Published October 1, 2024 | Version 1.0

Galactic Populations of LISA DWD Binaries

  • 1. ROR icon Goddard Space Flight Center
  • 2. ROR icon Carnegie Mellon University
  • 3. ROR icon Princeton University
  • 4. Rochester Institute of Technology

Description

These COSMIC simulation outputs and assembled galactic populations of
    Double White Dwarf (DWD) binaries
    represent the work published by V. Delfavero et al,
    in https://arxiv.org/abs/2409.15230

The COSMIC version used in these simulations is 3.4.10

The git repository for the accompanying code which built this dataset
    will be available at https://gitlab.com/xevra/basil-cosmic
    upon the publication of our article.

Also useful is the fork of ldasoft used in this pipeline:
    https://github.com/xevra/ldasoft

Please cite this work if you use the included data in a publication.

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Summary
-------------------------------------------------------------------------------
Params_[MODEL].ini
    This initialization file was used for COSMIC, 
       for the runs tagged with [MODEL].

[MODEL]_[KSTAR1]_[KSTAR2]_[METALLICITY_BIN].tar.gz
    This tarball contains the outputs from one run of COSMIC,
        using Params_[MODEL].ini, for a type of binary indicated by
        [KSTAR1] and [KSTAR2] according to COSMIC syntax,
        and for the [METALLICITY_BIN]'th metallicity bin.

[MODEL]_COSMIC.hdf5
    This hdf5 database holds the DWD population outputs for all 60
        COSMIC simulations in a compressed format.
    It only holds information about binary systems at the end
        of evolution (conv, according to COSMIC syntax).
    It does not contain the evolutionary history of individual binaries
        (the bpp information, according to COSMIC syntax).

[MODEL]_m12i-000_LISA.nal.hdf5
    This hdf5 database holds the LISA "resolved" population of DWD binaries
        for a single realization of a Milky-Way-like galaxy.
    It also stores many attributes indicating assumptions and various
        population statistics.
    The "nal" extension indicates that this database contains
        truncated Gaussian likelihood models for the resolved population
        of LISA DWDs,
        which can be loaded by the gwalk code (https://gitlab.com/xevra/gwalk).
    This database can also be explored by any hdf5 library (such as h5py).

[MODEL]_m12i-000_LISA.hdf5
    This hdf5 database holds all of the LISA-band binaries (f_GW > 10^-4 Hz)
        for a single galaxy realization.

[MODEL]_m12i-000_LISA.txt.gz
    This text file stores the inputs for ldasoft gbfisher analysis,
        for a specific galaxy realization under assumptions
        broadly described by [MODEL]

See README.txt for full description

-------------------------------------------------------------------------------
Funding
-------------------------------------------------------------------------------
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. ROS gratefully acknowledges support from NSF awards NSF PHY-1912632, PHY-2012057, PHY-2309172, AST-2206321, and the Simons Foundation. JB is supported by the NASA LISA Project Office.

We acknowledge software packages used in this publication, including NUMPY (Harris et al. 2020), SCIPY (Virtanen et al. 2020), MATPLOTLIB (Hunter 2007), ASTROPY (Astropy Collaboration et al. 2013, 2018), H5PY (Collette 2013), LEGWORK (Wagg et al. 2022), and ldasoft Littenberg et al. (2020). This research was done using resources provided by the Open Science Grid (Pordes et al. 2007; Sfiligoi et al. 2009), which is supported by the National Science Foundation awards #2030508 and #1836650, and the U.S. Department of Energy’s Office of Science

Files

README.txt

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Additional details

Related works

Is supplement to
Preprint: arXiv:2409.15230 (arXiv)

Software

Repository URL
https://gitlab.com/xevra/basil-cosmic
Development Status
Unsupported