  We present ${\tt NRPMw}$, an analytical model of gravitational-waves from
neutron star merger remnants informed using 618 numerical relativity (NR)
simulations. ${\tt NRPMw}$ is designed in the frequency domain using a
combination of complex Gaussian wavelets. The wavelet's parameters are
calibrated to equations of state (EOS) insensitive relations from NR data. The
NR simulations are computed with 21 EOS (7 of which are finite-temperature
microphysical models, and 3 of which contain quark phase transitions or
hyperonic degrees of freedom) and span total binary masses $M\in[2.4,3.4]~{\rm
M}_\odot$, mass ratios up to $q=2$, and (nonprecessing) dimensionless spins
magnitudes up to ${0.2}$. The theoretical uncertainties of the EOS-insensitive
relations are incorporated in ${\tt NRPMw}$ using recalibration parameters that
enhance the flexibility and accuracy of the model. ${\tt NRPMw}$ is NR-faithful
with fitting factors ${\gtrsim}0.9$ computed on an independent validation set
of 102 simulations.
