Prospects for Gravitational Wave Measurement of ZTFJ1539+5027

Abstract

The short-period eclipsing binary ZTFJ1539+5027 discovered by Burdge et al. (2019) will be a strong gravitational-wave source for the Laser Interferometer Space Antenna (LISA). We study how well LISA will constrain the parameters of this system by analyzing simulated gravitational wave data, and find that LISA observations will significantly improve measurements of the distance and inclination of the source, and allow for novel constraints to be placed on the speed of gravity.

5 pages, 3 figures. v2 updated Fig 3, added missing references. Accepted in ApJL

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Cited by in corpus (20)

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• An 8.8 minute orbital period eclipsing detached double white dwarf binary
• Identifying LISA verification binaries among the Galactic population of double white dwarfs
• Gravitational Wave Radiation of Double Degenerates with Extremely low-mass WD companions
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• A 1201 s Orbital Period Detached Binary: the First Double Helium Core White Dwarf LISA Verification Binary
• Circumbinary exoplanets and brown dwarfs with the Laser Interferometer Space Antenna
• Inferring the Presence of Tides in Detached White Dwarf Binaries
• Probing the speed of gravity with LVK, LISA, and joint observations
• Testing the Speed of Gravity with Black Hole Ringdown
• Possible Formation Scenarios of ZTF J153932.16+502738.8-A Gravitational Source Close to the Peak of LISA's Sensitivity
• The Discovery of Two LISA Sources within 0.5 kpc
• The LISA Data Challenge Radler Analysis and Time-dependent Ultra-compact Binary Catalogues
• Constraining the evolution of Newton's constant with slow inspirals observed from spaceborne gravitational-wave detectors
• Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
• Astrophysics with the Laser Interferometer Space Antenna
• PETRA: From the LISA global fit to a catalog of Galactic binaries
• LISA Galactic Binaries in the Roman Galactic Bulge Time-Domain Survey