We demonstrate how to quantify the frequencydomain amplitude and phase accuracy of waveform models,
The detection of GW170817, the first neutron starneutron star merger observed by Advanced LIGO and Virgo, and its following analyses represent the first contributions of gravitational wave data to understanding dense matter. Parameterizing the high density section of the equation of state of both neutron stars through spectral decomposition, and imposing a lower limit on the maximum mass value, led to an estimate of the stars’ radii of
 Award ID(s):
 1806962
 NSFPAR ID:
 10303213
 Publisher / Repository:
 IOP Publishing
 Date Published:
 Journal Name:
 Classical and Quantum Gravity
 Volume:
 37
 Issue:
 2
 ISSN:
 02649381
 Page Range / eLocation ID:
 Article No. 025008
 Format(s):
 Medium: X
 Sponsoring Org:
 National Science Foundation
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