Illarionov open his mouth and asked the uncomfortable question. What about radius? And he got to face the truth: that we don't have precise measurements at all. And it's because basically no optical telescope can resolve such a small, distant object. It has to be derived in an indirect way by any astrophysical process and since usually the radius comes together with the mass (compactness parameter: the mass to ratio quotient) the situation becomes hard. But there's a hope: gravitational waves. By measuring gravitational wave emissions from star oscillation is possible to get a good number for the radius. In contrast the mass values are well determined mainly by binary systems, as shown in this figure.

Probably LOFT can!
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