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97 results for “Helium”

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zenodo36/100

Electron Captures on 14N as a Trigger for Helium Shell Detonations

<p>MESA inlists, run_star_extras and patches associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2017ApJ...845...97B">Bauer et al. (2017)</a>. MESA version 8118.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.3847/1538-4357/aa7ffa">10.3847/1538-4357/aa7ffa</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

A possible formation channel for blue hook stars in globular cluster - II. Effects of metallicity, mass ratio, tidal enhancement efficiency and helium abundance

<p>MESA inlists and run_star_extras associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2016MNRAS.463.3449L">Lei et al. (2016)</a>. MESA version 7211.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.1093/mnras/stw2242">10.1093/mnras/stw2242</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Carbon Shell or Core Ignitions in White Dwarfs Accreting from Helium Stars

<p>MESA inlists and run_star_extras associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2016ApJ...821...28B">Brooks et al. (2016)</a>. MESA version 7624.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.3847/0004-637X/821/1/28">10.3847/0004-637X/821/1/28</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

AM Canum Venaticorum Progenitors with Helium Star Donors and the Resultant Explosions

<p>MESA inlists and run_star_extras associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2015ApJ...807...74B">Brooks et al. (2015)</a>. MESA version 5118.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.1088/0004-637X/807/1/74">10.1088/0004-637X/807/1/74</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Accretion-induced Collapse from Helium Star + White Dwarf Binaries

<p>MESA inlists and run_star_extras associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2017ApJ...843..151B">Brooks et al. (2017)</a>. MESA version 7624.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.3847/1538-4357/aa79a6">10.3847/1538-4357/aa79a6</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: evolution to the end of core helium burning

<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2015MNRAS.447.3115J">Jones et al. (2015)</a>. MESA version 3709.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.1093/mnras/stu2657">10.1093/mnras/stu2657</a></p> <p>Files are also available in a gihub repository <a href="https://github.com/swjones/mesa-Teile/tree/master/Jones.etal.2015.MNRAS.447.4.3115">here</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Dataset for strain-localisation in helium implanted tungsten: CPFE, Laue diffraction, AFM

<p>The folder includes dataset for helium-implanted tungsten and pure tungsten. The data includes measurement of the following for both materials&nbsp; as observed experimentally, and predicted using crystal-plasticity simulations:</p> <p>1. Surface morphology of nano-indents,</p> <p>2. Lattice-distortions around and under nano-indents</p> <p>3. Computed&nbsp;geometrically necessary dislocations field around and under nano-indents in both materials</p> <p>4. Load-displacement curves</p> <p>Guidelines for using dataset:</p> <p>1. Extracting the folder will generate five individual folders</p> <p>2. In the AFM plots folder, use the matlab code and dataset in the the folder to generate the surface morphology of nano-indents.</p> <p>3. In the &quot;CPFE implanted sample data&quot; folder --&gt; use &quot;CPFE implanted matlab code&quot; --&gt; load &quot;variables2&quot; --&gt; run the code (raw data is also provided in the folder)</p> <p>4.&nbsp;In the &quot;CPFE unimplanted sample data&quot; folder --&gt; use &quot;CPFE unimp matlab code&quot; --&gt; load &quot;variables3&quot; --&gt; run the code&nbsp;(raw data is also provided in the folder)</p> <p>5. In the &quot;Laue unimplanted data&quot; folder --&gt; use matlab code with relevant raw data provided in folder</p> <p>6. In the &quot;Laue implanted data&quot; folder --&gt; use matlab code with relevant raw data provided in folder</p> <p>7. Excel sheet provides nano-indentation and CPFE predictions of load-displacement curves</p> <p>8. The folder &quot;HR-EBSD code and data&quot; includes related raw data and codes.</p>

opencc-by-4.0May 2019View details →
zenodo36/100

Animations for "Remnants of Subdwarf Helium Donor Stars Ejected from Close Binaries with Thermonuclear Supernovae"

<p>Movies showing time evolution of the density in the z=0 plane for each of the seven Athena++ models in the paper. Each movie file corresponds to one model, labeled according to donor model number and the kinetic energy of the explosion in units of 10<sup>51</sup> ergs.</p>

opencc-by-4.0Oct 2019View details →
zenodo36/100

The variable evolution of accretor stars in binary systems due to accretion of increasingly helium-rich material

<p>Dataset for paper "The variable evolution of accretor stars in binary systems due to accretion of increasingly helium-rich material".</p> <p>You will need the <a href="https://github.com/Krytic/Kaitiaki">Kaitiaki code</a>.</p>

opencc-by-4.0Nov 2024View details →
zenodo36/100

Multidimensional Parameter Study of Double Detonation Type Ia Supernovae Originating from Thin Helium Shell White Dwarfs

<p>This dataset provides the end-state ejecta data for each of the simulations from Boos et al. 2021, along with condensed versions for use in radiative transfer calculations.</p>

opencc-by-4.0Sep 2021View details →
zenodo36/100

High-pressure x-ray diffraction data for arsenolite and its inclusion compound with helium

<p>X-ray diffraction data for arsenolite and its inclusion compound collected at the European Synchrotron Radiation Facility.</p>

opencc-by-4.0Oct 2021View details →
zenodo36/100

High-pressure X-ray diffraction data for arsenolite helium inclusion compound

<p>High-pressure x-ray diffraction data for arsenolite inclusion compound with helium collected at the European Synchrotron Radiation Facility.</p>

opencc-by-4.0Oct 2021View details →
zenodo36/100

Giant Tidal Tails of Helium Escaping the Hot Jupiter HAT-P-32 b

<p>This dataset contains materials presented&nbsp;in the paper ``Giant Tidal Tails of Helium Escaping the Hot Jupiter HAT-P-32 b&#39;&#39; (Zhang et al. 2023) accepted for publication by&nbsp;Science Advances. Please cite this paper&nbsp;and the&nbsp;Zenodo repository&nbsp;if these data&nbsp;are used in your work.</p> <p>Description of these files:&nbsp;</p> <ul> <li><strong>HPF_data.zip</strong> includes all 77 observed HPF spectral data of HAT-P-32 A+b.</li> <li><strong>HAT-P-32b_properties.csv</strong> includes our measured spectroscopic and&nbsp;physical properties of the planetary system. Columns of this file are explained in a README file&nbsp;<strong>README_HAT-P-32b_properties.dat</strong></li> <li><strong>3d_simulation_EW_vs_orbital_phase.dat</strong> includes the helium excess equivalent widths&nbsp;as a function of the planet&#39;s orbital phase, as predicted by&nbsp;our 3D hydrodynamic simulations</li> <li><strong>3d_simulation_orbital_phase_vs_helium_central_wavelength.dat</strong> includes the central wavelength of helium excess spectral feature (in the stellar restframe) as a function of the planet&#39;s orbital phase, as predicted by our 3D hydrodynamic simulations.&nbsp;</li> </ul>

opencc-by-4.0Apr 2023View details →
ClinicalTrials.gov36/100

Helium-oxygen Gas Mixtures Delivered by a High Flow Nasal Cannula in Bronchiolitis

ClinicalTrials.gov study NCT02373683. IPD Sharing: Not stated. Countries: 1. Publications: 10.

restrictedIPD-UNDECIDEDFeb 2026View details →
ClinicalTrials.gov36/100

Study of the Effect of VX-770 on Hyperpolarized Helium-3 Magnetic Resonance Imaging in Subjects With Cystic Fibrosis and the G551D Mutation

ClinicalTrials.gov study NCT01161537. IPD Sharing: Not stated. Countries: 1. Publications: 1.

restrictedIPD-UNDECIDEDFeb 2026View details →
dryad36/100

Alpha and helion particle charge radius difference by spectroscopy of quantum-degenerate helium

Open the record for dataset details and reuse information.

publicApr 2025View details →
dryad36/100

Data from: A pulsar-helium star compact binary system formed by common envelope evolution

Open the record for dataset details and reuse information.

publicAug 2025View details →
zenodo32/100

LiF data pack supporting "Observation of diffraction contrast in scanning helium microscopy"

<p>All the experimental data from the paper is included in this data pack including both the images and the z scans.&nbsp;</p> <p>Images from the paper are presented in three different formats with filenames scan00*****:</p> <p>1) .png file which is an unprocessed image of the raw data.&nbsp;<br> 2) .gwy file which is an unprocessed version of the data that can be opened in Gwyddion<br> 3) .mat file which contains all the measured data that can be opened in MATLAB</p> <p>The .mat file contains the most information and requires some explanation to easily understand.<br> The data is saved in a structure named meas, the key fields are as follows:</p> <p>meas.target - A matrix of the target position for each pixel, with a column for each of the x,y coordinates<br> meas.inputs - Input parameters used in the scanning program to collect the data<br> meas.initial_pos - Position of each the three stages at the start of the scan. The 3rd coordinate is the z scan and does not change throughout the scan<br> meas.data - A vector of the measured current at each pixel in Amps<br> meas.image &nbsp;- A matrix that represents the acquired image</p> <p>The remaining fields are explained at the bottom of the readme.</p> <p>The z scans are saved Z*****.mat and can be opened in MATALB.<br> The key variables in the data files are:</p> <p>z_position - Raw z coordinate of the positioner in nm<br> current_z - Measured current at each point in Amps<br> m - Horizontal scan gradient (approximately 1)<br> m2 - Vertical scan gradient (approximately 0)<br> step_pos - x coordiate at z_position=0<br> step_pos_v - y coordinate at z_position=0</p> <p>The x,y position at each point in the scan can then be obtained from<br> x=step_pos + m*(z_position)<br> y=step_pos_v + m2*(z_position)</p> <p><br> The true z distance between the pinhole and the sample in nm can be calculated from z=z_position-4295000</p> <p>The included data in the pack contains:</p> <p>Images presented in the paper:<br> scan001357<br> scan001361<br> scan001398<br> scan001415</p> <p>Z000006.mat - z scan of flat region<br> Z000008.mat - z scan of heavily distorted region<br> Z0000012.mat - z scan of lightly distorted region<br> Z000013.mat - z scan of HOPG</p> <p>z_scan_movie.avi - Video illustrating how the images vary with z<br> scan001401-scan001413 - Data to produce the video</p> <p>In addition, the analysis scripts have been included for reference.&nbsp;<br> The scripts can be used to regnerate the figures in the paper.</p> <p><br> The remaining fields in the meas structure are:<br> meas.date_time - Start date and time of the scan<br> meas.type - Scan pattern of the image. Always raster_jump<br> meas.p1 - Unused pressure<br> meas.p2 - Unused pressure<br> meas.p3 - Unused pressure<br> meas.p_srce - Source pressure at the start of the scan<br> meas.p_diff - Differential stage pressure at the start of the scan<br> meas.p_smpl - Sample pressure at the start of the scan<br> meas.p_det - Detector pressure at the start of the scan<br> meas.N_dwell - Number of current measurements taken at each pixel<br> meas.comments - comments (unused)<br> meas.det_params - Detector parameters used in the scan<br> meas.labtemp - A vector of the labtemp at each pixel (unused)<br> meas.return_state - Error status&nbsp;<br> &nbsp;</p>

opencc-by-4.0Dec 2019View details →
zenodo32/100

3D lookup tables for helium-graphene interaction for uniaxially strained graphene in the armchair direction

<p>Data files containing the 3D lookup tables for the helium-graphene Lennard Jones interaction for&nbsp;uniaxially strained graphene in the armchair direction from 0$\AA$ to 10$\AA$. Path integral Monte Carlo simulations can be performed using these data files and our open source code located <a href="https://code.delmaestro.org/">here</a>.</p>

opencc-by-4.0Jul 2020View details →
zenodo32/100

On The Impact of 22Ne On The Pulsation Periods of Carbon-Oxygen White Dwarfs With Helium Dominated Atmospheres

<p>This file contains the python scripts needed to re-produce figures 2-11&nbsp;in our paper. &nbsp;It also contains the information to re-run our 22Ne tests and other WD mass models. &nbsp;The README.md file contains a more detailed description of the data. &nbsp;</p>

opencc-by-4.0Sep 2020View details →

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allen-brain-atlas
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dandi-nwb
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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.

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