I have become utterly confused about times and velocities measured by different observers. Let us take the specific case of a Schwarzschild spacetime. When we say that there is a particle of mass m moving with 4-velocity $u^a = dx^a/d\tau$, $\tau$ is the proper time of the particle (i.e. the time registered by a clock sitting on the particle). But who is measuring the coordinate $x^a$? Is it measured by the asymptotic observer in Schwarzschild coordinates?
My next confusion is about the expression for the energy E of the particle as given by Frolov and Novikov in the book `Black Hole Physics' (p19, footnote). I am giving their argument below:
If $u^a$ is the 4-velocity of a particle of mass m moving freely in a stationary gravitational field with metric $\bf g$ (having signature $(-+++)$) then its energy \begin{align} E = - g_{00} ~c^2 ~m u^0 . \end{align} Then they claim that the energy in a static spacetime can be rewritten as \begin{align} E = \frac{\sqrt{-g_{00}}~m c^2}{\sqrt{1-v^2/c^2}} , \end{align} where $v$ is the physical three velocity s.t. \begin{align} v^2 = \frac{g_{\alpha\beta}}{-g_{00}}\frac{dx^\alpha dx^\beta}{dt^2} . \end{align} For example, for radial motion in Schwarzschild spacetime, \begin{align} E= mc^2 \frac{\sqrt{1-r_s/r}}{\sqrt{1-\dot r^2/(1-r_s/r)}} . \end{align} I do not understand how they arrived at the second expression for E in a static spacetime. I think they have used the result $$u^0 = \frac{1}{\sqrt{-g_{00}\left(1-v^2/c^2\right)}}$$ but I cannot see how it comes about.
Here, the indices $a,b,...$ run over spacetime coordinate values while $\alpha,\beta,...$ run over spatial ones. Any help would be greatly appreciated.