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6 results for “COMPAS”
Dataset from: Rapid stellar and binary population synthesis with COMPAS
<p>This data set is used to produce Figure 16 of the COMPAS Paper (<a href="https://arxiv.org/abs/2109.10352">Team COMPAS et al. 2021</a>).</p> <p>The file contains the output of 10,000,000 binaries evolved using COMPAS v02.21.00, using adaptive importance sampling (STROOPWAFEL) , sampling from a metallicity uniform in <span class="math-tex">\(\log(Z) \in [10^{-4},0.03]\)</span>. More details can be found in the `Run_Details` group.</p> <p>*****************************<br> Contents<br> *****************************</p> <ol> <li>COMPAS simulation output:<br> The hdf5 file Includes necessary information about the simulated binaries in the following groups:<br> <br> <strong>BSE_Double_Compact_Objects<br> BSE_Common_Envelopes<br> BSE_RLOF<br> BSE_Supernovae<br> BSE_System_Parameters<br> Run_</strong><strong>Details</strong><br> <br> We point the reader to the documentation at <a href="https://compas.science/docs">https://compas.science/docs</a>, for information and instructions regarding the contained data.<br> </li> <li><strong>Rate Data</strong><br> The hdf5 file contains 1 groups with BBH merger rate data for every BBH with an inspiral time that is smaller than the age of the Universe. This group contains a dataset "DCOmask" which can be used to point from the "DoubleCompactObjects" to the data contained in the respective rates datasets.<br> <br> We include the rates for one realization of the metallicity-dependent SFRD as discussed in the manuscript.<br> The metallicity-dependent SFRD used is the phenomenological metallicity-dependent SFRD as described in Neijssel et al. 2019, this contained in:<br> <strong>'Rates_mu00.035_muz-0.23_alpha0.0_sigma00.39_sigmaz0.0'</strong></li> </ol> <p>*****************************</p> <p>The rates were calculated by running ```FastCosmicIntegration.py``` from COMPAS's post-processing tools.<br> For a more detailed explanation of the workings of COMPAS's post-processing tools, please the docs <a href="https://compas.science/docs">https://compas.science/docs</a></p>
COMPAS v02.27.05 output at representative metallicities
<p>This dataset contains the output data of rapid binary population synthesis produced using COMPAS v02.27.05. The details of the initial conditions and setup are described in the "COMPAS_settings_table.pdf" file. We simulate 5 million binaries, at representative metallicities, and store them in HDF5 files, the default format for COMPAS simulations. Each HDF5 file contains the following groups:</p> <ul> <li> ‘/BSE_Common_Envelopes’</li> <li> ‘/BSE_Double_Compact_Objects’</li> <li> ‘/BSE_Supernovae’</li> <li> ‘/BSE_System_Parameters’</li> <li> ‘/Run_Details’</li> </ul> <p>For details about the data, such as variable names and attributes, visit the <a href="https://compas.readthedocs.io/en/latest/">compas.readthedocs.io</a>.<br> The metallicities chosen for the simulations are:</p> <ol> <li>Z=0.0001: the lowest metallicity accounted for in our stellar evolution tracks;</li> <li>Z=0.0002: a proxy metallicity for I Zwicky 18;</li> <li>Z=0.001;</li> <li>Z=0.0021: a proxy metallicity for the Small Magellanic Cloud;</li> <li>Z=0.0047: a proxy metallicity for the Large Magellanic Cloud;</li> <li>Z=0.01;</li> <li>Z=0.0142: a metallicity representative of the Sun;</li> <li>Z=0.02: a super-solar metallicity, aka "old Solar";</li> <li>Z=0.03: the highest metallicity accounted for in our stellar evolution tracks;</li> <li>U[log<sub>10</sub>(0.0001), log<sub>10</sub>(0.03)]: log-uniformly distributed metallicities from the COMPAS metallicities.</li> </ol> <p>This results in 50 million binaries in total.</p> <p>In addition to the Table in the "COMPAS_settings_table.pdf" file, we include a "Run Details" text file, which contains the setup as specified via COMPAS, for a particular batch of the Z=0.02 simulation. This file contains a representative description of the global properties of all the 10 simulations, but some details, e.g. Clock-Time, vary from batch to batch.</p> <p>For questions, comments, or suggestions, contact compas-user@googlegroups.com or visit <a href="https://compas.science/">compas.science/</a>.<br> Visit <a href="https://github.com/TeamCOMPAS/COMPAS">Team COMPAS Github page</a> to get access to the source code.<br> Finally, if you use any of these data, we kindly request that, in recognition of this team effort, the paper is cited as:</p> <p>Team COMPAS: J. Riley et al., “Rapid Stellar and Binary Population Synthesis with COMPAS”, <em>The Astrophysical Journal Supplement Series</em>, vol. 258, no. 2, 2022. <a href="https://iopscience.iop.org/article/10.3847/1538-4365/ac416c/meta">doi:10.3847/1538-4365/ac416c</a>.</p>
COMPAS (Clinical Otitis Media & Pneumonia Study): Pneumonia & Acute Otitis Media (AOM ) Efficacy Study of the Pneumococcal Conjugate Vaccine
ClinicalTrials.gov study NCT00466947. IPD Sharing: YES. Countries: 3. Publications: 3.
ComPAS Low-WAZ RCT Mali
ClinicalTrials.gov study NCT05248516. IPD Sharing: YES. Countries: 1. Publications: 1.
TMC114IFD3001 - Study Providing Continued Access to Treatment With Darunavir (DRV)/Ritonavir(Rtv) in HIV1 Infected Adults, Adolescents and Children Aged 3 Years or Above and Coming From Previous Compa
ClinicalTrials.gov study NCT01281813. IPD Sharing: Not stated. Countries: 8. Publications: 0.
An Immediate Implant Will be Placed Using the MiniNaviDent System and Static Guide. A Postoperative CBCT Scan Will Then be Acquired and Superimposed Onto the Preoperative CBCT Scan to Assess and Compa
ClinicalTrials.gov study NCT07380360. IPD Sharing: UNDECIDED. Countries: 1. Publications: 0.
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