and cognitive performance. The study was conducted at the National Resource Centre for Value Education in Engineering (NRCVEE), IIT Delhi.

The repository includes the following components:





Quantitative Datasets: Longitudinal data for clinical scales (GAD-7, PHQ-9, PSQI, POMS, SWLS, and PSS) and cognitive performance tasks (1-back, 2-back, and Trail Making Test A/B).




Qualitative Data: Anonymized participant feedback and experiential reflections collected post-intervention, prepared for Reflexive Thematic Analysis.




Demographic Data: Baseline participant information, including age, gender, and physical characteristics.




Statistical Analysis Pipeline: Four Jupyter Notebooks (.ipynb) providing the complete Python code for:





Baseline demographic comparisons.




Parametric testing (Welch’s t-tests, paired t-tests) and normality checks (Shapiro-Wilk, Kolmogorov-Smirnov).




Robust non-parametric testing (Mann-Whitney U, Wilcoxon signed-rank) and bootstrapped 95% confidence intervals.




Detailed subgroup analyses Segmented by clinical severity and gender.





These resources are provided to ensure the transparency and reproducibility of the study's results regarding yogic relaxation interventions.
DOI: 10.15468/dl.f5pf8z
title: Occurrence Download

description: A dataset containing 1970997 species occurrences available in GBIF matching the query:
{
 "and" : [
 "GadmGid is USA",
 "Geometry POLYGON((-127.52547 23.19591,-63.73949 23.19591,-63.73949 51.24512,-127.52547 51.24512,-127.52547 23.19591))",
 "OccurrenceStatus is Present",
 "TaxonKey is Nymphalidae",
 "Year 1925-2025"
 ]
}

 The dataset includes 1970997 records from 135 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0069358-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.5281/zenodo.18098328
title: Dataset for "Dynamical Classification of Galactic Open Clusters Using Virial Theorem"

description: This dataset contains the masses, observed and theoretical velocity dispersions, and dynamical states of 4,809 candidate clusters derived in this work. The data are drawn from Gaia DR3 astrometric measurements and the open cluster catalog by Hunter & Reffert (2024).
DOI: 10.5281/zenodo.18097852
title: Dataset for "Dynamical Classification of Galactic Open Clusters Using Virial Theorem"

description: This dataset contains the masses, observed and theoretical velocity dispersions, and dynamical states of 4,809 candidate clusters derived in this work. The data are drawn from Gaia DR3 astrometric measurements and the open cluster catalog by Hunter & Reffert (2024).
DOI: 10.48577/jpl.w5qql0
title: Post-Wildfire Sediment Fluxes and Turbidity Plumes in a Coastal-Draining Watershed

description: Coastal watersheds impacted by wildfires experience higher erosion resulting in increased sediment delivery to the ocean that alters limiting factors (i.e., light) for marine organisms. With increasing wildfire magnitude and severity, it is critical to explore changes in riverine discharges to the ocean to assess cascading hazards associated with wildfires. In situ data, remotely sensed turbidity data, and hydrological model (Soil and Water Assessment Tool “SWAT”) simulations have been adapted to capture and investigate fire-related land use change impacts on Malibu Creek, California, USA. Modifying SWAT land cover inputs using burn severity data had minimal impact on simulations, requiring additional parameterization for acceptable model performance. Remotely sensed turbidity, in situ discharge, rating curve sediment loads, and SWAT simulated discharge and sediment loads increased following the Woolsey Fire. When compared to in situ and rating curve data in similar non-fire water years, the 2019 Woolsey Fire water year in situ discharge was 1.8 times higher, SWAT simulated discharges were 1.4–1.7 times higher, and rating curve sediment load was 1.3 times higher. However, the SWAT simulated sediment loads were slightly lower (0.8–0.9 times) than rating curve sediment loads in similar non-fire water years. Mean coastal turbidity increased to 18.2 Formazin Nephelometric Unit (FNU) during the first storm post-fire (mean background value of 4.3 FNU). Synergies between methods demonstrated rapid coastal sediment exports (remote sensing) and ongoing erosion post-fire (SWAT). These data are essential to understanding fire-related marine ecological changes and implementing effective management and conservation initiatives.
DOI: 10.15468/dl.d27gkj
title: Occurrence Download

description: A dataset containing 748 species occurrences available in GBIF matching the query:
{
 "and" : [
 "OccurrenceStatus is Present",
 "TaxonKey is Chiasmocleis bassleri"
 ]
}

 The dataset includes 748 records from 42 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0069368-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.