DOI: 10.5281/zenodo.8161148
title: Popsyn Models for StarTrack Inference Interpolation

description: The StarTrack simulation results and population synthesis results associated with our paper, Iteratively Comparing Gravitational-Wave Observations to the Evolution of Massive Stellar Binaries. We were recently accepted by PRD, and you can find an earlier manuscript on the arxiv: https://arxiv.org/abs/2303.05436 The StarTrack version used to create these simulations is from October 5th, 2022. The summary is in the K_series.hdf5 file. This contains properties of each simulation, but not of individual binaries. There is a README.txt file included which describes the data. The StarTrack outputs are in the K0XXX.tar.gz format. Since Zenodo frowns on uploading hundreds of files, these are organized by which iteration they were generated in:<br> -it_0[a-o].tar.gz contain K0100-399 (in batches of roughly 20)<br> -it_1[a-e].tar.gz contain K0400-499 (in batches of roughly 20)<br> -it_2.tar.gz contains K0500-519<br> -it_3.tar.gz contains K0520-559<br> -it_4.tar.gz contains K0560-562<br> -it_5.tar.gz contains K0563-598<br> See Table 1 in the paper for more details about how these models were generated. The popsynth outputs are in the K0XXX_sfrX.hdf5 format.<br> All of the popsynth outputs used in the paper are in the sfr2_[a-e].tar.gz files (in batches of roughly 100).<br> sfr3 files were not used in the paper, but some of them are available.<br> <br> I provide the full set of binary properties for K0559 and K0565, for both sfr2 and sfr3 (K0XXX_sfrX_full.hdf5). Due to size limitations, we were unable to provide all of the K0XXX_sfr3.hdf5 or K0XXX_sfrX_full.hdf5 files, however the authors can make them available upon request (xevra86@gmail.com).
description: ROS and VD are supported by NSF AST-1909534 and PHY-2012057. ROS, VD, and AY are supported by NSF-PHY 2012057; ROS is also supported via NSF PHY-1912632 and AST-1909534. VD is supported by an appointment to the NASA Postdoctoral Program at the NASA Goddard Space Flight Center administered by Oak Ridge Associated Universities under contract NPP-GSFC-NOV21-0031. DW thanks the NSF (PHY-1912649, PHY-2207728) for support. KB acknowledges support from the Polish National Science Center (NCN) grant Maestro (2018/30/A/ST9/00050). This material is based upon work supported by NSF's LIGO Laboratory which is a major facility fully funded by the National Science Foundation. This research has made use of data, software and/or web tools obtained from the Gravitational Wave Open Science Center (https://www.gw-openscience.org/ ), a service of LIGO Laboratory, the LIGO Scientific Collaboration and the Virgo Collaboration. LIGO Laboratory and Advanced LIGO are funded by the United States National Science Foundation (NSF) as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. Virgo is funded through the European Gravitational Observatory (EGO), by the French Centre National de Recherche Scientifique (CNRS), the Italian Istituto Nazionale di Fisica Nucleare (INFN), and the Dutch Nikhef, with contributions by institutions from Belgium, Germany, Greece, Hungary, Ireland, Japan, Monaco, Poland, Portugal, Spain. The authors are grateful for computational resources provided by the LIGO Laboratory and supported by National Science Foundation Grants PHY-0757058 and PHY-0823459. This research was done using resources provided by the Open Science Grid, which is supported by the National Science Foundation awards #2030508 and #1836650, and the U.S. Department of Energy's Office of Science.