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We compute the macroscopic entropy of the supersymmetric rotating dyonicstrings carrying linear momentum in 6D (1,0) supergravity with curvaturesquared corrections. Our calculation is based on Sen's entropy functionformalism applied to the near-horizon geometry of the string solution takingthe form of an extremal BTZ$\times S^3$. The final entropy formula states thatthe two independent supersymmetric completions of Riemann tensor squaredcontribute equally to the entropy. A further $S^3$ compactification of the 6Dtheory results in a matter coupled 3D supergravity model in which thequantization condition of the SU(2)$_R$ Chern-Simons level implies the horizonvalue of the dilaton is not modified by higher derivative interactions beyondsupersymmetric curvature squared terms.

Attractor Mechanism and Non-Renormalization Theorem in 6D (1,0) Supergravity