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2,960 results for “elements”
Fig. 1 in Understanding UCEs: A Comprehensive Primer on Using Ultraconserved Elements for Arthropod Phylogenomics
Fig. 1. Breakdown of the number of arthropod UCEs-based publications per year (as of July 2019) by taxonomic group and taxonomic hierarchy.
Discontinuous Galerkin spatial discretisation of the neutron transport equation with pyramid finite elements and a discrete ordinate (SN) angular approximation.
<p>In accordance with EPSRC funding requirements this folder contains all raw data relevant to the named paper: </p> <p>Discontinuous Galerkin spatial discretisation of the neutron transport equation with pyramid finite elements and a discrete ordinate (SN) angular approximation.</p> <p><br> Journal: Annals of Nuclear Energy</p> <p> </p>
A Unified Framework to Analyze Transposable Element Insertion Polymorphisms using Graph Genomes
<p>GraffiTE_analyses_scripts_and_data_052924 <br>**********************************************</p> <p>Contact/info: goubert.clement@gmail.com </p> <p>Figures: <br>^^^^^^<br>This directory contains all the files and R script necessary to reproduce the data figures of the manuscript. </p> <p>GraffiTE pMEs datasets:<br>^^^^^^^^^^^^^^^^^^<br>This directory contains new pMEs datasets produced by GraffiTE for the different models presented in the manuscript. All datasets have been filtered according to the descriptions given in the Methods and Supplementary Methods sections of the manuscript. These data, along with more intermediate file, metadata and analysis script used to produce the figure are also available in the "Figures" directory.</p> <p> </p>
Metadata description regarding a study "Competitiveness and value creation: Longitudinal analysis of sawmills and wood construction element producers in Finland"
<p>This dataset is supplied by a commercial information service and is subject to usage restrictions. As such, the dataset itself cannot be publicly shared. This metadata description offers detailed information about the dataset's content and structure.</p>
De novo assemblies for the manuscrip "Candida albicans isolates contain frequent heterozygous structural variants and transposable elements within genes and centromeres"
Open the record for dataset details and reuse information.
Equilibrium chemical composition of impact-produced hot cloud during isentropic expansion. The initial temperature T0 is 4000 K, the initial pressure P0 is 5, 20, and 80 bar. Calculations are performed using the EQL program. Abundances of considered species are presented in molar fractions.The elemental composition of impact-produced cloud is taken as a mixture of CI chondrite, mare basalts, and ferroan anorthosite with a ratio of 1:25:25 by mass as in Berezhnoy (2013).
<p>Considered species include ions, neutral gas-phase species, and condensates. Ions are written as ...(+) (for example, Al(+)). Condensates (solids and liquids) are written as ...(c) or ...(c;...). Examples of condensates are Al2O3(c) and Al2O3(c; gamma). For species marked in theirs names as (cr, l) in Gurvich et al. (1989) (for example, Al2O3(cr, l)) it is possible to determine a state of matter (liquid or solid). The content of studied species is 0 if the relative molar fraction is less than 1e-21. </p> <p>The elemental composition of impact-produced cloud is taken as a mixture of CI chondrite, mare basalts, and ferroan anorthosite with a ratio of 1:25:25 by mass as in Berezhnoy (2013). </p> <p>Calculations of the equilibrium chemical composition of impact-produced clouds were performed starting from an initial temperature of 4000 K at different initial pressures of 5, 20, and 80 bar, corresponding to entropies equal to 7.2, 5.56, and 4.25 kJ / (kg×K), respectively. </p> <p>Berezhnoy, A.A., 2013. Chemistry of impact events on the Moon. Icarus 226, 205-211.</p> <p>Gurvich L.V., Veitz I.V. et al. Thermodynamic properties of individual substances. Fourth edition in 5 volumes. Hemisphere Pub Co. New York-London, 1989.</p>
Nutrients, alkalinity (AT), dissolved inorganic carbon (CT) and trace elements in Kongsfjorden, Svalbard July 2020
<p>Original data set for <strong>‘‘The Influence of Glaciers on Biogeochemical Cycles of Carbon, Nutrients and Trace Elements in Arctic Fjord Systems‘‘ </strong>contributing to <span>European Union’s Horizon 2020 research and innovation program under Grant Agreement No. 86938. </span> </p> <p>Data includes basic information (sample name, date, coordinates, depth), primary water column parameters (salinity, temperature, turbidity), dissolved (<22 µm) trace elements (dAl, dV, dFe, dMn, dCo, dNi, dCu, dZn, dCd, dPb), dissolved (<22 µm) nutrients (nitrate, nitrite, silicate, phosphate) and carbonate system parameters (alkalinity and dissolved inorganic carbon) for each sample.</p> <p> </p>
Evidence for compensatory evolution within pleiotropic regulatory elements
<p>In this archive we provide data and code to reproduce the results of our paper:<br>"Evidence for compensatory evolution within pleiotropic regulatory elements" by Kliesmete et al.</p>
Trace element and sulfur isotope study of sulfide chimneys from the basalt-hosted Daxi Vent Field: implications on the genesis of seafloor massive sulfide deposit at a segment end
<p>The dataset file is Table S1-S6 in the supporting information of the article entitled "Trace element and sulfur isotope study of sulfide chimneys from the basalt-hosted Daxi Vent Field: implications on the genesis of seafloor massive sulfide deposit at a segment end".</p>
Data for J-PLUS: Beyond spectroscopy III. Stellar parameters and elemental-abundance ratios for five million stars from DR3
<p>The table contains stellar atmospehric parameters (Teff, logg, [Fe/H]), luminosity classification, element abundance ratios ([C/Fe], [Mg/Fe] and [alpha/Fe]), distance and age for over five million stars derived using J-PLUS DR3 + Gaia EDR3.</p><p>It includes the following parameters:</p><p>ra: Right Ascension from J-PLUS DR3 (J2000)</p><p>dec: Declination from J-PLUS DR3 (J2000)</p><p>gl: Galactic longitude derived from ICRS coordinates</p><p>gb: Galactic latitude derived from ICRS coordinates</p><p>mag[12]: Magnitudes of J-PLUS twelve bands (r, g, i, z, u, J0378, J0395, J0410, J0430, J0515, J0660, J0861)</p><p>err_mag[12]&Uncertainties of magnitudes of J-PLUS twelve bands (r, g, i, z, u, J0378, J0395, J0410, J0430, J0515, J0660, J0861)</p><p>gp1/rp1/ip1: Magnitudes from Pan-STARRS1</p><p>err_gp1/rp1/ip1: Uncertainties of magnitudes from Pan-STARRS1</p><p>G/BP/RP: Magnitudes for the Gaia three bands from EDR3; note G represents a calibration-corrected G magnitude</p><p>err_G/BP/RP: Uncertainties of magnitudes for the three Gaia bands from EDR3</p><p>ebv_sfd: Value of E(B - V) from the extinction map of SFD98, corrected for a 14% systematic</p><p>[Fe/H]: Photometric metallicity</p><p>err_[Fe/H]: Uncertainty of photometric metallicity</p><p>flg_[Fe/H]: Quality flag of [Fe/H]</p><p>[C/Fe]: Photometric carbon-to-iron abundance ratio</p><p>err_[C/Fe]:Uncertainty of photometric carbon-to-iron abundance ratio</p><p>flg_[C/Fe]: Quality flag of [C/Fe]</p><p>[Mg/Fe]: Photometric magnesium-to-iron abundance ratio</p><p>err_[Mg/Fe]: Uncertainty of photometric magnesium-to-iron abundance ratio</p><p>flg_[Mg/Fe]: Quality flag of [Mg/Fe]</p><p>[alpha/Fe]: Photometric alpha-to-iron abundance ratio</p><p>err_[alpha/Fe]: Uncertainty of photometric alpha-to-iron abundance ratio</p><p>flg_[alpha/Fe]: Quality flag of [alpha/Fe]</p><p>Teff: Effective temperature</p><p>err_Teff: Uncertainty of effective temperature</p><p>logg: Surface gravity</p><p>err_logg: Uncertainty of surface gravity</p><p>dist: Distance </p><p>err_dist: Uncertainty of distance</p><p>flg_dist: Flag to indicate the method used to derive distance, which takes the values ``parallax", ``CMF", and ``NO"</p><p>age: Stellar age</p><p>err_age: Uncertainty of stellar age</p><p>rv: Radial velocity</p><p>err_rv: Uncertainty of radial velocity</p><p>flg_rv: Flag to indicate the source of radial velocity, which takes the values ``GALAH", ``APOGEE'', ``Gaia",``RAVE", ``LAMOST", ``SEGUE"</p><p>parallax: Parallax from {it Gaia} EDR3</p><p>err_parallax: Uncertainty of parallax from {it Gaia} EDR3</p><p>pmra: Proper motion in Right Ascension direction from Gaia EDR3</p><p>err_pmra: Uncertainty of proper motion in Right Ascension direction from Gaia EDR3</p><p>pmdec: Proper motion in Declination direction from Gaia EDR3</p><p>err_pmdec&Uncertainty of proper motion in Declination direction from Gaia EDR3</p><p>ruwe: Renormalised unit weight error from Gaia EDR3</p><p>type: Flag to indicate classifications of stars, which takes the values ``dwarf" and ``giant" </p><p>subtype: Flag to indicate further sub-classifications of dwarf stars, which takes the values ``TO", ``MS" and ``Binary"</p>
Geographic Information System of structural elements in the Niobe-Aphrodite Map Area of Venus: a tool for structural and geologic analysis.
<p>The Niobe Aphrodite Map Area covers over 25% of the surface of Venus and extends from 57N to 57S and 60E to 180E. The structural-element map presented here is derived from the1:10 M-scale geologic maps of Niobe Planitia, U.S. Geological Survey I-2467 and Aphrodite Terra, U.S. Geological Survey I-2476. Both maps are in various stages of review and revision overseen by the U.S. Geological Survey on behalf of NASA.</p> <p>Here we present a Geographic Information System (GIS) that contain the different structural elements of the area (deformation structures and lithodemic units), that can be used to analyze relationships between and among suites of structural elements across this large portion of Venus’ surface.</p> <p>Base images and data on which determination of the structural element determination is based can be accessed and downloaded directly in GIS-ready formats through the USGS Map a Planet website (https://astrogeology.usgs.gov/tools/map-a-planet-2).</p>
Supplementary material 1 from: Derkarabetian S, Starrett J, Tsurusaki N, Ubick D, Castillo S, Hedin M (2018) A stable phylogenomic classification of Travunioidea (Arachnida, Opiliones, Laniatores) based on sequence capture of ultraconserved elements. ZooKeys 760: 1-36. https://doi.org/10.3897/zookeys.760.24937
Data Table. Taxon sample and UCE sequencing results : Explanation note: Samples highlighted in red were sequenced for Starrett et al. (2017).
Files for "Ocellaris: a discontinuous Galerkin finite element solver for two-phase flows with high density differences"
<p>Input files and scripts sufficient to reproduce the results shown in the paper "Ocellaris: a discontinuous Galerkin finite element solver for high density ratio two phase flows".</p> <p>A version of Ocellaris similar to version 2019.0.1 was used and all results should be reproducible by this version of Ocellaris. See <a href="https://bitbucket.org/ocellarisproject/ocellaris/">the Ocellaris source code repository</a>, <a href="https://pypi.org/project/ocellaris/2019.0.1/">Ocellaris 2019.0.1 on PyPi</a>, or DOI <a href="https://zenodo.org/record/2558303">10.5281/zenodo.2558303</a>.</p> <p>The Ocellaris user guide can be found at <a href="https://www.ocellaris.org">www.ocellaris.org</a> and it includes guides to how to run Ocellaris in Singularity or Docker containers for ease of installation and testing. Containers for Ocellaris 2019.0.0 are available, for Docker run:</p> <pre><code class="language-bash"># On the host machine: docker run -it trlandet/fenics-dev:2018.1.0.r3 # Inside the Docker container pip3 install ocellaris==2019.0.1 --user </code></pre> <p> </p>
FIGURE 5. Trichomycterus zonatus, lateral views. A in The type specimens of Trichomycterus alternatus (Eigenmann, 1917) and Trichomycterus zonatus (Eigenmann, 1918), with elements for future revisionary work (Teleostei: Siluriformes: Trichomycteridae)
FIGURE 5. Trichomycterus zonatus, lateral views. A—holotype, FMNH 58573, 52.3 mm SL, Água Quente; B and C, paratypes, FMNH 58574, 42.8–46.9 mm SL, same locality as holotype (specimen C illustrated in Eigenmann (1918, pl 51, fig 1)); D—paratype, FMNH 58572, 50.7 mm SL, Cubatão, 7 miles west of Santos, São Paulo, Brazil.
FIGURE 1 in The type specimens of Trichomycterus alternatus (Eigenmann, 1917) and Trichomycterus zonatus (Eigenmann, 1918), with elements for future revisionary work (Teleostei: Siluriformes: Trichomycteridae)
FIGURE 1. Geographical provenance of type material of Trichomycterus alternatus and Trichomycterus zonatus. Red star— T. alternatus, holotype FMNH 58082 and paratypes FMNH 58083; yellow star—T. zonatus, holotype FMNH58573 and paratypes FMNH 58574; yellow circle—T. zonatus paratype FMNH 58572.
FIGURE 7 in The type specimens of Trichomycterus alternatus (Eigenmann, 1917) and Trichomycterus zonatus (Eigenmann, 1918), with elements for future revisionary work (Teleostei: Siluriformes: Trichomycteridae)
FIGURE 7. Stereo triplet of Trichomycterus zonatus holotype FMNH58573. 3D effects: A+B, dorsal view; B+C, ventral view. See text (Material and Methods) for further explanation.
lil, left ilium;; lti, left tibia; pd, pedal digits; and ub, unidentified bony element. The white box indicates the position from which the sample was taken for histological analysis. Scale bars, 10 mm (a, c, d), 20 mm (b). in A new Jurassic scansoriopterygid and the loss of membranous wings in theropod dinosaurs
lil, left ilium;; lti, left tibia; pd, pedal digits; and ub, unidentified bony element. The white box indicates the position from which the sample was taken for histological analysis. Scale bars, 10 mm (a, c, d), 20 mm (b).
Description of the monitoring analysis and evaluation of the new façade elements for building envelopes in both new construction and renovation.
<p>Deliverable with descritpion of Eco-Binder demo buildings</p>
Fig. 3. Select appendicular elements from RSM P2523.8. A in An Older and Exceptionally Large Adult Specimen of Tyrannosaurus rex
Fig. 3. Select appendicular elements from RSM P2523.8. A, The left scapula in lateral view. B, The right femur in anterior view. C, The right fibula in anterior view. D, Right pedal phalanx IV-1 in right lateral view.
text-fig. 20. Mandible of Erlikosaurus andrewsi (a) and Oviraptor philoceratops (b) in lateral view, illustrating different states for characters 72, 75, and 77. For sources of reconstructions and identifications of the elements, see ext-figur^ 6. Scale bars represent 50 mm. in The interrelationships and evolution of basal theropod dinosaurs
text-fig. 20. Mandible of Erlikosaurus andrewsi (a) and Oviraptor philoceratops (b) in lateral view, illustrating different states for characters 72, 75, and 77. For sources of reconstructions and identifications of the elements, see ext-figur^ 6. Scale bars represent 50 mm.
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Allen Brain Atlas
Allen Brain Atlas is an Allen Institute collection of brain map atlases, datasets, APIs, and analysis tools covering mouse, human, and non-human primate brain resources.
Annotated Behaviour and Observability Dataset (ABODe)
ABODe is a University of Edinburgh DataShare dataset for behavior classification in group-housed mice using home-cage video, identities, bounding boxes, ground-plate positions, and annotator labels.
DANDI Archive for NWB datasets
DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.
International Brain Laboratory public data
The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.
OpenNeuro
OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.