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4,634 results for “orbit”
Distribution. Angola, DR Congo, Malawi, Mozambique, Tanzania, and Zambia. Description. Head-body 46:5-47-8 cm (males), 44-45-5 cm (females), tail 40-43 cm (males), 38-39 cm (females), hindfoot 8:7-9-8 cm (males), 8-9 cm (females), ear 4-7-5-4 cm (males), 5-1-5-8 cm (females); weight 1-3-2 kg. The coat color is pale ocher, with brownish or grayish tones; melanistic individuals are quite common. The throat and chest are blackish, and the ventral pelage varies from creamy white to dirty white. The stripes and spots on the body vary from different hues of brown to black. The nuchal stripes run as two parallel lines from the nape to the shoulders, where they diverge and enlarge towards the elbows; they are not so conspicuously marked as in other genet species. Below them, a pair of thinner stripes and small spots are scattered on the shoulders and sides of the neck. A third pair of thinner, parallel stripes runs down the neck between the nuchal stripes, extending to about one fourth of the mid-dorsal line, where they vanish or diverge as the first row of flank spots. The black mid-dorsal line is continuous and is flanked on each side by four rows of oblong to squared spots, and by a few small-scattered spots below. There is a dorsal erectile crest. The face has a dark mask and a pair of white sub-ocular spots. The tail has seven to nine black rings, alternating with pale rings; the intervening white spaces are pigmented with a brownish tinge on the dorsal midline. The width of the pale rings relative to the dark rings in the middle of the tail is 50-75%; the tip of the tail is dark. The hindlimbs and forelimbs are black; there are white hairs on the metacarpals and metatarsals. [he posterior parts of the feet are dark. There are two pairs of teats. The posterior chamber of the auditory bulla is not ventrally inflated and has a continuous curve line on the external side. The ratio between the inter-orbital constriction and frontal width is 1-00 + 0-12. Dental formula: 13/3, C1/1,P 4/4, M 2/2 = 40. in Viverridae
Distribution. Angola, DR Congo, Malawi, Mozambique, Tanzania, and Zambia. Description. Head-body 46:5-47-8 cm (males), 44-45-5 cm (females), tail 40-43 cm (males), 38-39 cm (females), hindfoot 8:7-9-8 cm (males), 8-9 cm (females), ear 4-7-5-4 cm (males), 5-1-5-8 cm (females); weight 1-3-2 kg. The coat color is pale ocher, with brownish or grayish tones; melanistic individuals are quite common. The throat and chest are blackish, and the ventral pelage varies from creamy white to dirty white. The stripes and spots on the body vary from different hues of brown to black. The nuchal stripes run as two parallel lines from the nape to the shoulders, where they diverge and enlarge towards the elbows; they are not so conspicuously marked as in other genet species. Below them, a pair of thinner stripes and small spots are scattered on the shoulders and sides of the neck. A third pair of thinner, parallel stripes runs down the neck between the nuchal stripes, extending to about one fourth of the mid-dorsal line, where they vanish or diverge as the first row of flank spots. The black mid-dorsal line is continuous and is flanked on each side by four rows of oblong to squared spots, and by a few small-scattered spots below. There is a dorsal erectile crest. The face has a dark mask and a pair of white sub-ocular spots. The tail has seven to nine black rings, alternating with pale rings; the intervening white spaces are pigmented with a brownish tinge on the dorsal midline. The width of the pale rings relative to the dark rings in the middle of the tail is 50-75%; the tip of the tail is dark. The hindlimbs and forelimbs are black; there are white hairs on the metacarpals and metatarsals. [he posterior parts of the feet are dark. There are two pairs of teats. The posterior chamber of the auditory bulla is not ventrally inflated and has a continuous curve line on the external side. The ratio between the inter-orbital constriction and frontal width is 1-00 + 0-12. Dental formula: 13/3, C1/1,P 4/4, M 2/2 = 40.
Response of East Asian Precipitation to Precessional Orbital Forcing during Glacials –Sensitivity to Model Spatial Resolution
<p>Output data (precipitation, wind vector, etc) from three resolution experiments (F19,F09,F05) . LGM means Last glacial maximum. cntl means control run(21ka), HighSolin means the orbital year modified to 174ka. Please see more in the publication. </p>
accelerations from the accelerometer, orbit determination and CoM offset
<p>accelerations from the accelerometer, orbit determination and CoM offset</p>
Simulation data for the article "On the Effect of the Large Magellanic Cloud on the Orbital Poles of Milky Way Satellite Galaxies"
<p>This archive contains the data shared in the context of the "On the Effect of the Large Magellanic Cloud on the Orbital Poles of Milky Way Satellite Galaxies" article.</p> <p>In particular, it contains the initial conditions and final snapshots of our N-body simulation.</p>
Data for 'Experimental Determination of a Single Atom Ground State Orbital through Hyperfine Anisotropy'
<p>This folder contains the raw data and scripts used for the paper <em>'Experimental Determination of a Single Atom Ground State Orbital through Hyperfine Anisotropy'</em>.</p>
The Data for Gaseous Dynamical Friction on Elliptical Keplerian Orbits
<p>The results for the the changing orbital elements of single perturbers and equal mass binaries due to Gaseous Dynamical Friction. The arrays ecc0, Mp represent the eccentricities and Mach numbers over which the change in semi-major axis (adot) eccentricity (edot) and precession (omegadot) are calculated. </p>
Emergent flat band and topological Kondo semimetal driven by orbital-selective correlations
Open the record for dataset details and reuse information.
Data from: "Eddington envelopes: The fate of stars on parabolic orbits tidally disrupted by supermassive black holes" (Price et al. 2024)
<p>The paper by Price et al. (2024; <a href="https://arxiv.org/abs/2404.09381">arXiv:2404.09381</a>) simulates the tidal disruption of a one solar mass polytropic star by a million-solar-mass supermassive black hole, using the Phantom general relativistic smoothed particle hydrodynamics code (Price et al. 2018). The code used to perform the simulations is available at:</p> <p><a href="https://github.com/danieljprice/phantom">https://github.com/danieljprice/phantom</a></p> <p>This dataset contains:</p> <ol> <li>Scripts, intermediate data products and other small files used to create each figure in the paper</li> <li>Selected snapshots and other raw data from the four main calculations shown in the paper</li> </ol> <p>The main datasets contain parameter files and snapshots from the simulations used to create figures in the paper.small data files from the simulations and post-processing scripts used to create the scientific results and figures shown in the paper. Each simulation dataset contains:</p> <p><strong>.setup file:</strong> parameter file used by phantomsetup to create the initial conditions for the star itself<br><br><strong>.in file:</strong> parameter file used by phantom to perform the calculation<br><br><strong>tde_00000, tde_00100, tde_00200 etc:</strong> binary code snapshots containing raw data (particle positions, velocities, thermal energy, etc), these can be read/visualised/converted using the free and open source codes SPLASH (Price et al. 2007):<br><br><a href="https://github.com/danieljprice/splash">https://github.com/danieljprice/splash</a></p> <p>or Sarracen:</p> <p><a href="https://github.com/ttricco/sarracen">https://github.com/ttricco/sarracen</a></p> <p>SPLASH was used to create figures in the paper. The format and ways to read these data files are described in:</p> <p><a href="https://phantomsph.readthedocs.io/en/latest/user-guide/dumpfile.html">https://phantomsph.readthedocs.io/en/latest/user-guide/dumpfile.html</a></p> <p><strong>tde01.ev, tde02.ev etc:</strong> ascii files (see header) containing global quantities like total angular momentum, total momentum, total energy etc as a function of time. Each number corresponds to a restart of the code (i.e. resubmission of the job to the queue on the cluster).</p> <p><strong>tde01.log, tde02.log: </strong>output log from the simulations themselves, this contains some useful information like the unit scalings, typical timestep and code performance, hardware information etc.</p> <p><em><strong>.defaults, .limits, .units and .filenames:</strong> parameter files used by SPLASH to create particular figures. For example, to use the files lightcurve.defaults, lightcurve.units, lightcurve.limits and lightcurve.filenames one would plot using splash -p lightcurve</em></p> <p>The relevant raw data directories are:</p> <p><strong>beta1_hres: </strong>raw data from the adiabatic, beta=1 calculation</p> <p><strong>beta5_hres:</strong> raw data from the adiabatic, beta=5 calculation</p> <p><strong>beta1_isentropic: </strong>raw data from the isentropic, beta=1 calculation with a non-spinning black hole</p> <p><strong>beta1_isentropic_kerr_a99_i60:</strong> raw data from the isentropic, beta=1 calculation with a maximally-spinning black hole with the initial stellar orbit at an incliation of 60 degrees to the black hole spin</p> <p><strong>The procedure to recreate each figure and post-processing analysis used in the paper is explained in the README.md placed in each directory unpacked from the figureX.zip file</strong></p> <p> </p>
Diverse Orbital-scale Variations of Precipitation Oxygen Isotopes in the Northern Hemisphere Mid-latitudes: A Comparative Study Between East Asia and North America
<p>The isotope-enabled climate model output data and the corresponding NCL codes used for the paper "Li et al., 2024: Diverse orbital-scale variations of precipitation oxygen isotopes in the Northern Hemisphere mid-latitudes: A comparative study between East Asia and North America".</p>
Accompanying Files for "M/K-Dwarf Exoplanets With Similar Sizes and Instellations to Earth Typically Follow Near-Circular Orbits"
<p>=== gammaposteriors.tar.gz ===</p> <p>Each file (in the tarball) is named after the corresponding planetary object. The file contains samples drawn from the a-posteriori distribution of rho_{*,transit}/rho_{*,independent}. This ratio is referred to as gamma in the paper.</p> <p>=== stellarposteriors.tar.gz ===</p> <p>Each file contains the joint posterior distribution for the fundamental stellar parameters. The columns are:</p> <p>Mass (Solar masses), Radius (Solar radii), Density (kg/m^3)</p> <p>=== transittimes.tar.gz ===</p> <p>A pair of files are produced for each KOI/TOI, named appropriately. The pdf figure is a summary figure showing the TTV data with errors (black), along with the best fitting sinusoidal model in brown. We also report the FAP (false alarm probability) of that signal, the associated TTV period and amplitude as annotations on the figure. We also provide the actual transit times for each epoch, in the files *times.dat, using the columns...</p> <p>Epoch, Transit Time (BJD_UTC - 2,457,000), Error, TTV (mins), Error (mins)</p> <p>=== lightcurves.tar.gz ===</p> <p>Each file contains a detrended light curve, detrended using the method marginalisation process described in the paper. The columns are:</p> <p>Time (BJD_UTC - 2,400,000*)<br>Relative Intensity<br>Uncertainty</p> <p>For the TOIs, we include a fourth column which is the CROWDSAP value.</p> <p>* For TOIs, this becomes 2,457,000</p> <p>=== hbms -> *.tar.gz ===</p> <p>Each tarball contains samples drawn from the a-posteriori joint distribution of the Hierarchical Bayesian Model (HBM) fits. Each tarball is a distinct model, and thus HBM:</p> <p>exp.tar.gz - exponential distribution<br>beta.tar.gz - Beta distribution<br>rayleigh.tar.gz - Rayleigh distribution<br>tremaine.tar.gz - Tremaine distribution<br>exp_without4087.tar.gz - exponential distribution excluding KOI-4087.01<br>beta_without4087.tar.gz - Beta distribution excluding KOI-4087.01<br>exp_without4087_fake_0p0.tar.gz - exponential distribution excluding KOI-4087.01, but applied to fake data where e=0.0</p> <p>There are two types of files in each container.</p> <p>popchain_*.dat contains posterior samples of the population/hyper-parameters.<br>hkplate_*.dat contains posterior samples of the population/hyper-parameters.</p> <p>There are 20 walkers for each file type, labelled 1-20 at the suffix of the file. The columns in each file are organised as follows...</p> <p>popchain_exp*.dat<br>mu_e, var_e, loglike<br>popchain_rayl*.dat<br>mu_e, var_e, loglike<br>popchain_trem*.dat<br>mu_e, var_e, loglike<br>popchain_beta*.dat<br>mu_e, var_e, alpha, beta, loglike</p> <p>hkplatechain_*.dat<br>h'_1, k'_1, h'_2, k'_2,...</p>
Analysis of Orbital Sounding in Context with In Situ Ground Penetrating Radar at Jezero Crater, Mars
<p>This release includes all the SHARAD data used to produce analysis and figures in the paper, "Analysis of Orbital Sounding in Context with In Situ Ground Penetrating Radar at Jezero Crater, Mars", by M.C. Raguso et al., submitted to Geophysical Research Letters in February 2024.</p> <p>The manuscript is currently under review. The dataset will be released following the completion of the review process.</p> <p>This release also includes slides (pdf format) presented during the RIMFAX Science Team meeting (09/6/22-09/09/22).</p> <p>Preferred citation (DataCite format): </p> <p>Raguso, M.C., & Nunes, D.C. (2024). Analysis of Orbital Sounding in Context with In Situ Ground Penetrating Radar at Jezero Crater, Mars. [Dataset]. Zenodo. <a href="https://doi.org/10.5281/zenodo.10681430">https://doi.org/10.5281/zenodo.10681430</a></p> <p><em>For inquiries regarding the contents of this dataset, please contact the Corresponding Author listed in the README.txt file.</em></p>
Research data for: "Band Structure Interpolation using Optimized Local Orbitals from Linear-Scaling Density-Functional Theory"
<p>This file was created by Laura E. Ratcliff on 23rd March 2018. It contains the input files employed for the ONETEP and CASTEP calculations in the above publication.</p> <p>Directory Listing:</p> <p>castep/</p> <p>Contains the input files used to generate the CASTEP reference data.</p> <p>onetep/</p> <p>Contains the input files used to generate all of the ONETEP data, where filenames are labelled with the number of repeat CNT units, val (cond) indicates a valence (conduction) calculation and the suffixes follow a similar labelling convention to that employed in the manuscript.</p>
Supporting Data for the paper titled"Diurnal Variation of Liquid Water Path Derived from Two Polar-Orbiting FengYun-3 Microwave Radiation Imagers"
<p>The dataset contains:</p> <p>a) 4 files with name indicating collocated satellite, sensor, latitude,longitude and brightness temperature; format</p> <p>b) annual mean liquid water path derived from FY-3B/C Level 1 data; satellite,sensor, region; format</p> <p>c) annual mean amplitude and phase</p> <p>d) four seasons (winter,spring,summer, and autumn) mean amplitude</p> <p>d) 24 files with name indicating sensor, lwp, region, local solar time hour, format</p> <p>All files can be read by using matlab language.</p> <p> </p> <p>The first author was supported by National Natural Science Foundation of China Grant 91337218, and the second author was supported by NOAA grant NA14NES4320003 (Cooperative Institute for Climate and Satellites-CICS) at the University of Maryland/ESSIC.</p> <p>Corresponding author: Xiaolei Zou,xzou1@umd.edu</p>
Text-fig. 3. SMNK Ma1 MP 8, right maxilla and parts of the zygomatic and frontal bones of Hippopotamodon erymanthius from Mahmutgazi, Turkey. A) lingual view, B) lateral view (arrow shows the leading edge of the orbit) (scale 10 cm). in Hippopotamodon erymanthius (Suidae, Mammalia) from Mahmutgazi, Denizli-Çal basin, Turkey
Text-fig. 3. SMNK Ma1 MP 8, right maxilla and parts of the zygomatic and frontal bones of Hippopotamodon erymanthius from Mahmutgazi, Turkey. A) lingual view, B) lateral view (arrow shows the leading edge of the orbit) (scale 10 cm).
Minimum Orbital Period of Precataclysmic Variables
<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2018arXiv180803423N">Minimum Orbital Period of Precataclysmic Variables</a></p>
Supporting data for "Spectroscopy of Quantum Dot Orbitals with In-Plane Magnetic Fields"
<p>Supporting data for<br> "Hyperfine-phonon spin relaxation in a single-electron GaAs quantum dot"<br> Leon C. Camenzind, Liuqi Yu, Peter Stano, Jeramy D. Zimmerman, Arthur C. Gossard, Daniel Loss & Dominik M. Zumbühl</p> <p><em>Phys. Rev. Lett. <strong>122</strong>, 207701 – Published 22 May 2019</em></p>
Nanoresolution real-time 3D orbital tracking for studying mitochondrial trafficking in vertebrate axons in vivo - Data Set 2
<p>The data set was analyzed in main figures 2, 3 and supplementary figure 5.</p>
Nanoresolution real-time 3D orbital tracking for studying mitochondrial trafficking in vertebrate axons in vivo - Data Set 1
<p>24.01.2014 fish 5 was analyzed in main figures 1,2 and supplementary figure 4</p> <p>21.03.2014 fish 1 was analyzed in main figures 2,3 and supplementary figure 4</p>
text-fig. 11. heropod frontals in ventral view, illustrating character states for characters 37 and 64. a, stereophotographs of articulated frontals of Allosaurus fragilis (UMNH VP 5470); anterior is to the left, b, same as a; outline drawing, c, stereophotographs of articulated posterior skull roof (frontals, parietals, laterosphenoids) of Troödon formosus (AMNH 6174); anterior is to the top. D, same as c; outline drawing. Abbreviations: ce, facet for the cerebral hemispheres on the frontals; f, frontal; 1, facets for the lacrimals; Is, laterosphenoid; lsf, facets for the laterosphenoids; o, orbital facet; ob, facets for the olfactory bulbs on the frontals; pa, parietal; prf, contact with the prefrontal. Scale bars represent 10 mm. in The interrelationships and evolution of basal theropod dinosaurs
text-fig. 11. heropod frontals in ventral view, illustrating character states for characters 37 and 64. a, stereophotographs of articulated frontals of Allosaurus fragilis (UMNH VP 5470); anterior is to the left, b, same as a; outline drawing, c, stereophotographs of articulated posterior skull roof (frontals, parietals, laterosphenoids) of Troödon formosus (AMNH 6174); anterior is to the top. D, same as c; outline drawing. Abbreviations: ce, facet for the cerebral hemispheres on the frontals; f, frontal; 1, facets for the lacrimals; Is, laterosphenoid; lsf, facets for the laterosphenoids; o, orbital facet; ob, facets for the olfactory bulbs on the frontals; pa, parietal; prf, contact with the prefrontal. Scale bars represent 10 mm.
text-fig. 4. Skull reconstructions of representatives of riassic OTUs in left lateral view, a, Euparkeria capensis, Early Triassic (Scythian-Anisian), Beaufort Group, South Africa; redrawn from Ewer (1965). B, basal ornithischian Lesothosaurus diagnostics, Early Jurassic (Hettangian-Sinemurian), Elliot Formation, Lesotho; redrawn from Sereno (1991b). c, prosauropod sauropodomorph Plateosaurus sp., Late riassic (Norian), Knollenmergel, Germany; based on MB R. 1937. D, Eoraptor lunensis, Late Triassic (Camian), Ischigualasto Formation, Argentina; based on PVSJ 512. E, Herrerasaurus ischigualastensis, Late Triassic (Camian), Ischigualasto Formation, Argentina; redrawn from Sereno and Novas (1993). F, Coelophysis bauri, Late riassic (Norian), Chinle Formation, south-western USA; modified from Paul (1993). G, Lilienstemus lilienstemi, Late riassic (Norian), Knollenmergel, Germany; based on MB R. 2175, unpreserved elements shaded. H, Shuvosaurus inexpectatus, Late riassic (Norian), Dockum Group, Texas, USA; based on TU P 9280. Abbreviations: a, angular; aof, antorbital fenestra; d, dentary; emf, external mandibular fenestra; en, external nares; eo, exoccipital; f, frontal; itf, infratemporal fenestra; j, jugal; 1, lacrimal; m, maxilla; n, nasal; o, orbit; oc, occipital condyle; op, opisthotic; pa, parietal; pd, predentary; pm, premaxilla; pm-mf, premaxillary-maxillary fenestra; po, postorbital; pof, postfrontal; q, quadrate; qf, quadrate foramen; qj, quadratojugal; sa, surangular; saf, surangular foramen; snf, subnarial foramen; sob, supraorbital; soc, supraoccipital; sp, splenial; sq, squamosal; stf, supratemporal fenestra. Scale bars represent 10 mm (a-b) and 50 mm (c-H). in The interrelationships and evolution of basal theropod dinosaurs
text-fig. 4. Skull reconstructions of representatives of riassic OTUs in left lateral view, a, Euparkeria capensis, Early Triassic (Scythian-Anisian), Beaufort Group, South Africa; redrawn from Ewer (1965). B, basal ornithischian Lesothosaurus diagnostics, Early Jurassic (Hettangian-Sinemurian), Elliot Formation, Lesotho; redrawn from Sereno (1991b). c, prosauropod sauropodomorph Plateosaurus sp., Late riassic (Norian), Knollenmergel, Germany; based on MB R. 1937. D, Eoraptor lunensis, Late Triassic (Camian), Ischigualasto Formation, Argentina; based on PVSJ 512. E, Herrerasaurus ischigualastensis, Late Triassic (Camian), Ischigualasto Formation, Argentina; redrawn from Sereno and Novas (1993). F, Coelophysis bauri, Late riassic (Norian), Chinle Formation, south-western USA; modified from Paul (1993). G, Lilienstemus lilienstemi, Late riassic (Norian), Knollenmergel, Germany; based on MB R. 2175, unpreserved elements shaded. H, Shuvosaurus inexpectatus, Late riassic (Norian), Dockum Group, Texas, USA; based on TU P 9280. Abbreviations: a, angular; aof, antorbital fenestra; d, dentary; emf, external mandibular fenestra; en, external nares; eo, exoccipital; f, frontal; itf, infratemporal fenestra; j, jugal; 1, lacrimal; m, maxilla; n, nasal; o, orbit; oc, occipital condyle; op, opisthotic; pa, parietal; pd, predentary; pm, premaxilla; pm-mf, premaxillary-maxillary fenestra; po, postorbital; pof, postfrontal; q, quadrate; qf, quadrate foramen; qj, quadratojugal; sa, surangular; saf, surangular foramen; snf, subnarial foramen; sob, supraorbital; soc, supraoccipital; sp, splenial; sq, squamosal; stf, supratemporal fenestra. Scale bars represent 10 mm (a-b) and 50 mm (c-H).
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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.