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355 results for “collapses”

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zenodo36/100

Data relating to "Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal"

<p>Data describe the evolution of a population of millisecond pulsars (MSPs) born from Accretion Induced Collapse.</p> <p>Data entries are comma-separated.</p> <p>The formation and subsequent evolution of 9194 MSPs have been modelled with code based on the BSE Code [see&nbsp;Hurley, J. R., Pols, O. R. &amp; Tout, C. A. Comprehensive analytic formulae for stellar evolution as a function of mass and&nbsp;metallicity. Mon. Not. Roy. Astron. Soc. 315, 543&ndash;569 (2000)].</p> <p>For each MSP, the first row describes the magnetic field B (in Gauss) and the&nbsp;inclination angle (i,&nbsp;in radians) between magnetic &amp; rotational axes.</p> <p>These quantities (B,i) do not evolve.</p> <p>Thus, every row containing only two entries indicates the beginning of the data covering a separate&nbsp;MSP.<br> For subsequent rows, there are seven entries in each row.</p> <p>The first entry in each row is the (discretised) time in units of Gyr&nbsp;since the star formation event when the MSP is formed. 0.1 is the minimum time possible time for which an MSP can be born.&nbsp;Subsequent&nbsp;discrete time steps are&nbsp;0.1 Gyr.&nbsp;The last row for every MSP is for a time of 15.9 Gyr.&nbsp;</p> <p>Subsequent entries show (as a function of time)</p> <p>period (in s)</p> <p>period derivative dP/dt (s/s)</p> <p>NS mass (in units of solar masses)</p> <p>secondary mass&nbsp;(in units of solar masses)</p> <p>secondary type (for an explanation of secondary type label see&nbsp;Hurley, J. R., Pols, O. R. &amp; Tout, C. A. Comprehensive analytic formulae for stellar evolution as a function of mass and&nbsp;metallicity. Mon. Not. Roy. Astron. Soc. 315, 543&ndash;569 (2000).</p> <p>orbital separation</p>

opencc-by-4.0Mar 2022View details →
zenodo36/100

Dissipation-enhanced collapse singularity of a nonlocal fluid of light in a hot atomic vapor

<p>This repository contains the data presented in the manuscript titled &quot; Dissipation-enhanced collapse singularity of a nonlocal fluid of light in a hot atomic vapor &quot; by P.Azam et al., Phys. Rev. A <strong>104</strong>, 013515 &ndash; Published 15 July 2021</p> <p>The .zip file contains a folder for each figure, a folder (&quot;mesures&quot;) with the full dataset and analyzed measured and a code .mat to plot fig 1,2,3,6.</p> <p>Codes to plot fig 4 and 5 are in respective folders.</p>

opencc-by-4.0Apr 2022View details →
zenodo36/100

Supporting Information for "Geochemical evidence for diachronous uplift and synchronous collapse of the high elevation Variscan hinterland"

<p>Supplemental data for GLR manuscript submission.</p>

opencc-by-4.0Jul 2022View details →
zenodo36/100

Data for COLLAPSE: A representation learning framework for identification and characterization of protein structural sites

<p>Data for methods described in the paper&nbsp;&quot;COLLAPSE: A representation learning framework for identification and characterization of protein structural sites&quot; by Alexander Derry and Russ B. Altman (BioRxiv, 2022).&nbsp;https://www.biorxiv.org/content/10.1101/2022.07.20.500713v1</p>

opencc-by-4.0Jul 2022View details →
zenodo36/100

Collapse Light

We live in strange times, times in which it's difficult to know what we feel and even more to express it. In this moment caught between the collapse and the future, between apathy and tragedy, can the aesthetics be the answer? This model was made for the #CC0RemixChallenge, so you can use it for whatever you want, following the same philosophy. #CC0RemixChallenge Source: Objaverse 1.0 / Sketchfab

opencc-byMar 2020View details →
zenodo36/100

Collapsing Ancient Temple(4096x4096)

Ancient temple, overgrown and collapsing 4096x4096 TEXTURES Built to be slightly in ground, fairly simplistic If you use in a project, please email me and let me know, I'd loved to see what you've done! Source: Objaverse 1.0 / Sketchfab

opencc-byAug 2020View details →
zenodo36/100

Gene-collapsing analysis of clonal haematopoiesis in 136,401 Admixed Americans and 416,118 Europeans

<p>We performed gene-collapsing (gene burden) analysis of germline genetic variants identified from whole-exome sequencing (WES) to identify novel inherited genetic determinants of clonal haematopoiesis (CH). Here, we provide the summary statistics from CH gene-collapsing analysis performed on Admixed Americans recruited to the Mexico City Prospective Study (MCPS), Europeans recruited to the United Kingdom Biobank (UKB), and cross-ancestry meta-analysis of Admixed Americans and Europeans. Analyses was performed with&nbsp;<span>Fisher'</span>s exact test (for MCPS and UKB analysis)&nbsp;and Cochran&ndash;Mantel&ndash;Haenszel test (for meta-analysis).</p>

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

Multilayer test masses to enhance the collapse noise

<p>multilayer.nb - Main program</p>

opencc-by-4.0Oct 2018View details →
zenodo36/100

Asymmetric core collapse of rapidly rotating massive star

<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/#abs/2018MNRAS.474.2419G/abstract">Gilkis (2018)</a>. MESA version 7624.</p> <p>Publication DOI:&nbsp;10.1093/mnras/stx2934<a href="https://doi.org/10.1093/mnras/stx2934">10.1093/mnras/stx2934</a></p>

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

The Impact of Nuclear Reaction Rate Uncertainties on the Evolution of Core-collapse Supernova Progenitors

<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/#abs/2018ApJS..234...19F/abstract">Fields et al. (2018)</a>. MESA version 7624.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.3847/1538-4365/aaa29b">10.3847/1538-4365/aaa29b</a></p>

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

Light-curve and spectral properties of ultrastripped core-collapse supernovae leading to binary neutron stars

<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2017MNRAS.466.2085M">Moriya et al. (2017)</a>. MESA version 7624.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.1093/mnras/stw3225">10.1093/mnras/stw3225</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

Summary statistics of the gene-based collapsing analyses for COVID-19 severity within the DeCOI WGS data set

<p>These are the summary statistics of the gene-based collapsing analyses for COVID-19 severity within the DeCOI Whole-Genome Sequencing data set from the European subcohort (n=1,017).</p> <p>Case - control definitions:<br>Ex (file: DeCOI_EUR_Ex_RVAS.tsv.gz): 272 cases (required mechanical ventilation or died because of COVID-19 = WHO score 6-10); 362 controls (not hospitalized = WHO score 1-3)<br>B1 (file: DeCOI_EUR_B1_RVAS.tsv.gz): 655 cases (at least hospitalized = WHO score 4-10); 362 controls (not hospitalized = WHO score 1-3)</p> <p>Column description:<br>CHROM: Chromosome of the respective gene<br>ID: Column of the format: [Ensemble Gene ID].[mask which was used to select variants].[upper alle frequency cut-off]<br>ALLELE0: The reference allele<br>ALLELE1: The alternative allele and the effect allele - here all variants which pass allele frequency and mask filters (see ID-column)<br>A1FREQ: Total frequency of Allele 1<br>A1FREQ_CASES: Frequency of Allele 1 in cases<br>A1FREQ_CONTROLS: Frequency of Allele 1 in controls<br>N: Count of individuals that were used in the analysis<br>N_CASES: Count of cases that were used in the analysis<br>N_CONTROLS: Count of controls that were used in the analysis<br>TEST: Test-mode of regenie - here an additive model was used<br>BETA: Estimated effect size given as beta<br>SE: Standard error of BETA<br>LOG10P: Negative decadic logarithm of the p-value</p> <p>Method:<br>Please refer to our accompanying manuscript for a detailed description. We conducted gene-based collapsing analysis using regenie 3.2.4 in logistic regression mode (without step 1). Covariates used were sex, age, age*age, age*sex and the first 10 principal components derived from common variants.</p> <p>Contact for further information:<br>dac_decoi_hostgenetics@listen.uni-bonn.de</p>

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

Collapse of a freestanding rock pillar at Matterhorn Hörnligrat: daily high-resolution images show kinematic precursor

<p>Animated time series of manually selected pictures highlights the visible displacement of a freestanding rock pillar at Matterhorn H&ouml;rnligrat two weeks prior the collapse. Data used are available under https://doi.pangaea.de/10.1594/PANGAEA.967586 (Weber et al., 2024).</p>

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

Three-dimensional simulations of rapidly rotating core-collapse supernovae: finding a neutrino-powered explosion aided by non-axisymmetric flows

<p>Those are movies of numerical supernova models, which appear&nbsp;in&nbsp;Takiwaki, Kotake, and Suwa 2016&nbsp;Monthly Notices of the Royal Astronomical Society: Letters, Volume 461, Issue 1, p.L112-L116.</p> <p>&nbsp;</p> <p>&nbsp;</p>

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

Yields from paper: ALUMINIUM-26 FROM MASSIVE BINARY STARS II. ROTATING SINGLE STARS UP TO CORE-COLLAPSE AND THEIR IMPACT ON THE EARLY SOLAR SYSTEM

<p>Title: Aluminium-26 From Massive Binary Stars II: ROTATING SINGLE STARS UP TO CORE-COLLAPSE AND THEIR IMPACT ON THE EARLY SOLAR SYSTEM<br> Authors: Brinkman H.E., den Hartogh J. W., Doherty C.L., Pignatari M., Lugaro M.<br> ================================================================================<br> Description of contents: A .tar.gz package containing three files with the complete set<br> of yields from the models presented in this paper. YieldsNR.txt contains the yields for the<br> non-rotating models and Yields150.txt and Yields300.txt the yields for the models<br> rotating at an initial velocity of 150 and 300 km/s, respectively.</p> <p>================================================================================</p>

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

Performance and limits of a shallow-water model for landslide-generated tsunamis: from laboratory experiments to simulations of flank collapses at Montagne Pelée (Martinique) - DATASETS

<p>Datasets of the 6 presented experiments with 4mm beads presented in the paper &quot;Performance and limits of a shallow-water model for landslide-generated tsunamis: from laboratory experiments to simulations of flank collapses at Montagne Pel&eacute;e (Martinique)&quot;.</p> <p>Each datasets (csv file) corresponds to the hand picked profile of either the water free surface or the granular material at 0.1 second of interval.&nbsp;</p> <p>The third&nbsp;dataset for each experiment corespond of the gauges records.</p>

opencc-by-4.0Nov 2022View details →
zenodo36/100

Supplemental Information in Support of "Moment tensor event identification for collapses"

<p>Supplemental Information in support of manuscript &quot;Moment tensor event identification for collapses&quot;.</p> <p>File 00_Collapse_MT_Table.csv is a summary of moment tensor solutions for all of the collapses in this manuscript.</p> <p>A Jupyter notebook (file 00_Collapse_MT_Table.ipynb) is provided which loads the information from the provided table and creates an example plot of one of the full moment tensor solutions and plots all the solutions on a global map. The notebook creates two PNG images mt.png and map.png which are also provided.</p> <p>Directories (e.g., 1980-06-12_Southern_Nevada) contain figures showing waveform fits for the collapses. For each event, the waveforms to the left show displacement data (black) and synthetics (red - used in inversion, blue - predicted only) for the vertical, radial, and transverse components.&nbsp; Detailed information about the event and the moment tensor solution are provided on the right-hand side of the last figure.</p>

opencc-by-4.0Dec 2022View details →
zenodo36/100

Implications of large binding energies of massive stripped core collapse supernova progenitors on the explosion mechanism

<p>Inlist files&nbsp;(r15140) used for the creation of the core-collapse progenitor models in the paper &quot;The implications of large binding energies of massive, stripped, core-collapse supernova progenitors on the explosion mechanism&quot;. Based on the&nbsp;&lsquo;20M pre ms to core collapse&rsquo; example from MESA r22.05, adapted for use in r15140, and include several variations as detailed in the paper appendix A. See README.txt for running details and example script.</p> <p>Also included are the full simulation list and the&nbsp;profiles of the 52 simulated cases, including the pre-collapse profiles&nbsp;at the point of termination for the 27 models that reached collapse. Profiles are at central oxygen depletion (5% abundance at center), central silicon depletion (5% abundance at center) and collapse, as defined in the paper.</p>

opencc-by-4.0Jan 2023View details →
dryad36/100

Data on range-wide breeding habitat use of the critically endangered Yellow-breasted Bunting Emberiza aureola after population collapse

<p>The population of the Yellow-breasted Bunting <em>Emberiza aureola</em>, a formerly widely distributed and abundant songbird of northern Eurasia, suffered a catastrophic decline and a strong range contraction between 1980 and 2013. There is evidence that the decline was driven by illegal trapping during migration, but potential contributions of other factors to the decline, such as land-use change, have not yet been evaluated. Before effects of land-use change can be evaluated, a basic understanding of the ecological requirements of the species is needed. We therefore compared habitat use in ten remaining breeding regions across the range, from European Russia to Japan and the Russian Far East. We also assessed large-scale variation in habitat parameters across the breeding range.</p> <p>We found large variation in habitat use, within and between populations. Differences were related to the cover and height of trees and shrubs at Yellow-breasted Bunting territories. In many regions, Yellow-breasted Buntings occupied early successional stages, including anthropogenic habitats characterized by mowing, grazing or fire regimes. We found that the probability of presence can be best predicted with the cover of shrubs, herbs and grasses. Highest probabilities were found at shrub cover values of 40 to 70 %.</p> <p>Differences in habitat use along a longitudinal gradient were small, but we found strong differences across latitudes, possibly related to habitat availability. We conclude that the remaining Yellow-breasted Bunting populations are not limited to specific habitat types. Our results provide important baseline information to model the range-wide distribution of this critically endangered species and to guide targeted conservation measures.</p>

opencc-zeroFeb 2022View details →

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