It's good advise not to use old-fashioned concepts from times where the mathematics of SR hasn't been understood in its whole glory yet. That was a very short period between 1905 and 1907, when Minkowski introduced the four-dimensional tensor formalism of the spacetime manifold, named after him Minkowski space, which is a pseudo-Euclidean affine space with a pseudometric of signature (1,3) or equivalently (3,1), depending on the convention you are used to. I'm used to the high-energy-particle physicists' "west-coast convention" with the (1,3) signature.
This leads to the covariant definition of the fundamental dynamical quantities energy, and momentum. Using the fact that after introducing a Minkowski reference frame (inertial frame) you can describe the trajectory of a massive particle by the world line, ##x^{\mu}=x^{\mu}(\tau)##, where ##x^{\mu}## are the (contravariant) components ##(x^{\mu})=(x^0,\vec{x})=(ct,\vec{x})## where ##c## is the speed of light in a vacuum, and ##\tau## is the proper time of the particle, defined by
$$\mathrm{d} \tau=\frac{1}{c} \mathrm{d} s = \frac{1}{c} \sqrt{\eta_{\mu \nu} \mathrm{d} x^{\mu} \mathrm{d} x^{\nu}}, \qquad (*)$$
where ##(\eta_{\mu \nu}=\mathrm{diag}(1,-1,-1,-1)## are the Minkowski-metric components.
Then with the invariant (Minkowski scalar) mass of the particle one defines the four-momentum (which is a Minkowski four-vector) by its components
$$p^{\mu}=m \frac{\mathrm{d} x^{\mu}}{\mathrm{d} \tau}.$$
It obeys the constraint
$$p_{\mu} p^{\mu} = (p^0)^2-\vec{p}^2=m^2 c^2,$$
which follows from the definition of the proper-time increment.
To interpret the components we check the non-relativistic limit, when ##|\vec{v}|=|\mathrm{d} \vec{x}/\mathrm{d} t| \ll c##. To that end we express the four-momentum in terms of derivatives with respect to the coordinate time. The spatial components are
$$\vec{p}=m \frac{\mathrm{d} \vec{x}}{\mathrm{d} \tau} = m \frac{\mathrm{d} \vec{x}}{\mathrm{d} t} \frac{\mathrm{d} t}{\mathrm{d} \tau} = m \gamma \vec{v},$$
where
$$\gamma=\frac{1}{\sqrt{1-\vec{v}^2/c^2}} \simeq 1+\frac{1}{2} \frac{\vec{v}^2}{c^2} + \mathcal{O(v^4/c^4)}.$$
Thus for ##|\vec{v}| \ll \vec{c}## we see that
$$\vec{p} \simeq m \vec{v} [1+\mathcal{O}(v^2/c^2)],$$
which identifies the invariant mass, ##m##, with the Newtonian limit of the mass, i.e., ##m## is just the mass known from Newtonian mechanics.
For the temporal component
$$p^0=\sqrt{m^2 c^2 + \vec{p}^2} =m c \sqrt{1+\vec{p}^2/(mc)^2} \simeq m c[1+\vec{v}^2/(2 c^2) + \mathcal{O}(v^4/c^4) ] \simeq \left (m c^2 + \frac{m}{2} \vec{v}^2 \right) \frac{1}{c}.$$
Thus we have
$$c p^0= E =c \sqrt{m^2 c^2+\vec{p}^2} \simeq m c^2+\frac{m}{2} \vec{v}^2,$$
i.e., up to an additive constant ##E_0=m c^2## (the socalled "rest energy of the particle") ##E## is the relativistic generalization of kinetic energy of Newtonian mechanics. That the rest energy is included here is crucial to make ##(p^{\mu})=(E/c,\vec{p})## a four-vector, i.e., up to a unit-conversion factor ##1/c## energy and momentum are components of a four-vector.
To describe relativistically moving particles and find corresponding dynamical laws, it's much simpler to use the manifest covariant four-vector formalism than to guess around with the non-covariant (1+3)-dimensional formalism of the early days of relativity! That's why it's not wise to use old-fashioned ideas of "relativistic mass" (sometimes they had to distinguish even between "longitudinal" and "transverse mass", leading to a complete mess compared to the modern treatment in terms of Minkowski's four-dimensional tensor formalism).