Listening to the Horizon: Probing Near-Horizon Reflectivity with GW250114

Testing the horizon properties of astrophysical black holes is a central goal of gravitational-wave astronomy. The recently identified Direct Wave (DW), a prompt non-quasinormal component of GW250114, provides a new probe of near-horizon physics. While it remains unclear whether the DW itself carries horizon information, we show that it enables a novel null test of horizon reflectivity. If the remnant is an exotic compact object (ECO) with a partially reflecting surface, inward plunge radiation is reflected and leaks back through the gravitational potential barrier, producing a delayed DW echo whose amplitude is set by the surface reflectivity ($\mathrm{\mid }{\mathcal{R}}_s\mathrm{\mid }$). We construct the corresponding echo template, normalized by the observed DW, and search for it in quasinormal-mode-filtered data. We find no evidence for an echo ($\ln \mathcal{B}=-2.9$) and obtain the 90% credible bound $\mathrm{\mid }{\mathcal{R}}_s\mathrm{\mid }<0.06$, corresponding to a reflected energy fraction below $0.4\mathrm{\%}$, for surfaces from $0.1M_f$ to a Planck length from the would-be horizon. Our method thus turns the prompt ringdown signal into a direct test of horizon reflectivity.