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

Prospects for Gravitational Wave Measurement of ZTFJ1539+5027