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10 results for “interstellar medium”
Run 0 video in "Ram pressure stripping in elliptical galaxies – I. The impact of the interstellar medium turbulence"
<p>Run 0 presented in the paper "Ram pressure stripping in elliptical galaxies – I. The impact of the interstellar medium turbulence" (http://adsabs.harvard.edu/abs/2013MNRAS.428..804S or https://doi.org/10.1093/mnras/sts071).</p>
Run 5 video in "Ram pressure stripping in elliptical galaxies – I. The impact of the interstellar medium turbulence"
<p>Run 5 presented in the paper "Ram pressure stripping in elliptical galaxies – I. The impact of the interstellar medium turbulence" (http://adsabs.harvard.edu/abs/2013MNRAS.428..804S or https://doi.org/10.1093/mnras/sts071).</p>
Fig. 3 in The Deuterium Abundance in the Local Interstellar Medium
Fig. 3. Comparison of molariforms of two taxa of Megalonyx from South Carolina. A. SCSM 2006.1.101, Megalonyx leptostomus from the late Blancan Walrus Ditch Local Fauna near Summerville, in Dorchester County, South Carolina, in occlusal (A1) and lateral (A2) views. B. SCSM 2004.1.26.2, Megalonyx wheatleyi/jeffersonii from the late Irvingtonian Camelot Local Fauna near Harleyville, in Dorchester County, South Carolina, in occlusal (B1) and lateral (B2) views. While M. jeffersonii is larger than both M. leptostomus and M. wheatleyi, hypsodonty indices were statistically the same in all species.
Fig. 1 in The Deuterium Abundance in the Local Interstellar Medium
Fig. 1. Measurements used to calculate hypsodonty index (HI) in Megalonyx. HI is calculated as the depth of the mandible (DM), usually measured below the third molariform tooth (see B), divided by the length of the tooth row (LTR; see A), and multiplied by 100. Specimen displayed is AMNH F:AM 99187—mandible of Megalonyx wheatleyi from the middle Irvingtonian McLeod Mine, Florida, in occlusal (A) and lateral (B) views.
Fig. 2 in The Deuterium Abundance in the Local Interstellar Medium
Fig. 2. Drawing of Megalonyx skull, based on Leidy (1855: pls. 1 and 3) showing upper dentition in left lateral (A) and occlusal (B) views. Positions of caniniforms and molariforms are indicated. Not to scale.
Fragmentation cross-sections for cosmic ray nuclei in the interstellar medium
<p>Table of the cumulative (included ghost nuclei) and direct fragmentation cross sections <strong>on H target</strong> generated with the <a href="https://github.com/carmeloevoli/XS4GCR">XS4GCR</a> code.</p> <p>More than 3800 channels are included from Ni64 to H1.</p> <ul> <li>Tables are saved as txt files with ' ' as delimiter.</li> <li>For each row the first 4 integers represent: fragment Z, fragment A, projectile Z and projectile A</li> <li>The following 160 values are the cross sections (in mbarn) as a function of the projectile kinetic energy per nucleon</li> <li>The first row is identified with 0 0 0 0 as the first 4 values and contains the values of the kinetic energy per nucleon (log spaced between 10 MeV/n and 1 TeV/n) at which the cross sections are computed.</li> </ul>
Data from: Survival of polycyclic aromatic hydrocarbon knockout fragments in the interstellar medium
<p>Original and published data for the paper "Survival of polycyclic aromatic hydrocarbon knockout fragments in the interstellar medium", published in Nature Communications, from measurements at the DESIREE facility. See original publication for experimental details.</p> <p> </p> <p><strong>Folder structure:</strong></p> <p><em>Raw_Data</em> contains the raw particle-detector data obtained from the measurements as csv-files in two separate subdirectories. The <em>Beam_Dump</em> folder contains measurements where the ion beam is dumped onto a detector after a different time delays. The <em>Spontaneous_Decay</em> folder contains measurements of neutral particle counts as a function of ion storage time. Metadata is present in the included json-files.</p> <p>Figure_Data contains the processed data presented in the figures of the original publication as csv-files. Metadata is present in the included json-file.</p>
Derivative products: "Very Local Interstellar Medium Revealed by Complete Solar Cycle of Interstellar Neutral Helium Observations with IBEX" by Swaczyna et al.
<p>Derivative products from: Swaczyna et al. 2022, "Very Local Interstellar Medium Revealed by Complete Solar Cycle of Interstellar Neutral Helium Observations with IBEX", ApJS, under review</p>
Cartesian coordinates and rate constants obtained in "Radical Addition and H Abstraction Reactions in Ethane, Ethylene and Acetylene: A Gateway for Ethyl and Vinyl Bearing Molecules in the Interstellar Medium"
<p>Set of cartesian coordinates for reactants, pre-reactant complexes, transition states and products for the reactions presented in the manuscript "Radical Addition and H Abstraction Reactions in Ethane, Ethylene and Acetylene: A Gateway for Ethyl and Vinyl Bearing Molecules in the Interstellar Medium". </p> <p>The energy level employed in the optimisation was UMN15-D3BJ/def2-TZVP using a grid=ultrafine and the dispersion correction parameters recommended in Goerigk et al 2017 (https://pubs.rsc.org/en/content/articlelanding/2017/cp/c7cp04913g), all geometries and energies were obtained using Gaussian16 interfaced to ChemShell. </p> <p>Edit: The comment line of every structure includes its electronic energy (in Eh) and the Zero Point Vibrational Energy (in Eh).</p> <p>Edit: Additionally we included the reaction rate constants obtained with the instanton method at the level of theory mentioned above. These values serve as data behind the figure for the article. The first column of the rate constant file correspond to 1000/T in 1/K whereas the second column present the rate constant in s<sup>-1</sup></p> <p> </p>
Supplementary material "Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 μm line at z ∼ 0"
<p>Repository with supplementary material to the paper: "Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 μm line at z ∼ 0" published in Astronomy & Astrophysics.</p> <p>It contains the final datasets of luminosity predictions for the [C II] luminosity in the different EAGLE galaxies.</p>
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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.