Fig. A.1.
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Coefficients of 2an in Eq. (A.1) for the neutron star models constructed with two different crust EOSs, NV (Negele & Vautherin 1973) and DH (Douchin & Haensel 2001). For the interior (core), we use the APR and WFF3 EOS. The open and filled marks correspond to results with NV and DH EOS, while the solid, dashed, and dotted lines correspond to the results for the 1.4M⊙, 2.0M⊙ neutron star models for the APR EOS, and 1.4M⊙ neutron star models for the WFF3 EOS.
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