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ShareScore release 0.9.0
Dataset results
3 results for “GW190521”
Data release - A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr
<p>Data release accompanying the manuscript</p> <p> "<strong>A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr</strong>" - <a href="https://arxiv.org/abs/2009.14057">Chen et al. (2020)</a></p> <p>assuming an association between the LIGO-Virgo gravitational wave signal <a href="https://www.gw-openscience.org/eventapi/html/O3_Discovery_Papers/GW190521/">GW190521</a> and the electromagnetic signal ZTF19abanrhr as identified by <a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.124.251102">Graham et al 2020</a>.</p> <p>The posterior samples for the GW analyses are available from <a href="https://doi.org/10.5281/zenodo.4057130">Isi (2020)</a> and <a href="https://dcc.ligo.org/LIGO-P2000158/public">LVC (2020)</a> respectively.</p>
Dataset: "GW190521: tracing imprints of spin-precession on the most massive black hole binary"
<p>This dataset contains the results presented in "<em>GW190521: tracing imprints of spin-precession on the most massive black hole binary</em>": <a href="https://arxiv.org/abs/2310.01544">https://arxiv.org/abs/2310.01544</a>.</p> <p>The accompanying repository used to take this data and generate the figures in the paper can be found at <a href="https://github.com/simonajmiller/gw190521-timedomain-release/">https://github.com/simonajmiller/gw190521-timedomain-release/</a>.</p>
GW190521: posterior samples conditional on AGN J1249+3449
<p>Posterior samples for the LIGO-Virgo gravitational wave signal <a href="https://www.gw-openscience.org/eventapi/html/O3_Discovery_Papers/GW190521/">GW190521</a> conditional on the location of AGN J1249+3449. This dataset contains a file with results fixing the sky location to J1249+3449 (<em>posterior_samples_GW190521_J1249+3449.h5</em>), and another additionally fixing the luminosity distance to 2511 Mpc (<em>posterior_samples_GW190521_J1249+3449_2511Mpc.h5</em>). These analyses are motivated by <a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.124.251102">Graham et al 2020</a>.</p> <p>The posteriors were sampled using LALInference (<a href="https://arxiv.org/abs/1409.7215">Veitch et al 2015</a>) with the same configuration as in the LIGO-Virgo analyses (<a href="https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.125.101102">Abbott et al 2020 PRL</a> and <a href="https://iopscience.iop.org/article/10.3847/2041-8213/aba493">Abbott et al 2020 ApJL</a>). The results were packaged using <a href="https://arxiv.org/abs/2006.06639">PESummary</a>.</p> <p>For instructions on how to load the result files, please see the PESummary <a href="https://docs.ligo.org/lscsoft/pesummary/igwn_pinned/core/read_pesummary.html">documentation</a>.</p>
ScienceDex guides
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