10.5281/zenodo.4751656
https://zenodo.org/records/4751656
oai:zenodo.org:4751656
Héctor Estellés
Héctor Estellés
0000-0001-6143-5532
University of the Balearic Islands
Sascha Husa
Sascha Husa
0000-0002-0445-1971
University of the Balearic Islands
Marta Colleoni
Marta Colleoni
0000-0002-7214-9088
University of the Balearic Islands
Maite Mateu-Lucena
Maite Mateu-Lucena
0000-0003-4817-6913
University of the Balearic Islands
Maria de Lluc Planas
Maria de Lluc Planas
0000-0001-8278-7406
University of the Balearic Islands
Cecilio García-Quirós
Cecilio García-Quirós
0000-0002-8059-2477
University of the Balearic Islands
David Keitel
David Keitel
0000-0002-2824-626X
University of the Balearic Islands
Antoni Ramos-Buades
Antoni Ramos-Buades
0000-0002-6874-7421
Max Planck Institut für Gravitationsphysik and University of the Balearic Islands
Data release for the paper "A detailed analysis of GW190521 with phenomenological waveform models"
Zenodo
2021
Gravitational Waves
Parameter Estimation
2021-05-13
eng
10.5281/zenodo.4751655
Creative Commons Attribution 4.0 International
Data release for an extensive analysis of the GW190521 gravitational wave event, which is consistent with a high mass binary black hole system with a very short signal, detected during the O3a observation run of the Advanced LIGO and Virgo detectors. In this analysis we use the current generation of phenomenological waveform model families, IMRPhenomX and IMRPhenomT, as implemented in the LALSuite code (https://doi.org/10.7935/GT1W-FZ16). This data release corresponds to the paper "A detailed analysis of GW190521 with phenomenological waveform models" (https://arxiv.org/abs/2105.06360), which should be cited when using these data. It contains the posterior samples of the default runs using IMRPhenomXPHM and IMRPhenomTPHM, carried out using the Markov Chain Monte Carlo (MCMC) sampling implementation of the LALInference code and their corresponding command line.