TY - JOUR
T1 - Multi-messenger parameter inference of gravitational-wave and electromagnetic observations of white dwarf binaries
AU - Johnson, Peyton T.
AU - Coughlin, Michael W.
AU - Hamilton, Ashlie
AU - José Bustamante-Rosell, María
AU - Ashton, Gregory
AU - Corey, Samuel
AU - Kupfer, Thomas
AU - Littenberg, Tyson B.
AU - Reed, Draco
AU - Zimmerman, Aaron
PY - 2021/11/1
Y1 - 2021/11/1
N2 - The upcoming Laser Interferometer Space Antenna (LISA) will detect a
large gravitational-wave foreground of Galactic white dwarf binaries.
These sources are exceptional for their probable detection at
electromagnetic wavelengths, some long before LISA flies. Studies in
both gravitational and electromagnetic waves will yield strong
constraints on system parameters not achievable through measurements of
one messenger alone. In this work, we present a Bayesian inference
pipeline and simulation suite in which we study potential constraints on
binaries in a variety of configurations. We show how using LISA
detections and parameter estimation can significantly improve
constraints on system parameters when used as a prior for the
electromagnetic analyses. We also provide rules of thumb for how current
measurements will benefit from LISA measurements in the future.
AB - The upcoming Laser Interferometer Space Antenna (LISA) will detect a
large gravitational-wave foreground of Galactic white dwarf binaries.
These sources are exceptional for their probable detection at
electromagnetic wavelengths, some long before LISA flies. Studies in
both gravitational and electromagnetic waves will yield strong
constraints on system parameters not achievable through measurements of
one messenger alone. In this work, we present a Bayesian inference
pipeline and simulation suite in which we study potential constraints on
binaries in a variety of configurations. We show how using LISA
detections and parameter estimation can significantly improve
constraints on system parameters when used as a prior for the
electromagnetic analyses. We also provide rules of thumb for how current
measurements will benefit from LISA measurements in the future.
KW - Astrophysics - Instrumentation and Methods for Astrophysics
KW - Astrophysics - High Energy Astrophysical Phenomena
KW - General Relativity and Quantum Cosmology
M3 - Article
SN - 0035-8711
VL - 525
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 3
ER -